Redshifts of candidate gamma-ray blazars

J. P. Halpern, M. Eracleous, J. R. Mattox

Research output: Contribution to journalArticlepeer-review

29 Scopus citations

Abstract

We identify 16 optical counterparts of blazars that have been suggested as sources of high-energy gamma-ray emission detected by the EGRET instrument on board the Compton Gamma-Ray Observatory. Nine new redshifts are obtained, as well one contradiction and two confirmations of published redshifts ranging from z = 0.566 to z = 3.00. The optical spectra of four objects are featureless, including high signal-to-noise spectra of the likely counterparts of 3EG J0433+2908 and GeV J0508+0540, which, if at low redshift, would be attractive targets to search for TeV emission using atmospheric Cerenkov telescopes, because they emit above 10 GeV. However, the combination of spectroscopy and CCD imaging of those objects shows no evidence for their underlying host galaxies, which probably means that z > 0.3, diminishing their prospects as TeV sources.

Original languageEnglish (US)
Pages (from-to)572-579
Number of pages8
JournalAstronomical Journal
Volume125
Issue number2 1766
DOIs
StatePublished - 2003

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Redshifts of candidate gamma-ray blazars'. Together they form a unique fingerprint.

Cite this