DRAFT
2024-12-25 01:43:21
Type: Object/s-Data/Analysis
ZTF and Gemini Observations of the Fast-fading Luminous Optical Transient AT2024aehp
Authors: Jason Sevilla, Anna Y. Q. Ho (Cornell), Gokul Srinivasaragavan (UMD)
Source Group: ZTF
Abstract:
We report ZTF observations of a rapidly fading transient, AT2024aehp (ZTF24abygbss). The spectroscopic redshift of the host galaxy is z = 0.170, implying a peak absolute magnitude of M_g ~ -20.5 AB mag.

At UTC 2024-04-21 08:37:22, ZTF detected a new transient candidate (ZTF24abybgss) 0.1” offset from a possible host galaxy in SDSS and Legacy Survey.

 

ZTF24abygbss was discovered at a position (J2000) of:

RA = 08:21:07.47

Dec = +28:44:22.20

 

The transient’s peak magnitude was g = 19.1 +/- 0.1 mag, and exhibited blue colors (g - r = -0.3 mag, corrected for Milky Way extinction [1]). The transient was reported to the Transient Name Server by the Automatic Learning for the Rapid Classification of Events (ALeRCE) broker as AT2024aehp [2]. ZTF photometry observed a fade rate of 0.2 mag/day over the next five days. 

 

The fast fading and possible high peak luminosity from the photometric redshift of the host galaxy (SDSS z_ph = 0.17 ± 0.09, implying M < -20 mag) motivated us to trigger follow-up observations. We acquired spectroscopy of the candidate using GMOS-S at Gemini Observatory on 2024-12-23, under the target-of-opportunity program GS-2024B-Q-121 (PI Ho). The spectrum shows galactic Hɑ, [N II], and [S II] emission lines that correspond to a redshift of z=0.170 and implies a peak absolute magnitude of M_g = -20.5 AB mag for the transient.

 

As the absolute magnitude, blue colors, and fast fading are consistent with an FBOT similar to AT2018cow, we encourage multiwavelength follow-up observations.

 

[1] Schlafly, E. F., & Finkbeiner, D. P. (2011), ApJ, 737, 103

[2] Munoz-Arancibia et al. (2024), TNS Discovery Report No. 2024-4959

 

We thank the Gemini Observatory staff for assistance in rapidly obtaining these observations.

 

Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Oskar Klein Center at Stockholm University, the University of Maryland, University of California, Berkeley , the University of Wisconsin at Milwaukee, University of Warwick, Ruhr University Bochum, Cornell University, Northwestern University and Drexel University. Operations are conducted by COO, IPAC, and UW.

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 2024aehp [ZTF24abygbss] 08:21:07.471 +28:44:22.30 SDSS J082107.46+284422.0 08:21:07.471 +28:44:22.30

Comments