Detection of an outburst one year prior to the explosion of SN 2011ht
arXiv:1309.4695 · doi:10.1088/2041-8205/779/1/L8
Abstract
Using imaging from the Pan-STARRS1 survey, we identify a precursor outburst at epochs 287 and 170 days prior to the reported explosion of the purported Type IIn supernova (SN) 2011ht. In the Pan-STARRS data, a source coincident with SN 2011ht is detected exclusively in the \zps\ and \yps-bands. An absolute magnitude of M-11.8 suggests that this was an outburst of the progenitor star. Unfiltered, archival Catalina Real Time Transient survey images also reveal a coincident source from at least 258 to 138 days before the main event. We suggest that the outburst is likely to be an intrinsically red eruption, although we cannot conclusively exclude a series of erratic outbursts which were observed only in the redder bands by chance. This is only the fourth detection of an outburst prior to a claimed SN, and lends credence to the possibility that many more interacting transients have pre-explosion outbursts, which have been missed by current surveys.
Revised version following referee report
References in corpus (8)
- A giant outburst two years before the core-collapse of a massive star
- SN 2006jc: A Wolf-Rayet Star Exploding in a Dense He-Rich Circumstellar Medium
- A panchromatic view of the restless SN2009ip reveals the explosive ejection of a massive star envelope
- Luminous Blue Variables as the progenitors of supernovae with quasi-periodic radio modulations
- SN 2009ip and SN 2010mc: Core-collapse Type IIn supernovae arising from blue supergiants
- SN 1994W: An Interacting Supernova or Two Interacting Shells?
- SN 2005 gj: Evidence for LBV supernovae progenitors?
- SN 2009kn - the twin of the Type IIn supernova 1994W
Cited by in corpus (71)
- Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
- The Zwicky Transient Facility: Science Objectives
- Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
- Precursors prior to Type IIn supernova explosions are common: precursor rates, properties, and correlations
- Ejection of the massive Hydrogen-rich envelope timed with the collapse of the stripped SN2014C
- Interacting Supernovae: Types IIn and Ibn
- PTF11iqb: Cool supergiant mass loss that bridges the gap between Type IIn and normal supernovae
- Luminous Red Novae: Stellar Mergers or Giant Eruptions?
- Bright, months-long stellar outbursts announce the explosion of interaction-powered supernovae
- Super-Eddington Stellar Winds Driven by Near-Surface Energy Deposition
- Mass-loss histories of Type IIn supernova progenitors within decades before their explosion
- Towards a Realistic Explosion Landscape for Binary Population Synthesis
- Shock breakout theory
- Multi-epoch spectropolarimetry of SN 2009ip: direct evidence for aspherical circumstellar material
- Type IIn supernova light-curve properties measured from an untargeted survey sample
- The supernova CSS121015:004244+132827: a clue for understanding super-luminous supernovae
- Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)
- Electron-capture supernovae exploding within their progenitor wind
- Interaction-powered supernovae: Rise-time vs. peak-luminosity correlation and the shock-breakout velocity
- Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle
- Diversity of GRB energetics vs. SN homogeneity: supernova 2013cq associated with the gamma-ray burst 130427A
- SN 2015bh: NGC 2770's 4th supernova or a luminous blue variable on its way to a Wolf-Rayet star?
- Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational wave source GW150914
- Interacting supernovae and supernova impostors. LSQ13zm: an outburst heralds the death of a massive star
- The bumpy light curve of supernova iPTF13z
- SN 2009ip at late times - an interacting transient at +2 years
- Supernova Impostors and other Gap Transients
- Supernova Progenitors, Their Variability, and the Type IIP Supernova ASASSN-16fq in M66
- Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions
- Evidence for past interaction with an asymmetric circumstellar shell in the young SNR Cassiopeia A
- The Physics of Flash (Supernova) Spectroscopy
- SN Hunt 248: a super-Eddington outburst from a massive cool hypergiant
- The Nearby Type Ibn Supernova 2015G: Signatures of Asymmetry and Progenitor Constraints
- Massive stars exploding in a He-rich circumstellar medium. VI. Observations of two distant Type Ibn supernova candidates discovered by La Silla-QUEST
- PTF 13efv - An outburst 500 days prior to the SNHunt 275 explosion and its radiative efficiency
- Super-Eddington stellar winds: unifying radiative-enthalpy vs. flux-driven models
- Constraints on Type IIn Supernova Progenitor Outbursts from the Lick Observatory Supernova Search
- SN 2018bsz: a Type I superluminous supernova with aspherical circumstellar material
- Mass loss of massive stars near the Eddington luminosity by core neutrino emission shortly before their explosion
- Search for precursor eruptions among Type IIb supernovae
- SN 2012aa - a transient between Type Ibc core-collapse and superluminous supernovae
- Interacting supernovae and supernova impostors. SN 2007sv: the major eruption of a massive star in UGC 5979
- Circumstellar and explosion properties of Type Ibn supernovae
- The Candidate Progenitor of the Type IIn SN 2010jl is Not an Optically Luminous Star
- Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)
- Massive stars exploding in a He-rich circumstellar medium - VIII. PSN J07285387+3349106, a highly reddened supernova Ibn
- Supernova PTF12glz: a possible shock breakout driven through an aspherical wind
- Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae
- SN 2020bqj: a Type Ibn supernova with a long lasting peak plateau
- PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
- Radiative Acceleration of Dense Circumstellar Material in Interacting Supernovae
- Radio Analysis of SN 2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse
- On the Progenitor of the Type Ic Supernova 2012fh
- A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf
- Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova
- SN 2015as: A low luminosity Type IIb supernova without an early light curve peak
- Core-collapse supernovae in dense environments -- particle acceleration and non-thermal emission
- Searching for precursor activity of Type IIn Supernovae
- Comparison between the first and second mass eruptions from progenitors of Type IIn supernovae
- Inferring CSM Properties of Type II SNe Using a Magnitude-Limited ZTF Sample
- A survey of eight hot Jupiters in secondary eclipse using WIRCam at CFHT
- Early light curves of Type II supernovae interacting with a circumstellar disk
- The Carnegie Supernova Project II. Observations of SN 2014ab possibly revealing a 2010jl-like SN IIn with pre-existing dust
- SN 2020pvb: a Type IIn-P supernova with a precursor outburst
- Hydrodynamic Modelling of Early Peaks in Type Ibc Supernovae with Circumstellar Interaction
- Modeling the light curve of Type IIn-P SN 2005cl with red supergiant progenitors featuring pre-SN ourbursts
- A six year image-subtraction light curve of SN 2010jl
- Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter
- Hubble Space Telescope Imaging Reveals That SN 2015bh Is Much Fainter than Its Progenitor
- Radiation-Driven Stellar Eruptions
- Finding Fast Transients in Real Time Using Novel Light Curve Analysis Algorithm