Multi-Wavelength Analysis of AT 2023sva: a Luminous Orphan Afterglow With Evidence for a Structured Jet
Gokul P Srinivasaragavan, Daniel A Perley, Anna Y. Q Ho, Brendan O'Connor, Antonio de Ugarte Postigo, Nikhil Sarin, S. Bradley Cenko, Jesper Sollerman, Lauren Rhodes, David A Green, …
We present multi-wavelength analysis of ZTF23abelseb (AT 2023sva), an
optically discovered fast-fading ($\Delta m_r = 2.2$ mag in $\Delta t = 0.74 $
days), luminous ($M_r \sim -30.0$ mag) and red ($g-r = 0.50$ mag) transient at
$z = 2.28$ with accompanying luminous radio emission. AT 2023sva does not
possess a $\gamma$-ray burst (GRB) counterpart to an isotropic equivalent
energy limit of $E_{\rm{\gamma, \, iso}} < 1.6 \times 10^{52}$ erg, determined
through searching $\gamma$-ray satellite archives between the last
non-detection and first detection, making it the sixth example of an
optically-discovered afterglow with a redshift measurement and no detected GRB
counterpart. We analyze AT 2023sva's optical, radio, and X-ray observations to
characterize the source. From radio analyses, we find the clear presence of
strong interstellar scintillation (ISS) 72 days after the initial explosion,
allowing us to place constraints on the source's angular size and bulk Lorentz
factor. When comparing the source sizes derived from ISS of orphan events to
those of the classical GRB population, we find orphan events have statistically
smaller source sizes. We also utilize Bayesian techniques to model the
multi-wavelength afterglow. Within this framework, we find evidence that AT
2023sva possesses a shallow power-law structured jet viewed slightly off-axis
($\theta_{\rm{v}} = 0.07 \pm 0.02$) just outside of the jet's core opening
angle ($\theta_{\rm{c}} = 0.06 \pm 0.02$). We determine this is likely the
reason for the lack of a detected GRB counterpart, but also investigate other
scenarios. AT 2023sva's evidence for possessing a structured jet stresses the
importance of broadening orphan afterglow search strategies to a diverse range
of GRB jet angular energy profiles, to maximize the return of future optical
surveys.
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Title
Multi-Wavelength Analysis of AT 2023sva: a Luminous Orphan Afterglow With Evidence for a Structured Jet
Creators
Gokul P Srinivasaragavan
Daniel A Perley
Anna Y. Q Ho
Brendan O'Connor
Antonio de Ugarte Postigo
Nikhil Sarin
S. Bradley Cenko
Jesper Sollerman
Lauren Rhodes
David A Green
Dmitry S Svinkin
Varun Bhalerao
Gaurav Waratkar
A. J Nayana
Poonam Chandra
M. Coleman Miller
Daniele B Malesani
Geoffrey Ryan
Suryansh Srijan
Eric C Bellm
Eric Burns
David J Titterington
Maria B Stone
Josiah Purdum
Tomás Ahumada
G. C Anupama
Sudhanshu Barway
Michael W Coughlin
Andrew Drake
Rob Fender
José F. AgüÍ Fernández
Dmitry D Frederiks
Stefan Geier
Matthew J Graham
Mansi M Kasliwal
S. R Kulkarni
Harsh Kumar
Maggie L Li
Russ R Laher
Alexandra L Lysenko
Gopal Parwani
Richard A Perley
Anna V Ridnaia
Anirudh Salgundi
Roger Smith
Niharika Sravan
Vishwajeet Swain
Christina C Thöne
Anastasia E Tsvetkova
Mikhail V Ulanov
Jada Vail
Jacob L Wise
Avery Wold
Resource Type
Preprint
Language
English
Academic Unit
Physics
Other Identifier
991022016381704721
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