daniel holz
daniel holz
Enrico Fermi Institute, Department of Physics, Department of Astronomy & Astrophysics, and Kavli
Verified email at uchicago.edu - Homepage
Title
Cited by
Cited by
Year
Observation of gravitational waves from a binary black hole merger
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (6), 061102, 2016
109482016
GW170817: observation of gravitational waves from a binary neutron star inspiral
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical Review Letters 119 (16), 161101, 2017
62222017
GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (24), 241103, 2016
33622016
GW170104: observation of a 50-solar-mass binary black hole coalescence at redshift 0.2
L Scientific, BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, ...
Physical review letters 118 (22), 221101, 2017
24222017
Multi-messenger observations of a binary neutron star merger
BP Abbott, S Bloemen, P Canizares, H Falcke, RP Fender, S Ghosh, ...
23452017
Gravitational waves and gamma-rays from a binary neutron star merger: GW170817 and GRB 170817A
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
The Astrophysical Journal Letters 848 (2), L13, 2017
20082017
GWTC-1: a gravitational-wave transient catalog of compact binary mergers observed by LIGO and Virgo during the first and second observing runs
BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, ...
Physical Review X 9 (3), 031040, 2019
1988*2019
GW170814: A three-detector observation of gravitational waves from a binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical review letters 119 (14), 141101, 2017
19002017
Toward a halo mass function for precision cosmology: the limits of universality
J Tinker, AV Kravtsov, A Klypin, K Abazajian, M Warren, G Yepes, ...
The Astrophysical Journal 688 (2), 709, 2008
17542008
Binary black hole mergers in the first advanced LIGO observing run
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical Review X 6 (4), 041015, 2016
14342016
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, ...
Living reviews in relativity 23 (1), 1-69, 2020
14292020
Tests of general relativity with GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
arXiv preprint arXiv:1602.03841, 2016
12012016
GW170817: Measurements of neutron star radii and equation of state
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical review letters 121 (16), 161101, 2018
11052018
GW170608: observation of a 19 solar-mass binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
The Astrophysical Journal Letters 851 (2), L35, 2017
10352017
A gravitational-wave standard siren measurement of the Hubble constant
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
arXiv preprint arXiv:1710.05835, 2017
9032017
Properties of the binary black hole merger GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (24), 241102, 2016
7992016
Exploring the sensitivity of next generation gravitational wave detectors
BP Abbott, R Abbott, TD Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and Quantum Gravity 34 (4), 044001, 2017
7272017
GW190425: Observation of a compact binary coalescence with total mass∼ 3.4 M⊙
BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, ...
The Astrophysical Journal Letters 892 (1), L3, 2020
7002020
Astrophysical implications of the binary black hole merger GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
The Astrophysical Journal Letters 818 (2), L22, 2016
6992016
The first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range
K Belczynski, DE Holz, T Bulik, R O’Shaughnessy
Nature 534 (7608), 512-515, 2016
6752016
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