AstroNote 2024-106

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DRAFT
2024-04-11 21:37:56
Type: Object/s-Data/Analysis
AT2024fkm: Updated g-band photometry with AST3 and GRANDMA
Authors: Tian-Rui Sun (Purple Mountain Observatory), P. Hello (IJCLAB), Xue-Feng Wu, Xiao-Yan Li (Nanjing Institute of Astronomical Observation Technology),Xiang-Yan Yuan, Lifan Wang (TAMU), Xiao-Feng Wang (Tsinghua University), M. Masek (FZU), S. Agayeva (ShAO), Y. Rajabov (UBAI), T. Bonzi (Berkeley), S. Antier (OCA), S. Karpov (FZU), T. Hussenot (IJCLAB), T. du Laz (Caltech), M. Coughlin (UMN)
Keywords: Supernova
Abstract:
We present follow-up photometry of AT2024fkm using AST3.

We observed AT2024fkm with AST3 (Antarctic Survey Telescope 3-3) at Yaoan Astronomy Observation Station (China, Yunnan) with 60 240 second exposures spanning 2024-04-07T15:07:27.731 to 2024-04-07T19:08:34.228 by AST3-3 in g-band.

The stacked image was analyzed by stdpipe (Karpov et al., 2020) using PS1 reference images. The depth is 22.1 magnitude in g-band and the flux of the transient on the top of the galaxy contribution is 20.13
+/- 0.03.

We extracted a g-ZTF stacked image from 2018-03-28, composed of 8x30s individual images in rsa.ipac.caltech.edu. The depth of the reference is 21.2 g-band. We measured a flux of the galaxy at the location of the transient of 21.16 +/- 0.20.

We finally measured the flux of the transient (without the galaxy contribution) of 20.66 +/- 0.14

The source faded > 0.5 mag in 3 days, according to the last ZTF public report.

Show current TNS values
CatalogNameReported RAReported DECReported Obj-TypeReported RedshiftHost NameHost RedshiftRemarksTNS RATNS DECTNS Obj-TypeTNS Redshift
TNS2024fkm13:53:08.582+35:43:14.2713:53:08.564+35:43:14.38SN IIb0.04113