<i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501

We report the results of flux and spectral variability studies of all seven <i>Nuclear Spectroscopic Telescope Array (NuSTAR)</i> observations of TeV <inline-formula><math display="inline"><semantics><mrow><mi>γ</mi><mo>-</mo><...

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Main Author: Ashwani Pandey
Format: Article
Language:English
Published: MDPI AG 2020-07-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/3/55
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author Ashwani Pandey
author_facet Ashwani Pandey
author_sort Ashwani Pandey
collection DOAJ
description We report the results of flux and spectral variability studies of all seven <i>Nuclear Spectroscopic Telescope Array (NuSTAR)</i> observations of TeV <inline-formula><math display="inline"><semantics><mrow><mi>γ</mi><mo>-</mo></mrow></semantics></math></inline-formula>ray emitting blazar Markarian (or Mrk) 501. We found strong evidence of intraday variability in 3–79 keV X-ray light curves (LCs) of Mrk 501 during four out of these seven observations. We examined spectral variability using a model-independent hardness-ratio analysis and found a general “harder-when-brighter” behaviour in two observations. We also investigated the nature of 3–79 keV X-ray spectra of TeV blazar Mrk 501 and found that five out of seven spectra are well described by the curved log-parabola models with photon indices (at 10 keV) <inline-formula><math display="inline"><semantics><mrow><mi>α</mi><mo>∼</mo></mrow></semantics></math></inline-formula> 2.12–2.32 and a curvature <inline-formula><math display="inline"><semantics><mrow><mi>β</mi><mo>∼</mo></mrow></semantics></math></inline-formula> 0.15–0.28. The two other spectra are somewhat better represented by simple power-law models with photon indices 2.70 and 2.75. We briefly discuss available physical models to explain our results.
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spelling doaj.art-5bafe378c0a54ecbbc9b75ff914460f52023-11-20T07:58:39ZengMDPI AGGalaxies2075-44342020-07-01835510.3390/galaxies8030055<i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501Ashwani Pandey0Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263001, IndiaWe report the results of flux and spectral variability studies of all seven <i>Nuclear Spectroscopic Telescope Array (NuSTAR)</i> observations of TeV <inline-formula><math display="inline"><semantics><mrow><mi>γ</mi><mo>-</mo></mrow></semantics></math></inline-formula>ray emitting blazar Markarian (or Mrk) 501. We found strong evidence of intraday variability in 3–79 keV X-ray light curves (LCs) of Mrk 501 during four out of these seven observations. We examined spectral variability using a model-independent hardness-ratio analysis and found a general “harder-when-brighter” behaviour in two observations. We also investigated the nature of 3–79 keV X-ray spectra of TeV blazar Mrk 501 and found that five out of seven spectra are well described by the curved log-parabola models with photon indices (at 10 keV) <inline-formula><math display="inline"><semantics><mrow><mi>α</mi><mo>∼</mo></mrow></semantics></math></inline-formula> 2.12–2.32 and a curvature <inline-formula><math display="inline"><semantics><mrow><mi>β</mi><mo>∼</mo></mrow></semantics></math></inline-formula> 0.15–0.28. The two other spectra are somewhat better represented by simple power-law models with photon indices 2.70 and 2.75. We briefly discuss available physical models to explain our results.https://www.mdpi.com/2075-4434/8/3/55galaxies: activeBL lacertae objects: generalBL lacertae objects: individual (mrk 501)
spellingShingle Ashwani Pandey
<i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
Galaxies
galaxies: active
BL lacertae objects: general
BL lacertae objects: individual (mrk 501)
title <i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
title_full <i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
title_fullStr <i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
title_full_unstemmed <i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
title_short <i><b>NuSTAR</b></i> View of TeV Blazar Mrk 501
title_sort i b nustar b i view of tev blazar mrk 501
topic galaxies: active
BL lacertae objects: general
BL lacertae objects: individual (mrk 501)
url https://www.mdpi.com/2075-4434/8/3/55
work_keys_str_mv AT ashwanipandey ibnustarbiviewoftevblazarmrk501