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Title: A Mid-IR Selected Changing-look Quasar and Physical Scenarios for Abrupt AGN Fading

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1];  [2]; ORCiD logo [3];  [2];  [4]; ORCiD logo [5]; ORCiD logo [6];  [7];  [3]; ORCiD logo [8];  [3]; ORCiD logo [3];  [1];  [9]
  1. California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
  2. Borough of Manhattan Community College, New York, NY (United States). Dept. of Science; American Museum of Natural History (AMNH), New York, NY (United States); City Univ. (CUNY), NY (United States)
  3. California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Cahill Center for Astronomy and Astrophysics
  4. Univ. of Edinburgh, Scotland (United Kingdom). Inst. for Astronomy
  5. Berkeley Center or Cosmological Physics, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  6. Núcleo de Astronomía de la Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Santiago (Chile)
  7. California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Cahill Center for Astronomy and Astrophysics; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  8. National Optical Astronomy Observatory (NOAO), Tuscon, AZ (United States) and La Serena (Chile)
  9. Korea Inst. for Advanced Study, Seoul (Republic of Korea). School of Physics

We report a new changing-look quasar, WISE J105203.55+151929.5 at $$z$$ = 0.303, found by identifying highly mid-IR-variable quasars in the Wide-field Infrared Survey Explorer (WISE)/Near-Earth Object WISE Reactivation (NEOWISE) data stream. Compared to multiepoch mid-IR photometry of a large sample of SDSS-confirmed quasars, WISE J1052+1519 is an extreme photometric outlier, fading by more than a factor of two at 3.4 and 4.6 $$μ$$m since 2009. Swift target-of-opportunity observations in 2017 show even stronger fading in the soft X-rays compared to the ROSAT detection of this source in 1995, with at least a factor of 15 decrease. We obtained second-epoch spectroscopy with the Palomar telescope in 2017 that, when compared with the 2006 archival SDSS spectrum, reveals that the broad H$$β$$ emission has vanished and that the quasar has become significantly redder. The two most likely interpretations for this dramatic change are source fading or obscuration, where the latter is strongly disfavored by the mid-IR data. We discuss various physical scenarios that could cause such changes in the quasar luminosity over this timescale, and favor changes in the innermost regions of the accretion disk that occur on the thermal and heating/cooling front timescales. We discuss possible physical triggers that could cause these changes, and predict the multiwavelength signatures that could distinguish these physical scenarios.

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Organization:
USDOE
OSTI ID:
1544065
Journal Information:
The Astrophysical Journal (Online), Vol. 864, Issue 1; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 79 works
Citation information provided by
Web of Science

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NuSTAR and XMM-Newton observations of NGC 1365: Extreme absorption variability and a constant inner accretion disk text January 2014
First Results from the Catalina Real-time Transient Survey text January 2008
The thermal-viscous disk instability model in the AGN context text January 2009
Turbulent Stresses in Local Simulations of Radiation-Dominated Accretion Disks, and the Possibility of the LIghtman-Eardley Instability text January 2009
Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux text January 2009
The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance text January 2010
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A Global Three Dimensional Radiation Magneto-hydrodynamic Simulation of Super-Eddington Accretion Disks text January 2014
WISE photometry for 400 million SDSS sources text January 2014
A possible close supermassive black-hole binary in a quasar with optical periodicity text January 2015
The Multi-Layer Variable Absorbers in NGC 1365 Revealed by XMM-Newton and NuSTAR text January 2015
A systematic search for close supermassive black hole binaries in the Catalina Real-Time Transient Survey text January 2015
Towards an Understanding of Changing-Look Quasars: An Archival Spectroscopic Search in SDSS text January 2015
Migration Traps in Disks Around Supermassive Black Holes text January 2015
Infrared Time Lags for the Periodic Quasar PG 1302-102 preprint January 2015
IC 751: a new changing-look AGN discovered by NuSTAR text January 2016
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The Close AGN Reference Survey (CARS) - What is causing Mrk1018's return to the shadows after 30 years? text January 2016
iPTF16fnl: a faint and fast tidal disruption event in an E+A galaxy text January 2017
Cooling timescale of dust tori in dying active galactic nuclei text January 2017
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Correcting for the Effects of Interstellar Extinction text January 1998

Cited By (31)

A new class of flares from accreting supermassive black holes journal January 2019
Results of a systematic search for outburst events in 1.4 million galaxies journal October 2018
Rapid luminosity decline and subsequent reformation of the innermost dust distribution in the changing-look AGN Mrk 590 journal December 2019
The ‘Big Dipper’: the nature of the extreme variability of the AGN SDSS J2232−0806 journal February 2019
MUSE observations of a changing-look AGN – I. The reappearance of the broad emission lines journal March 2019
Extreme AGN variability: evidence of magnetically elevated accretion? journal November 2018
LIGO tells us LINERs are not optically thick RIAFs journal October 2019
A Luminous Transient Event in a Sample of WISE -selected Variable AGNs journal October 2018
Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 10 4 yr journal January 2019
Changing-look Quasar Candidates: First Results from Follow-up Spectroscopy of Highly Optically Variable Quasars journal March 2019
Rapid “Turn-on” of Type-1 AGN in a Quiescent Early-type Galaxy SDSS1115+0544 journal March 2019
Gemini Imaging of the Host Galaxies of Changing-look Quasars journal May 2019
1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months journal September 2019
A New Class of Changing-look LINERs journal September 2019
The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars journal September 2019
The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar journal October 2019
An Unusual Mid-infrared Flare in a Type 2 AGN: An Obscured Turning-on AGN or Tidal Disruption Event? journal November 2019
Two New “Turn-off” Changing-look Active Galactic Nuclei and Implication on “Partially Obscured” AGNs journal December 2019
Initial Results from a Systematic Search for Changing-look Active Galactic Nuclei Selected via Mid-infrared Variability journal January 2020
More unWISE Coadd Epochs from 2016 NEOWISE-reactivation Imaging journal October 2018
The Nearby “Changing Look” Seyfert NGC 1346 journal April 2019
On the origin of the dramatic spectral variability of WPVS 007 journal May 2019
A Luminous Transient Event in a Sample of WISE-Selected Variable AGN text January 2018
Changing-Look Quasar Candidates: First Results from Follow-up Spectroscopy of Highly Optically Variable Quasars text January 2018
Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within $10^4$ years text January 2018
The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-Look Quasars text January 2019
MUSE observations of a changing-look AGN I: The re-appearance of the broad emission lines text January 2019
Rapid Luminosity Decline and Subsequent Reformation of the Innermost Dust Distribution in the Changing-look AGN Mrk 590 text January 2019
Initial results from a systematic search for changing-look active galactic nuclei selected via mid-infrared variability text January 2019
On the Origin of the Dramatic Spectral Variability of WPVS 007 text January 2019
The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar text January 2019

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