학술논문
The Gravity Collective: A Comprehensive Analysis of the Electromagnetic Search for the Binary Neutron Star Merger GW190425
Document Type
Working Paper
Author
Coulter, D. A.; Kilpatrick, C. D.; Jones, D. O.; Foley, R. J.; Filippenko, A. V.; Zheng, W.; Swift, J. J.; Rahman, G. S.; Stacey, H. E.; Piro, A. L.; Rojas-Bravo, C.; Vilchez, J. Anais; Muñoz-Elgueta, N.; Arcavi, I.; Dimitriadis, G.; Siebert, M. R.; Bloom, J. S.; Bustamante-Rosell, M. J.; Clever, K. E.; Davis, K. W.; Kutcka, J.; Macias, P.; McGill, P.; Quiñonez, P. J.; Ramirez-Ruiz, E.; Siellez, K.; Tinyanont, S.; Cenko, S. B.; Drout, M. R.; Hausen, R.; Jacobson-Galán, W. V.; Howell, D. Andrew; Kasen, D.; McCully, C.; Rest, A.; Taggart, K.; Valenti, S.
Source
Subject
Language
Abstract
We present an ultraviolet-to-infrared search for the electromagnetic (EM) counterpart to GW190425, the second-ever binary neutron star (BNS) merger discovered by the LIGO-Virgo-KAGRA Collaboration (LVK). GW190425 was more distant and had a larger localization area than GW170817, therefore we use a new tool teglon to redistribute the GW190425 localization probability in the context of galaxy catalogs within the final localization volume. We derive a 90th percentile area of 6,688 deg$^{2}$, a $\sim$1.5$\times$ improvement relative to the LIGO/Virgo map, and show how teglon provides an order of magnitude boost to the search efficiency of small ($\leq$1 deg$^{2}$) field-of-view instruments. We combine our data with all publicly reported imaging data, covering 9,078.59 deg$^2$ of unique area and 48.13% of the LIGO/Virgo-assigned localization probability, to calculate the most comprehensive kilonova, short gamma-ray burst (sGRB) afterglow, and model-independent constraints on the EM emission from a hypothetical counterpart to GW190425 to date under the assumption that no counterpart was found in these data. If the counterpart were similar to AT 2017gfo, there was a 28.4% chance that it would have been detected in the combined dataset. We are relatively insensitive to an on-axis sGRB, and rule out a generic transient with a similar peak luminosity and decline rate as AT 2017gfo to 30% confidence. Finally, across our new imaging and all publicly-reported data, we find 28 candidate optical counterparts that we cannot rule out as being associated with GW190425, finding that 4 such counterparts discovered within the localization volume and within 5 days of merger exhibit luminosities consistent with a kilonova.
Comment: 41 pages, 11 figures, Submitted to ApJ
Comment: 41 pages, 11 figures, Submitted to ApJ