English

The variability analysis of PKS 2155-304

Astrophysics 2007-05-23 v1

Abstract

In this paper, the post-1977 photometric observations of PKS 2155-304 are compiled and used to discuss the variation periodicity. Largest amplitude variations (ΔU=1m.5\Delta U = 1^{m}.5; ΔB=1m.65\Delta B = 1^{m}.65; ΔV=1m.85\Delta V = 1^{m}.85 ; ΔR=1m.25\Delta R = 1^{m}.25; ΔI=1m.14\Delta I = 1^{m}.14 ) and color indices ((BV)=0.30±0.06(B-V) = 0.30\pm 0.06; (UB)=0.72±0.08(U-B) = -0.72\pm 0.08; (BR)=0.62±0.07(B-R) = 0.62\pm 0.07; (VR)=0.32±0.04(V-R) = 0.32\pm 0.04) are found. The Jurkevich's method and DCF (Discrete Correlation Function) method indicate possible periods of 4.16-year and 7.0-year in the V light curve.

Keywords

Cite

@article{arxiv.astro-ph/0001028,
  title  = {The variability analysis of PKS 2155-304},
  author = {J. H. Fan and R. G. Lin},
  journal= {arXiv preprint arXiv:astro-ph/0001028},
  year   = {2007}
}

Comments

11 pages, 4 figures, A&A (accepted)