activity
20002008
most citedTesting the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71. I. Simultaneous broadband observations during November 2003

72 citations · 90 across the 4 of their papers we have counts for

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astro-ph20088 cited

The Rosette Eye: the key transition phase in the birth of a massive star

J. Z. Li, M. D. Smith, R. Gredel +2

Massive protostars dramatically influence their surroundings via accretion-induced outflows and intense radiation fields. They evolve rapidly, the disk and infalling envelope being…

astro-ph200610 cited

The 2dF BL Lac Survey II

D. Londish, S. M. Croom, J. Heidt +6

We report on our further analysis of the expanded and revised sample of potential BL Lac objects (the 2BL) optically identified from two catalogues of blue-selected (UV excess) poi…

astro-ph200672 cited

Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71. I. Simultaneous broadband observations during November 2003

L. Ostorero, S. J. Wagner, J. Gracia +6

Some intra-day variable, compact extra-galactic radio sources show brightness temperatures severely exceeding 10^{12} K, the limit set by catastrophic inverse-Compton (IC) cooling…

astro-ph2005

Faint Radio Sources in the NOAO Bootes Field. VLBA Imaging and Optical Identifications

J. M. Wrobel, G. B. Taylor, T. A. Rector +2

As a step toward investigating the parsec-scale properties of faint extragalactic radio sources, the Very Long Baseline Array (VLBA) was used at 5.0 GHz to obtain phase-referenced…

astro-ph2005

Intrinsic Curvature in the X-ray Spectra of BL Lacertae Objects

Eric S. Perlman, Greg Madejski, Markos Georganopoulos +10

We report results from {\it XMM-Newton} observations of thirteen X-ray bright BL Lacertae objects, selected from the {\it Einstein} Slew Survey sample. The survey was designed to l…

astro-ph2004

Image-Processing Techniques for the Creation of Presentation-Quality Astronomical Images

T. A. Rector, Z. G. Levay, L. M. Frattare +2

The quality of modern astronomical data, the power of modern computers and the agility of current image-processing software enable the creation of high-quality images in a purely d…