Multiwavelength temporal and spectral study of TeV blazar 1ES 1727+502 during 2014–2021

Author:

Prince Raj1ORCID,Khatoon Rukaiya23,Majumdar Pratik45,Czerny Bożena1,Gupta Nayantara6

Affiliation:

1. Center for Theoretical Physics, Polish Academy of Sciences , Al.Lotnikow 32/46, PL-02-668 Warsaw, Poland

2. Tezpur University , Napaam 784028, Tezpur, India

3. Inter-University Center for Astronomy and Astrophysics , Post Bag 4, Ganeshkhind, Pune 411007, India

4. Saha Institute of Nuclear Physics , HBNI, Kolkata 700064, India

5. Faculty of Physics and Applied Informatics, Department of Astrophysics, University of Lodz , PL-90236 Lodz, Poland

6. Raman Research Institute , Sadashivanagar, Bangalore 560080, India

Abstract

ABSTRACT One of the most important questions in blazar physics is the origin of broad-band emission and fast-flux variation. In this work, we studied the broad-band temporal and spectral properties of a TeV blazar 1ES 1727+502 and explore the one-zone synchrotron self-Compton (SSC) model to fit the broad-band spectral energy distribution (SED). We collected the long-term (2014–2021) multiband data that include both the low- and high-flux states of the source. The entire light curve is divided into three segments of different flux states and the best-fitting parameters obtained by broad-band SED modelling corresponding to three flux states were then compared. The TeV blazar 1ES 1727+502 has been observed to show the brightest flaring episode in the X-ray followed by the optical–UV and γ-rays. The fractional variability estimated during various segments behaves differently in multiple wavebands, suggesting a complex nature of emission in this source. This source has shown a range of variability time from days scale to month scale during this long period of observations between 2014 and 2021. A ‘harder-when-brighter’ trend is not prominent in the X-ray but seen in the optical–UV and an opposite trend is observed in the γ-ray. The complex nature of correlation among various bands is observed. The SED modelling suggests that the one-zone SSC emission model can reproduce the broad-band spectrum in the energy range from optical–UV to very high energy γ-ray.

Funder

National Science Centre

MNiSW

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Broadband Multiwavelength Study of LHAASO-detected Active Galactic Nuclei;The Astrophysical Journal Supplement Series;2024-02-15

2. Probing the disc–jet coupling in S4 0954+65, PKS 0903−57, and 4C +01.02 with γ-rays;Monthly Notices of the Royal Astronomical Society;2023-11-06

3. Multiwavelength study of TeV blazar 1ES 1218+304 using gamma-ray, X-ray and optical observations;Monthly Notices of the Royal Astronomical Society;2023-07-14

4. Gamma-ray flares and broad-band spectral study of PKS 0402-362;Monthly Notices of the Royal Astronomical Society;2023-03-07

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