The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814

Autor(es):Mostrar menos -

Kilpatrick, Charles D. ^[1] ; Coulter, David A. ^[2] ; Arcavi, Iair ^{[3, 4]} ; Brink, Thomas G. ^[5] ; Dimitriadis, Georgios ^[2] ; Filippenko, V, Alexei ; Foley, Ryan J. ^[2] ; Howell, D. Andrew ^{[6, 7]} ; Jones, David O. ^[2] ; Kasen, Daniel ^{[8, 9, 10, 11]} ; Makler, Martin ^{[12, 13, 14, 15]} ; Piro, Anthony L. ^[16] ; Rojas-Bravo, Cesar ^[2] ; Sand, David J. ^[17] ; Swift, Jonathan J. ^[18] ; Tucker, Douglas ^[19] ; Zheng, WeiKang ^[11] ; Allam, Sahar S. ^[19] ; Annis, James T. ^[19] ; Antilen, Juanita ^[20] ; Bachmann, Tristan G. ^[21] ; Bloom, Joshua S. ^{[11, 22]} ; Bom, Clecio R. ^{[13, 23]} ; Bostroem, K. Azalee ^[24] ; Brout, Dillon ^[25] ; Burke, Jamison ^{[6, 7]} ; Butler, Robert E. ^[26] ; Butner, Melissa ^[27] ; Campillay, Abdo ^[28] ; Clever, Karoli E. ^[2] ; Conselice, Christopher J. ^[29] ; Cooke, Jeff ^{[30, 31]} ; Dage, Kristen C. ^{[32, 33, 34]} ; de Carvalho, Reinaldo R. ^[35] ; de Jaeger, Thomas ^{[36, 11]} ; Desai, Shantanu ^[37] ; Garcia, Alyssa ^[38] ; Garcia-Bellido, Juan ^[39] ; Gill, Mandeep S. S. ^[40] ; Girish, Nachiket ^[11] ; Hallakoun, Na'ama ^{[3, 41]} ; Herner, Kenneth ^[19] ; Hiramatsu, Daichi ^{[6, 7]} ; Holz, Daniel E. ^{[42, 43]} ; Huber, Grace ^[18] ; Kawash, Adam M. ^[34] ; McCully, Curtis ^{[6, 7]} ; Medallon, Sophia A. ^[2] ; Metzger, Brian D. ^{[44, 45]} ; Modak, Shaunak ^[11] ; Morgan, Robert ^[46] ; Munoz, Ricardo R. ^[20] ; Munoz-Elgueta, Nahir ^[47] ; Murakami, Yukei S. ^[11] ; Felipe Olivares, E. ^[48] ; Palmese, Antonella ^[19] ; Patra, Kishore C. ^[11] ; Pereira, Maria E. S. ^[38] ; Pessi, Thallis L. ^{[49, 50]} ; Pineda-Garcia, J. ^[51] ; Quirola-Vasquez, Jonathan ^{[52, 53]} ; Ramirez-Ruiz, Enrico ^[2] ; Rembold, Sandro Barboza ^[49] ; Rest, Armin ^{[54, 55]} ; Rodriguez, Osmar ^[3] ; Santana-Silva, Luidhy ^[35] ; Sherman, Nora F. ^[38] ; Siebert, Matthew R. ^[2] ; Smith, Carli ^[2] ; Smith, J. Allyn ^[56] ; Soares-Santos, Marcelle ^[38] ; Stacey, Holland ^[18] ; Stahl, Benjamin E. ^[11] ; Strader, Jay ^[34] ; Strasburger, Erika ^[11] ; Sunseri, James ^[11] ; Tinyanont, Samaporn ^[2] ; Tucker, Brad E. ^{[57, 58, 59]} ; Ulloa, Natalie ^[28] ; Valenti, Stefano ^[24] ; Vasylyev, Sergiy S. ^[11] ; Wiesner, Matthew P. ^[60] ; Zhang, Keto D. ^[11]

Afiliação do(s) autor(es):Mostrar menos -

^[1] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys, Evanston, IL 60208 - USA

^[2] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 - USA

^[3] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv - Israel

^[4] CIFAR, CIFAR Azrieli Global Scholars Program, Toronto, ON - Canada

^[5] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 - USA

^[6] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 - USA

^[7] Las Cumbres Observ, 6740 Cortona Dr, Suite 102, Goleta, CA 93117 - USA

^[8] Univ Calif Berkeley, Theoret Astrophys Ctr, Berkeley, CA 94720 - USA

^[9] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 - USA

^[10] Lawrence Berkeley Natl Lab, Nucl Sci Div, Berkeley, CA 94720 - USA

^[11] Filippenko, Alexei, V, Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 - USA

^[12] Consejo Nacl Invest Cient & Tecn, RA-1650 Buenos Aires, DF - Argentina

^[13] Ctr Brasileiro Pesquisas Fis, Rua Dr Xavier Sigaud 150, BR-22290180 Rio De Janeiro, RJ - Brazil

^[14] ECyT UNSAM, Int Ctr Adv Studies, RA-1650 Buenos Aires, DF - Argentina

^[15] ECyT UNSAM, Inst Ciencias Fis, RA-1650 Buenos Aires, DF - Argentina

^[16] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 - USA

^[17] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 - USA

^[18] Thacher Sch, Thacher Observ, 5025 Thacher Rd, Ojai, CA 93023 - USA

^[19] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 - USA

^[20] Univ Chile, Dept Astron, Camino El Observ 1515, Santiago - Chile

^[21] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 - USA

^[22] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, MS 50B-4206, Berkeley, CA 94720 - USA

^[23] Ctr Fed Educ Tecnol Celso Suckow da Fonseca, Rodovia Mario Covas, Lote J2, Quadra J, BR-23810000 Itaguai, RJ - Brazil

^[24] Univ Calif Davis, Dept Phys & Astron, Davis, CA 95616 - USA

^[25] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 - USA

^[26] Indiana Univ, Dept Astron, 727 E Third St, Bloomington, IN 47405 - USA

^[27] East Tennessee State Univ, Dept Phys & Astron, Johnson City, TN 37614 - USA

^[28] Las Campanas Observ, Carnegie Observ, Casilla 601, La Serena - Chile

^[29] Univ Manchester, Jodrell Bank, Ctr Astrophys, Oxford Rd, Manchester, Lancs - England

^[30] Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, H29, Hawthorn, Vic 3122 - Australia

^[31] Swinburne Univ Technol, Australian Res Council Ctr Excellence Gravitat Wa, Hawthorn, Vic 3122 - Australia

^[32] McGill Univ, Dept Phys, 3600 Univ St, Montreal, PQ H3A 2T8 - Canada

^[33] McGill Univ, McGill Space Inst, 3550 Univ St, Montreal, PQ H3A 2A7 - Canada

^[34] Michigan State Univ, Ctr Data Intens & Time Domain Astron, Dept Phys & Astron, E Lansing, MI 48824 - USA

^[35] Univ Cidade Sao Paul, NAT Univ Cruzeiro do Sul, Rua Galvao Bueno 868, BR-01506000 Sao Paulo, SP - Brazil

^[36] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 - USA

^[37] Indian Inst Technol, Kandi 502285, Telangana - India

^[38] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 - USA

^[39] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid - Spain

^[40] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 - USA

^[41] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot - Israel

^[42] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 - USA

^[43] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 - USA

^[44] Columbia Univ, Columbia Astrophys Lab, 538 W 120th St, New York, NY 10027 - USA

^[45] Flatiron Inst, Ctr Computat Astrophys, 162 W 5th Ave, New York, NY 10011 - USA

^[46] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 - USA

^[47] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching - Germany

^[48] Univ Atacama, Inst Astron & Ciencias Planetarias, Copayapu 485, Copiapo - Chile

^[49] Univ Fed Santa Maria, Ctr Ciencias Nat & Exatas, Dept Fis, BR-97105900 Santa Maria, RS - Brazil

^[50] Univ Diego Portales, Nucleo Astron, Av Ejercito 441, Santiago - Chile

^[51] Univ Andres Bello, Dept Ciencias Fis, Avda Republ 252, Santiago - Chile

^[52] Pontificia Univ Catolica Chile, Inst Astrofis, Casilla 306, Santiago 22 - Chile

^[53] Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100, Santiago - Chile

^[54] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 - USA

^[55] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 - USA

^[56] Austin Peay State Univ, Dept Phys Engn & Astron, POB 4608, Clarksville, TN 37044 - USA

^[57] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Canberra, ACT - Australia

^[58] Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Canberra, ACT 2601 - Australia

^[59] Australian Natl Univ, Natl Ctr Publ Awareness Sci, Canberra, ACT 2611 - Australia

^[60] Benedictine Univ, Dept Phys, 5700 Coll Rd, Lisle, IL 60532 - USA

• Tipo de documento: Artigo Científico
• Fonte: ASTROPHYSICAL JOURNAL; v. 923, n. 2 DEC 2021.
• Citações Web of Science: 0

Resumo

We present optical follow-up imaging obtained with the Katzman Automatic Imaging Telescope, Las Cumbres Observatory Global Telescope Network, Nickel Telescope, Swope Telescope, and Thacher Telescope of the LIGO/Virgo gravitational wave (GW) signal from the neutron star-black hole (NSBH) merger GW190814. We searched the GW190814 localization region (19 deg(2) for the 90th percentile best localization), covering a total of 51 deg(2) and 94.6% of the two-dimensional localization region. Analyzing the properties of 189 transients that we consider as candidate counterparts to the NSBH merger, including their localizations, discovery times from merger, optical spectra, likely host galaxy redshifts, and photometric evolution, we conclude that none of these objects are likely to be associated with GW190814. Based on this finding, we consider the likely optical properties of an electromagnetic counterpart to GW190814, including possible kilonovae and short gamma-ray burst afterglows. Using the joint limits from our follow-up imaging, we conclude that a counterpart with an r-band decline rate of 0.68 mag day(-1), similar to the kilonova AT 2017gfo, could peak at an absolute magnitude of at most -17.8 mag (50% confidence). Our data are not constraining for ``red{''} kilonovae and rule out ``blue{''} kilonovae with M > 0.5 M (circle dot) (30% confidence). We strongly rule out all known types of short gamma-ray burst afterglows with viewing angles <17 degrees assuming an initial jet opening angle of similar to 5.degrees 2 and explosion energies and circumburst densities similar to afterglows explored in the literature. Finally, we explore the possibility that GW190814 merged in the disk of an active galactic nucleus, of which we find four in the localization region, but we do not find any candidate counterparts among these sources. (AU)

• Processo FAPESP: 20/03301-5 - Determinando as propriedades de galáxias hospedeiras de ondas gravitacionais
• Beneficiário: Luidhy Santana da Silva
• Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado
• Processo FAPESP: 14/11156-4 - O que determina o crescimento da massa estelar de galáxias elípticas? Intrínseco ou ambiente: a saga contínua
• Beneficiário: Reinaldo Ramos de Carvalho
• Modalidade de apoio: Auxílio à Pesquisa - Temático