Swift/UVOT discovery of Swift J221951−484240: a UV luminous ambiguous nuclear transient
- Department of Physics, Lancaster University , Lancaster LA1 4YB , UK; School of Physics and Astronomy & Institute for Gravitational Wave Astronomy, University of Birmingham , Birmingham, B15 2TT , UK
- University College London, Mullard Space Science Laboratory , Holmbury St Mary, Dorking RH5 6NT , UK
- School of Physics and Astronomy & Institute for Gravitational Wave Astronomy, University of Birmingham , Birmingham, B15 2TT , UK; Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast , Belfast BT7 1NN , UK
- Astrophysics Science Division, NASA Goddard Space Flight Center , Greenbelt, MD 20771 , USA
- School of Physics and Astronomy & Institute for Gravitational Wave Astronomy, University of Birmingham , Birmingham, B15 2TT , UK
- Cerro Tololo Inter-American Observatory/NSFs NOIRLab , Casilla 603, La Serena , Chile; Las Campanas Observatory , Carnegie Observatories, Colina El Pino, Casilla 601, La Serena , Chile
- South African Astronomical Observatory , PO Box 9, Observatory 7935, Cape Town , South Africa; Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701 , South Africa; Department of Physics, University of the Free State , PO Box 339, Bloemfontein 9300 , South Africa
- Astrophysics Science Division, NASA Goddard Space Flight Center , Greenbelt, MD 20771 , USA; Joint Space-Science Institute, Computer and Space Sciences Building, University of Maryland , College Park, MD 20742 , USA
- University of Messina, MIFT Department , Polo Papardo, Viale F.S. D’Alcontres 31, I-98166 Messina , Italy
- Australia Telescope National Facility, CSIRO Space and Astronomy , PO Box 76, Epping, NSW 1710 , Australia
- Astronomical Observatory, University of Warsaw , Al. Ujazdowskie 4, PL-00-478 Warszawa , Poland
- Aryabhatta Research Institute of Observational Sciences (ARIES) , Manora Peak, Nainital-263002 , India; Department of Physics, Deen Dayal Upadhyaya Gorakhpur University , Gorakhpur-273009 , India
- Astrophysics Science Division, NASA Goddard Space Flight Center , Greenbelt, MD 20771 , USA; Center for Space Science and Technology, University of Maryland Baltimore County , 1000 Hilltop Circle, Baltimore, MD 21250 , USA; Center for Research and Exploration in Space Science and Technology, NASA/GSFC , Greenbelt, MD 20771 , USA
- Las Campanas Observatory , Carnegie Observatories, Colina El Pino, Casilla 601, La Serena , Chile
- Department of Astronomy, University of Wisconsin , 475 N. Charter Str, Madison, WI 53704 , USA; INAF-Osservatorio di Padova , vicolo dell Osservatorio 5, I-35122 Padova , Italy
- Aryabhatta Research Institute of Observational Sciences (ARIES) , Manora Peak, Nainital-263002 , India
- School of Physics and Astronomy, University of Leicester , Leicester LE1 7RH , UK
- Max-Planck-Institut für Extraterrestrische Physik , Giessenbachstraße 1, D-85748 Garching , Germany
- Department of Physics, University of Bath , Bath BA2 7AY , UK
- Australia Telescope National Facility, CSIRO Space and Astronomy , 1828 Yarrie Lake Road, Narrabri, NSW 2390 , Australia
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Mitchell Physics Building, Texas A&M University, Department of Physics and Astronomy , College Station, TX 77843 , USA
- Department of Astronomy and Astrophysics, The Pennsylvania State University , University Park, PA 16802 , USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802 , USA
- Department of Astronomy and Astrophysics, The Pennsylvania State University , University Park, PA 16802 , USA
- Department of Astronomy and Astrophysics, University of Toronto , Toronto, ON, M5S 3H4 , Canada
- INAF – IASF Palermo , Via Ugo La Malfa 153, I-90146 Palermo , Italy
- INAF – Osservatorio Astronomico di Brera , Via Bianchi 46, I-23807 Merate , Italy
- Dipartimento di Fisica e Astronomia, Universitá di Padova , 35122 Padova , Italy
- INAF–Osservatorio Astronomico di Roma , Via Frascati 33, I-00040 Monteporzio Catone , Italy; Space Science Data Center (SSDC) – Agenzia Spaziale Italiana (ASI) , I-00133 Roma , Italy
- Space Science Data Center (SSDC) – Agenzia Spaziale Italiana (ASI) , I-00133 Roma , Italy
- Department of Physics and Astronomy, Clemson University , Kinard Lab of Physics, Clemson, SC 29634-0978 , USA
- National Science Foundation , Alexandria, VA 22314 , USA
- Department of Astrophysics/IMAPP, Radboud University , NL-6525 AJ Nijmegen , the Netherlands; Cosmic Dawn Center (DAWN) , Denmark; Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200 Copenhagen N , Denmark
- INAF–Osservatorio Astronomico di Roma , Via Frascati 33, I-00040 Monteporzio Catone , Italy
- Los Alamos National Laboratory , B244, Los Alamos, NM 87545 , USA
- Space Science Data Center (SSDC) – Agenzia Spaziale Italiana (ASI) , I-00133 Roma , Italy; INAF–Osservatorio Astronomico di Roma , Via Frascati 33, I-00040 Monteporzio Catone , Italy
- Department of Physics and Mathematics, Aoyama Gakuin University , Sagamihara, Kanagawa, 252-5258 , Japan
- INAF – IASF Palermo , Via Ugo La Malfa 153, I-90146 Palermo , Italy; Department of Astronomy and Astrophysics, The Pennsylvania State University , University Park, PA 16802 , USA
- Department of Physics, University of Rome Tor Vergata , via della Ricerca Scientifica 1, I-00100 Rome , Italy; INAF, Via del Fosso del Cavaliere , 100, I-00133 Rome , Italy
- INAF, Via del Fosso del Cavaliere , 100, I-00133 Rome , Italy; Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101 , China
We report the discovery of Swift J221951−484240 (hereafter: J221951), a luminous slow-evolving blue transient that was detected by the Neil Gehrels Swift Observatory Ultraviolet/Optical Telescope (Swift/UVOT) during the follow-up of gravitational wave alert S190930t, to which it is unrelated. Swift/UVOT photometry shows the UV spectral energy distribution of the transient to be well modelled by a slowly shrinking blackbody with an approximately constant temperature of T ∼ 2.5 × 104 K. At a redshift z = 0.5205, J221951 had a peak absolute magnitude of Mu,AB = −23 mag, peak bolometric luminosity Lmax = 1.1 x 1045 ergs-1 and a total radiated energy of E > 2.6 × 1052 erg. The archival Wide-field Infrared Survey Explorer IR photometry shows a slow rise prior to a peak near the discovery date. Spectroscopic UV observations display broad absorption lines in N V and O VI, pointing towards an outflow at coronal temperatures. The lack of emission in the higher H α lines, N I and other neutral lines is consistent with a viewing angle close to the plane of the accretion or debris disc. The origin of J221951 cannot be determined with certainty but has properties consistent with a tidal disruption event and the turn-on of an active galactic nucleus.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); Scientific and Technological Research Council of Turkey (TÜBITAK); United Kingdom Space Agency; Italian Space Agency; Italian Ministry of Foreign Affairs and International Cooperation; European Union’s Horizon 2020; Danish National Research Foundation
- Contributing Organization:
- LIGO Scientific Collaboration; Virgo Scientific Collaboration
- Grant/Contract Number:
- 89233218CNA000001
- OSTI ID:
- 2340879
- Report Number(s):
- LA-UR--23-24498
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 530; ISSN 0035-8711
- Publisher:
- Oxford University PressCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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