Document List by Author

AndrewLawrence Miller of University of Florida is listed as an author on the following documents:
(List events moderated by AndrewLawrence Miller)

LIGO-Number Title Author(s) Topic(s) Last Updated
P2100098-v14 Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run LIGO Scientific Collaboration et al. Continuous Wave
Stochastic
08 May 2024
P2300439-v1 Erratum: Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run AndrewLawrence Miller et al. Continuous Wave
Stochastic
12 Feb 2024
P2100367-v13 All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data LIGO Scientific Collaboration et al. Continuous Wave
17 Jun 2022
P2100343-v8 All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data LIGO Scientific Collaboration et al. Continuous Wave
30 Nov 2021
G2200599-v1 LVK webinar series: Known continuous wave sources Ian Jones et al. Continuous Wave
27 Mar 2022
G2200241-v2 LVK webinar slides: Searching for continuous gravitational waves from unknown sources Brynmor Haskell et al. Continuous Wave
Education, Outreach
24 Feb 2022
P2000500-v11 Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs LIGO Scientific Collaboration et al. Stochastic
01 Feb 2022
P2000407-v17 Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910 LIGO Scientific Collaboration et al. Continuous Wave
28 Apr 2021
P1800391-v9 Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run LIGO Scientific Collaboration et al. Continuous Wave
28 Nov 2019
P1800195-v13 Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817 LIGO Scientific Collaboration et al. Continuous Wave
Stochastic
04 Oct 2019

Number of documents found: 10


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