stanford.bib

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@article{Cao2024,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2024ApJ...971L..45C},
	archiveprefix = {arXiv},
	author = {{Cao}, Zhen and {Aharonian}, F. and {Axikegu} and {Bai}, Y.~X. and {Bao}, Y.~W. and {Bastieri}, D. and {Bi}, X.~J. and {Bi}, Y.~J. and {Bian}, W. and {Bukevich}, A.~V. and {Cao}, Q. and {Cao}, W.~Y. and {Cao}, Zhe and {Chang}, J. and {Chang}, J.~F. and {Chen}, A.~M. and {Chen}, E.~S. and {Chen}, H.~X. and {Chen}, Liang and {Chen}, Lin and {Chen}, Long and {Chen}, M.~J. and {Chen}, M.~L. and {Chen}, Q.~H. and {Chen}, S. and {Chen}, S.~H. and {Chen}, S.~Z. and {Chen}, T.~L. and {Chen}, Y. and {Cheng}, N. and {Cheng}, Y.~D. and {Cui}, M.~Y. and {Cui}, S.~W. and {Cui}, X.~H. and {Cui}, Y.~D. and {Dai}, B.~Z. and {Dai}, H.~L. and {Dai}, Z.~G. and {Danzengluobu} and {Dong}, X.~Q. and {Duan}, K.~K. and {Fan}, J.~H. and {Fan}, Y.~Z. and {Fang}, J. and {Fang}, J.~H. and {Fang}, K. and {Feng}, C.~F. and {Feng}, H. and {Feng}, L. and {Feng}, S.~H. and {Feng}, X.~T. and {Feng}, Y. and {Feng}, Y.~L. and {Gabici}, S. and {Gao}, B. and {Gao}, C.~D. and {Gao}, Q. and {Gao}, W. and {Gao}, W.~K. and {Ge}, M.~M. and {Geng}, L.~S. and {Giacinti}, G. and {Gong}, G.~H. and {Gou}, Q.~B. and {Gu}, M.~H. and {Guo}, F.~L. and {Guo}, X.~L. and {Guo}, Y.~Q. and {Guo}, Y.~Y. and {Han}, Y.~A. and {Hasan}, M. and {He}, H.~H. and {He}, H.~N. and {He}, J.~Y. and {He}, Y. and {Hor}, Y.~K. and {Hou}, B.~W. and {Hou}, C. and {Hou}, X. and {Hu}, H.~B. and {Hu}, Q. and {Hu}, S.~C. and {Huang}, D.~H. and {Huang}, T.~Q. and {Huang}, W.~J. and {Huang}, X.~T. and {Huang}, X.~Y. and {Huang}, Y. and {Ji}, X.~L. and {Jia}, H.~Y. and {Jia}, K. and {Jiang}, K. and {Jiang}, X.~W. and {Jiang}, Z.~J. and {Jin}, M. and {Kang}, M.~M. and {Karpikov}, I. and {Kuleshov}, D. and {Kurinov}, K. and {Li}, B.~B. and {Li}, C.~M. and {Li}, Cheng and {Li}, Cong and {Li}, D. and {Li}, F. and {Li}, H.~B. and {Li}, H.~C. and {Li}, Jian and {Li}, Jie and {Li}, K. and {Li}, S.~D. and {Li}, W.~L. and {Li}, W.~L. and {Li}, X.~R. and {Li}, Xin and {Li}, Y.~Z. and {Li}, Zhe and {Li}, Zhuo and {Liang}, E.~W. and {Liang}, Y.~F. and {Lin}, S.~J. and {Liu}, B. and {Liu}, C. and {Liu}, D. and {Liu}, D.~B. and {Liu}, H. and {Liu}, H.~D. and {Liu}, J. and {Liu}, J.~L. and {Liu}, M.~Y. and {Liu}, R.~Y. and {Liu}, S.~M. and {Liu}, W. and {Liu}, Y. and {Liu}, Y.~N. and {Luo}, Q. and {Luo}, Y. and {Lv}, H.~K. and {Ma}, B.~Q. and {Ma}, L.~L. and {Ma}, X.~H. and {Mao}, J.~R. and {Min}, Z. and {Mitthumsiri}, W. and {Mu}, H.~J. and {Nan}, Y.~C. and {Neronov}, A. and {Ou}, L.~J. and {Pattarakijwanich}, P. and {Pei}, Z.~Y. and {Qi}, J.~C. and {Qi}, M.~Y. and {Qiao}, B.~Q. and {Qin}, J.~J. and {Raza}, A. and {Ruffolo}, D. and {S{\'a}iz}, A. and {Saeed}, M. and {Semikoz}, D. and {Shao}, L. and {Shchegolev}, O. and {Sheng}, X.~D. and {Shu}, F.~W. and {Song}, H.~C. and {Stenkin}, Yu. V. and {Stepanov}, V. and {Su}, Y. and {Sun}, D.~X. and {Sun}, Q.~N. and {Sun}, X.~N. and {Sun}, Z.~B. and {Takata}, J. and {Tam}, P.~H.~T. and {Tang}, Q.~W. and {Tang}, R. and {Tang}, Z.~B. and {Tian}, W.~W. and {Wang}, C. and {Wang}, C.~B. and {Wang}, G.~W. and {Wang}, H.~G. and {Wang}, H.~H. and {Wang}, J.~C. and {Wang}, Kai and {Wang}, Kai and {Wang}, L.~P. and {Wang}, L.~Y. and {Wang}, P.~H. and {Wang}, R. and {Wang}, W. and {Wang}, X.~G. and {Wang}, X.~Y. and {Wang}, Y. and {Wang}, Y.~D. and {Wang}, Y.~J. and {Wang}, Z.~H. and {Wang}, Z.~X. and {Wang}, Zhen and {Wang}, Zheng and {Wei}, D.~M. and {Wei}, J.~J. and {Wei}, Y.~J. and {Wen}, T. and {Wu}, C.~Y. and {Wu}, H.~R. and {Wu}, Q.~W. and {Wu}, S. and {Wu}, X.~F. and {Wu}, Y.~S. and {Xi}, S.~Q. and {Xia}, J. and {Xiang}, G.~M. and {Xiao}, D.~X. and {Xiao}, G. and {Xin}, Y.~L. and {Xing}, Y. and {Xiong}, D.~R. and {Xiong}, Z. and {Xu}, D.~L. and {Xu}, R.~F. and {Xu}, R.~X. and {Xu}, W.~L. and {Xue}, L. and {Yan}, D.~H. and {Yan}, J.~Z. and {Yan}, T. and {Yang}, C.~W. and {Yang}, C.~Y. and {Yang}, F. and {Yang}, F.~F. and {Yang}, L.~L. and {Yang}, M.~J. and {Yang}, R.~Z. and {Yang}, W.~X. and {Yao}, Y.~H. and {Yao}, Z.~G. and {Yin}, L.~Q. and {Yin}, N. and {You}, X.~H. and {You}, Z.~Y. and {Yu}, Y.~H. and {Yuan}, Q. and {Yue}, H. and {Zeng}, H.~D. and {Zeng}, T.~X. and {Zeng}, W. and {Zha}, M. and {Zhang}, B.~B. and {Zhang}, F. and {Zhang}, H. and {Zhang}, H.~M. and {Zhang}, H.~Y. and {Zhang}, J.~L. and {Zhang}, Li and {Zhang}, P.~F. and {Zhang}, P.~P. and {Zhang}, R. and {Zhang}, S.~B. and {Zhang}, S.~R. and {Zhang}, S.~S. and {Zhang}, X. and {Zhang}, X.~P. and {Zhang}, Y.~F. and {Zhang}, Yi and {Zhang}, Yong and {Zhao}, B. and {Zhao}, J. and {Zhao}, L. and {Zhao}, L.~Z. and {Zhao}, S.~P. and {Zhao}, X.~H. and {Zheng}, F. and {Zhong}, W.~J. and {Zhou}, B. and {Zhou}, H. and {Zhou}, J.~N. and {Zhou}, M. and {Zhou}, P. and {Zhou}, R. and {Zhou}, X.~X. and {Zhou}, X.~X. and {Zhu}, B.~Y. and {Zhu}, C.~G. and {Zhu}, F.~R. and {Zhu}, H. and {Zhu}, K.~J. and {Zou}, Y.~C. and {Zuo}, X. and {The Lhaaso Collaboration}},
	date-added = {2024-08-26 11:47:40 -0500},
	date-modified = {2024-08-26 11:47:42 -0500},
	doi = {10.3847/2041-8213/ad5e6d},
	eid = {L45},
	eprint = {2405.07691},
	journal = {\apjl},
	keywords = {High energy astrophysics, Gamma-ray astronomy, Low-luminosity active galactic nuclei, LINER galaxies, Blazars, Fanaroff-Riley radio galaxies, 739, 628, 2033, 925, 164, 526, Astrophysics - High Energy Astrophysical Phenomena},
	month = aug,
	number = {2},
	pages = {L45},
	primaryclass = {astro-ph.HE},
	title = {{Discovery of Very High Energy Gamma-Ray Emissions from the Low-luminosity AGN NGC 4278 by LHAASO}},
	volume = {971},
	year = 2024,
	bdsk-url-1 = {https://doi.org/10.3847/2041-8213/ad5e6d}}

@article{Colpi2014,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2014SSRv..183..189C},
	archiveprefix = {arXiv},
	author = {{Colpi}, Monica},
	date-added = {2024-06-11 14:22:34 -0700},
	date-modified = {2024-06-11 14:22:36 -0700},
	doi = {10.1007/s11214-014-0067-1},
	eprint = {1407.3102},
	journal = {\ssr},
	keywords = {Black hole physics, Dynamics, Galaxy mergers, Black hole binaries, Astrophysics - Astrophysics of Galaxies},
	month = sep,
	number = {1-4},
	pages = {189-221},
	primaryclass = {astro-ph.GA},
	title = {{Massive Binary Black Holes in Galactic Nuclei and Their Path to Coalescence}},
	volume = {183},
	year = 2014,
	bdsk-url-1 = {https://doi.org/10.1007/s11214-014-0067-1}}

@article{Adam2017,
	abstract = {Quark--gluon plasma is an exotic state of matter that can emerge in heavy nuclei high-energy collisions. The ALICE collaboration reports the first observation of strangeness enhancement in proton--proton collisions, a possible signature of this state.},
	annote = {Cited in FAPESP project},
	author = {Adam, J. and Adamov{\'a}, D. and Aggarwal, M. M. and Rinella, G. Aglieri and Agnello, M. and Agrawal, N. and Ahammed, Z. and Ahmad, S. and Ahn, S. U. and Aiola, S. and Akindinov, A. and Alam, S. N. and Albuquerque, D. S. D. and Aleksandrov, D. and Alessandro, B. and Alexandre, D. and Molina, R. Alfaro and Alici, A. and Alkin, A. and Alme, J. and Alt, T. and Altinpinar, S. and Altsybeev, I. and Prado, C. Alves Garcia and An, M. and Andrei, C. and Andrews, H. A. and Andronic, A. and Anguelov, V. and Anti{\v c}i{\'c}, T. and Antinori, F. and Antonioli, P. and Aphecetche, L. and Appelsh{\"a}user, H. and Arcelli, S. and Arnaldi, R. and Arnold, O. W. and Arsene, I. C. and Arslandok, M. and Audurier, B. and Augustinus, A. and Averbeck, R. and Azmi, M. D. and Badal{\`a}, A. and Baek, Y. W. and Bagnasco, S. and Bailhache, R. and Bala, R. and Balasubramanian, S. and Baldisseri, A. and Baral, R. C. and Barbano, A. M. and Barbera, R. and Barile, F. and Barnaf{\"o}ldi, G. G. and Barnby, L. S. and Barret, V. and Bartalini, P. and Barth, K. and Bartke, J. and Bartsch, E. and Basile, M. and Bastid, N. and Basu, S. and Bathen, B. and Batigne, G. and Camejo, A. Batista and Batyunya, B. and Batzing, P. C. and Bearden, I. G. and Beck, H. and Bedda, C. and Behera, N. K. and Belikov, I. and Bellini, F. and Martinez, H. Bello and Bellwied, R. and Belmont, R. and Belmont-Moreno, E. and Beltran, L. G. E. and Belyaev, V. and Bencedi, G. and Beole, S. and Berceanu, I. and Bercuci, A. and Berdnikov, Y. and Berenyi, D. and Bertens, R. A. and Berzano, D. and Betev, L. and Bhasin, A. and Bhat, I. R. and Bhati, A. K. and Bhattacharjee, B. and Bhom, J. and Bianchi, L. and Bianchi, N. and Bianchin, C. and Biel{\v c}{\'\i}k, J. and Biel{\v c}{\'\i}kov{\'a}, J. and Bilandzic, A. and Biro, G. and Biswas, R. and Biswas, S. and Bjelogrlic, S. and Blair, J. T. and Blau, D. and Blume, C. and Bock, F. and Bogdanov, A. and B{\o}ggild, H. and Boldizs{\'a}r, L. and Bombara, M. and Bonora, M. and Book, J. and Borel, H. and Borissov, A. and Borri, M. and Boss{\'u}, F. and Botta, E. and Bourjau, C. and Braun-Munzinger, P. and Bregant, M. and Breitner, T. and Broker, T. A. and Browning, T. A. and Broz, M. and Brucken, E. J. and Bruna, E. and Bruno, G. E. and Budnikov, D. and Buesching, H. and Bufalino, S. and Buncic, P. and Busch, O. and Buthelezi, Z. and Butt, J. B. and Buxton, J. T. and Cabala, J. and Caffarri, D. and Cai, X. and Caines, H. and Diaz, L. Calero and Caliva, A. and Villar, E. Calvo and Camerini, P. and Carena, F. and Carena, W. and Carnesecchi, F. and Castellanos, J. Castillo and Castro, A. J. and Casula, E. A. R. and Sanchez, C. Ceballos and Cepila, J. and Cerello, P. and Cerkala, J. and Chang, B. and Chapeland, S. and Chartier, M. and Charvet, J. L. and Chattopadhyay, S. and Chattopadhyay, S. and Chauvin, A. and Chelnokov, V. and Cherney, M. and Cheshkov, C. and Cheynis, B. and Barroso, V. Chibante and Chinellato, D. D. and Cho, S. and Chochula, P. and Choi, K. and Chojnacki, M. and Choudhury, S. and Christakoglou, P. and Christensen, C. H. and Christiansen, P. and Chujo, T. and Chung, S. U. and Cicalo, C. and Cifarelli, L. and Cindolo, F. and Cleymans, J. and Colamaria, F. and Colella, D. and Collu, A. and Colocci, M. and Balbastre, G. Conesa and del Valle, Z. Conesa and Connors, M. E. and Contreras, J. G. and Cormier, T. M. and Morales, Y. Corrales and Maldonado, I. Cort{\'e}s and Cortese, P. and Cosentino, M. R. and Costa, F. and Crkovska, J. and Crochet, P. and Albino, R. Cruz and Cuautle, E. and Cunqueiro, L. and Dahms, T. and Dainese, A. and Danisch, M. C. and Danu, A. and Das, D. and Das, I. and Das, S. and Dash, A. and Dash, S. and De, S. and De Caro, A. and de Cataldo, G. and de Conti, C. and de Cuveland, J. and De Falco, A. and De Gruttola, D. and De Marco, N. and De Pasquale, S. and De Souza, R. D. and Deisting, A. and Deloff, A. and D{\'e}nes, E. and Deplano, C. and Dhankher, P. and Di Bari, D. and Di Mauro, A. and Di Nezza, P. and Di Ruzza, B. and Corchero, M. A. Diaz and Dietel, T. and Dillenseger, P. and Divi{\`a}, R. and Djuvsland, {\O}. and Dobrin, A. and Gimenez, D. Domenicis and D{\"o}nigus, B. and Dordic, O. and Drozhzhova, T. and Dubey, A. K. and Dubla, A. and Ducroux, L. and Dupieux, P. and Ehlers, R. J. and Elia, D. and Endress, E. and Engel, H. and Epple, E. and Erazmus, B. and Erdemir, I. and Erhardt, F. and Espagnon, B. and Estienne, M. and Esumi, S. and Eum, J. and Evans, D. and Evdokimov, S. and Eyyubova, G. and Fabbietti, L. and Fabris, D. and Faivre, J. and Fantoni, A. and Fasel, M. and Feldkamp, L. and Feliciello, A. and Feofilov, G. and Ferencei, J. and T{\'e}llez, A. Fern{\'a}ndez and Ferreiro, E. G. and Ferretti, A. and Festanti, A. and Feuillard, V. J. G. and Figiel, J. and Figueredo, M. A. S. and Filchagin, S. and Finogeev, D. and Fionda, F. M. and Fiore, E. M. and Floris, M. and Foertsch, S. and Foka, P. and Fokin, S. and Fragiacomo, E. and Francescon, A. and Francisco, A. and Frankenfeld, U. and Fronze, G. G. and Fuchs, U. and Furget, C. and Furs, A. and Girard, M. Fusco and Gaardh{\o}je, J. J. and Gagliardi, M. and Gago, A. M. and Gajdosova, K. and Gallio, M. and Galvan, C. D. and Gangadharan, D. R. and ALICE Collaboration},
	date = {2017/06/01},
	date-added = {2024-05-06 17:25:39 -0700},
	date-modified = {2024-05-06 17:25:57 -0700},
	doi = {10.1038/nphys4111},
	id = {Adam2017},
	isbn = {1745-2481},
	journal = {Nature Physics},
	number = {6},
	pages = {535--539},
	title = {Enhanced production of multi-strange hadrons in high-multiplicity proton--proton collisions},
	url = {https://doi.org/10.1038/nphys4111},
	volume = {13},
	year = {2017},
	bdsk-url-1 = {https://doi.org/10.1038/nphys4111}}

@article{Thompson2019,
	abstract = {As material falls toward a black hole, it heats up and emits x-rays. Almost all black holes are discovered by this x-ray emission. Thompson et al. observed light from a giant star that is Doppler shifted, indicating an orbit around a binary companion. The companion object must weigh more than 2.6 solar masses, but it emits no light, including x-rays. This indicates the presence of a black hole that is not currently consuming any material. There may be a population of similarly hidden black holes that have been missed by x-ray observations. Science, this issue p. 637 A binary star contains a noninteracting compact object, probably a previously hidden black hole. Black hole binary systems with companion stars are typically found via their x-ray emission, generated by interaction and accretion. Noninteracting binaries are expected to be plentiful in the Galaxy but must be observed using other methods. We combine radial velocity and photometric variability data to show that the bright, rapidly rotating giant star 2MASS J05215658+4359220 is in a binary system with a massive unseen companion. The system has an orbital period of ~83 days and near-zero eccentricity. The photometric variability period of the giant is consistent with the orbital period, indicating star spots and tidal synchronization. Constraints on the giant's mass and radius imply that the unseen companion is 3.3−0.7+2.8 solar masses, indicating that it is a noninteracting low-mass black hole or an unexpectedly massive neutron star.},
	author = {Todd A. Thompson and Christopher S. Kochanek and Krzysztof Z. Stanek and Carles Badenes and Richard S. Post and Tharindu Jayasinghe and David W. Latham and Allyson Bieryla and Gilbert A. Esquerdo and Perry Berlind and Michael L. Calkins and Jamie Tayar and Lennart Lindegren and Jennifer A. Johnson and Thomas W.-S. Holoien and Katie Auchettl and Kevin Covey},
	date-added = {2024-03-11 21:02:26 -0700},
	date-modified = {2024-03-11 21:02:26 -0700},
	doi = {10.1126/science.aau4005},
	eprint = {https://www.science.org/doi/pdf/10.1126/science.aau4005},
	journal = {Science},
	number = {6465},
	pages = {637-640},
	title = {A noninteracting low-mass black hole--giant star binary system},
	url = {https://www.science.org/doi/abs/10.1126/science.aau4005},
	volume = {366},
	year = {2019},
	bdsk-url-1 = {https://www.science.org/doi/abs/10.1126/science.aau4005},
	bdsk-url-2 = {https://doi.org/10.1126/science.aau4005}}

@article{Barr2024,
	abstract = {Some compact objects observed in gravitational wave events have masses in the gap between known neutron stars (NSs) and black holes (BHs). The nature of these mass gap objects is unknown, as is the formation of their host binary systems. We report pulsar timing observations made with the Karoo Array Telescope (MeerKAT) of PSR J0514−4002E, an eccentric binary millisecond pulsar in the globular cluster NGC 1851. We found a total binary mass of 3.887 $\pm$ 0.004 solar masses (M⊙), and multiwavelength observations show that the pulsar's binary companion is also a compact object. The companion's mass (2.09 to 2.71 M⊙, 95\% confidence interval) is in the mass gap, indicating either a very massive NS or a low-mass BH. We propose that the companion formed in a merger between two earlier NSs. There is a substantial gap between the masses of the heaviest measured neutron star and the lightest measured black hole. This mass gap carries information about how both types of object form during supernovae (see the Perspective by Fishbach). Barr et al. used pulsar timing to investigate a binary system in a dense star cluster. They found that the pulsar's binary companion is an object in the mass gap, but could not determine whether it is an unusually high-mass neutron star or an unusually low-mass black hole. Either way, the authors argue that it formed by the earlier merger of two other neutron stars. ---Keith T. Smith Radio timing of a pulsar indicates that it has a binary companion in the mass gap between neutron stars and black holes.},
	author = {Ewan D. Barr and Arunima Dutta and Paulo C. C. Freire and Mario Cadelano and Tasha Gautam and Michael Kramer and Cristina Pallanca and Scott M. Ransom and Alessandro Ridolfi and Benjamin W. Stappers and Thomas M. Tauris and Vivek Venkatraman Krishnan and Norbert Wex and Matthew Bailes and Jan Behrend and Sarah Buchner and Marta Burgay and Weiwei Chen and David J. Champion and C.-H. Rosie Chen and Alessandro Corongiu and Marisa Geyer and Y. P. Men and Prajwal Voraganti Padmanabh and Andrea Possenti},
	date-added = {2024-03-11 21:02:21 -0700},
	date-modified = {2024-03-11 21:02:21 -0700},
	doi = {10.1126/science.adg3005},
	eprint = {https://www.science.org/doi/pdf/10.1126/science.adg3005},
	journal = {Science},
	number = {6680},
	pages = {275-279},
	title = {A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes},
	url = {https://www.science.org/doi/abs/10.1126/science.adg3005},
	volume = {383},
	year = {2024},
	bdsk-url-1 = {https://www.science.org/doi/abs/10.1126/science.adg3005},
	bdsk-url-2 = {https://doi.org/10.1126/science.adg3005}}

@article{Connors2021,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...909..146C},
	archiveprefix = {arXiv},
	author = {{Connors}, Riley M.~T. and {Garc{\'\i}a}, Javier A. and {Tomsick}, John and {Hare}, Jeremy and {Dauser}, Thomas and {Grinberg}, Victoria and {Steiner}, James F. and {Mastroserio}, Guglielmo and {Sridhar}, Navin and {Fabian}, Andrew C. and {Jiang}, Jiachen and {Parker}, Michael L. and {Harrison}, Fiona and {Kallman}, Timothy R.},
	date-added = {2024-02-20 10:47:45 -0800},
	date-modified = {2024-02-20 10:47:46 -0800},
	doi = {10.3847/1538-4357/abdd2c},
	eid = {146},
	eprint = {2101.06343},
	journal = {\apj},
	keywords = {Accretion, Stellar accretion disks, black hole physics, Atomic physics, Low-mass x-ray binary stars, 14, 1579, 159, 2063, 939, Astrophysics - High Energy Astrophysical Phenomena},
	month = mar,
	number = {2},
	pages = {146},
	primaryclass = {astro-ph.HE},
	title = {{Reflection Modeling of the Black Hole Binary 4U 1630-47: The Disk Density and Returning Radiation}},
	volume = {909},
	year = 2021,
	bdsk-url-1 = {https://doi.org/10.3847/1538-4357/abdd2c}}

@article{Sridhar2020,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...890...53S},
	archiveprefix = {arXiv},
	author = {{Sridhar}, Navin and {Garc{\'\i}a}, Javier A. and {Steiner}, James F. and {Connors}, Riley M.~T. and {Grinberg}, Victoria and {Harrison}, Fiona A.},
	date-added = {2024-02-20 10:46:51 -0800},
	date-modified = {2024-02-20 10:46:52 -0800},
	doi = {10.3847/1538-4357/ab64f5},
	eid = {53},
	eprint = {1912.11447},
	journal = {\apj},
	keywords = {High energy astrophysics, Compact objects, Black hole physics, Low-mass x-ray binary stars, Accretion, X-ray astronomy, Spectroscopy, Astronomy data modeling, X-ray sources, General relativity, Gravitation, Astrophysical black holes, 739, 288, 159, 939, 14, 1810, 1558, 1859, 1822, 641, 661, 98, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology, High Energy Physics - Experiment, Physics - Data Analysis, Statistics and Probability, Physics - Plasma Physics},
	month = feb,
	number = {1},
	pages = {53},
	primaryclass = {astro-ph.HE},
	title = {{Evolution of the Accretion Disk-Corona during the Bright Hard-to-soft State Transition: A Reflection Spectroscopic Study with GX 339-4}},
	volume = {890},
	year = 2020,
	bdsk-url-1 = {https://doi.org/10.3847/1538-4357/ab64f5}}

@article{Gierlinski1999,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/1999MNRAS.309..496G},
	archiveprefix = {arXiv},
	author = {{Gierli{\'n}ski}, Marek and {Zdziarski}, Andrzej A. and {Poutanen}, Juri and {Coppi}, Paolo S. and {Ebisawa}, Ken and {Johnson}, W. Neil},
	date-added = {2024-01-29 16:28:10 -0800},
	date-modified = {2024-01-29 16:28:11 -0800},
	doi = {10.1046/j.1365-8711.1999.02875.x},
	eprint = {astro-ph/9905146},
	journal = {\mnras},
	keywords = {Astrophysics},
	month = oct,
	number = {2},
	pages = {496-512},
	primaryclass = {astro-ph},
	title = {{Radiation mechanisms and geometry of Cygnus X-1 in the soft state}},
	volume = {309},
	year = 1999,
	bdsk-url-1 = {https://doi.org/10.1046/j.1365-8711.1999.02875.x}}

@article{Hankla2022,
	abstract = {{X-ray binaries exhibit a soft spectral state comprising thermal blackbody emission at 1 keV and a power-law tail above 10 keV. Empirical models fit the high-energy power-law tail to radiation from a non-thermal electron distribution, but the physical location of the non-thermal electrons and the reason for their power-law index and high-energy cut-off are still largely unknown. Here, we propose that the non-thermal electrons originate from within the black hole's innermost stable circular orbit (the `plunging region'). Using an analytic model for the plunging region dynamics and electron distribution function properties from particle-in-cell simulations, we outline a steady-state model that can reproduce the observed spectral features. In particular, our model reproduces photon indices of Γ ≳ 2 and power-law luminosities of the order of a few per cent of the disc luminosity for strong magnetic fields, consistent with observations of the soft state. Because the emission originates so close to the black hole, we predict that the power-law luminosity should strongly depend on the system inclination angle and black hole spin. This model could be extended to the power-law tails observed above 400 keV in the hard state of X-ray binaries.}},
	author = {Hankla, Amelia M and Scepi, Nicolas and Dexter, Jason},
	date-added = {2024-01-25 16:00:46 -0800},
	date-modified = {2024-01-25 16:00:55 -0800},
	doi = {10.1093/mnras/stac1785},
	eprint = {https://academic.oup.com/mnras/article-pdf/515/1/775/45026821/stac1785.pdf},
	issn = {0035-8711},
	journal = {\mnras},
	month = {06},
	number = {1},
	pages = {775-784},
	title = {{Non-thermal emission from the plunging region: a model for the high-energy tail of black hole X-ray binary soft states}},
	url = {https://doi.org/10.1093/mnras/stac1785},
	volume = {515},
	year = {2022},
	bdsk-url-1 = {https://doi.org/10.1093/mnras/stac1785}}

@article{Fabian2020,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.5389F},
	archiveprefix = {arXiv},
	author = {{Fabian}, A.~C. and {Buisson}, D.~J. and {Kosec}, P. and {Reynolds}, C.~S. and {Wilkins}, D.~R. and {Tomsick}, J.~A. and {Walton}, D.~J. and {Gandhi}, P. and {Altamirano}, D. and {Arzoumanian}, Z. and {Cackett}, E.~M. and {Dyda}, S. and {Garcia}, J.~A. and {Gendreau}, K.~C. and {Grefenstette}, B.~W. and {Homan}, J. and {Kara}, E. and {Ludlam}, R.~M. and {Miller}, J.~M. and {Steiner}, J.~F.},
	date-added = {2024-01-25 15:52:34 -0800},
	date-modified = {2024-01-25 15:52:35 -0800},
	doi = {10.1093/mnras/staa564},
	eprint = {2002.09691},
	journal = {\mnras},
	keywords = {accretion, accretion discs, X-rays: binaries, black hole physics, Astrophysics - High Energy Astrophysical Phenomena},
	month = apr,
	number = {4},
	pages = {5389-5396},
	primaryclass = {astro-ph.HE},
	title = {{The soft state of the black hole transient source MAXI J1820+070: emission from the edge of the plunge region?}},
	volume = {493},
	year = 2020,
	bdsk-url-1 = {https://doi.org/10.1093/mnras/staa564}}

@article{Agazie2023,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2023ApJ...952L..37A},
	archiveprefix = {arXiv},
	author = {{Agazie}, Gabriella and {Anumarlapudi}, Akash and {Archibald}, Anne M. and {Baker}, Paul T. and {B{\'e}csy}, Bence and {Blecha}, Laura and {Bonilla}, Alexander and {Brazier}, Adam and {Brook}, Paul R. and {Burke-Spolaor}, Sarah and {Burnette}, Rand and {Case}, Robin and {Casey-Clyde}, J. Andrew and {Charisi}, Maria and {Chatterjee}, Shami and {Chatziioannou}, Katerina and {Cheeseboro}, Belinda D. and {Chen}, Siyuan and {Cohen}, Tyler and {Cordes}, James M. and {Cornish}, Neil J. and {Crawford}, Fronefield and {Cromartie}, H. Thankful and {Crowter}, Kathryn and {Cutler}, Curt J. and {D'Orazio}, Daniel J. and {Decesar}, Megan E. and {Degan}, Dallas and {Demorest}, Paul B. and {Deng}, Heling and {Dolch}, Timothy and {Drachler}, Brendan and {Ferrara}, Elizabeth C. and {Fiore}, William and {Fonseca}, Emmanuel and {Freedman}, Gabriel E. and {Gardiner}, Emiko and {Garver-Daniels}, Nate and {Gentile}, Peter A. and {Gersbach}, Kyle A. and {Glaser}, Joseph and {Good}, Deborah C. and {G{\"u}ltekin}, Kayhan and {Hazboun}, Jeffrey S. and {Hourihane}, Sophie and {Islo}, Kristina and {Jennings}, Ross J. and {Johnson}, Aaron and {Jones}, Megan L. and {Kaiser}, Andrew R. and {Kaplan}, David L. and {Kelley}, Luke Zoltan and {Kerr}, Matthew and {Key}, Joey S. and {Laal}, Nima and {Lam}, Michael T. and {Lamb}, William G. and {Lazio}, T. Joseph W. and {Lewandowska}, Natalia and {Littenberg}, Tyson B. and {Liu}, Tingting and {Luo}, Jing and {Lynch}, Ryan S. and {Ma}, Chung-Pei and {Madison}, Dustin R. and {McEwen}, Alexander and {McKee}, James W. and {McLaughlin}, Maura A. and {McMann}, Natasha and {Meyers}, Bradley W. and {Meyers}, Patrick M. and {Mingarelli}, Chiara M.~F. and {Mitridate}, Andrea and {Natarajan}, Priyamvada and {Ng}, Cherry and {Nice}, David J. and {Ocker}, Stella Koch and {Olum}, Ken D. and {Pennucci}, Timothy T. and {Perera}, Benetge B.~P. and {Petrov}, Polina and {Pol}, Nihan S. and {Radovan}, Henri A. and {Ransom}, Scott M. and {Ray}, Paul S. and {Romano}, Joseph D. and {Runnoe}, Jessie C. and {Sardesai}, Shashwat C. and {Schmiedekamp}, Ann and {Schmiedekamp}, Carl and {Schmitz}, Kai and {Schult}, Levi and {Shapiro-Albert}, Brent J. and {Siemens}, Xavier and {Simon}, Joseph and {Siwek}, Magdalena S. and {Stairs}, Ingrid H. and {Stinebring}, Daniel R. and {Stovall}, Kevin and {Sun}, Jerry P. and {Susobhanan}, Abhimanyu and {Swiggum}, Joseph K. and {Taylor}, Jacob and {Taylor}, Stephen R. and {Turner}, Jacob E. and {Unal}, Caner and {Vallisneri}, Michele and {Vigeland}, Sarah J. and {Wachter}, Jeremy M. and {Wahl}, Haley M. and {Wang}, Qiaohong and {Witt}, Caitlin A. and {Wright}, David and {Young}, Olivia and {Nanograv Collaboration}},
	date-added = {2023-10-30 16:23:57 -0700},
	date-modified = {2023-10-30 16:23:58 -0700},
	doi = {10.3847/2041-8213/ace18b},
	eid = {L37},
	eprint = {2306.16220},
	journal = {\apjl},
	keywords = {Gravitational waves, Supermassive black holes, Galaxy evolution, 678, 1663, 594, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology},
	month = aug,
	number = {2},
	pages = {L37},
	primaryclass = {astro-ph.HE},
	title = {{The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background}},
	volume = {952},
	year = 2023,
	bdsk-url-1 = {https://doi.org/10.3847/2041-8213/ace18b}}

@article{Karouzos2019,
	abstract = {Mitchell C. Begelman, Professor in the Department of Astrophysical and Planetary Sciences at the University of Colorado Boulder and a black hole expert, discusses the start of the field with Nature Astronomy.},
	author = {Karouzos, Marios},
	date = {2019/01/01},
	date-added = {2023-09-03 10:00:43 -0700},
	date-modified = {2023-09-03 10:00:43 -0700},
	doi = {10.1038/s41550-018-0671-1},
	id = {Karouzos2019},
	isbn = {2397-3366},
	journal = {Nature Astronomy},
	number = {1},
	pages = {2--5},
	title = {Black holes},
	url = {https://doi.org/10.1038/s41550-018-0671-1},
	volume = {3},
	year = {2019},
	bdsk-url-1 = {https://doi.org/10.1038/s41550-018-0671-1}}

@article{Mandarakas2019,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...623A..61M},
	archiveprefix = {arXiv},
	author = {{Mandarakas}, N. and {Blinov}, D. and {Liodakis}, I. and {Kouroumpatzakis}, K. and {Zezas}, A. and {Panopoulou}, G.~V. and {Myserlis}, I. and {Angelakis}, E. and {Hovatta}, T. and {Kiehlmann}, S. and {Kokolakis}, K. and {Paleologou}, E. and {Pouliasi}, A. and {Skalidis}, R. and {Pavlidou}, V.},
	date-added = {2023-09-03 09:59:09 -0700},
	date-modified = {2023-09-03 09:59:10 -0700},
	doi = {10.1051/0004-6361/201834458},
	eid = {A61},
	eprint = {1810.06312},
	journal = {\aap},
	keywords = {techniques: polarimetric, galaxies: active, gamma rays: galaxies, Astrophysics - High Energy Astrophysical Phenomena},
	month = mar,
	pages = {A61},
	primaryclass = {astro-ph.HE},
	title = {{Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique}},
	volume = {623},
	year = 2019,
	bdsk-url-1 = {https://doi.org/10.1051/0004-6361/201834458}}

@article{Schutte2022,
	abstract = {Black-hole-driven outflows have been observed in some dwarf galaxies with active galactic nuclei1, and probably play a role in heating and expelling gas (thereby suppressing star formation), as they do in larger galaxies2. The extent to which black-hole outflows can trigger star formation in dwarf galaxies is unclear, because work in this area has previously focused on massive galaxies and the observational evidence is scarce3--5. Henize 2-10 is a dwarf starburst galaxy previously reported to have a central massive black hole6--9, although that interpretation has been disputed because some aspects of the observational evidence are also consistent with a supernova remnant10,11. At a distance of approximately 9 Mpc, it presents an opportunity to resolve the central region and to determine if there is evidence for a black-hole outflow influencing star formation. Here we report optical observations of Henize 2-10 with a linear resolution of a few parsecs. We find an approximately 150-pc-long ionized filament connecting the region of the black hole with a site of recent star formation. Spectroscopy reveals a sinusoid-like position--velocity structure that is well described by a simple precessing bipolar outflow. We conclude that this black-hole outflow triggered the star formation.},
	author = {Schutte, Zachary and Reines, Amy E.},
	date = {2022/01/01},
	date-added = {2023-09-03 09:55:56 -0700},
	date-modified = {2023-09-03 09:55:56 -0700},
	doi = {10.1038/s41586-021-04215-6},
	id = {Schutte2022},
	isbn = {1476-4687},
	journal = {Nature},
	number = {7893},
	pages = {329--333},
	title = {Black-hole-triggered star formation in the dwarf galaxy Henize 2-10},
	url = {https://doi.org/10.1038/s41586-021-04215-6},
	volume = {601},
	year = {2022},
	bdsk-url-1 = {https://doi.org/10.1038/s41586-021-04215-6}}

@article{Neilsen2011,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2011PNAS..10812641N},
	archiveprefix = {arXiv},
	author = {{Neilsen}, D. and {Lehner}, L. and {Palenzuela}, C. and {Hirschmann}, E.~W. and {Liebling}, S.~L. and {Motl}, P.~M. and {Garrett}, T.},
	date-added = {2023-05-15 17:46:22 -0700},
	date-modified = {2023-05-15 17:46:23 -0700},
	doi = {10.1073/pnas.1019618108},
	eprint = {1012.5661},
	journal = {Proceedings of the National Academy of Science},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology},
	month = aug,
	number = {31},
	pages = {12641-12646},
	primaryclass = {astro-ph.HE},
	title = {{Boosting jet power in black hole spacetimes}},
	volume = {108},
	year = 2011,
	bdsk-url-1 = {https://doi.org/10.1073/pnas.1019618108}}

@article{Combi2022,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...928..187C},
	archiveprefix = {arXiv},
	author = {{Combi}, Luciano and {Lopez Armengol}, Federico G. and {Campanelli}, Manuela and {Noble}, Scott C. and {Avara}, Mark and {Krolik}, Julian H. and {Bowen}, Dennis},
	date-added = {2023-05-15 17:10:27 -0700},
	date-modified = {2023-05-15 17:10:29 -0700},
	doi = {10.3847/1538-4357/ac532a},
	eid = {187},
	eprint = {2109.01307},
	journal = {\apj},
	keywords = {Supermassive black holes, Jets, Compact objects, Magnetohydrodynamical simulations, 1663, 870, 288, 1966, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = apr,
	number = {2},
	pages = {187},
	primaryclass = {astro-ph.HE},
	title = {{Minidisk Accretion onto Spinning Black Hole Binaries: Quasi-periodicities and Outflows}},
	volume = {928},
	year = 2022,
	bdsk-url-1 = {https://doi.org/10.3847/1538-4357/ac532a}}

@article{Paschalidis2021,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...910L..26P},
	archiveprefix = {arXiv},
	author = {{Paschalidis}, Vasileios and {Bright}, Jane and {Ruiz}, Milton and {Gold}, Roman},
	date-added = {2023-05-15 17:10:20 -0700},
	date-modified = {2023-05-15 17:10:21 -0700},
	doi = {10.3847/2041-8213/abee21},
	eid = {L26},
	eprint = {2102.06712},
	journal = {\apjl},
	keywords = {High energy astrophysics, Astrophysical black holes, black hole physics, Accretion, Gravitation, Gravitational wave sources, 739, 98, 159, 14, 661, 677, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, General Relativity and Quantum Cosmology},
	month = apr,
	number = {2},
	pages = {L26},
	primaryclass = {astro-ph.HE},
	title = {{Minidisk Dynamics in Accreting, Spinning Black Hole Binaries: Simulations in Full General Relativity}},
	volume = {910},
	year = 2021,
	bdsk-url-1 = {https://doi.org/10.3847/2041-8213/abee21}}

@article{Palenzuela2010,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2010PhRvD..82d4045P},
	archiveprefix = {arXiv},
	author = {{Palenzuela}, Carlos and {Garrett}, Travis and {Lehner}, Luis and {Liebling}, Steven L.},
	date-added = {2023-05-15 16:55:26 -0700},
	date-modified = {2023-05-15 16:55:27 -0700},
	doi = {10.1103/PhysRevD.82.044045},
	eid = {044045},
	eprint = {1007.1198},
	journal = {\prd},
	keywords = {04.25.dg, Numerical studies of black holes and black-hole binaries, General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = aug,
	number = {4},
	pages = {044045},
	primaryclass = {gr-qc},
	title = {{Magnetospheres of black hole systems in force-free plasma}},
	volume = {82},
	year = 2010,
	bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.82.044045}}

@article{Goldreich1969,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/1969ApJ...156...59G},
	author = {{Goldreich}, P. and {Lynden-Bell}, D.},
	date-added = {2023-05-11 16:20:10 -0700},
	date-modified = {2023-05-11 16:20:11 -0700},
	doi = {10.1086/149947},
	journal = {\apj},
	month = apr,
	pages = {59-78},
	title = {{Io, a jovian unipolar inductor}},
	volume = {156},
	year = 1969,
	bdsk-url-1 = {https://doi.org/10.1086/149947}}

@article{Piddington1968,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/1968Natur.217..935P},
	author = {{Piddington}, J.~H. and {Drake}, J.~F.},
	date-added = {2023-05-11 16:17:50 -0700},
	date-modified = {2023-05-11 16:17:51 -0700},
	doi = {10.1038/217935a0},
	journal = {\nat},
	month = mar,
	number = {5132},
	pages = {935-937},
	title = {{Electrodynamic Effects of Jupiter's Satellite Io}},
	volume = {217},
	year = 1968,
	bdsk-url-1 = {https://doi.org/10.1038/217935a0}}

@article{Gurnett1972,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/1972ApJ...175..525G},
	author = {{Gurnett}, Donald A.},
	date-added = {2023-05-11 16:12:59 -0700},
	date-modified = {2023-05-11 16:12:59 -0700},
	doi = {10.1086/151576},
	journal = {\apj},
	month = jul,
	pages = {525},
	title = {{Sheath Effects and Related Charged-Particle Acceleration by Jupiter's Satellite IO}},
	volume = {175},
	year = 1972,
	bdsk-url-1 = {https://doi.org/10.1086/151576}}

@inproceedings{Shawhan1975,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/1975ASSL...52..375S},
	author = {{Shawhan}, S.~D. and {Goertz}, C.~K. and {Hubbard}, R.~F. and {Gurnett}, D.~A. and {Joyce}, G.},
	booktitle = {The Magnetospheres of the Earth and Jupiter},
	date-added = {2023-05-11 16:12:20 -0700},
	date-modified = {2023-05-11 16:12:21 -0700},
	doi = {10.1007/978-94-010-1789-3_31},
	editor = {{Formisano}, V.},
	keywords = {Io, Jupiter Atmosphere, Particle Acceleration, Plasma Sheaths, Atmospheric Models, Earth Magnetosphere, Electrons, Emission Spectra, Ion Motion, Pioneer 10 Space Probe, Lunar and Planetary Exploration},
	month = jan,
	pages = {375},
	series = {Astrophysics and Space Science Library},
	title = {{Io Accelerated Electrons and Ions}},
	volume = {52},
	year = 1975,
	bdsk-url-1 = {https://doi.org/10.1007/978-94-010-1789-3_31}}

@article{Goicoechea2020,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...637A..89G},
	archiveprefix = {arXiv},
	author = {{Goicoechea}, L.~J. and {Artamonov}, B.~P. and {Shalyapin}, V.~N. and {Sergeyev}, A.~V. and {Burkhonov}, O.~A. and {Akhunov}, T.~A. and {Asfandiyarov}, I.~M. and {Bruevich}, V.~V. and {Ehgamberdiev}, S.~A. and {Shimanovskaya}, E.~V. and {Zheleznyak}, A.~P.},
	date-added = {2023-03-16 15:32:18 -0700},
	date-modified = {2023-03-16 15:32:19 -0700},
	doi = {10.1051/0004-6361/202037902},
	eid = {A89},
	eprint = {2004.04991},
	journal = {\aap},
	keywords = {techniques: photometric, methods: data analysis, gravitational lensing: strong, gravitational lensing: micro, quasars: individual: QSO 2237+0305, Astrophysics - Astrophysics of Galaxies},
	month = may,
	pages = {A89},
	primaryclass = {astro-ph.GA},
	title = {{Liverpool-Maidanak monitoring of the Einstein Cross in 2006-2019. I. Light curves in the gVrRI optical bands and microlensing signatures}},
	volume = {637},
	year = 2020,
	bdsk-url-1 = {https://doi.org/10.1051/0004-6361/202037902}}

@article{Millon2022,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...668A..77M},
	archiveprefix = {arXiv},
	author = {{Millon}, M. and {Dalang}, C. and {Lemon}, C. and {Sluse}, D. and {Paic}, E. and {Chan}, J.~H.~H. and {Courbin}, F.},
	date-added = {2023-03-16 15:31:47 -0700},
	date-modified = {2023-03-16 15:31:48 -0700},
	doi = {10.1051/0004-6361/202244440},
	eid = {A77},
	eprint = {2207.00598},
	journal = {\aap},
	keywords = {gravitational lensing: micro, quasars: supermassive black holes, methods: data analysis, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena},
	month = dec,
	pages = {A77},
	primaryclass = {astro-ph.GA},
	title = {{Evidence for a milliparsec-separation supermassive binary black hole with quasar microlensing}},
	volume = {668},
	year = 2022,
	bdsk-url-1 = {https://doi.org/10.1051/0004-6361/202244440}}