Multiwavelength analysis of Fermi-LAT blazars with high-significance periodicity: detection of a long-term rising emission in PG 1553+113

Author:

Peñil P1,Westernacher-Schneider J R12,Ajello M1,Domínguez A3ORCID,Buson S4,Otero-Santos J567,Marcotulli L8,Torres−Albà N1,Zrake J1ORCID

Affiliation:

1. Department of Physics and Astronomy, Clemson University , Kinard Lab of Physics, Clemson, SC 29634-0978 , USA

2. Leiden Observatory, Leiden University , PO Box 9513, NL-2300 RA Leiden , the Netherlands

3. IPARCOS and Department of EMFTEL, Universidad Complutense de Madrid , E-28040 Madrid , Spain

4. Julius-Maximilians-Universität , Würzburg D-97070 , Germany

5. Instituto de Astrofísica de Canarias (IAC) , E-38200 La Laguna, Tenerife , Spain

6. Universidad de La Laguna (ULL), Departamento de Astrofísica , E-38206 La Laguna, Tenerife , Spain

7. Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n , E-18008 Granada , Spain

8. Department of Physics, Yale University , 52 Hillhouse Avenue, New Haven, CT 06511 , USA

Abstract

ABSTRACT Blazars display variable emission across the entire electromagnetic spectrum, with time-scales that can range from a few minutes to several years. Our recent work has shown that a sample of five blazars exhibit hints of periodicity with a global significance ${\gtrsim}2\, \sigma$ at γ-ray energies, in the range of 0.1 GeV < E < 800 GeV. In this work, we study their multiwavelength emission, covering the X-ray, ultraviolet, optical, and radio bands. We show that three of these blazars present similar periodic patterns in the optical and radio bands. Additionally, fluxes in the different bands of the five blazars are correlated, suggesting a co-spatial origin. Moreover, we detect a long-term (≈10 yr) rising trend in the light curves of PG 1553+113, and we use it to infer possible constraints on the binary black hole hypothesis.

Funder

MEXT

JAXA

Swedish Research Council

MINECO

MICINN

NSF

Gordon and Betty Moore Foundation

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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