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19972026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2010Show all

18 papers · 1 filter

astro-ph.HE2010★ 102 cited

Spectral Energy Distribution of Markarian 501: Quiescent State vs. Extreme Outburst

The VERITAS Collaboration, V. A. Acciari, T. Arlen +225

The very high energy (VHE; E > 100 GeV) blazar Markarian 501 has a well-studied history of extreme spectral variability and is an excellent laboratory for studying the physical pro…

astro-ph.HE2010★ 239 cited

Insights Into the High-Energy Gamma-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era

LAT collaboration, A. A. Abdo et al., the MAGIC collaboration +6

We report on the gamma-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average LAT gamma-ray spectrum of Mrk 501 can be well descr…

astro-ph.HE2010★ 87 cited

Multi-wavelength Observations of the Flaring Gamma-ray Blazar 3C 66A in 2008 October

LAT collaboration, A. A. Abdo et al., the VERITAS collaboration +4

The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GA…

astro-ph.CO2010★ 79 cited

The Sudden Death of the Nearest Quasar

Kevin Schawinski, Daniel A. Evans, Shanil Virani +13

Galaxy formation is significantly modulated by energy output from supermassive black holes at the centers of galaxies which grow in highly efficient luminous quasar phases. The tim…

astro-ph.GA2010★ 30 cited

Massive Star Formation of the Sgr A East HII Regions Near the Galactic Center

F. Yusef-Zadeh, J. H. Lacy, M. Wardle +4

A group of four compact HII regions associated with the well-known 50 km/s molecular cloud is the closest site of on-going star formation to the dynamical center of the Galaxy, at…

astro-ph.GA2010★ 10 cited

Occultation of the Quiescent Emission from Sgr A* by IR Flares

F. Yusef-Zadeh, M. Wardle, H. Bushouse +2

We have investigated the nature of flare emission from Sgr A* during multi-wavelength observations of this source that took place in 2004, 2005 and 2006. We present evidence for di…