Multi-Frequency Monitoring of Three Gamma-Ray Quasars

Details Multi-Frequency Monitoring of Three Gamma-Ray Quasars Multi-Frequency Monitoring of Three Gamma-Ray Quasars

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..714..202j&link_type=abstract

X-RAY TIMING 2003: Rossie and Beyond. AIP Conference Proceedings, Volume 714, pp. 202-208 (2004).

Physics

3

Galactic Center, Bar, Circumnuclear Matter, And Bulge, X-Ray, Intergalactic Matter, Quasar Absorption And Emission-Line Systems, Lyman Forest

Scientific paper

We have performed two campaigns of intensive monitoring of the blazars 3C 273, 3C 279, and PKS 1510-089 in the X-ray, optical, near-IR, and radio regions in March and April 2002. The quasar 3C 279 reveals significant interday variability at all wavelengths. The quasar 3C 273 shows smooth variations in the X-ray and near-IR regions on time scales of 2-3 days. For both quasars the results indicate close connection between X-ray and near-IR emission with a delay of X-rays from 0 to 3 days. The quasar PKS 1510-089 was in a low emission state at all frequencies during the campaigns.

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