EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371

C. Von Montigny; G. Kanbach; H. A. Mayer-Hasselwander; K. Pinkau; H. Rothermel; M. Sommer; D. L. Bertsch; C. E. Fichtel; R. C. Hartman; S. D. Hunter; P. W. Kwok; J. R. Mattox; P. Sreekumar; D. J. Thompson; Y. C. Lin; P. F. Michelson; P. L. Nolan; D. A. Kniffen; E. Schneid

doi:10.1063/1.44278

EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371

C. Von Montigny
, G. Kanbach
, H. A. Mayer-Hasselwander
, K. Pinkau
, H. Rothermel
, M. Sommer
, D. L. Bertsch
, C. E. Fichtel
, R. C. Hartman
, S. D. Hunter
, P. W. Kwok
, J. R. Mattox
, P. Sreekumar
, D. J. Thompson
, Y. C. Lin
, P. F. Michelson
, P. L. Nolan
, D. A. Kniffen
, E. Schneid

Manipal Centre for Natural Sciences, Manipal

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

4 Citations (Scopus)

Abstract

Most of the active galactic nuclei (AGN) detected by EGRET are known or suspected to be superluminal sources. We report here the results of the observations of the blazars 3C 345, BL Lac and 3C 371, which have been selected from the list of known and possible superluminal sources. For none of them we found a signal in high energy γ-rays. The 20 upper limits for the γ-ray fluxes for energies above 100 MeV (equivalent to 95% confidence) are presented.

Original language	English
Title of host publication	Compton Gamma-Ray Observatory
Editors	Neil Gehrels, Michael W. Friedlander, Daryl J. Macomb
Publisher	American Institute of Physics Inc.
Pages	518-522
Number of pages	5
ISBN (Electronic)	1563961040
DOIs	https://doi.org/10.1063/1.44278
Publication status	Published - 1993
Event	Compton Symposium - St. Louis, United States Duration: 15-10-1992 → 17-10-1992

Publication series

Name	AIP Conference Proceedings
Volume	280
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	Compton Symposium
Country/Territory	United States
City	St. Louis
Period	15-10-92 → 17-10-92

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

Access to Document

10.1063/1.44278

Cite this

Von Montigny, C., Kanbach, G., Mayer-Hasselwander, H. A., Pinkau, K., Rothermel, H., Sommer, M., Bertsch, D. L., Fichtel, C. E., Hartman, R. C., Hunter, S. D., Kwok, P. W., Mattox, J. R., Sreekumar, P., Thompson, D. J., Lin, Y. C., Michelson, P. F., Nolan, P. L., Kniffen, D. A., & Schneid, E. (1993). EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371. In N. Gehrels, M. W. Friedlander, & D. J. Macomb (Eds.), Compton Gamma-Ray Observatory (pp. 518-522). (AIP Conference Proceedings; Vol. 280). American Institute of Physics Inc.. https://doi.org/10.1063/1.44278

@inproceedings{d4425fe8478241d4b7711c50fa70b6de,

title = "EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371",

abstract = "Most of the active galactic nuclei (AGN) detected by EGRET are known or suspected to be superluminal sources. We report here the results of the observations of the blazars 3C 345, BL Lac and 3C 371, which have been selected from the list of known and possible superluminal sources. For none of them we found a signal in high energy γ-rays. The 20 upper limits for the γ-ray fluxes for energies above 100 MeV (equivalent to 95\% confidence) are presented.",

author = "\{Von Montigny\}, C. and G. Kanbach and Mayer-Hasselwander, \{H. A.\} and K. Pinkau and H. Rothermel and M. Sommer and Bertsch, \{D. L.\} and Fichtel, \{C. E.\} and Hartman, \{R. C.\} and Hunter, \{S. D.\} and Kwok, \{P. W.\} and Mattox, \{J. R.\} and P. Sreekumar and Thompson, \{D. J.\} and Lin, \{Y. C.\} and Michelson, \{P. F.\} and Nolan, \{P. L.\} and Kniffen, \{D. A.\} and E. Schneid",

note = "Publisher Copyright: {\textcopyright} 1993 American Institute of Physics.; Compton Symposium ; Conference date: 15-10-1992 Through 17-10-1992",

year = "1993",

doi = "10.1063/1.44278",

language = "English",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "518--522",

editor = "Neil Gehrels and Friedlander, \{Michael W.\} and Macomb, \{Daryl J.\}",

booktitle = "Compton Gamma-Ray Observatory",

}

Von Montigny, C, Kanbach, G, Mayer-Hasselwander, HA, Pinkau, K, Rothermel, H, Sommer, M, Bertsch, DL, Fichtel, CE, Hartman, RC, Hunter, SD, Kwok, PW, Mattox, JR, Sreekumar, P, Thompson, DJ, Lin, YC, Michelson, PF, Nolan, PL, Kniffen, DA & Schneid, E 1993, EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371. in N Gehrels, MW Friedlander & DJ Macomb (eds), Compton Gamma-Ray Observatory. AIP Conference Proceedings, vol. 280, American Institute of Physics Inc., pp. 518-522, Compton Symposium, St. Louis, United States, 15-10-92. https://doi.org/10.1063/1.44278

EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371. / Von Montigny, C.; Kanbach, G.; Mayer-Hasselwander, H. A. et al.
Compton Gamma-Ray Observatory. ed. / Neil Gehrels; Michael W. Friedlander; Daryl J. Macomb. American Institute of Physics Inc., 1993. p. 518-522 (AIP Conference Proceedings; Vol. 280).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371

AU - Von Montigny, C.

AU - Kanbach, G.

AU - Mayer-Hasselwander, H. A.

AU - Pinkau, K.

AU - Rothermel, H.

AU - Sommer, M.

AU - Bertsch, D. L.

AU - Fichtel, C. E.

AU - Hartman, R. C.

AU - Hunter, S. D.

AU - Kwok, P. W.

AU - Mattox, J. R.

AU - Sreekumar, P.

AU - Thompson, D. J.

AU - Lin, Y. C.

AU - Michelson, P. F.

AU - Nolan, P. L.

AU - Kniffen, D. A.

AU - Schneid, E.

PY - 1993

Y1 - 1993

N2 - Most of the active galactic nuclei (AGN) detected by EGRET are known or suspected to be superluminal sources. We report here the results of the observations of the blazars 3C 345, BL Lac and 3C 371, which have been selected from the list of known and possible superluminal sources. For none of them we found a signal in high energy γ-rays. The 20 upper limits for the γ-ray fluxes for energies above 100 MeV (equivalent to 95% confidence) are presented.

AB - Most of the active galactic nuclei (AGN) detected by EGRET are known or suspected to be superluminal sources. We report here the results of the observations of the blazars 3C 345, BL Lac and 3C 371, which have been selected from the list of known and possible superluminal sources. For none of them we found a signal in high energy γ-rays. The 20 upper limits for the γ-ray fluxes for energies above 100 MeV (equivalent to 95% confidence) are presented.

UR - https://www.scopus.com/pages/publications/85063816574

UR - https://www.scopus.com/pages/publications/85063816574#tab=citedBy

U2 - 10.1063/1.44278

DO - 10.1063/1.44278

M3 - Conference contribution

AN - SCOPUS:85063816574

T3 - AIP Conference Proceedings

SP - 518

EP - 522

BT - Compton Gamma-Ray Observatory

A2 - Gehrels, Neil

A2 - Friedlander, Michael W.

A2 - Macomb, Daryl J.

PB - American Institute of Physics Inc.

T2 - Compton Symposium

Y2 - 15 October 1992 through 17 October 1992

ER -

EGRET upper limits for the blazars 3C 345, BL Lac and 3C 371

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