activity
20142023
most citedSearching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

76 citations · 158 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.GA20242 cited

Growth of high redshift supermassive black holes from heavy seeds in the BRAHMA cosmological simulations: Implications of overmassive black holes

Aklant K Bhowmick, Laura Blecha, Paul Torrey +6

JWST has recently revealed a large population of accreting black holes (BHs) in the early Universe. Even after accounting for possible systematic biases, the high-z $M_*-M_{\rm \rm…

astro-ph.HE20241 cited

Signatures of Circumbinary Disk Dynamics in Multi-Messenger Population Studies of Massive Black Hole Binaries

Magdalena Siwek, Luke Zoltan Kelley, Lars Hernquist

We investigate the effect of cutting-edge circumbinary disk (CBD) evolution models on massive black hole binary (MBHB) populations and the gravitational wave background (GWB). We s…

astro-ph.GA2024

AGN feedback in isolated galaxies with a SMUGGLE multiphase ISM

Aneesh Sivasankaran, Laura Blecha, Paul Torrey +6

Feedback from active galactic nuclei (AGN) can strongly impact the host galaxies by driving high-velocity winds that impart substantial energy and momentum to the interstellar medi…

astro-ph.GA20242 cited

Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

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

The first "seeds" of supermassive black holes (BH) can range from . However, the lowest mass seeds () are inaccessible to most cosm…

astro-ph.GA20232 cited

Representing low mass black hole seeds in cosmological simulations: A new sub-grid stochastic seed model

Aklant K Bhowmick, Laura Blecha, Paul Torrey +5

The nature of the first seeds of supermassive black holes (SMBHs) is currently unknown, with postulated initial masses ranging from to as low as $\sim10^2~M_{\…

astro-ph.HE2023380 cited

The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background

Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald +111

The NANOGrav 15-year data set shows evidence for the presence of a low-frequency gravitational-wave background (GWB). While many physical processes can source such low-frequency gr…