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most citedMultiwavelength Observations of Markarian 421 in March 2001: an Unprecedented View on the X-ray/TeV Correlated Variability

220 citations · 220 across the 2 of their papers we have counts for

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astro-ph2007★ 220 cited

Multiwavelength Observations of Markarian 421 in March 2001: an Unprecedented View on the X-ray/TeV Correlated Variability

G. Fossati, J. H. Buckley, I. H. Bond +26

(Abridged) We present a detailed analysis of week-long simultaneous observations of the blazar Mrk421 at 2-60 keV X-rays (RXTE) and TeV gamma-rays (Whipple and HEGRA) in 2001. The…

astro-ph2005

Multiwavelength Observations of 3C 66A during the WEBT campaign of 2003 - 2004

M. Boettcher, J. Harvey, M. Joshi

The BL Lac object 3C 66A was the target of an extensive multiwavelength monitoring campaign from July 2003 through April 2004, involving observations throughout the electromagnetic…

astro-ph2003

Multiwavelength Observations of Strong Flares From the TeV-Blazar 1ES 1959+650

H. Krawczynski, S. B. Hughes, D. Horan +16

Following the detection of strong TeV gamma-ray flares from the BL Lac object 1ES 1959+650 with the Whipple 10 m Cherenkov telescope on May 16 and 17, 2002, we performed intensive…

astro-ph2000

Demographics of Blazars

G. Fossati

We discuss the preliminary results of an extensive effort to address the fundamental, and yet un-answered, question that can be trivialized as: ``are there more blue or red blazars…

astro-ph2000

Looking for High Energy Peaked Blazars

L. Costamante, G. Ghisellini, A. Celotti +10

Blazars can be classified on the basis of their overall Spectral Energy Distribution (SED). BL Lac objects are usually divided in LBL or HBL (Low or High energy peaked BL Lacs), ac…

astro-ph1999

The concave X-ray spectrum of the blazar ON 231: the signature of intermediate BL Lac objects

G. Tagliaferri, G. Ghisellini, P. Giommi +17

ON 231 was observed with BeppoSAX in May and June 1998, following an exceptional optical outburst which occured in April--May. We measured the X-ray spectrum from 0.1 up to 100 keV…