REM near-IR and optical multiband observations of PKS2155-304 in 2005
arXiv:0704.0265 · doi:10.1051/0004-6361:20066477
Abstract
Spectral variability is the main tool for constraining emission models of BL Lac objects. By means of systematic observations of the BL Lac prototype PKS 2155-304 in the infrared-optical band, we explore variability on the scales of months, days and hours. We made our observations with the robotic 60 cm telescope REM located at La Silla, Chile. VRIJHK filters were used. PKS 2155-304 was observed from May to December 2005. The wavelength interval explored, the total number of photometric points and the short integration time render our photometry substantially superior to previous ones for this source. On the basis of the intensity and colour we distinguish three different states of the source, each of duration of months, which include all those described in the literature. In particular, we report the highest state ever detected in the H band. The source varied by a factor of 4 in this band, much more than in the V band (a factor ~2). The source softened with increasing intensity, contrary to the general pattern observed in the UV-X-ray bands. On five nights of November we had nearly continuous monitoring for 2-3 hours. A variability episode with a time scale of ~24 h is well documented, a much more rapid flare with t=1-2 h, is also apparent, but is supported by relatively few points.
This paper is the corrected version of the paper published in A&A 469 503. It contains the material in the "Errata Corrrige", in press in A&A
References in corpus (11)
- REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination
- Stochastic particle acceleration and synchrotron self--Compton radiation in TeV blazars
- The Intra-Night Optical Variability of the bright BL Lac object S5 0716+714
- Correlation between the TeV and X-ray emission in high--energy peaked BL Lac objects
- XMM-Newton View of PKS 2155-304: Characterizing the X-ray Variability Properties with EPIC-PN
- A rapid and dramatic outburst in Blazar 3C 454.3 during May 2005 - Optical and infrared observations with REM and AIT
- XMM-Newton view of PKS 2155-304: hardness ratio and cross-correlation analysis of EPIC pn observations
- Optical spectroscopy of BL Lacertae objects. Broad lines, companion galaxies and redshift lower limits
- Dissipation of jet bulk kinetic energy in powerful blazars
- Multiwavelength Observations of the BL Lacertae Object PKS 2155-304 with XMM-Newton
- Multiband Photometry of the Blazar PKS 0537-441: A Major Active State in December 2004 - March 2005
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- Infrared to X-ray observations of PKS 2155-304 in a low state
- Spectral energy distributions of the BL Lac PKS 2155-304 from XMM-Newton
- Flux and spectral variability of the blazar PKS 2155-304 with XMM-Newton: Evidence of Particle Acceleration and Synchrotron Cooling
- AGILE observation of a gamma-ray flare from the blazar 3C 279
- New Multiwavelength Observations of PKS 2155-304 and Implications for the Coordinated Variability Patterns of Blazars