activity
20182026
most citedCharacterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes

107 citations · 785 across the 63 of their papers we have counts for

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Showing 2020Show all

9 papers · 1 filter

astro-ph.IM2020

Automating the Inclusion of Subthreshold Signal-to-Noise Ratios for Rapid Gravitational-Wave Localization

Cody Messick, Surabhi Sachdev, Kipp Cannon +29

The accurate localization of gravitational-wave (GW) events in low-latency is a crucial element in the search for further multimessenger signals from these cataclysmic events. The…

astro-ph.IM2020

GstLAL: A software framework for gravitational wave discovery

Kipp Cannon, Sarah Caudill, Chiwai Chan +28

The GstLAL library, derived from Gstreamer and the LIGO Algorithm Library, supports a stream-based approach to gravitational-wave data processing. Although GstLAL was primarily des…

astro-ph.HE2020★ 79 cited

An early warning system for electromagnetic follow-up of gravitational-wave events

Surabhi Sachdev, Ryan Magee, Chad Hanna +28

Binary neutron stars (BNSs) will spend -- 15 minutes in the band of Advanced LIGO and Virgo detectors at design sensitivity. Matched-filtering of gravitational-wave (GW…

astro-ph.IM2020★ 1 cited

Improving the background estimation technique in the GstLAL inspiral pipeline with the time-reversed template bank

Chiwai Chan, Kipp Cannon, Sarah Caudill +20

Background estimation is important for determining the statistical significance of a gravitational-wave event. Currently, the background model is constructed numerically from the s…

gr-qc2020★ 9 cited

Overview of KAGRA : KAGRA science

KAGRA Collaboration, T. Akutsu, M. Ando +240

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured a…

astro-ph.HE2020★ 20 cited

Intermediate Luminosity Red Transients by Black Holes Born from Erupting Massive Stars

Daichi Tsuna, Ayako Ishii, Naoto Kuriyama +2

We consider black hole formation in failed supernovae when a dense circumstellar medium (CSM) is present around the massive star progenitor. By utilizing radiation hydrodynamical s…