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20092026
most citedBlazars in the Fermi Era: The OVRO 40-m Telescope Monitoring Program

549 citations · 7.2k across the 125 of their papers we have counts for

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Showing 2013Show all

13 papers · 1 filter

astro-ph.HE2013★ 31 cited

Multiwavelength observations of the gamma-ray emitting narrow-line Seyfert 1 PMN J0948+0022 in 2011

F. D'Ammando, J. Larsson, M. Orienti +13

We report on radio-to-gamma-ray observations during 2011 May-September of PMN J0948+0022, the first narrow-line Seyfert 1 (NLSy1) galaxy detected in gamma-rays by Fermi-LAT. Strong…

astro-ph.HE2013★ 99 cited

Connecting radio variability to the characteristics of gamma-ray blazars

Joseph L. Richards, Talvikki Hovatta, Walter Max-Moerbeck +3

We present results from four years of twice-weekly 15 GHz radio monitoring of about 1500 blazars with the Owens Valley Radio Observatory 40 m telescope. Using the intrinsic modulat…

astro-ph.HE2013★ 40 cited

MAGIC observations and multifrequency properties of the Flat Spectrum Radio Quasar 3C 279 in 2011

J. Aleksić, S. Ansoldi, L. A. Antonelli +168

We study the multifrequency emission and spectral properties of the quasar 3C 279. We observed 3C 279 in very high energy (VHE, E>100GeV) gamma rays, with the MAGIC telescopes duri…

astro-ph.CO2013★ 278 cited

The Cosmic Evolution of Fermi BL Lacertae Objects

M. Ajello, R. W. Romani, D. Gasparrini +14

Fermi has provided the largest sample of gamma-ray selected blazars to date. In this work we use a uniformly selected set of 211 BL Lacertae (BL Lac) objects detected by it Fermi d…

astro-ph.HE2013★ 8 cited

An Exceptional Radio Flare in Markarian 421

Joseph L. Richards, Talvikki Hovatta, Matthew L. Lister +9

In September 2012, the high-synchrotron-peaked (HSP) blazar Markarian 421 underwent a rapid wideband radio flare, reaching nearly twice the brightest level observed in the centimet…

astro-ph.CO2013★ 1 cited

Intrinsic brightness temperatures of blazar jets at 15 GHz

T. Hovatta, E. M. Leitch, D. C. Homan +5

We have developed a new Bayesian Markov Chain Monte Carlo method to deconvolve light curves of blazars into individual flares, including proper estimation of the fit errors. We use…