papers

Publications (18)

astro-ph.GA2021

Event Horizon Telescope observations of the jet launching and collimation in Centaurus A

Michael Janssen, Heino Falcke, Matthias Kadler +236

Very-long-baseline interferometry (VLBI) observations of active galactic nuclei at millimeter wavelengths have the power to reveal the launching and initial collimation region of e…

astro-ph.GA2013

Observations of gas flows inside a protoplanetary gap

Simon Casassus, Gerrit van der Plas, Sebastian Perez M. +16

Gaseous giant planet formation is thought to occur in the first few million years following stellar birth. Models predict that giant planet formation carves a deep gap in the dust…

astro-ph.IM2019

Calibration of ALMA as a phased array: ALMA observations during the 2017 VLBI campaign

Ciriaco Goddi, Ivan Marti-Vidal, Hugo Messias +14

We present a detailed description of the special procedures for calibration and quality assurance of Atacama Large Millimeter/submillimeter Array (ALMA) observations in Very Long B…

physics.geo-ph2009

Precise geodesy with the Very Long Baseline Array

Leonid Petrov, David Gordon, John Gipson +5

We report on a program of geodetic measurements between 1994 and 2007 which used the Very Long Baseline Array and up to 10 globally distributed antennas. One of the goals of this p…

astro-ph.HE2023

Comparison of Polarized Radiative Transfer Codes used by the EHT Collaboration

Ben S. Prather, Cora Prather, Jason Dexter +271

Interpretation of resolved polarized images of black holes by the Event Horizon Telescope (EHT) requires predictions of the polarized emission observable by an Earth-based instrume…

astro-ph.HE2021

The Polarized Image of a Synchrotron Emitting Ring of Gas Orbiting a Black Hole

Ramesh Narayan, Daniel C. M. Palumbo, Michael D. Johnson +237

Synchrotron radiation from hot gas near a black hole results in a polarized image. The image polarization is determined by effects including the orientation of the magnetic field i…

astro-ph.EP2020

Long Baseline Observations of the HD100546 Protoplanetary Disk with ALMA

Sebastián Pérez, Simon Casassus, Antonio Hales +9

Using the Atacama Large Millimeter/submillimeter Array (ALMA), we observed the young Herbig star HD 100546, host to a prominent disk with a deep, wide gap in the dust. The high-res…

astro-ph2003

VLBA Calibrator Survey: Astrometric and Image Results

Leonid Petrov, David Grodon, Anthony Beasley +1

Positions and maps of 1608 new compact sources were obtained in twelve sessions observed during 1994--2002 at the VLBA network at 8.4/2.3 GHz. These sources are recommended for use…

astro-ph.CO2010

The Position/Structure Stability of Four ICRF2 Sources

Ed Fomalont, Kenneth Johnston, Alan Fey +3

Four close radio sources in the International Celestial Reference Frame (ICRF) catalog were observed using phase referencing with the VLBA at 43, 23 and 8.6 GHz, and with VERA at 2…

astro-ph.HE2023

The internal Faraday screen of Sagittarius A*

Maciek Wielgus, Sara Issaoun, Ivan Marti-Vidal +5

We report on 85-101 GHz light curves of the Galactic Center supermassive black hole, Sagittarius A* (Sgr A*), observed in April 2017 with the Atacama Large Millimeter/submillimeter…

astro-ph.HE2023

A search for pulsars around Sgr A* in the first Event Horizon Telescope dataset

Pablo Torne, Kuo Liu, Ralph P. Eatough +282

The Event Horizon Telescope (EHT) observed in 2017 the supermassive black hole at the center of the Milky Way, Sagittarius A* (Sgr A*), at a frequency of 228.1 GHz (=1.3 mm). T…

astro-ph.HE2022

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…

gr-qc2020

Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole

Dimitrios Psaltis, Lia Medeiros, Pierre Christian +185

The 2017 Event Horizon Telescope (EHT) observations of the central source in M87 have led to the first measurement of the size of a black-hole shadow. This observation offers a new…

astro-ph.IM2019

Total Power Map to Visibilities (TP2VIS): Joint Deconvolution of ALMA 12m, 7m, and Total Power Array Data

Jin Koda, Peter Teuben, Tsuyoshi Sawada +2

We present a new package for joint deconvolution of ALMA 12m, 7m, and Total Power (TP) data, dubbed ``Total Power Map to Visibilities (TP2VIS)". It converts a TP (single-dish) map…

gr-qc2002

General relativistic model for experimental measurement of the speed of propagation of gravity by VLBI

Sergei Kopeikin, Ed Fomalont

A relativistic sub-picosecond model of gravitational time delay in radio astronomical observations is worked out and a new experimental test of general relativity is discussed in w…

gr-qc2021

Constraints on black-hole charges with the 2017 EHT observations of M87*

Prashant Kocherlakota, Luciano Rezzolla, Heino Falcke +234

Our understanding of strong gravity near supermassive compact objects has recently improved thanks to the measurements made by the Event Horizon Telescope (EHT). We use here the M8…

astro-ph.IM2014

Astrometry of Cassini with the VLBA to Improve the Saturn Ephemeris

Dayton L. Jones, William M. Folkner, Robert A. Jacobson +4

Planetary ephemerides have been developed and improved over centuries. They are a fundamental tool for understanding solar system dynamics, and essential for planetary and small bo…

astro-ph.IM2014

Phase Characteristics of the ALMA 3 km Baseline Data

Satoki Matsushita, Yoshiharu Asaki, Ryohei Kawabe +3

We present the phase characteristics study of the Atacama Large Millimeter/submillimeter Array (ALMA) long (up to 3 km) baseline, which is the longest baseline tested so far using…