Radio and X-ray observations of the luminous Fast Blue Optical Transient AT2020xnd
arXiv:2110.05514 · doi:10.3847/1538-4357/ac4506
Abstract
We present deep X-ray and radio observations of the Fast Blue Optical Transient (FBOT) AT2020xnd/ZTF20acigmel at from d to d after explosion. AT2020xnd belongs to the category of optically luminous FBOTs with similarities to the archetypal event AT2018cow. AT2020xnd shows luminous radio emission reaching ergsHz at 20GHz and d post explosion, accompanied by luminous and rapidly fading soft X-ray emission peaking at ergs. Interpreting the radio emission in the context of synchrotron radiation from the explosion's shock interaction with the environment we find that AT2020xnd launched a high-velocity outflow (0.1-0.2) propagating into a dense circumstellar medium (effective yr for an assumed wind velocity of kms). Similar to AT2018cow, the detected X-ray emission is in excess compared to the extrapolated synchrotron spectrum and constitutes a different emission component, possibly powered by accretion onto a newly formed black hole or neutron star. These properties make AT2020xnd a high-redshift analog to AT2018cow, and establish AT2020xnd as the fourth member of the class of optically-luminous FBOTs with luminous multi-wavelength counterparts.
21 pages, 6 figures, 6 tables. Submitted to ApJ
References in corpus (20)
- X-ray Properties of Black-Hole Binaries
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- WSClean: an implementation of a fast, generic wide-field imager for radio astronomy
- The Zwicky Transient Facility: Science Objectives
- The 1% Concordance Hubble Constant
- Rapidly-Evolving and Luminous Transients from Pan-STARRS1
- Circumstellar Emission from Type Ib and Ic Supernovae
- An optimized algorithm for multi-scale wideband deconvolution of radio astronomical images
- The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics
- Radio interferometric gain calibration as a complex optimization problem
- Radio Properties of Tidal Disruption Events
- Non-linear Kalman filters for calibration in radio interferometry
- An extremely powerful long-lived superluminal ejection from the black hole MAXI J1820+070
- The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at
- A mildly relativistic outflow from the energetic, fast-rising blue optical transient CSS161010 in a dwarf galaxy
- A Luminous, Fast Rising UV-Transient Discovered by ROTSE: a Tidal Disruption Event?
- Gamma-ray Thermalization and Leakage from Millisecond Magnetar Nebulae: Towards a Self-Consistent Model for Superluminous Supernovae
- uGMRT observations of a Fast and Blue Optical Transient -- AT 2018cow
- Rapidly Evolving Transients from the Hyper Suprime-Cam SSP Transient Survey
- A detailed radio study of the energetic, nearby and puzzling GRB 171010A
Cited by in corpus (31)
- A Search for Extragalactic Fast Blue Optical Transients in ZTF and the Rate of AT2018cow-like Transients
- Science objectives of the Einstein Probe mission
- Luminous Millimeter, Radio, and X-ray Emission from ZTF20acigmel (AT2020xnd)
- Shocked jets in CCSNe can power the zoo of fast blue optical transients
- A common envelope jets supernova (CEJSN) impostor scenario for fast blue optical transients
- The population of tidal disruption events discovered with eROSITA
- A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
- Minutes-duration Optical Flares with Supernova Luminosities
- An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
- Dust Echoes from Luminous Fast Blue Optical Transients
- Synchrotron Afterglow Model for AT 2022cmc: Jetted Tidal Disruption Event or Engine-Powered Supernova?
- Late-time Hubble Space Telescope Observations of AT 2018cow. II. Evolution of a UV bright Underlying Source 2--4 Yr Post-discovery
- A flash of polarized optical light points to an aspherical "cow"
- Particle Acceleration in Mildly Relativistic Outflows of Fast Energetic Transient Sources
- On the nature of Fast Blue Optical Transients
- O'TRAIN: a robust and flexible Real/Bogus classifier for the study of the optical transient sky
- Neutrino Emission from Luminous Fast Blue Optical Transients
- Multi-wavelength observations of the Luminous Fast Blue Optical Transient AT2023fhn
- The Luminosity Phase Space of Galactic and Extragalactic X-ray Transients Out to Intermediate Redshifts
- Late-time Hubble Space Telescope Observations of AT 2018cow. I. Further Constraints on the Fading Prompt Emission and Thermal Properties 50--60 Days Post-discovery
- A Population Study on the Radio Emission of Fast Blue Optical Transients
- Prospects for Time-Domain and Multi-Messenger Science with eXTP
- The soft X-ray transient EP241021a: A cosmic explosion with a complex off-axis jet and cocoon from a massive progenitor
- Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
- Searching for Radio Transients with Inverted Spectra in Epoch 1 of VLASS and VCSS, and Identification of a Sample of Candidate Relativistic Nuclear Transients
- The Emission and Suppression of Line Features in Luminous Transients
- Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium CoreBlack Hole Mergers Following Delayed Dynamical Instability
- The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
- Light-curve Modelling for The Initial Rising Phase of Rapidly-evolving Transients Powered by Continuous Outflow
- AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission
- Luminous Fast Blue Optical Transients and Type Ibn/Icn SNe from Wolf-Rayet/Black Hole Mergers