DRAFT
2021-08-18 13:15:03
Type: Object/s-Data/Analysis
Pan-STARRS follow-up of AT2021qvw: A rapidly evolving LBV outburst turning into an SN like event.
Authors: M. Fulton, S. J. Smartt, K. W. Smith (QUB), K. C. Chambers, M. Huber (IfA, Hawaii), S. Srivastav, D. R. Young, J. Gillanders, S. Sim (QUB), T. de Boer, J. Bulger, J. Fairlamb, C.-C. Lin, T. Lowe, E. Magnier, A. Schultz, R. J. Wainscoat, M. Willman (IfA), T.-W. Chen (Stockholm), D. E. Wright (University of Minnesota), C. Stubbs (Harvard), A. Rest (STScI)
Source Group: Pan-STARRS
Abstract:
We report the Pan-STARRS follow-up of the intrinsically faint transient AT2021qvw as an LBV-turning-supernova like event in the host galaxy CGCG 454-019, at a redshift of z = 0.025, or d = 111 Mpc (from NED). The transient initially faded quickly over a period of 10 days (to r~23), but has now brightened to r=19.4. This transient resembles a 2009ip-like explosion in its early phases; therefore, spectroscopic classification is strongly encouraged.

We are carrying out the "Pan-STARRS Search for Kilonovae", which is a focused search for intrinsically faint transients, or rapidly evolving transients in galaxies that are closer than 200 Mpc in the ongoing Pan-STARRS Near-Earth Object surveys (see Smartt et al. AstroNote 2019-48 for details). In normal survey mode, Pan-STARRS1 and Pan-STARRS2 telescopes take 4 x 45s exposures in w, i or z each night, reaching 5 sigma magnitudes of w<22, i<21 and z<20.5 in each frame (see Chambers et al. 2016, 1612.05560). The w-band filter is a broad g+r+i composite. 

We report the Pan-STARRS follow-up of the intrinsically faint transient AT2021qvw (Fulton et al. AstroNote 2021-179), which indicates that it may be an LBV eruption that is turning into a supernova like event in the host galaxy CGCG 454-019, at a redshift of z = 0.025, or d = 111 Mpc (from NED).

The transient was discovered on MJD 59386.55 (2021-06-21, 13:14:16 UT) at mag m_w = 21.40 +/- 0.16 (see Fulton et al. AstroNote 2021-179 for further details) and followed extensively over ten days. Decline rates of 0.32 +/- 0.07 mag/day, 0.15 +/- 0.03 mag/day, 0.17 +/- 0.04 mag/day and 0.13 +/- 0.04 mag/day were measured in the PS1 w, r, i and z bands respectively.

We revisited the transient's location on MJD 59437.41 (2021-08-11, 9:53:16 UTC), observing the transient had rebrightened. On MJD 59443.46 (2021-08-17, 11:01:38 UTC) we measured magnitudes of g = 19.59 +/- 0.04, r = 19.35 +/- 0.03 and i = 19.38 +/- 0.03, implying incline rates of >0.5 mag per day in each filter over three days. This transient may be a luminous LBV eruption, which rapidly declined and then undergone a supernova like explosion, similar to the events in SN2009ip (e.g. Mauerhan et al. 2013 MNRAS, 430, 18;  Pastorello et al. 2013, ApJ 767, 1). Spectroscopic classification and follow-up are strongly encouraged.

Operation of the Pan-STARRS1 and Pan-STARRS2 telescopes is primarily supported by the National Aeronautics and Space Administration under Grant No. NNX12AR65G and Grant No. NNX14AM74G issued through the SSO Near-Earth Object (NEO) Observations Program. The discoveries from the "Pan-STARRS Search for Kilonovae" program are a byproduct of the Pan-STARRS NEO survey observations. Data are processed at Queen's University Belfast enabled through the STFC grants ST/P000312/1 and ST/T000198/1. 

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2021qvw [PS21gqd] 23:16:38.285 +15:53:39.97 CGCG 454-019 0.025364 23:16:38.286 +15:53:40.01 SN II 0.025364

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