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20102026
most citedThe NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

1.5k citations · 7.4k across the 56 of their papers we have counts for

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Showing 2021Show all

9 papers · 1 filter

gr-qc2021★ 62 cited

The NANOGrav 12.5-year data set: Search for Non-Einsteinian Polarization Modes in theGravitational-Wave Background

Zaven Arzoumanian, Paul T. Baker, Harsha Blumer +68

We search NANOGrav's 12.5-year data set for evidence of a gravitational wave background (GWB) with all the spatial correlations allowed by general metric theories of gravity. We fi…

astro-ph.GA2021★ 11 cited

Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function

Megan Taylor Tillman, Sarah Wellons, Claude-André Faucher-Giguère +2

Observations of massive galaxies at low redshift have revealed approximately linear scaling relations between the mass of a supermassive black hole (SMBH) and properties of its hos…

astro-ph.HE2021★ 37 cited

Gravitational Self-Lensing in Populations of Massive Black Hole Binaries

Luke Zoltan Kelley, Daniel J. D'Orazio, Rosanne Di Stefano

The community may be on the verge of detecting low-frequency gravitational waves from massive black hole binaries (MBHBs), but no examples of binary active galactic nuclei (AGN) ha…

astro-ph.GA2021★ 23 cited

Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse

Aklant K. Bhowmick, Laura Blecha, Paul Torrey +5

Direct collapse black holes~(BH) are promising candidates for producing massive quasars, but their formation requires fine-tuned conditions. In this work, we use cosmo…

astro-ph.HE2021★ 41 cited

Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts

Simone S. Bavera, Tassos Fragos, Emmanouil Zapartas +15

Long-duration gamma-ray bursts are thought to be associated with the core-collapse of massive, rapidly spinning stars and the formation of black holes. However, efficient angular m…

astro-ph.GA2021★ 16 cited

Impact of gas based seeding on supermassive black hole populations at

Aklant K. Bhowmick, Laura Blecha, Paul Torrey +6

Deciphering the formation of supermassive black holes~(SMBHs) is a key science goal for upcoming observational facilities. In most theoretical channels proposed so far, the seed fo…

astro-ph.CO2021★ 125 cited

Searching For Gravitational Waves From Cosmological Phase Transitions With The NANOGrav 12.5-year dataset

Zaven Arzoumanian, Paul T. Baker, Harsha Blumer +62

We search for a first-order phase transition gravitational wave signal in 45 pulsars from the NANOGrav 12.5 year dataset. We find that the data can be modeled in terms of a strong…

astro-ph.GA2021★ 35 cited

The NANOGrav 11yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500Mpc

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +54

Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At sub-parsec separations, binaries become strong sources of low-…

astro-ph.GA2021★ 69 cited

Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently

Linhao Ma, Philip F. Hopkins, Xiangcheng Ma +3

Possible formation scenarios of supermassive black holes in the early universe include rapid growth from less massive seed black holes (BHs) via super-Eddington accretion or runawa…