{
  "createdOn": 1710635907067,
  "submittedHow": "web",
  "submitter": "S. Srivastav at Oxford <shubhamsrivastav@gmail.com>",
  "bibcode": "2024GCN.35933....1S",
  "body": "S. Srivastav, S. J. Smartt (Oxford), M. D. Fulton and K. W. Smith (QUB) report on behalf of a larger collaboration:\n\nWe report follow-up photometry of AT2024eju, the possible optical counterpart (Srivastav et al., GCN 35932) of the fast X-ray transient EP240315a (Zhang et al., GCN 35931). The images were obtained with the 2m Liverpool Telescope in g, r and i bands starting on MJD 60385.848, 1.01 days following the discovery of the X-ray transient.\n\nThe transient was not detected in any of the 3 bands with the following upper limits:\n\nMJD\tFilter\tLimit (AB mag)\n60385.848\tg\t>19.55\n60385.851\tr\t>19.72\n60385.853\ti\t>20.02\n\nThis suggests that AT2024eju has likely faded since the ATLAS detection ~1 day ago, further follow-up observations are encouraged.\n",
  "subject": "AT2024eju: followup observations with Liverpool Telescope suggest a fading transient",
  "circularId": 35933
}