Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Renneby, Malin Nicole - 1990- [verfasserIn] Henriques, Bruno M. B. [verfasserIn] Hilbert, Stefan - 1976- [verfasserIn] Nelson, Dylan [verfasserIn] Vogelsberger, Mark - 1978- [verfasserIn] Angulo, Raul E. [verfasserIn] Springel, Volker - 1970- [verfasserIn] Hernquist, Lars - 1954- [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2020 September 4 |
|---|
| Anmerkung: |
Gesehen am 02.08.2022 |
|---|---|
| Umfang: |
30 |
| Übergeordnetes Werk: |
Enthalten in: Monthly notices of the Royal Astronomical Society - Royal Astronomical Society, Oxford : Oxford Univ. Press, 1827, 498(2020), 4, Seite 5804-5833 |
|---|---|
| Übergeordnetes Werk: |
volume:498 ; year:2020 ; number:4 ; pages:5804-5833 ; extent:30 |
| Links: |
|---|
| DOI / URN: |
10.1093/mnras/staa2675 |
|---|
| Katalog-ID: |
1810991188 |
|---|
| LEADER | 01000caa a2200265 4500 | ||
|---|---|---|---|
| 001 | 1810991188 | ||
| 003 | DE-627 | ||
| 005 | 20240416193759.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 220720s2020 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1093/mnras/staa2675 |2 doi | |
| 035 | |a (DE-627)1810991188 | ||
| 035 | |a (DE-599)KXP1810991188 | ||
| 035 | |a (OCoLC)1341464073 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 100 | 1 | |a Renneby, Malin Nicole |d 1990- |e verfasserin |0 (DE-588)1192997557 |0 (DE-627)1671548698 |4 aut | |
| 245 | 1 | 0 | |a Joint galaxy-galaxy lensing and clustering constraints on galaxy formation |c Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist |
| 264 | 1 | |c 2020 September 4 | |
| 300 | |a 30 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 02.08.2022 | ||
| 520 | |a We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. | ||
| 700 | 1 | |a Henriques, Bruno M. B. |e verfasserin |0 (DE-588)1264156901 |0 (DE-627)181282291X |4 aut | |
| 700 | 1 | |a Hilbert, Stefan |d 1976- |e verfasserin |0 (DE-588)135796474 |0 (DE-627)57166220X |0 (DE-576)300651112 |4 aut | |
| 700 | 1 | |a Nelson, Dylan |e verfasserin |0 (DE-588)115182805X |0 (DE-627)101233600X |0 (DE-576)42382581X |4 aut | |
| 700 | 1 | |a Vogelsberger, Mark |d 1978- |e verfasserin |0 (DE-588)133437698 |0 (DE-627)546058434 |0 (DE-576)299848299 |4 aut | |
| 700 | 1 | |a Angulo, Raul E. |e verfasserin |0 (DE-588)1161140662 |0 (DE-627)1024541320 |0 (DE-576)506376567 |4 aut | |
| 700 | 1 | |a Springel, Volker |d 1970- |e verfasserin |0 (DE-588)122321391 |0 (DE-627)705861503 |0 (DE-576)293218463 |4 aut | |
| 700 | 1 | |a Hernquist, Lars |d 1954- |e verfasserin |0 (DE-588)1264244401 |0 (DE-627)1813088241 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |a Royal Astronomical Society |t Monthly notices of the Royal Astronomical Society |d Oxford : Oxford Univ. Press, 1827 |g 498(2020), 4, Seite 5804-5833 |h Online-Ressource |w (DE-627)314059164 |w (DE-600)2016084-7 |w (DE-576)090955420 |x 1365-2966 |7 nnns |
| 773 | 1 | 8 | |g volume:498 |g year:2020 |g number:4 |g pages:5804-5833 |g extent:30 |
| 856 | 4 | 0 | |u https://doi.org/10.1093/mnras/staa2675 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_U | ||
| 912 | |a GBV_ILN_2013 | ||
| 912 | |a ISIL_DE-16-250 | ||
| 912 | |a SYSFLAG_1 | ||
| 912 | |a GBV_KXP | ||
| 912 | |a GBV_ILN_11 | ||
| 912 | |a GBV_ILN_20 | ||
| 912 | |a GBV_ILN_22 | ||
| 912 | |a GBV_ILN_23 | ||
| 912 | |a GBV_ILN_24 | ||
| 912 | |a GBV_ILN_31 | ||
| 912 | |a GBV_ILN_39 | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_60 | ||
| 912 | |a GBV_ILN_62 | ||
| 912 | |a GBV_ILN_63 | ||
| 912 | |a GBV_ILN_69 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_73 | ||
| 912 | |a GBV_ILN_74 | ||
| 912 | |a GBV_ILN_95 | ||
| 912 | |a GBV_ILN_100 | ||
| 912 | |a GBV_ILN_105 | ||
| 912 | |a GBV_ILN_110 | ||
| 912 | |a GBV_ILN_120 | ||
| 912 | |a GBV_ILN_151 | ||
| 912 | |a GBV_ILN_161 | ||
| 912 | |a GBV_ILN_170 | ||
| 912 | |a GBV_ILN_213 | ||
| 912 | |a GBV_ILN_224 | ||
| 912 | |a GBV_ILN_230 | ||
| 912 | |a GBV_ILN_285 | ||
| 912 | |a GBV_ILN_293 | ||
| 912 | |a GBV_ILN_370 | ||
| 912 | |a GBV_ILN_602 | ||
| 912 | |a GBV_ILN_702 | ||
| 912 | |a GBV_ILN_2001 | ||
| 912 | |a GBV_ILN_2003 | ||
| 912 | |a GBV_ILN_2007 | ||
| 912 | |a GBV_ILN_2008 | ||
| 912 | |a GBV_ILN_2009 | ||
| 912 | |a GBV_ILN_2010 | ||
| 912 | |a GBV_ILN_2014 | ||
| 912 | |a GBV_ILN_2015 | ||
| 912 | |a GBV_ILN_2018 | ||
| 912 | |a GBV_ILN_2026 | ||
| 912 | |a GBV_ILN_2088 | ||
| 912 | |a GBV_ILN_2112 | ||
| 912 | |a GBV_ILN_2190 | ||
| 912 | |a GBV_ILN_2810 | ||
| 912 | |a GBV_ILN_4012 | ||
| 912 | |a GBV_ILN_4035 | ||
| 912 | |a GBV_ILN_4037 | ||
| 912 | |a GBV_ILN_4046 | ||
| 912 | |a GBV_ILN_4112 | ||
| 912 | |a GBV_ILN_4125 | ||
| 912 | |a GBV_ILN_4126 | ||
| 912 | |a GBV_ILN_4246 | ||
| 912 | |a GBV_ILN_4249 | ||
| 912 | |a GBV_ILN_4305 | ||
| 912 | |a GBV_ILN_4306 | ||
| 912 | |a GBV_ILN_4307 | ||
| 912 | |a GBV_ILN_4313 | ||
| 912 | |a GBV_ILN_4322 | ||
| 912 | |a GBV_ILN_4323 | ||
| 912 | |a GBV_ILN_4324 | ||
| 912 | |a GBV_ILN_4325 | ||
| 912 | |a GBV_ILN_4335 | ||
| 912 | |a GBV_ILN_4338 | ||
| 912 | |a GBV_ILN_4367 | ||
| 912 | |a GBV_ILN_4700 | ||
| 951 | |a AR | ||
| 952 | |d 498 |j 2020 |e 4 |h 5804-5833 |g 30 | ||
| 980 | |2 2013 |1 01 |x DE-16-250 |b 4170756150 |c 00 |f --%%-- |d --%%-- |e --%%-- |j --%%-- |y l01 |z 20-07-22 | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 00 |s s |a hd2020 | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 01 |s s |0 (DE-627)1410508463 |a wissenschaftlicher Artikel (Zeitschrift) | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 02 |s s |a per_8 | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 03 |s s |a s_30 | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 04 |s p |0 (DE-627)1750174588 |a Nelson, Dylan | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 04 |s k |0 (DE-627)1416822720 |a Extern | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 04 |s k |0 (DE-627)1583940421 |a Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 04 |s s |0 (DE-627)1410501914 |a Verfasser | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 04 |s s |a pos_4 | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 05 |s p |0 (DE-627)1475299141 |a Springel, Volker | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 05 |s k |0 (DE-627)1416822720 |a Extern | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 05 |s s |0 (DE-627)1410501914 |a Verfasser | ||
| 982 | |2 2013 |1 01 |x DE-16-250 |8 05 |s s |a pos_7 | ||
| author_variant |
m n r mn mnr b m b h bmb bmbh s h sh d n dn m v mv r e a re rea v s vs l h lh |
|---|---|
| matchkey_str |
article:13652966:2020----::onglxglxlnigncutrncntans |
| oclc_num |
1341464073 |
| hierarchy_sort_str |
2020 September 4 |
| publishDate |
2020 |
| allfields |
10.1093/mnras/staa2675 doi (DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 DE-627 ger DE-627 rda eng Renneby, Malin Nicole 1990- verfasserin (DE-588)1192997557 (DE-627)1671548698 aut Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist 2020 September 4 30 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 02.08.2022 We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Henriques, Bruno M. B. verfasserin (DE-588)1264156901 (DE-627)181282291X aut Hilbert, Stefan 1976- verfasserin (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 aut Nelson, Dylan verfasserin (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X aut Vogelsberger, Mark 1978- verfasserin (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 aut Angulo, Raul E. verfasserin (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 aut Springel, Volker 1970- verfasserin (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 aut Hernquist, Lars 1954- verfasserin (DE-588)1264244401 (DE-627)1813088241 aut Enthalten in Royal Astronomical Society Monthly notices of the Royal Astronomical Society Oxford : Oxford Univ. Press, 1827 498(2020), 4, Seite 5804-5833 Online-Ressource (DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 1365-2966 nnns volume:498 year:2020 number:4 pages:5804-5833 extent:30 https://doi.org/10.1093/mnras/staa2675 Verlag Resolving-System lizenzpflichtig Volltext GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 498 2020 4 5804-5833 30 2013 01 DE-16-250 4170756150 00 --%%-- --%%-- --%%-- --%%-- l01 20-07-22 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 |
| spelling |
10.1093/mnras/staa2675 doi (DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 DE-627 ger DE-627 rda eng Renneby, Malin Nicole 1990- verfasserin (DE-588)1192997557 (DE-627)1671548698 aut Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist 2020 September 4 30 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 02.08.2022 We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Henriques, Bruno M. B. verfasserin (DE-588)1264156901 (DE-627)181282291X aut Hilbert, Stefan 1976- verfasserin (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 aut Nelson, Dylan verfasserin (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X aut Vogelsberger, Mark 1978- verfasserin (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 aut Angulo, Raul E. verfasserin (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 aut Springel, Volker 1970- verfasserin (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 aut Hernquist, Lars 1954- verfasserin (DE-588)1264244401 (DE-627)1813088241 aut Enthalten in Royal Astronomical Society Monthly notices of the Royal Astronomical Society Oxford : Oxford Univ. Press, 1827 498(2020), 4, Seite 5804-5833 Online-Ressource (DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 1365-2966 nnns volume:498 year:2020 number:4 pages:5804-5833 extent:30 https://doi.org/10.1093/mnras/staa2675 Verlag Resolving-System lizenzpflichtig Volltext GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 498 2020 4 5804-5833 30 2013 01 DE-16-250 4170756150 00 --%%-- --%%-- --%%-- --%%-- l01 20-07-22 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 |
| allfields_unstemmed |
10.1093/mnras/staa2675 doi (DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 DE-627 ger DE-627 rda eng Renneby, Malin Nicole 1990- verfasserin (DE-588)1192997557 (DE-627)1671548698 aut Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist 2020 September 4 30 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 02.08.2022 We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Henriques, Bruno M. B. verfasserin (DE-588)1264156901 (DE-627)181282291X aut Hilbert, Stefan 1976- verfasserin (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 aut Nelson, Dylan verfasserin (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X aut Vogelsberger, Mark 1978- verfasserin (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 aut Angulo, Raul E. verfasserin (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 aut Springel, Volker 1970- verfasserin (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 aut Hernquist, Lars 1954- verfasserin (DE-588)1264244401 (DE-627)1813088241 aut Enthalten in Royal Astronomical Society Monthly notices of the Royal Astronomical Society Oxford : Oxford Univ. Press, 1827 498(2020), 4, Seite 5804-5833 Online-Ressource (DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 1365-2966 nnns volume:498 year:2020 number:4 pages:5804-5833 extent:30 https://doi.org/10.1093/mnras/staa2675 Verlag Resolving-System lizenzpflichtig Volltext GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 498 2020 4 5804-5833 30 2013 01 DE-16-250 4170756150 00 --%%-- --%%-- --%%-- --%%-- l01 20-07-22 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 |
| allfieldsGer |
10.1093/mnras/staa2675 doi (DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 DE-627 ger DE-627 rda eng Renneby, Malin Nicole 1990- verfasserin (DE-588)1192997557 (DE-627)1671548698 aut Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist 2020 September 4 30 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 02.08.2022 We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Henriques, Bruno M. B. verfasserin (DE-588)1264156901 (DE-627)181282291X aut Hilbert, Stefan 1976- verfasserin (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 aut Nelson, Dylan verfasserin (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X aut Vogelsberger, Mark 1978- verfasserin (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 aut Angulo, Raul E. verfasserin (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 aut Springel, Volker 1970- verfasserin (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 aut Hernquist, Lars 1954- verfasserin (DE-588)1264244401 (DE-627)1813088241 aut Enthalten in Royal Astronomical Society Monthly notices of the Royal Astronomical Society Oxford : Oxford Univ. Press, 1827 498(2020), 4, Seite 5804-5833 Online-Ressource (DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 1365-2966 nnns volume:498 year:2020 number:4 pages:5804-5833 extent:30 https://doi.org/10.1093/mnras/staa2675 Verlag Resolving-System lizenzpflichtig Volltext GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 498 2020 4 5804-5833 30 2013 01 DE-16-250 4170756150 00 --%%-- --%%-- --%%-- --%%-- l01 20-07-22 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 |
| allfieldsSound |
10.1093/mnras/staa2675 doi (DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 DE-627 ger DE-627 rda eng Renneby, Malin Nicole 1990- verfasserin (DE-588)1192997557 (DE-627)1671548698 aut Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist 2020 September 4 30 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 02.08.2022 We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Henriques, Bruno M. B. verfasserin (DE-588)1264156901 (DE-627)181282291X aut Hilbert, Stefan 1976- verfasserin (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 aut Nelson, Dylan verfasserin (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X aut Vogelsberger, Mark 1978- verfasserin (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 aut Angulo, Raul E. verfasserin (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 aut Springel, Volker 1970- verfasserin (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 aut Hernquist, Lars 1954- verfasserin (DE-588)1264244401 (DE-627)1813088241 aut Enthalten in Royal Astronomical Society Monthly notices of the Royal Astronomical Society Oxford : Oxford Univ. Press, 1827 498(2020), 4, Seite 5804-5833 Online-Ressource (DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 1365-2966 nnns volume:498 year:2020 number:4 pages:5804-5833 extent:30 https://doi.org/10.1093/mnras/staa2675 Verlag Resolving-System lizenzpflichtig Volltext GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 498 2020 4 5804-5833 30 2013 01 DE-16-250 4170756150 00 --%%-- --%%-- --%%-- --%%-- l01 20-07-22 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 |
| language |
English |
| source |
Enthalten in Monthly notices of the Royal Astronomical Society 498(2020), 4, Seite 5804-5833 volume:498 year:2020 number:4 pages:5804-5833 extent:30 |
| sourceStr |
Enthalten in Monthly notices of the Royal Astronomical Society 498(2020), 4, Seite 5804-5833 volume:498 year:2020 number:4 pages:5804-5833 extent:30 |
| format_phy_str_mv |
Article |
| building |
2013:0 |
| institution |
findex.gbv.de |
| selectbib_iln_str_mv |
2013@01 |
| sw_local_iln_str_mv |
2013:hd2020 DE-16-250:hd2020 2013:wissenschaftlicher Artikel (Zeitschrift) DE-16-250:wissenschaftlicher Artikel (Zeitschrift) 2013:per_8 DE-16-250:per_8 2013:s_30 DE-16-250:s_30 2013:Nelson, Dylan DE-16-250:Nelson, Dylan 2013:Extern DE-16-250:Extern 2013:Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" DE-16-250:Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013:Verfasser DE-16-250:Verfasser 2013:pos_4 DE-16-250:pos_4 2013:Springel, Volker DE-16-250:Springel, Volker 2013:pos_7 DE-16-250:pos_7 |
| isfreeaccess_bool |
false |
| container_title |
Monthly notices of the Royal Astronomical Society |
| authorswithroles_txt_mv |
Renneby, Malin Nicole @@aut@@ Henriques, Bruno M. B. @@aut@@ Hilbert, Stefan @@aut@@ Nelson, Dylan @@aut@@ Vogelsberger, Mark @@aut@@ Angulo, Raul E. @@aut@@ Springel, Volker @@aut@@ Hernquist, Lars @@aut@@ |
| publishDateDaySort_date |
2020-01-01T00:00:00Z |
| hierarchy_top_id |
314059164 |
| id |
1810991188 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">1810991188</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240416193759.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">220720s2020 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1093/mnras/staa2675</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)1810991188</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)KXP1810991188</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1341464073</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Renneby, Malin Nicole</subfield><subfield code="d">1990-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1192997557</subfield><subfield code="0">(DE-627)1671548698</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Joint galaxy-galaxy lensing and clustering constraints on galaxy formation</subfield><subfield code="c">Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020 September 4</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">30</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Gesehen am 02.08.2022</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Henriques, Bruno M. B.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1264156901</subfield><subfield code="0">(DE-627)181282291X</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hilbert, Stefan</subfield><subfield code="d">1976-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)135796474</subfield><subfield code="0">(DE-627)57166220X</subfield><subfield code="0">(DE-576)300651112</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nelson, Dylan</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)115182805X</subfield><subfield code="0">(DE-627)101233600X</subfield><subfield code="0">(DE-576)42382581X</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Vogelsberger, Mark</subfield><subfield code="d">1978-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)133437698</subfield><subfield code="0">(DE-627)546058434</subfield><subfield code="0">(DE-576)299848299</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Angulo, Raul E.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1161140662</subfield><subfield code="0">(DE-627)1024541320</subfield><subfield code="0">(DE-576)506376567</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Springel, Volker</subfield><subfield code="d">1970-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)122321391</subfield><subfield code="0">(DE-627)705861503</subfield><subfield code="0">(DE-576)293218463</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hernquist, Lars</subfield><subfield code="d">1954-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1264244401</subfield><subfield code="0">(DE-627)1813088241</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="a">Royal Astronomical Society</subfield><subfield code="t">Monthly notices of the Royal Astronomical Society</subfield><subfield code="d">Oxford : Oxford Univ. Press, 1827</subfield><subfield code="g">498(2020), 4, Seite 5804-5833</subfield><subfield code="h">Online-Ressource</subfield><subfield code="w">(DE-627)314059164</subfield><subfield code="w">(DE-600)2016084-7</subfield><subfield code="w">(DE-576)090955420</subfield><subfield code="x">1365-2966</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:498</subfield><subfield code="g">year:2020</subfield><subfield code="g">number:4</subfield><subfield code="g">pages:5804-5833</subfield><subfield code="g">extent:30</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1093/mnras/staa2675</subfield><subfield code="x">Verlag</subfield><subfield code="x">Resolving-System</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2013</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ISIL_DE-16-250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_1</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_KXP</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_74</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_100</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_120</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_213</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_224</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2001</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2003</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2007</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2008</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2009</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2010</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2015</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2026</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2088</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2190</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2810</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4035</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4246</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">498</subfield><subfield code="j">2020</subfield><subfield code="e">4</subfield><subfield code="h">5804-5833</subfield><subfield code="g">30</subfield></datafield><datafield tag="980" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="b">4170756150</subfield><subfield code="c">00</subfield><subfield code="f">--%%--</subfield><subfield code="d">--%%--</subfield><subfield code="e">--%%--</subfield><subfield code="j">--%%--</subfield><subfield code="y">l01</subfield><subfield code="z">20-07-22</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">00</subfield><subfield code="s">s</subfield><subfield code="a">hd2020</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">01</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410508463</subfield><subfield code="a">wissenschaftlicher Artikel (Zeitschrift)</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">02</subfield><subfield code="s">s</subfield><subfield code="a">per_8</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">03</subfield><subfield code="s">s</subfield><subfield code="a">s_30</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1750174588</subfield><subfield code="a">Nelson, Dylan</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1416822720</subfield><subfield code="a">Extern</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1583940421</subfield><subfield code="a">Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten"</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="a">pos_4</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1475299141</subfield><subfield code="a">Springel, Volker</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1416822720</subfield><subfield code="a">Extern</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">s</subfield><subfield code="a">pos_7</subfield></datafield></record></collection>
|
| standort_str_mv |
--%%-- |
| standort_iln_str_mv |
2013:--%%-- DE-16-250:--%%-- |
| author |
Renneby, Malin Nicole 1990- |
| spellingShingle |
Renneby, Malin Nicole 1990- 2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_8 2013 s_30 2013 Nelson, Dylan 2013 Extern 2013 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 Verfasser 2013 pos_4 2013 Springel, Volker 2013 pos_7 Joint galaxy-galaxy lensing and clustering constraints on galaxy formation |
| authorStr |
Renneby, Malin Nicole 1990- |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)314059164 |
| format |
electronic Article |
| delete_txt_mv |
keep |
| author_role |
aut aut aut aut aut aut aut aut |
| typewithnormlink_str_mv |
Person@(DE-588)1192997557 DifferentiatedPerson@(DE-588)1192997557 DifferentiatedPerson@(DE-588)1264156901 Person@(DE-588)1264156901 Person@(DE-588)135796474 DifferentiatedPerson@(DE-588)135796474 Person@(DE-588)115182805X DifferentiatedPerson@(DE-588)115182805X Person@(DE-588)133437698 DifferentiatedPerson@(DE-588)133437698 Person@(DE-588)1161140662 DifferentiatedPerson@(DE-588)1161140662 Person@(DE-588)122321391 DifferentiatedPerson@(DE-588)122321391 DifferentiatedPerson@(DE-588)1264244401 Person@(DE-588)1264244401 |
| collection |
KXP SWB GVK |
| remote_str |
true |
| last_changed_iln_str_mv |
2013@20-07-22 |
| illustrated |
Not Illustrated |
| issn |
1365-2966 |
| topic_title |
2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_8 2013 01 DE-16-250 03 s s_30 2013 01 DE-16-250 04 p (DE-627)1750174588 Nelson, Dylan 2013 01 DE-16-250 04 k (DE-627)1416822720 Extern 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_4 2013 01 DE-16-250 05 p (DE-627)1475299141 Springel, Volker 2013 01 DE-16-250 05 k (DE-627)1416822720 Extern 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_7 Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist |
| topic |
2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_8 2013 s_30 2013 Nelson, Dylan 2013 Extern 2013 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 Verfasser 2013 pos_4 2013 Springel, Volker 2013 pos_7 |
| topic_unstemmed |
2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_8 2013 s_30 2013 Nelson, Dylan 2013 Extern 2013 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 Verfasser 2013 pos_4 2013 Springel, Volker 2013 pos_7 |
| topic_browse |
2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_8 2013 s_30 2013 Nelson, Dylan 2013 Extern 2013 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 Verfasser 2013 pos_4 2013 Springel, Volker 2013 pos_7 |
| format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
| standort_txtP_mv |
--%%-- |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
cr |
| hierarchy_parent_title |
Monthly notices of the Royal Astronomical Society |
| normlinkwithtype_str_mv |
(DE-588)1192997557@Person (DE-588)1192997557@DifferentiatedPerson (DE-588)1264156901@DifferentiatedPerson (DE-588)1264156901@Person (DE-588)135796474@Person (DE-588)135796474@DifferentiatedPerson (DE-588)115182805X@Person (DE-588)115182805X@DifferentiatedPerson (DE-588)133437698@Person (DE-588)133437698@DifferentiatedPerson (DE-588)1161140662@Person (DE-588)1161140662@DifferentiatedPerson (DE-588)122321391@Person (DE-588)122321391@DifferentiatedPerson (DE-588)1264244401@DifferentiatedPerson (DE-588)1264244401@Person |
| hierarchy_parent_id |
314059164 |
| signature |
--%%-- |
| signature_str_mv |
--%%-- |
| hierarchy_top_title |
Monthly notices of the Royal Astronomical Society |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)314059164 (DE-600)2016084-7 (DE-576)090955420 |
| normlinkwithrole_str_mv |
(DE-588)1192997557@@aut@@ (DE-588)1264156901@@aut@@ (DE-588)135796474@@aut@@ (DE-588)115182805X@@aut@@ (DE-588)133437698@@aut@@ (DE-588)1161140662@@aut@@ (DE-588)122321391@@aut@@ (DE-588)1264244401@@aut@@ |
| title |
Joint galaxy-galaxy lensing and clustering constraints on galaxy formation |
| ctrlnum |
(DE-627)1810991188 (DE-599)KXP1810991188 (OCoLC)1341464073 |
| title_full |
Joint galaxy-galaxy lensing and clustering constraints on galaxy formation Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist |
| author_sort |
Renneby, Malin Nicole 1990- |
| journal |
Monthly notices of the Royal Astronomical Society |
| journalStr |
Monthly notices of the Royal Astronomical Society |
| callnumber-first-code |
- |
| lang_code |
eng |
| isOA_bool |
false |
| recordtype |
marc |
| publishDateSort |
2020 |
| contenttype_str_mv |
txt |
| container_start_page |
5804 |
| author_browse |
Renneby, Malin Nicole Henriques, Bruno M. B. Hilbert, Stefan Nelson, Dylan Vogelsberger, Mark Angulo, Raul E. Springel, Volker Hernquist, Lars |
| selectkey |
2013:l |
| container_volume |
498 |
| physical |
30 |
| format_se |
Elektronische Aufsätze |
| author-letter |
Renneby, Malin Nicole |
| doi_str_mv |
10.1093/mnras/staa2675 |
| normlink |
1192997557 1671548698 1264156901 181282291X 135796474 57166220X 300651112 115182805X 101233600X 42382581X 133437698 546058434 299848299 1161140662 1024541320 506376567 122321391 705861503 293218463 1264244401 1813088241 1410508463 1750174588 1416822720 1583940421 1410501914 1475299141 |
| normlink_prefix_str_mv |
(DE-588)1192997557 (DE-627)1671548698 (DE-588)1264156901 (DE-627)181282291X (DE-588)135796474 (DE-627)57166220X (DE-576)300651112 (DE-588)115182805X (DE-627)101233600X (DE-576)42382581X (DE-588)133437698 (DE-627)546058434 (DE-576)299848299 (DE-588)1161140662 (DE-627)1024541320 (DE-576)506376567 (DE-588)122321391 (DE-627)705861503 (DE-576)293218463 (DE-588)1264244401 (DE-627)1813088241 (DE-627)1410508463 (DE-627)1750174588 (DE-627)1416822720 (DE-627)1583940421 (DE-627)1410501914 (DE-627)1475299141 |
| author2-role |
verfasserin |
| title_sort |
joint galaxy-galaxy lensing and clustering constraints on galaxy formation |
| title_auth |
Joint galaxy-galaxy lensing and clustering constraints on galaxy formation |
| abstract |
We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Gesehen am 02.08.2022 |
| abstractGer |
We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Gesehen am 02.08.2022 |
| abstract_unstemmed |
We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development. Gesehen am 02.08.2022 |
| collection_details |
GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2026 GBV_ILN_2088 GBV_ILN_2112 GBV_ILN_2190 GBV_ILN_2810 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 |
| container_issue |
4 |
| title_short |
Joint galaxy-galaxy lensing and clustering constraints on galaxy formation |
| url |
https://doi.org/10.1093/mnras/staa2675 |
| ausleihindikator_str_mv |
2013:- |
| rolewithnormlink_str_mv |
@@aut@@(DE-588)1192997557 @@aut@@(DE-588)1264156901 @@aut@@(DE-588)135796474 @@aut@@(DE-588)115182805X @@aut@@(DE-588)133437698 @@aut@@(DE-588)1161140662 @@aut@@(DE-588)122321391 @@aut@@(DE-588)1264244401 |
| remote_bool |
true |
| author2 |
Henriques, Bruno M. B. Hilbert, Stefan 1976- Nelson, Dylan Vogelsberger, Mark 1978- Angulo, Raul E. Springel, Volker 1970- Hernquist, Lars 1954- |
| author2Str |
Henriques, Bruno M. B. Hilbert, Stefan 1976- Nelson, Dylan Vogelsberger, Mark 1978- Angulo, Raul E. Springel, Volker 1970- Hernquist, Lars 1954- |
| ppnlink |
314059164 |
| GND_str_mv |
Renneby, Malin Renneby, Malin Nicole Henriques, Bruno Henriques, Bruno M. B. Hilbert, S. Hilbert, S. J. Hilbert, Stefan Johannes Hibert, Stefan J. Hilbert, Stefan Nelson, D. Nelson, Dylan Vogelsberger, Mark P. Vogelsberger, Mark Philipp Vogelsberger, Mark Angulo, Raul E. Springel, V. Springel, Volker Hernquist, Lars E. Hernquist, Lars Eric Hernquist, Lars |
| GND_txt_mv |
Renneby, Malin Renneby, Malin Nicole Henriques, Bruno Henriques, Bruno M. B. Hilbert, S. Hilbert, S. J. Hilbert, Stefan Johannes Hibert, Stefan J. Hilbert, Stefan Nelson, D. Nelson, Dylan Vogelsberger, Mark P. Vogelsberger, Mark Philipp Vogelsberger, Mark Angulo, Raul E. Springel, V. Springel, Volker Hernquist, Lars E. Hernquist, Lars Eric Hernquist, Lars |
| GND_txtF_mv |
Renneby, Malin Renneby, Malin Nicole Henriques, Bruno Henriques, Bruno M. B. Hilbert, S. Hilbert, S. J. Hilbert, Stefan Johannes Hibert, Stefan J. Hilbert, Stefan Nelson, D. Nelson, Dylan Vogelsberger, Mark P. Vogelsberger, Mark Philipp Vogelsberger, Mark Angulo, Raul E. Springel, V. Springel, Volker Hernquist, Lars E. Hernquist, Lars Eric Hernquist, Lars |
| mediatype_str_mv |
c |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1093/mnras/staa2675 |
| callnumber-a |
--%%-- |
| up_date |
2024-07-04T18:41:46.978Z |
| _version_ |
1803674983576109056 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">1810991188</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240416193759.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">220720s2020 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1093/mnras/staa2675</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)1810991188</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)KXP1810991188</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1341464073</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Renneby, Malin Nicole</subfield><subfield code="d">1990-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1192997557</subfield><subfield code="0">(DE-627)1671548698</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Joint galaxy-galaxy lensing and clustering constraints on galaxy formation</subfield><subfield code="c">Malin Renneby, Bruno M.B. Henriques, Stefan Hilbert, Dylan Nelson, Mark Vogelsberger, Raúl E. Angulo, Volker Springel and Lars Hernquist</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020 September 4</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">30</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Gesehen am 02.08.2022</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We compare predictions for galaxy-galaxy lensing profiles and clustering from the Henriques et al. public version of the Munich semi-analytical model (SAM) of galaxy formation and the IllustrisTNG suite, primarily TNG300, with observations from KiDS + GAMA and SDSS-DR7 using four different selection functions for the lenses (stellar mass, stellar mass and group membership, stellar mass and isolation criteria, and stellar mass and colour). We find that this version of the SAM does not agree well with the current data for stellar mass-only lenses with $M_\ast \gt 10^{11}\, \mathrm{ M}_\odot$. By decreasing the merger time for satellite galaxies as well as reducing the radio-mode active galactic nucleus accretion efficiency in the SAM, we obtain better agreement, both for the lensing and the clustering, at the high-mass end. We show that the new model is consistent with the signals for central galaxies presented in Velliscig et al. Turning to the hydrodynamical simulation, TNG300 produces good lensing predictions, both for stellar mass-only (χ2 = 1.81 compared to χ2 = 7.79 for the SAM) and locally brightest galaxy samples (χ2 = 3.80 compared to χ2 = 5.01). With added dust corrections to the colours it matches the SDSS clustering signal well for red low-mass galaxies. We find that both the SAMs and TNG300 predict $\sim 50\, {{\ \rm per\ cent}}$ excessive lensing signals for intermediate-mass red galaxies with 10.2 < log10M*[M⊙] < 11.2 at $r \approx 0.6\, h^{-1}\, \text{Mpc}$, which require further theoretical development.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Henriques, Bruno M. B.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1264156901</subfield><subfield code="0">(DE-627)181282291X</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hilbert, Stefan</subfield><subfield code="d">1976-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)135796474</subfield><subfield code="0">(DE-627)57166220X</subfield><subfield code="0">(DE-576)300651112</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nelson, Dylan</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)115182805X</subfield><subfield code="0">(DE-627)101233600X</subfield><subfield code="0">(DE-576)42382581X</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Vogelsberger, Mark</subfield><subfield code="d">1978-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)133437698</subfield><subfield code="0">(DE-627)546058434</subfield><subfield code="0">(DE-576)299848299</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Angulo, Raul E.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1161140662</subfield><subfield code="0">(DE-627)1024541320</subfield><subfield code="0">(DE-576)506376567</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Springel, Volker</subfield><subfield code="d">1970-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)122321391</subfield><subfield code="0">(DE-627)705861503</subfield><subfield code="0">(DE-576)293218463</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hernquist, Lars</subfield><subfield code="d">1954-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1264244401</subfield><subfield code="0">(DE-627)1813088241</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="a">Royal Astronomical Society</subfield><subfield code="t">Monthly notices of the Royal Astronomical Society</subfield><subfield code="d">Oxford : Oxford Univ. Press, 1827</subfield><subfield code="g">498(2020), 4, Seite 5804-5833</subfield><subfield code="h">Online-Ressource</subfield><subfield code="w">(DE-627)314059164</subfield><subfield code="w">(DE-600)2016084-7</subfield><subfield code="w">(DE-576)090955420</subfield><subfield code="x">1365-2966</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:498</subfield><subfield code="g">year:2020</subfield><subfield code="g">number:4</subfield><subfield code="g">pages:5804-5833</subfield><subfield code="g">extent:30</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1093/mnras/staa2675</subfield><subfield code="x">Verlag</subfield><subfield code="x">Resolving-System</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2013</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ISIL_DE-16-250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_1</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_KXP</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_74</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_100</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_120</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_213</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_224</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2001</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2003</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2007</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2008</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2009</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2010</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2015</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2026</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2088</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2190</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2810</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4035</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4246</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">498</subfield><subfield code="j">2020</subfield><subfield code="e">4</subfield><subfield code="h">5804-5833</subfield><subfield code="g">30</subfield></datafield><datafield tag="980" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="b">4170756150</subfield><subfield code="c">00</subfield><subfield code="f">--%%--</subfield><subfield code="d">--%%--</subfield><subfield code="e">--%%--</subfield><subfield code="j">--%%--</subfield><subfield code="y">l01</subfield><subfield code="z">20-07-22</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">00</subfield><subfield code="s">s</subfield><subfield code="a">hd2020</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">01</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410508463</subfield><subfield code="a">wissenschaftlicher Artikel (Zeitschrift)</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">02</subfield><subfield code="s">s</subfield><subfield code="a">per_8</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">03</subfield><subfield code="s">s</subfield><subfield code="a">s_30</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1750174588</subfield><subfield code="a">Nelson, Dylan</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1416822720</subfield><subfield code="a">Extern</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1583940421</subfield><subfield code="a">Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten"</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="a">pos_4</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1475299141</subfield><subfield code="a">Springel, Volker</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1416822720</subfield><subfield code="a">Extern</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">05</subfield><subfield code="s">s</subfield><subfield code="a">pos_7</subfield></datafield></record></collection>
|
| score |
7.40158 |