activity
19952026
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 · 22.7k across the 285 of their papers we have counts for

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Showing 2009Show all

7 papers · 1 filter

astro-ph.CO2009★ 65 cited

A 3.5mm Polarimetric Survey of Radio-loud Active Galactic Nuclei

I. Agudo, C. Thum, H. Wiesemeyer +1

We present the results from the first large (>100 source) 3.5 mm polarimetric survey of radio loud active galactic nuclei (AGN). The I, Q, U, and V Stokes parameter observations we…

astro-ph.HE2009★ 104 cited

Multiwavelength monitoring of the enigmatic Narrow-Line Seyfert 1 PMN J0948+0022 in March-July 2009

LAT Collaboration, E. Angelakis, C. Bailyn +39

Following the recent discovery of gamma rays from the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 (z=0.5846), we started a multiwavelength campaign from radio to gamma r…

astro-ph.CO2009★ 8 cited

Very Long Baseline Array observations of the Intraday Variable source J1128+592

K. E. Gabanyi, N. Marchili, T. P. Krichbaum +5

Short time-scale flux density variations of flat spectrum radio sources are often explained by the scattering of radio waves in the turbulent, ionized Interstellar Matter of the Mi…

astro-ph.GA2009

AGN astrophysics via multi-frequency monitoring of gamma-ray blazars in the Fermi-GST era

E. Angelakis, L. Fuhrmann, J. A. Zensus +10

The F-GAMMA-project is the coordinated effort of several observatories to understand the AGN phenomenon and specifically blazars via multi-frequency monitoring in collaboration wit…

astro-ph.CO2009★ 28 cited

The radio lightcurve of SN 2008iz in M82 revealed by Urumqi observations

N. Marchili, I. Marti-Vidal, A. Brunthaler +7

We report on a set of 5 GHz Urumqi observations of the galaxy M82, made between August 2005 and May 2009. From the resulting flux densities, we detect a strong flare, starting in M…

astro-ph.CO2009★ 81 cited

Imaging an Event Horizon: submm-VLBI of a Super Massive Black Hole

Sheperd Doeleman, Eric Agol, Don Backer +20

A long standing goal in astrophysics is to directly observe the immediate environment of a black hole with angular resolution comparable to the event horizon. Realizing this goal w…