An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23)
This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and H...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lam, Casey [verfasserIn] Lu, Jessica R. [verfasserIn] Udalski, Andrzej [verfasserIn] Bond, Ian [verfasserIn] Bennett, David P. [verfasserIn] Skowron, Jan [verfasserIn] Mróz, Przemek [verfasserIn] Poleski, Radek [verfasserIn] Sumi, Takahiro [verfasserIn] Szymański, Micha\l K. [verfasserIn] Koz\lowski, Szymon [verfasserIn] Pietrukowicz, Pawe\l [verfasserIn] Soszyński, Igor [verfasserIn] Ulaczyk, Krzysztof [verfasserIn] Wyrzykowski, \Lukasz [verfasserIn] Miyazaki, Shota [verfasserIn] Suzuki, Daisuke [verfasserIn] Koshimoto, Naoki [verfasserIn] Rattenbury, Nicholas J. [verfasserIn] Hosek, Matthew W. [verfasserIn] Abe, Fumio [verfasserIn] Barry, Richard [verfasserIn] Bhattacharya, Aparna [verfasserIn] Fukui, Akihiko [verfasserIn] Fujii, Hirosane [verfasserIn] Hirao, Yuki [verfasserIn] Itow, Yoshitaka [verfasserIn] Kirikawa, Rintaro [verfasserIn] Kondo, Iona [verfasserIn] Matsubara, Yutaka [verfasserIn] Matsumoto, Sho [verfasserIn] Muraki, Yasushi [verfasserIn] Olmschenk, Greg [verfasserIn] Ranc, Clément [verfasserIn] Okamura, Arisa [verfasserIn] Satoh, Yuki K. [verfasserIn] Silva, Stela Ishitani [verfasserIn] Toda, Taiga [verfasserIn] Tristram, Paul J. [verfasserIn] Vandorou, Aikaterini [verfasserIn] Yama, Hibiki [verfasserIn] Abrams, Natasha S. [verfasserIn] Agarwal, Shrihan [verfasserIn] Rose, Sam [verfasserIn] Terry, Sean K. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 July 6 |
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| Anmerkung: |
Gesehen am 08.08.2022 |
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| Umfang: |
42 |
| Übergeordnetes Werk: |
Enthalten in: The astrophysical journal. Supplement series - London : Institute of Physics Publ., 1996, 260(2022), 2, Artikel-ID 55, Seite 1-42 |
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| Übergeordnetes Werk: |
volume:260 ; year:2022 ; number:2 ; elocationid:55 ; pages:1-42 ; extent:42 |
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| DOI / URN: |
10.3847/1538-4365/ac7441 |
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| Katalog-ID: |
181340934X |
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| 100 | 1 | |a Lam, Casey |e verfasserin |0 (DE-588)1264818203 |0 (DE-627)1813409978 |4 aut | |
| 245 | 1 | 3 | |a An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) |c Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry |
| 264 | 1 | |c 2022 July 6 | |
| 300 | |a 42 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
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| 500 | |a Gesehen am 08.08.2022 | ||
| 520 | |a This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). | ||
| 700 | 1 | |a Lu, Jessica R. |e verfasserin |4 aut | |
| 700 | 1 | |a Udalski, Andrzej |e verfasserin |4 aut | |
| 700 | 1 | |a Bond, Ian |e verfasserin |4 aut | |
| 700 | 1 | |a Bennett, David P. |e verfasserin |0 (DE-588)1283262819 |0 (DE-627)1839065133 |4 aut | |
| 700 | 1 | |a Skowron, Jan |e verfasserin |4 aut | |
| 700 | 1 | |a Mróz, Przemek |e verfasserin |4 aut | |
| 700 | 1 | |a Poleski, Radek |e verfasserin |4 aut | |
| 700 | 1 | |a Sumi, Takahiro |e verfasserin |4 aut | |
| 700 | 1 | |a Szymański, Micha\l K. |e verfasserin |4 aut | |
| 700 | 1 | |a Koz\lowski, Szymon |e verfasserin |4 aut | |
| 700 | 1 | |a Pietrukowicz, Pawe\l |e verfasserin |4 aut | |
| 700 | 1 | |a Soszyński, Igor |e verfasserin |4 aut | |
| 700 | 1 | |a Ulaczyk, Krzysztof |e verfasserin |4 aut | |
| 700 | 1 | |a Wyrzykowski, \Lukasz |e verfasserin |4 aut | |
| 700 | 1 | |a Miyazaki, Shota |e verfasserin |4 aut | |
| 700 | 1 | |a Suzuki, Daisuke |e verfasserin |4 aut | |
| 700 | 1 | |a Koshimoto, Naoki |e verfasserin |4 aut | |
| 700 | 1 | |a Rattenbury, Nicholas J. |e verfasserin |4 aut | |
| 700 | 1 | |a Hosek, Matthew W. |e verfasserin |4 aut | |
| 700 | 1 | |a Abe, Fumio |e verfasserin |4 aut | |
| 700 | 1 | |a Barry, Richard |e verfasserin |4 aut | |
| 700 | 1 | |a Bhattacharya, Aparna |e verfasserin |4 aut | |
| 700 | 1 | |a Fukui, Akihiko |e verfasserin |4 aut | |
| 700 | 1 | |a Fujii, Hirosane |e verfasserin |4 aut | |
| 700 | 1 | |a Hirao, Yuki |e verfasserin |4 aut | |
| 700 | 1 | |a Itow, Yoshitaka |e verfasserin |4 aut | |
| 700 | 1 | |a Kirikawa, Rintaro |e verfasserin |4 aut | |
| 700 | 1 | |a Kondo, Iona |e verfasserin |4 aut | |
| 700 | 1 | |a Matsubara, Yutaka |e verfasserin |4 aut | |
| 700 | 1 | |a Matsumoto, Sho |e verfasserin |4 aut | |
| 700 | 1 | |a Muraki, Yasushi |e verfasserin |4 aut | |
| 700 | 1 | |a Olmschenk, Greg |e verfasserin |4 aut | |
| 700 | 1 | |a Ranc, Clément |e verfasserin |0 (DE-588)1204147469 |0 (DE-627)1689284927 |4 aut | |
| 700 | 1 | |a Okamura, Arisa |e verfasserin |4 aut | |
| 700 | 1 | |a Satoh, Yuki K. |e verfasserin |0 (DE-588)1315041014 |0 (DE-627)1877269689 |4 aut | |
| 700 | 1 | |a Silva, Stela Ishitani |e verfasserin |4 aut | |
| 700 | 1 | |a Toda, Taiga |e verfasserin |4 aut | |
| 700 | 1 | |a Tristram, Paul J. |e verfasserin |4 aut | |
| 700 | 1 | |a Vandorou, Aikaterini |e verfasserin |4 aut | |
| 700 | 1 | |a Yama, Hibiki |e verfasserin |4 aut | |
| 700 | 1 | |a Abrams, Natasha S. |e verfasserin |4 aut | |
| 700 | 1 | |a Agarwal, Shrihan |e verfasserin |4 aut | |
| 700 | 1 | |a Rose, Sam |e verfasserin |4 aut | |
| 700 | 1 | |a Terry, Sean K. |e verfasserin |4 aut | |
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10.3847/1538-4365/ac7441 doi (DE-627)181340934X (DE-599)KXP181340934X (OCoLC)1361713329 DE-627 ger DE-627 rda eng Lam, Casey verfasserin (DE-588)1264818203 (DE-627)1813409978 aut An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry 2022 July 6 42 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 08.08.2022 This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Lu, Jessica R. verfasserin aut Udalski, Andrzej verfasserin aut Bond, Ian verfasserin aut Bennett, David P. verfasserin (DE-588)1283262819 (DE-627)1839065133 aut Skowron, Jan verfasserin aut Mróz, Przemek verfasserin aut Poleski, Radek verfasserin aut Sumi, Takahiro verfasserin aut Szymański, Micha\l K. verfasserin aut Koz\lowski, Szymon verfasserin aut Pietrukowicz, Pawe\l verfasserin aut Soszyński, Igor verfasserin aut Ulaczyk, Krzysztof verfasserin aut Wyrzykowski, \Lukasz verfasserin aut Miyazaki, Shota verfasserin aut Suzuki, Daisuke verfasserin aut Koshimoto, Naoki verfasserin aut Rattenbury, Nicholas J. verfasserin aut Hosek, Matthew W. verfasserin aut Abe, Fumio verfasserin aut Barry, Richard verfasserin aut Bhattacharya, Aparna verfasserin aut Fukui, Akihiko verfasserin aut Fujii, Hirosane verfasserin aut Hirao, Yuki verfasserin aut Itow, Yoshitaka verfasserin aut Kirikawa, Rintaro verfasserin aut Kondo, Iona verfasserin aut Matsubara, Yutaka verfasserin aut Matsumoto, Sho verfasserin aut Muraki, Yasushi verfasserin aut Olmschenk, Greg verfasserin aut Ranc, Clément verfasserin (DE-588)1204147469 (DE-627)1689284927 aut Okamura, Arisa verfasserin aut Satoh, Yuki K. verfasserin (DE-588)1315041014 (DE-627)1877269689 aut Silva, Stela Ishitani verfasserin aut Toda, Taiga verfasserin aut Tristram, Paul J. verfasserin aut Vandorou, Aikaterini verfasserin aut Yama, Hibiki verfasserin aut Abrams, Natasha S. verfasserin aut Agarwal, Shrihan verfasserin aut Rose, Sam verfasserin aut Terry, Sean K. verfasserin aut Enthalten in The astrophysical journal. Supplement series London : Institute of Physics Publ., 1996 260(2022), 2, Artikel-ID 55, Seite 1-42 Online-Ressource (DE-627)312200196 (DE-600)2006860-8 (DE-576)090890892 1538-4365 nnns volume:260 year:2022 number:2 elocationid:55 pages:1-42 extent:42 https://doi.org/10.3847/1538-4365/ac7441 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_65 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_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 260 2022 2 55 1-42 42 2013 01 DE-16-250 4176843403 00 --%%-- --%%-- --%%-- --%%-- l01 08-08-22 2013 01 DE-16-250 00 s hd2022 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_45 2013 01 DE-16-250 03 s s_42 2013 01 DE-16-250 04 p (DE-627)1809686113 Ranc, Clément 2013 01 DE-16-250 04 k (DE-627)1416733728 ZAH Astronomisches Recheninstitut 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_34 |
| spelling |
10.3847/1538-4365/ac7441 doi (DE-627)181340934X (DE-599)KXP181340934X (OCoLC)1361713329 DE-627 ger DE-627 rda eng Lam, Casey verfasserin (DE-588)1264818203 (DE-627)1813409978 aut An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry 2022 July 6 42 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 08.08.2022 This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Lu, Jessica R. verfasserin aut Udalski, Andrzej verfasserin aut Bond, Ian verfasserin aut Bennett, David P. verfasserin (DE-588)1283262819 (DE-627)1839065133 aut Skowron, Jan verfasserin aut Mróz, Przemek verfasserin aut Poleski, Radek verfasserin aut Sumi, Takahiro verfasserin aut Szymański, Micha\l K. verfasserin aut Koz\lowski, Szymon verfasserin aut Pietrukowicz, Pawe\l verfasserin aut Soszyński, Igor verfasserin aut Ulaczyk, Krzysztof verfasserin aut Wyrzykowski, \Lukasz verfasserin aut Miyazaki, Shota verfasserin aut Suzuki, Daisuke verfasserin aut Koshimoto, Naoki verfasserin aut Rattenbury, Nicholas J. verfasserin aut Hosek, Matthew W. verfasserin aut Abe, Fumio verfasserin aut Barry, Richard verfasserin aut Bhattacharya, Aparna verfasserin aut Fukui, Akihiko verfasserin aut Fujii, Hirosane verfasserin aut Hirao, Yuki verfasserin aut Itow, Yoshitaka verfasserin aut Kirikawa, Rintaro verfasserin aut Kondo, Iona verfasserin aut Matsubara, Yutaka verfasserin aut Matsumoto, Sho verfasserin aut Muraki, Yasushi verfasserin aut Olmschenk, Greg verfasserin aut Ranc, Clément verfasserin (DE-588)1204147469 (DE-627)1689284927 aut Okamura, Arisa verfasserin aut Satoh, Yuki K. verfasserin (DE-588)1315041014 (DE-627)1877269689 aut Silva, Stela Ishitani verfasserin aut Toda, Taiga verfasserin aut Tristram, Paul J. verfasserin aut Vandorou, Aikaterini verfasserin aut Yama, Hibiki verfasserin aut Abrams, Natasha S. verfasserin aut Agarwal, Shrihan verfasserin aut Rose, Sam verfasserin aut Terry, Sean K. verfasserin aut Enthalten in The astrophysical journal. Supplement series London : Institute of Physics Publ., 1996 260(2022), 2, Artikel-ID 55, Seite 1-42 Online-Ressource (DE-627)312200196 (DE-600)2006860-8 (DE-576)090890892 1538-4365 nnns volume:260 year:2022 number:2 elocationid:55 pages:1-42 extent:42 https://doi.org/10.3847/1538-4365/ac7441 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_65 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_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 260 2022 2 55 1-42 42 2013 01 DE-16-250 4176843403 00 --%%-- --%%-- --%%-- --%%-- l01 08-08-22 2013 01 DE-16-250 00 s hd2022 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_45 2013 01 DE-16-250 03 s s_42 2013 01 DE-16-250 04 p (DE-627)1809686113 Ranc, Clément 2013 01 DE-16-250 04 k (DE-627)1416733728 ZAH Astronomisches Recheninstitut 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_34 |
| allfields_unstemmed |
10.3847/1538-4365/ac7441 doi (DE-627)181340934X (DE-599)KXP181340934X (OCoLC)1361713329 DE-627 ger DE-627 rda eng Lam, Casey verfasserin (DE-588)1264818203 (DE-627)1813409978 aut An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry 2022 July 6 42 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 08.08.2022 This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Lu, Jessica R. verfasserin aut Udalski, Andrzej verfasserin aut Bond, Ian verfasserin aut Bennett, David P. verfasserin (DE-588)1283262819 (DE-627)1839065133 aut Skowron, Jan verfasserin aut Mróz, Przemek verfasserin aut Poleski, Radek verfasserin aut Sumi, Takahiro verfasserin aut Szymański, Micha\l K. verfasserin aut Koz\lowski, Szymon verfasserin aut Pietrukowicz, Pawe\l verfasserin aut Soszyński, Igor verfasserin aut Ulaczyk, Krzysztof verfasserin aut Wyrzykowski, \Lukasz verfasserin aut Miyazaki, Shota verfasserin aut Suzuki, Daisuke verfasserin aut Koshimoto, Naoki verfasserin aut Rattenbury, Nicholas J. verfasserin aut Hosek, Matthew W. verfasserin aut Abe, Fumio verfasserin aut Barry, Richard verfasserin aut Bhattacharya, Aparna verfasserin aut Fukui, Akihiko verfasserin aut Fujii, Hirosane verfasserin aut Hirao, Yuki verfasserin aut Itow, Yoshitaka verfasserin aut Kirikawa, Rintaro verfasserin aut Kondo, Iona verfasserin aut Matsubara, Yutaka verfasserin aut Matsumoto, Sho verfasserin aut Muraki, Yasushi verfasserin aut Olmschenk, Greg verfasserin aut Ranc, Clément verfasserin (DE-588)1204147469 (DE-627)1689284927 aut Okamura, Arisa verfasserin aut Satoh, Yuki K. verfasserin (DE-588)1315041014 (DE-627)1877269689 aut Silva, Stela Ishitani verfasserin aut Toda, Taiga verfasserin aut Tristram, Paul J. verfasserin aut Vandorou, Aikaterini verfasserin aut Yama, Hibiki verfasserin aut Abrams, Natasha S. verfasserin aut Agarwal, Shrihan verfasserin aut Rose, Sam verfasserin aut Terry, Sean K. verfasserin aut Enthalten in The astrophysical journal. Supplement series London : Institute of Physics Publ., 1996 260(2022), 2, Artikel-ID 55, Seite 1-42 Online-Ressource (DE-627)312200196 (DE-600)2006860-8 (DE-576)090890892 1538-4365 nnns volume:260 year:2022 number:2 elocationid:55 pages:1-42 extent:42 https://doi.org/10.3847/1538-4365/ac7441 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_65 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_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 260 2022 2 55 1-42 42 2013 01 DE-16-250 4176843403 00 --%%-- --%%-- --%%-- --%%-- l01 08-08-22 2013 01 DE-16-250 00 s hd2022 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_45 2013 01 DE-16-250 03 s s_42 2013 01 DE-16-250 04 p (DE-627)1809686113 Ranc, Clément 2013 01 DE-16-250 04 k (DE-627)1416733728 ZAH Astronomisches Recheninstitut 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_34 |
| allfieldsGer |
10.3847/1538-4365/ac7441 doi (DE-627)181340934X (DE-599)KXP181340934X (OCoLC)1361713329 DE-627 ger DE-627 rda eng Lam, Casey verfasserin (DE-588)1264818203 (DE-627)1813409978 aut An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry 2022 July 6 42 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 08.08.2022 This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Lu, Jessica R. verfasserin aut Udalski, Andrzej verfasserin aut Bond, Ian verfasserin aut Bennett, David P. verfasserin (DE-588)1283262819 (DE-627)1839065133 aut Skowron, Jan verfasserin aut Mróz, Przemek verfasserin aut Poleski, Radek verfasserin aut Sumi, Takahiro verfasserin aut Szymański, Micha\l K. verfasserin aut Koz\lowski, Szymon verfasserin aut Pietrukowicz, Pawe\l verfasserin aut Soszyński, Igor verfasserin aut Ulaczyk, Krzysztof verfasserin aut Wyrzykowski, \Lukasz verfasserin aut Miyazaki, Shota verfasserin aut Suzuki, Daisuke verfasserin aut Koshimoto, Naoki verfasserin aut Rattenbury, Nicholas J. verfasserin aut Hosek, Matthew W. verfasserin aut Abe, Fumio verfasserin aut Barry, Richard verfasserin aut Bhattacharya, Aparna verfasserin aut Fukui, Akihiko verfasserin aut Fujii, Hirosane verfasserin aut Hirao, Yuki verfasserin aut Itow, Yoshitaka verfasserin aut Kirikawa, Rintaro verfasserin aut Kondo, Iona verfasserin aut Matsubara, Yutaka verfasserin aut Matsumoto, Sho verfasserin aut Muraki, Yasushi verfasserin aut Olmschenk, Greg verfasserin aut Ranc, Clément verfasserin (DE-588)1204147469 (DE-627)1689284927 aut Okamura, Arisa verfasserin aut Satoh, Yuki K. verfasserin (DE-588)1315041014 (DE-627)1877269689 aut Silva, Stela Ishitani verfasserin aut Toda, Taiga verfasserin aut Tristram, Paul J. verfasserin aut Vandorou, Aikaterini verfasserin aut Yama, Hibiki verfasserin aut Abrams, Natasha S. verfasserin aut Agarwal, Shrihan verfasserin aut Rose, Sam verfasserin aut Terry, Sean K. verfasserin aut Enthalten in The astrophysical journal. Supplement series London : Institute of Physics Publ., 1996 260(2022), 2, Artikel-ID 55, Seite 1-42 Online-Ressource (DE-627)312200196 (DE-600)2006860-8 (DE-576)090890892 1538-4365 nnns volume:260 year:2022 number:2 elocationid:55 pages:1-42 extent:42 https://doi.org/10.3847/1538-4365/ac7441 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_65 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_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 260 2022 2 55 1-42 42 2013 01 DE-16-250 4176843403 00 --%%-- --%%-- --%%-- --%%-- l01 08-08-22 2013 01 DE-16-250 00 s hd2022 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_45 2013 01 DE-16-250 03 s s_42 2013 01 DE-16-250 04 p (DE-627)1809686113 Ranc, Clément 2013 01 DE-16-250 04 k (DE-627)1416733728 ZAH Astronomisches Recheninstitut 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_34 |
| allfieldsSound |
10.3847/1538-4365/ac7441 doi (DE-627)181340934X (DE-599)KXP181340934X (OCoLC)1361713329 DE-627 ger DE-627 rda eng Lam, Casey verfasserin (DE-588)1264818203 (DE-627)1813409978 aut An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mróz, Radek Poleski, Takahiro Sumi, Michał K. Szymański, Szymon Kozłowski, Paweł Pietrukowicz, Igor Soszyński, Krzysztof Ulaczyk, Łukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek, Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clément Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, and Sean K. Terry 2022 July 6 42 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 08.08.2022 This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Lu, Jessica R. verfasserin aut Udalski, Andrzej verfasserin aut Bond, Ian verfasserin aut Bennett, David P. verfasserin (DE-588)1283262819 (DE-627)1839065133 aut Skowron, Jan verfasserin aut Mróz, Przemek verfasserin aut Poleski, Radek verfasserin aut Sumi, Takahiro verfasserin aut Szymański, Micha\l K. verfasserin aut Koz\lowski, Szymon verfasserin aut Pietrukowicz, Pawe\l verfasserin aut Soszyński, Igor verfasserin aut Ulaczyk, Krzysztof verfasserin aut Wyrzykowski, \Lukasz verfasserin aut Miyazaki, Shota verfasserin aut Suzuki, Daisuke verfasserin aut Koshimoto, Naoki verfasserin aut Rattenbury, Nicholas J. verfasserin aut Hosek, Matthew W. verfasserin aut Abe, Fumio verfasserin aut Barry, Richard verfasserin aut Bhattacharya, Aparna verfasserin aut Fukui, Akihiko verfasserin aut Fujii, Hirosane verfasserin aut Hirao, Yuki verfasserin aut Itow, Yoshitaka verfasserin aut Kirikawa, Rintaro verfasserin aut Kondo, Iona verfasserin aut Matsubara, Yutaka verfasserin aut Matsumoto, Sho verfasserin aut Muraki, Yasushi verfasserin aut Olmschenk, Greg verfasserin aut Ranc, Clément verfasserin (DE-588)1204147469 (DE-627)1689284927 aut Okamura, Arisa verfasserin aut Satoh, Yuki K. verfasserin (DE-588)1315041014 (DE-627)1877269689 aut Silva, Stela Ishitani verfasserin aut Toda, Taiga verfasserin aut Tristram, Paul J. verfasserin aut Vandorou, Aikaterini verfasserin aut Yama, Hibiki verfasserin aut Abrams, Natasha S. verfasserin aut Agarwal, Shrihan verfasserin aut Rose, Sam verfasserin aut Terry, Sean K. verfasserin aut Enthalten in The astrophysical journal. Supplement series London : Institute of Physics Publ., 1996 260(2022), 2, Artikel-ID 55, Seite 1-42 Online-Ressource (DE-627)312200196 (DE-600)2006860-8 (DE-576)090890892 1538-4365 nnns volume:260 year:2022 number:2 elocationid:55 pages:1-42 extent:42 https://doi.org/10.3847/1538-4365/ac7441 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_65 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_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 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 260 2022 2 55 1-42 42 2013 01 DE-16-250 4176843403 00 --%%-- --%%-- --%%-- --%%-- l01 08-08-22 2013 01 DE-16-250 00 s hd2022 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_45 2013 01 DE-16-250 03 s s_42 2013 01 DE-16-250 04 p (DE-627)1809686113 Ranc, Clément 2013 01 DE-16-250 04 k (DE-627)1416733728 ZAH Astronomisches Recheninstitut 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_34 |
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An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) |
| abstract |
This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Gesehen am 08.08.2022 |
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This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Gesehen am 08.08.2022 |
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This supplement provides supporting material for Lam et al. We briefly summarize past gravitational microlensing searches for black holes (BHs) and present details of the observations, analysis, and modeling of five BH candidates observed with both ground-based photometric microlensing surveys and Hubble Space Telescope astrometry and photometry. We present detailed results for four of the five candidates that show no or low probability for the lens to be a BH. In these cases, the lens masses are <2 M ⊙, and two of the four are likely white dwarfs or neutron stars. We also present detailed methods for comparing the full sample of five candidates to theoretical expectations of the number of BHs in the Milky Way (∼108). Gesehen am 08.08.2022 |
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An isolated mass-gap black hole or neutron star detected with astrometric microlensing (2022, ApJL, 933, L23) |
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Lu, Jessica R. Udalski, Andrzej Bond, Ian Bennett, David P. Skowron, Jan Mróz, Przemek Poleski, Radek Sumi, Takahiro Szymański, Micha\l K. Koz\lowski, Szymon Pietrukowicz, Pawe\l Soszyński, Igor Ulaczyk, Krzysztof Wyrzykowski, \Lukasz Miyazaki, Shota Suzuki, Daisuke Koshimoto, Naoki Rattenbury, Nicholas J. Hosek, Matthew W. Abe, Fumio Barry, Richard Bhattacharya, Aparna Fukui, Akihiko Fujii, Hirosane Hirao, Yuki Itow, Yoshitaka Kirikawa, Rintaro Kondo, Iona Matsubara, Yutaka Matsumoto, Sho Muraki, Yasushi Olmschenk, Greg Ranc, Clément Okamura, Arisa Satoh, Yuki K. Silva, Stela Ishitani Toda, Taiga Tristram, Paul J. Vandorou, Aikaterini Yama, Hibiki Abrams, Natasha S. Agarwal, Shrihan Rose, Sam Terry, Sean K. |
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Lu, Jessica R. Udalski, Andrzej Bond, Ian Bennett, David P. Skowron, Jan Mróz, Przemek Poleski, Radek Sumi, Takahiro Szymański, Micha\l K. Koz\lowski, Szymon Pietrukowicz, Pawe\l Soszyński, Igor Ulaczyk, Krzysztof Wyrzykowski, \Lukasz Miyazaki, Shota Suzuki, Daisuke Koshimoto, Naoki Rattenbury, Nicholas J. Hosek, Matthew W. Abe, Fumio Barry, Richard Bhattacharya, Aparna Fukui, Akihiko Fujii, Hirosane Hirao, Yuki Itow, Yoshitaka Kirikawa, Rintaro Kondo, Iona Matsubara, Yutaka Matsumoto, Sho Muraki, Yasushi Olmschenk, Greg Ranc, Clément Okamura, Arisa Satoh, Yuki K. Silva, Stela Ishitani Toda, Taiga Tristram, Paul J. Vandorou, Aikaterini Yama, Hibiki Abrams, Natasha S. Agarwal, Shrihan Rose, Sam Terry, Sean K. |
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