Articles Citing

Inferring the pair-instability mass gap from gravitational wave data

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¹Gravity Exploration Institute, School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
²Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, Illinois 60637, USA
³DAMTP, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, United Kingdom
⁴Kavli Institute for Cosmology, Madingley Road, Cambridge, CB3 0HA, United Kingdom
⁵H. H. Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL, United Kingdom
⁶Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, 1800 Sherman Avenue, Evanston, Illinois 60201, USA

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Articles Citing

Inferring the pair-instability mass gap from gravitational wave data

Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses

Signatures of a Subpopulation of Hierarchical Mergers in the GWTC-4 Gravitational-Wave Dataset

Subpopulation of low-mass, spinning black holes: Signatures of dynamical assembly

Low-mass failed supernovae and the 10M⊙ peak in the merging black hole mass distribution

Measurement prospects for the pair-instability mass cutoff with gravitational waves

Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold

Evidence of the pair-instability gap from black-hole masses

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars

Heavy black-holes also matter in standard siren cosmology

Reexamining Evidence of a Pair-instability Mass Gap in the Binary Black Hole Population

Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5

GWTC-4.0: Population Properties of Merging Compact Binaries

Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the 35 M ⊙ Peak

GW231123: Likely a Product of Successive Mergers from ∼10 Stellar-mass Black Holes

Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals

When black holes align: A subpopulation of aligned massive binary black holes observed via gravitational waves

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