GCN Circular 28947
Subject
IceCube-201114A: DECam observations and candidate optical counterpart
Event
Date
2020-11-23T22:45:57Z (5 years ago)
From
Robert Morgan at U. of Wisconsin-Madison <robert.morgan@wisc.edu>
Robert Morgan (U of Wisconsin-Madison), Ken Herner (Fermilab), Alyssa Garcia (U of Michigan), Robert Gruendl (NCSA), Keith Bechtol (U of Wisconsin-Madison), Kathy Vivas (NOIRLab), Clara E. Mart�nez-V�zquez (NOIRLab), Claudio Aguilera (NOIRLab), Alex Drlica-Wagner (Fermilab), Julio Carballo-Bello (U de Tarapac�), Peter Ferguson (Texas A&M U), Alex Goater (U of Surrey), Jeff Cooke (Swinburne U), Timothy M. C. Abbott (NOIRLab)
We triggered the Dark Energy Camera (DECam) at Cerro Tololo Inter-American Observatory in Chile on the localization area of the GOLD neutrino event detected by IceCube (IceCube-201114A, GCN 28887). Observations took place on 2020-11-14, 2020-11-15, and 2020-11-18 in the gri bands, using 150 second exposures, and reaching 10-sigma limiting magnitudes of approximately 23 mag*. Each night, the ~95% of the 90% localization area was covered by DECam. We reduced the DECam images using the DESGW difference imaging pipeline (Herner et al. 2020), using the 2020-11-14 images as reference images, to find candidate counterparts.
We required that candidate counterparts are (1) not found in GAIA DR2, (2) detected on 2 nights by Source Extractor with 1 of the detections also passing a machine learning artifact detection program (autoscan, Goldstein et. al 2015), (3) detected in multiple bands on at least one night, (4) not found in a spatial-temporal look-up in the Minor Planet Center or Near Earth Object Catalog, (5) not ruled out as an artifact by visual inspection.
We find one optical counterpart candidate:
| NAME | TNS | RA | DEC | HOST |
| DESNU-c-882497 | AT2020aava