High redshift Fermi blazars observed by GROND and Swift
arXiv:1209.2514 · doi:10.1093/mnras/sts140
Abstract
We observed 5 gamma-ray loud blazars at redshift greater than 2 with the X-Ray Telescope (XRT) and the UltraViolet and Optical Telescope (UVOT) onboard the Swift satellite, and the Gamma-Ray burst Optical Near-Infrared Detector (GROND) instrument. These observations were quasi simultaneous, usually within a few hours. For 4 of these blazars the near-IR to UV data show the presence of an accretion disc, and we could reliably estimate its accretion rate and black hole mass. One of them, PKS 1348+007, was found in an extraordinarily high IR-optical state, almost two orders of magnitude brighter than at the epoch of the Sloan Digital Sky Survey observations. For all the 5 quasars the physical parameters of the jet emitting zone, derived by applying a one-zone emission model, are similar to that found for the bulk of other gamma-ray loud quasars. With our observations we have X-ray data for the full sample of blazars at z>2 present in the Fermi 2-yrs (2LAC) catalog. This allows to have a rather complete view of the spectral energy distribution of all high-redshift Fermi blazars, and to draw some conclusions about their properties, and especially about the relation between the accretion rate and the jet power.
11 pages, 6 figures, submitted to MNRAS
References in corpus (6)
- GROND - a 7-channel imager
- Swift and infra-red observations of the blazar 3C~454.3 during the giant X-ray flare of May 2005
- INTEGRAL observations of the blazar 3C454.3 in outburst
- Blue Fermi Flat Spectrum Radio Quasars
- SDSS J102623.61+254259.5: the second most distant blazar at z=5.3
- Dissipation of jet bulk kinetic energy in powerful blazars
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- SDSS J013127.34-032100.1: a candidate blazar with a 11 billion solar mass black hole at =5.18
- Constraints on the location of -ray emitting region for a sample of blazars with radio core-shift measurements
- Jets, black holes and disks in blazars
- Awakening of The High Redshift Blazar CGRaBS J0809+5341
- VLBI observations of a flared optical quasar CGRaBS J0809+5341
- Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
- Extragalactic astrophysics with next-generation CMB experiments