Joint cluster reconstructions - combing free-form lensing and X-rays

Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a...
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Autor*in:	Huber, Korbinian - 1987- [verfasserIn] Tchernin, Céline [verfasserIn] Merten, Julian [verfasserIn] Hilbert, Stefan [verfasserIn] Bartelmann, Matthias - 1965- [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	15 July 2019

Anmerkung:	Gesehen am 28.04.2020
Umfang:	14

Übergeordnetes Werk:	Enthalten in: Astronomy and astrophysics - Les Ulis : EDP Sciences, 1969, 627(2019) Artikel-Nummer A143, 14 Seiten
Übergeordnetes Werk:	volume:627 ; year:2019 ; extent:14

Links:	Volltext Volltext

DOI / URN:	10.1051/0004-6361/201834928

Katalog-ID:	1696304598

Internformat


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245	1	0	\|a Joint cluster reconstructions - combing free-form lensing and X-rays \|c Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann
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520			\|a Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two.
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matchkey_str	article:14320746:2019----::oncutreosrcincmigreom
oclc_num	1341317075
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publishDate	2019
allfields	10.1051/0004-6361/201834928 doi (DE-627)1696304598 (DE-599)KXP1696304598 (OCoLC)1341317075 DE-627 ger DE-627 rda eng Huber, Korbinian 1987- verfasserin (DE-588)1179981510 (DE-627)1067593934 (DE-576)518453553 aut Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann 15 July 2019 14 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 28.04.2020 Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Tchernin, Céline verfasserin (DE-588)1139868659 (DE-627)897775961 (DE-576)493514163 aut Merten, Julian verfasserin aut Hilbert, Stefan verfasserin aut Bartelmann, Matthias 1965- verfasserin (DE-588)141554185 (DE-627)629953090 (DE-576)170611779 aut Enthalten in Astronomy and astrophysics Les Ulis : EDP Sciences, 1969 627(2019) Artikel-Nummer A143, 14 Seiten Online-Ressource (DE-627)253390222 (DE-600)1458466-9 (DE-576)072283351 1432-0746 nnns volume:627 year:2019 extent:14 https://doi.org/10.1051/0004-6361/201834928 Verlag Resolving-System lizenzpflichtig Volltext https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html Verlag 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2021 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 627 2019 14 627(2019) Artikel-Nummer A143, 14 Seiten 2013 01 DE-16-250 363953543X 00 --%%-- --%%-- --%%-- --%%-- l01 28-04-20 2013 01 DE-16-250 00 s hd2019 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_5 2013 01 DE-16-250 03 s s_14 2013 01 DE-16-250 04 p (DE-627)1581690878 Tchernin, Céline 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_2 2013 01 DE-16-250 05 p (DE-627)1433881497 Bartelmann, Matthias 2013 01 DE-16-250 05 k (DE-627)1416535187 Institut für Theoretische Physik 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_5
spelling	10.1051/0004-6361/201834928 doi (DE-627)1696304598 (DE-599)KXP1696304598 (OCoLC)1341317075 DE-627 ger DE-627 rda eng Huber, Korbinian 1987- verfasserin (DE-588)1179981510 (DE-627)1067593934 (DE-576)518453553 aut Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann 15 July 2019 14 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 28.04.2020 Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Tchernin, Céline verfasserin (DE-588)1139868659 (DE-627)897775961 (DE-576)493514163 aut Merten, Julian verfasserin aut Hilbert, Stefan verfasserin aut Bartelmann, Matthias 1965- verfasserin (DE-588)141554185 (DE-627)629953090 (DE-576)170611779 aut Enthalten in Astronomy and astrophysics Les Ulis : EDP Sciences, 1969 627(2019) Artikel-Nummer A143, 14 Seiten Online-Ressource (DE-627)253390222 (DE-600)1458466-9 (DE-576)072283351 1432-0746 nnns volume:627 year:2019 extent:14 https://doi.org/10.1051/0004-6361/201834928 Verlag Resolving-System lizenzpflichtig Volltext https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html Verlag 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2021 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 627 2019 14 627(2019) Artikel-Nummer A143, 14 Seiten 2013 01 DE-16-250 363953543X 00 --%%-- --%%-- --%%-- --%%-- l01 28-04-20 2013 01 DE-16-250 00 s hd2019 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_5 2013 01 DE-16-250 03 s s_14 2013 01 DE-16-250 04 p (DE-627)1581690878 Tchernin, Céline 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_2 2013 01 DE-16-250 05 p (DE-627)1433881497 Bartelmann, Matthias 2013 01 DE-16-250 05 k (DE-627)1416535187 Institut für Theoretische Physik 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_5
allfields_unstemmed	10.1051/0004-6361/201834928 doi (DE-627)1696304598 (DE-599)KXP1696304598 (OCoLC)1341317075 DE-627 ger DE-627 rda eng Huber, Korbinian 1987- verfasserin (DE-588)1179981510 (DE-627)1067593934 (DE-576)518453553 aut Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann 15 July 2019 14 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 28.04.2020 Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Tchernin, Céline verfasserin (DE-588)1139868659 (DE-627)897775961 (DE-576)493514163 aut Merten, Julian verfasserin aut Hilbert, Stefan verfasserin aut Bartelmann, Matthias 1965- verfasserin (DE-588)141554185 (DE-627)629953090 (DE-576)170611779 aut Enthalten in Astronomy and astrophysics Les Ulis : EDP Sciences, 1969 627(2019) Artikel-Nummer A143, 14 Seiten Online-Ressource (DE-627)253390222 (DE-600)1458466-9 (DE-576)072283351 1432-0746 nnns volume:627 year:2019 extent:14 https://doi.org/10.1051/0004-6361/201834928 Verlag Resolving-System lizenzpflichtig Volltext https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html Verlag 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2021 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 627 2019 14 627(2019) Artikel-Nummer A143, 14 Seiten 2013 01 DE-16-250 363953543X 00 --%%-- --%%-- --%%-- --%%-- l01 28-04-20 2013 01 DE-16-250 00 s hd2019 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_5 2013 01 DE-16-250 03 s s_14 2013 01 DE-16-250 04 p (DE-627)1581690878 Tchernin, Céline 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_2 2013 01 DE-16-250 05 p (DE-627)1433881497 Bartelmann, Matthias 2013 01 DE-16-250 05 k (DE-627)1416535187 Institut für Theoretische Physik 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_5
allfieldsGer	10.1051/0004-6361/201834928 doi (DE-627)1696304598 (DE-599)KXP1696304598 (OCoLC)1341317075 DE-627 ger DE-627 rda eng Huber, Korbinian 1987- verfasserin (DE-588)1179981510 (DE-627)1067593934 (DE-576)518453553 aut Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann 15 July 2019 14 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 28.04.2020 Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Tchernin, Céline verfasserin (DE-588)1139868659 (DE-627)897775961 (DE-576)493514163 aut Merten, Julian verfasserin aut Hilbert, Stefan verfasserin aut Bartelmann, Matthias 1965- verfasserin (DE-588)141554185 (DE-627)629953090 (DE-576)170611779 aut Enthalten in Astronomy and astrophysics Les Ulis : EDP Sciences, 1969 627(2019) Artikel-Nummer A143, 14 Seiten Online-Ressource (DE-627)253390222 (DE-600)1458466-9 (DE-576)072283351 1432-0746 nnns volume:627 year:2019 extent:14 https://doi.org/10.1051/0004-6361/201834928 Verlag Resolving-System lizenzpflichtig Volltext https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html Verlag 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2021 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 627 2019 14 627(2019) Artikel-Nummer A143, 14 Seiten 2013 01 DE-16-250 363953543X 00 --%%-- --%%-- --%%-- --%%-- l01 28-04-20 2013 01 DE-16-250 00 s hd2019 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_5 2013 01 DE-16-250 03 s s_14 2013 01 DE-16-250 04 p (DE-627)1581690878 Tchernin, Céline 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_2 2013 01 DE-16-250 05 p (DE-627)1433881497 Bartelmann, Matthias 2013 01 DE-16-250 05 k (DE-627)1416535187 Institut für Theoretische Physik 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_5
allfieldsSound	10.1051/0004-6361/201834928 doi (DE-627)1696304598 (DE-599)KXP1696304598 (OCoLC)1341317075 DE-627 ger DE-627 rda eng Huber, Korbinian 1987- verfasserin (DE-588)1179981510 (DE-627)1067593934 (DE-576)518453553 aut Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann 15 July 2019 14 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 28.04.2020 Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Tchernin, Céline verfasserin (DE-588)1139868659 (DE-627)897775961 (DE-576)493514163 aut Merten, Julian verfasserin aut Hilbert, Stefan verfasserin aut Bartelmann, Matthias 1965- verfasserin (DE-588)141554185 (DE-627)629953090 (DE-576)170611779 aut Enthalten in Astronomy and astrophysics Les Ulis : EDP Sciences, 1969 627(2019) Artikel-Nummer A143, 14 Seiten Online-Ressource (DE-627)253390222 (DE-600)1458466-9 (DE-576)072283351 1432-0746 nnns volume:627 year:2019 extent:14 https://doi.org/10.1051/0004-6361/201834928 Verlag Resolving-System lizenzpflichtig Volltext https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html Verlag 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2021 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 627 2019 14 627(2019) Artikel-Nummer A143, 14 Seiten 2013 01 DE-16-250 363953543X 00 --%%-- --%%-- --%%-- --%%-- l01 28-04-20 2013 01 DE-16-250 00 s hd2019 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_5 2013 01 DE-16-250 03 s s_14 2013 01 DE-16-250 04 p (DE-627)1581690878 Tchernin, Céline 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_2 2013 01 DE-16-250 05 p (DE-627)1433881497 Bartelmann, Matthias 2013 01 DE-16-250 05 k (DE-627)1416535187 Institut für Theoretische Physik 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_5
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source	Enthalten in Astronomy and astrophysics 627(2019) Artikel-Nummer A143, 14 Seiten volume:627 year:2019 extent:14
sourceStr	Enthalten in Astronomy and astrophysics 627(2019) Artikel-Nummer A143, 14 Seiten volume:627 year:2019 extent:14
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container_title	Astronomy and astrophysics
authorswithroles_txt_mv	Huber, Korbinian @@aut@@ Tchernin, Céline @@aut@@ Merten, Julian @@aut@@ Hilbert, Stefan @@aut@@ Bartelmann, Matthias @@aut@@
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We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. 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title	Joint cluster reconstructions - combing free-form lensing and X-rays
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title_full	Joint cluster reconstructions - combing free-form lensing and X-rays Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann
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title_sort	joint cluster reconstructions - combing free-form lensing and x-rays
title_auth	Joint cluster reconstructions - combing free-form lensing and X-rays
abstract	Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Gesehen am 28.04.2020
abstractGer	Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Gesehen am 28.04.2020
abstract_unstemmed	Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. We show how the combination of X-ray and weak lensing data can affect a free-form reconstruction, improving the accuracy in the central region in some cases by a factor of two. Gesehen am 28.04.2020
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title_short	Joint cluster reconstructions - combing free-form lensing and X-rays
url	https://doi.org/10.1051/0004-6361/201834928 https://www.aanda.org/articles/aa/abs/2019/07/aa34928-18/aa34928-18.html
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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">1696304598</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220818055005.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">200428s2019 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1051/0004-6361/201834928</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)1696304598</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)KXP1696304598</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1341317075</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">Huber, Korbinian</subfield><subfield code="d">1987-</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1179981510</subfield><subfield code="0">(DE-627)1067593934</subfield><subfield code="0">(DE-576)518453553</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Joint cluster reconstructions - combing free-form lensing and X-rays</subfield><subfield code="c">Korbinian Huber, Céline Tchernin, Julian Merten, Stefan Hilbert, and Matthias Bartelmann</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">15 July 2019</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">14</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 28.04.2020</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.<i>Aims<i/>. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models.<i>Methods<i/>. We make use of the lensing reconstruction code SAWLENS2, and expand its capabilities by incorporating an estimate of the projected gravitational potential based on X-ray data that are deprojected using the local Richardson-Lucy method and used to infer the Newtonian potential of the cluster. We discuss how potentially arising numerical artefacts can be treated.<i>Results<i/>. We demonstrate the feasibility of our method on a simplified mock Navarro-Frenk-White (NFW) halo and on a cluster from a realistic hydrodynamical simulation. 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Joint cluster reconstructions - combing free-form lensing and X-rays

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