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Title: RTN-008: Rubin Observatory Processing of Gravitational Wave TOO Data in the Early Operations Era

Abstract

Since the watershed discovery of an electromagnetic counterpart to the LIGO/VIRGO gravitational wave source GW170817, multi-messenger astrophysics has emerged as a major area of strategic focus for the NSF. Rubin Observatory’s depth, survey speed, and data management systems will make it a key asset in the search for EM counterparts. Exploiting this capability during the phases of Rubin commissioning and early operations that coincide with GW observing run O4 may require special actions, however. We discuss potential approaches to data access, template building, and special data processing.

Authors:
ORCiD logo
  1. Dept. of Astronomy, University of Washington
Publication Date:
Other Number(s):
Vera C. Rubin Observatory Technical Note RTN-008
DOE Contract Number:  
AC02-76SF00515
Research Org.:
NSF-DOE Vera C. Rubin Observatory
Sponsoring Org.:
U.S. National Science Foundation; U.S. Department of Energy Office of Science
Subject:
79 ASTRONOMY AND ASTROPHYSICS
OSTI Identifier:
2997564
DOI:
https://doi.org/10.71929/rubin/2997564

Citation Formats

Bellm, Eric C. RTN-008: Rubin Observatory Processing of Gravitational Wave TOO Data in the Early Operations Era. United States: N. p., 2022. Web. doi:10.71929/rubin/2997564.
Bellm, Eric C. RTN-008: Rubin Observatory Processing of Gravitational Wave TOO Data in the Early Operations Era. United States. doi:https://doi.org/10.71929/rubin/2997564
Bellm, Eric C. 2022. "RTN-008: Rubin Observatory Processing of Gravitational Wave TOO Data in the Early Operations Era". United States. doi:https://doi.org/10.71929/rubin/2997564. https://www.osti.gov/servlets/purl/2997564. Pub date:Wed Aug 03 04:00:00 UTC 2022
@article{osti_2997564,
title = {RTN-008: Rubin Observatory Processing of Gravitational Wave TOO Data in the Early Operations Era},
author = {Bellm, Eric C.},
abstractNote = {Since the watershed discovery of an electromagnetic counterpart to the LIGO/VIRGO gravitational wave source GW170817, multi-messenger astrophysics has emerged as a major area of strategic focus for the NSF. Rubin Observatory’s depth, survey speed, and data management systems will make it a key asset in the search for EM counterparts. Exploiting this capability during the phases of Rubin commissioning and early operations that coincide with GW observing run O4 may require special actions, however. We discuss potential approaches to data access, template building, and special data processing.},
doi = {10.71929/rubin/2997564},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Wed Aug 03 04:00:00 UTC 2022},
month = {Wed Aug 03 04:00:00 UTC 2022}
}