{
  "circularId": 45157,
  "eventId": "IceCube-260712A",
  "submittedHow": "web",
  "subject": "IceCube-260712A: LAST optical follow-up observations of the IceCube neutrino candidate",
  "format": "text/plain",
  "body": "S. Garrappa (WIS), R. Konno (WIS), E. A. Zimmerman (WIS), A. Horowicz (WIS), E. O. Ofek (WIS), S. Ben-Ami (WIS), D. Polishook (WIS), O. Yaron (WIS), S. Fainer (WIS), A. Krassilchtchikov (WIS), Y. M. Shani (WIS), E. Segre (WIS), A. Gal-Yam (WIS), and S. Spitzer (WIS) on behalf of the LAST Collaboration.\n\nWe report observations of the IceCube Bronze neutrino candidate IC-260712A (GCN#45141) with the Large Array Survey Telescope (LAST, Ofek et al. 2023; Ben-Ami et al. 2023). We observed the field of IC-260712A using four telescopes (one unit), each with a FoV of 7.4 sq. deg and no filter (clear - similar to the GAIA Bp band) over several epochs. In each epoch, we stack  20 x 20 s images.\nWe began observations on 13 07 2026 at 18:54:08 UTC (T-T0 = 31.8 hours). The observations covered the full 90% neutrino footprint reported in GCN#45141 with a single LAST telescope. \n\nWe find no candidate transient optical counterpart in the automatic transient-detection pipeline (Konno et al. 2026). For each epoch, the average 5-sigma limiting magnitude in the neutrino footprint, is 20.1 (AB).\n\nLAST is a survey telescope array of the Weizmann Astrophysical Observatory (https://www.weizmann.ac.il/wao/).\n",
  "bibcode": "2026GCN.45157....1G",
  "createdOn": 1784041538449,
  "submitter": "Simone Garrappa at Weizmann Institute of Science <simone.garrappa@weizmann.ac.il>"
}