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20142026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 8.2k across the 102 of their papers we have counts for

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21 papers · 1 filter

astro-ph.HE2022★ 29 cited

Using Machine Learning to Link Black Hole Accretion Flows with Spatially Resolved Polarimetric Observables

Richard Qiu, Angelo Ricarte, Ramesh Narayan +3

We introduce a new library of 535,194 model images of the supermassive black holes and Event Horizon Telescope (EHT) targets Sgr A* and M87*, computed by performing general relativ…

astro-ph.GA2022★ 16 cited

Constraints from dwarf galaxies on black hole seeding and growth models with current and future surveys

Urmila Chadayammuri, Akos Bogdan, Angelo Ricarte +1

Dwarf galaxies are promising test beds for constraining models of supermassive and intermediate-mass black holes (MBH) via their black hole occupation fraction (BHOF). Disentanglin…

astro-ph.HE2022★ 22 cited

Accretion Flow Morphology in Numerical Simulations of Black Holes from the ngEHT Model Library: The Impact of Radiation Physics

Koushik Chatterjee, Andrew Chael, Paul Tiede +18

In the past few years, the Event Horizon Telescope (EHT) has provided the first-ever event horizon-scale images of the supermassive black holes (BHs) (M87*) and Sagittarius A (…

astro-ph.CO2022

Expectations for Horizon-Scale Supermassive Black Hole Population Studies with the ngEHT

Dominic W. Pesce, Daniel C. M. Palumbo, Angelo Ricarte +5

We present estimates for the number of supermassive black holes (SMBHs) for which the next-generation Event Horizon Telescope (ngEHT) can identify the black hole ``shadow,'' along…

astro-ph.GA2022

Tracing the hot spot motion using the next generation Event Horizon Telescope (ngEHT)

Razieh Emami, Paul Tiede, Sheperd S. Doeleman +19

We propose to trace the dynamical motion of a shearing hot spot near the SgrA* source through a dynamical image reconstruction algorithm, StarWarps. Such a hot spot may form as the…

astro-ph.HE2022

Probing plasma composition with the next generation Event Horizon Telescope (ngEHT)

Razieh Emami, Richard Anantua, Angelo Ricarte +15

We explore the plasma matter content in the innermost accretion disk/jet in M87* as relevant for an enthusiastic search for the signatures of anti-matter in the next generation of…

astro-ph.HE2022

Emission Modeling in the EHT-ngEHT Age

Richard Anantua, Joaquín Dúran, Nathan Ngata +9

This work proposes a methodology to test phenomenologically-motivated emission processes that account for the flux and polarization distribution and global structure of the 230 GHz…

astro-ph.HE2022★ 1 cited

The ngEHT's Role in Measuring Supermassive Black Hole Spins

Angelo Ricarte, Paul Tiede, Razieh Emami +2

While supermassive black hole masses have been cataloged across cosmic time, only a few dozen of them have robust spin measurements. By extending and improving the existing Event H…

astro-ph.HE2022★ 16 cited

How Spatially Resolved Polarimetry Informs Black Hole Accretion Flow Models

Angelo Ricarte, Michael D. Johnson, Yuri Y. Kovalev +2

The Event Horizon Telescope (EHT) Collaboration has successfully produced images of two supermassive black holes, enabling novel tests of black holes and their accretion flows on h…

gr-qc2022★ 36 cited

Observational Signatures of Frame Dragging in Strong Gravity

Angelo Ricarte, Daniel C. M. Palumbo, Ramesh Narayan +2

Objects orbiting in the presence of a rotating massive body experience a gravitomagnetic frame-dragging effect, known as the Lense-Thirring effect, that has been experimentally con…

astro-ph.GA2022★ 1 cited

A vast population of wandering and merging IMBHs at cosmic noon

Tiziana Di Matteo, Yueying Ni, Nianyi Chen +5

Massive black holes in the centers of galaxies today must have grown by several orders of magnitude from seed black holes formed at early times. Detecting a population of intermedi…

astro-ph.HE2022★ 37 cited

Multi-frequency Black Hole Imaging for the Next-Generation Event Horizon Telescope

Andrew Chael, Sara Issaoun, Dominic W. Pesce +4

The Event Horizon Telescope (EHT) has produced images of the plasma flow around the supermassive black holes in Sgr A* and M87* with a resolution comparable to the projected size o…

astro-ph.GA2022★ 32 cited

Unraveling Twisty Linear Polarization Morphologies in Black Hole Images

Razieh Emami, Angelo Ricarte, George N. Wong +23

We investigate general relativistic magnetohydrodynamic simulations (GRMHD) to determine the physical origin of the twisty patterns of linear polarization seen in spatially resolve…

astro-ph.HE2022★ 69 cited

The Photon Ring in M87*

Avery E. Broderick, Dominic W. Pesce, Paul Tiede +48

We report measurements of the gravitationally lensed secondary image -- the first in an infinite series of so-called "photon rings" -- around the supermassive black hole M87* via s…

astro-ph.HE2022★ 47 cited

Resolving the inner parsec of the blazar J1924-2914 with the Event Horizon Telescope

Sara Issaoun, Maciek Wielgus, Svetlana Jorstad +27

The blazar J1924-2914 is a primary Event Horizon Telescope (EHT) calibrator for the Galactic Center's black hole Sagittarius A*. Here we present the first total and linearly polari…

astro-ph.HE2022★ 112 cited

Millimeter light curves of Sagittarius A* observed during the 2017 Event Horizon Telescope campaign

Maciek Wielgus, Nicola Marchili, Ivan Marti-Vidal +28

The Event Horizon Telescope (EHT) observed the compact radio source, Sagittarius A* (Sgr A*), in the Galactic Center on 2017 April 5-11 in the 1.3 millimeter wavelength band. At th…

astro-ph.HE2022

PATOKA: Simulating Electromagnetic Observables of Black Hole Accretion

George N. Wong, Ben S. Prather, Vedant Dhruv +11

The Event Horizon Telescope (EHT) has released analyses of reconstructed images of horizon-scale millimeter emission near the supermassive black hole at the center of the M87 galax…

gr-qc2022★ 6 cited

Astrophysics with the Laser Interferometer Space Antenna

Pau Amaro Seoane, Jeff Andrews, Manuel Arca Sedda +156

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many…

astro-ph.GA2022★ 23 cited

A hidden population of massive black holes in simulated dwarf galaxies

Ray S. Sharma, Alyson M. Brooks, Michael Tremmel +3

We explore the characteristics of actively accreting MBHs within dwarf galaxies in the \textsc{Romulus25} cosmological hydrodynamic simulation. We examine the MBH occupation fracti…

astro-ph.GA2022★ 2 cited

Prospects to Explore High-redshift Black Hole Formation with Multi-band Gravitational Waves Observatories

Hsin-Yu Chen, Angelo Ricarte, Fabio Pacucci

The assembly of massive black holes in the early universe remains a poorly constrained open question in astrophysics. The merger and accretion of light seeds (remnants of Populatio…

astro-ph.HE2022★ 15 cited

Probing Plasma Physics with Spectral Index Maps of Accreting Black Holes on Event Horizon Scales

Angelo Ricarte, Charles Gammie, Ramesh Narayan +1

The Event Horizon Telescope (EHT) collaboration has produced the first resolved images of the supermassive black holes at the centre of our galaxy and at the centre of the elliptic…