TITLE: GCN CIRCULAR NUMBER: 35933 SUBJECT: AT2024eju: followup observations with Liverpool Telescope suggest a fading transient DATE: 24/03/17 00:38:27 GMT FROM: S. Srivastav at Oxford <shubhamsrivastav@gmail.com> S. Srivastav, S. J. Smartt (Oxford), M. D. Fulton and K. W. Smith (QUB) report on behalf of a larger collaboration: We 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. The transient was not detected in any of the 3 bands with the following upper limits: MJD Filter Limit (AB mag) 60385.848 g >19.55 60385.851 r >19.72 60385.853 i >20.02 This suggests that AT2024eju has likely faded since the ATLAS detection ~1 day ago, further follow-up observations are encouraged. View this GCN Circular online at https://gcn.nasa.gov/circulars/35933. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...