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EGRET observations of BL Lacertae objects with redshifts below 0.2

  • Y. C. Lin*
  • , D. L. Bertsch
  • , B. L. Dingus
  • , J. A. Esposito
  • , C. E. Fichtel
  • , R. C. Hartman
  • , S. D. Hunter
  • , G. Kanbach
  • , D. A. Kniffen
  • , J. R. Mattox
  • , H. A. Mayer-Hasselwander
  • , P. F. Michelson
  • , C. Von Montigny
  • , R. Mukherjee
  • , P. L. Nolan
  • , E. J. Schneid
  • , P. Sreekumar
  • , D. J. Thompson
  • , T. D. Willis
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

In the "Revised and Updated Catalog of QuasiStellar Objects" of Hewitt & Burbidge (1993), 90 sources are designated as BL Lacertae Objects. 11 of these 90 BL Lac objects have redshifts below 0.1, out of which EGRET has detected 3, while 13 of these 90 BL Lac objects have redshifts between 0.1 and 0.2, out of which EGRET has detected 2 more, during Phase 1 and Phase 2 of the Compton Observatory's viewing programs. There seems to be a duty cycle of about 25% for EGRET to detect a close BL Lac object with redshift below 0.2. For the other close BL Lac objects which EGRET did not detect, co-adding of EGRET data also yields no detectable flux. These EGRET results are discussed in the paper.

Original languageEnglish
Pages (from-to)499-502
Number of pages4
JournalAstronomy and Astrophysics Supplement Series
Volume120
Issue number4
Publication statusPublished - 1996

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

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