Performance of the low-latency GstLAL inspiral search towards LIGO, Virgo, and KAGRA's fourth observing run

The authors are grateful for computational resources provided by the LIGO Laboratory and supported by National Science Foundation Grants No. PHY-0757058 and No. PHY-0823459. This material is based upon work supported by NSF’s LIGO Laboratory which is a major facility fully funded by the National Science Foundation. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation (NSF) and operates under cooperative Agreement No. PHY-1764464. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors are grateful for computational resources provided by the Pennsylvania State University’s Institute for Computational and Data Sciences (ICDS) and the University of Wisconsin Milwaukee Nemo and support by Grants No. NSF PHY-2011865, No. NSF OAC-2103662, No. NSF PHY-1626190, No. NSF PHY-1700765, and No. NSF PHY-2207728. This paper carries LIGO Document No. LIGO-P2300124. M. W. C. acknowledges support from the National Science Foundation with Grant No. PHY-2010970 and OAC- 2117997. R. E. is supported by the Natural Sciences & Engineering Research Council of Canada (NSERC).