Day-scale variability of 3C 279 and searches for correlations in gamma-ray, x-ray, and optical bands

Citation
Rc. Hartman et al., Day-scale variability of 3C 279 and searches for correlations in gamma-ray, x-ray, and optical bands, ASTROPHYS J, 558(2), 2001, pp. 583-589
Citations number
42
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
558
Issue
2
Year of publication
2001
Part
1
Pages
583 - 589
Database
ISI
SICI code
0004-637X(20010910)558:2<583:DVO32A>2.0.ZU;2-N
Abstract
Light curves of 3C 279 are presented in optical (R band), X-rays (RXTE/PCA) , and gamma rays (CGRO/ EGRET) for 1999 January-February and 2000 January-M arch. During both of those epochs the gamma -ray levels were high and all t hree observed bands demonstrated substantial variation, on timescales as sh ort as 1 day. Correlation analyses provided no consistent pattern, although a rather significant optical/gamma -ray correlation was seen in 1999, with a gamma -ray lag of similar to2.5 days, and there are other suggestions of correlations in the light curves. For comparison, correlation analysis is also presented for the gamma -ray and X-ray light curves during the large g amma ray flare in 1996 February and the two gamma -bright weeks leading up to it; the correlation at that time was strong, with a gamma -ray/X-ray off set of no more than 1 day.