DRAFT
2023-08-27 16:56:11
Type: Object/s-Data/Analysis
ZTF Observations of the Candidate Optical Afterglow AT 2023qxj
Authors: Maggie L. Li, Jada L. Vail, Anna Y. Q. Ho (Cornell University), Michael Coughlin (University of Minnesota), Daniel Perley (LJMU), Anirudh Salgundi, Vishwajeet Swain, Gaurav Waratkar (IITB)
Keywords: Optical
Abstract:
We report observations of a fast-evolving red transient. AT 2023qxj is a likely optical afterglow with a GRB counterpart discovered by Fermi.

We report the discovery of a fast-evolving red transient by the Zwicky Transient Facility (ZTF). The transient has a coincident Fermi GRB counterpart [1].

AT 2023qxj (ZTF23abaanxz) was discovered at the position (J2000) of:

RA = 19:58:33.55 (299.6397739 deg)

Dec = +54:27:48.02 (54.4633396 deg)

on 2023-08-27 07:10:10.94 UT by ZTF at r = 17.11 +/- 0.04 mag (MJD=60183.26872). ZTF obtained a non-detection 1 day prior (MJD=60182.26553) at r > 20.18 mag, indicating a fast rise rate of >3 mag/day in r. ZTF also obtained detections later that night at r = 18.88 +/- 0.08 mag (MJD=60183.33919) and g = 19.27 +/- 0.16 mag (MJD=60183.40719), implying that the transient was red and fading quickly.

The Galactic latitude of AT 2023qxj is 12.8 degrees, and the Galactic reddening toward the direction of AT 2023qxj is: E_(g-r) = 0.227 from Schlafly & Finkbeiner (2011).

The fast rise, fast decay, red color, and lack of archival optical counterpart of AT 2023qxj make it a strong candidate afterglow. We identify the coincident GRB 230827256 discovered by Fermi at the position (J2000) of:

RA = 19:57:16.8 

Dec = +56:28:12

with an error radius of 2.17 deg. The time of the GRB trigger was 2023-08-27 06:08:31 UT (MJD=60183.25591), 18.45 minutes prior to the first ZTF detection of AT 2023qxj.

ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, and IN2P3, France. Operations are conducted by COO, IPAC, and UW.

[1] https://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3hdprods.pl?files=P&Tar…

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 2023qxj 19:58:33.546 +54:27:48.02 Afterglow 19:58:33.546 +54:27:48.02

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