Multiwavelength periodicity study of Markarian 501
arXiv:0904.4392 · doi:10.1051/0004-6361/200911814
Abstract
Context: Active Galactic Nuclei are highly variable emitters of electromagnetic waves from the radio to the gamma-ray regime. This variability may be periodic, which in turn could be the signature of a binary black hole. Systems of black holes are strong emitters of gravitational waves whose amplitude depends on the binary orbital parameters as the component mass, the orbital semi-major-axis and eccentricity. Aims: It is our aim to prove the existence of periodicity of the AGN Markarian 501 from several observations in different wavelengths. A simultaneous periodicity in different wavelengths provides evidence for bound binary black holes in the core of AGN. Methods: Existing data sets from observations by Whipple, SWIFT, RXTE and MAGIC have been analysed with the Lomb-Scargle method, the epoch folding technique and the SigSpec software. Results: Our analysis shows a 72-day period, which could not be seen in previous works due to the limited length of observations. This does not contradict a 23-day period which can be derived as a higher harmonic from the 72-day period.
9 pages, 15 figures, accepted at A&A
References in corpus (6)
- Variable VHE gamma-ray emission from Markarian 501
- SigSpec - I. Frequency- and Phase-Resolved Significance in Fourier Space
- X-ray Detection of the Proto Supermassive Binary Black Hole at the Centre of Abell 400
- Modeling of Emission Signatures of Massive Black Hole Binaries: I Methods
- Supermassive binary black holes among cosmic gamma-ray sources
- A possible disk mechanism for the 23d QPO in Mkn~501
Cited by in corpus (6)
- Blazar Mrk 501 shows rhythmic oscillations in its -ray emission
- Multi-color optical monitoring of Mrk 501 from 2010 to 2015
- Electromagnetic signatures of supermassive black hole binaries resolved by PTAs
- Search for intra-day optical variability in Mrk 501
- Not so Swift: 20 years of multiwavelength observations of Mrk 421 and Mrk 501
- A Supermassive Binary Black Hole Candidate in Mrk 501