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Title: A significant hardening and rising shape detected in the MeV/GeV νFν spectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February

Abstract

In this paper, we report on Fermi Large Area Telescope (LAT) and multi-wavelength results on the recently discovered very-high-energy (VHE, E > 100 GeV) blazar S4 0954+65 (z = 0.368) during an exceptionally bright optical flare in 2015 February. During the time period (2015 February 13/14, or MJD 57067) when the MAGIC telescope detected VHE γ-ray emission from the source, the Fermi-LAT data indicated a significant spectral hardening at GeV energies, with a power-law photon index of 1.8 ± 0.1—compared with the 3FGL (The Fermi LAT 4-Year Point Source Catalog) value (averaged over four years of observation) of 2.34 ± 0.04. In contrast, Swift X-Ray Telescope data showed a softening of the X-ray spectrum, with a photon index of 1.72 ± 0.08 (compared with 1.38 ± 0.03 averaged during the flare from MJD 57066 to 57077), possibly indicating a modest contribution of synchrotron photons by the highest-energy electrons superposed on the inverse Compton component. Fitting of the quasi-simultaneous (<1 d) broad-band spectrum with a one-zone synchrotron plus inverse-Compton model revealed that GeV/TeV emission could be produced by inverse-Compton scattering of external photons from the dust torus. Finally, we emphasize that a flaring blazar showing high flux of ≳1.0 × 10-6more » photons cm-2s-1 (E > 100 MeV) and a hard spectral index of ΓGeV < 2.0 detected by Fermi-LAT on daily timescales is a promising target for TeV follow-up by ground-based Cherenkov telescopes to discover high-redshift blazars, investigate their temporal variability and spectral features in the VHE band, and also constrain the intensity of the extragalactic background light.« less

Authors:
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Publication Date:
Research Org.:
Hiroshima Univ., Higashihiroshima (Japan); NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
Sponsoring Org.:
USDOE; National Aeronautics and Space Administration (NASA); Japan Society for the Promotion of Science (JSPS) (Japan)
Contributing Org.:
Fermi LAT Collaboration
OSTI Identifier:
1355691
Grant/Contract Number:  
NNH12ZDA001N; NNH13ZDA001N-FERMI; 15K17652
Resource Type:
Accepted Manuscript
Journal Name:
Publications of the Astronomical Society of Japan
Additional Journal Information:
Journal Volume: 68; Journal Issue: 4; Journal ID: ISSN 0004-6264
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; BL Lacertae objects; active galaxies; galaxies jets; gamma rays; X-rays

Citation Formats

Tanaka, Yasuyuki T., Becerra Gonzalez, Josefa, Itoh, Ryosuke, Finke, Justin D., Inoue, Yoshiyuki, Ojha, Roopesh, Carpenter, Bryce, Lindfors, Elina, Krauß, Felicia, Desiante, Rachele, Shiki, Kensei, Fukazawa, Yasushi, Longo, Francesco, McEnery, Julie E., Buson, Sara, Nilsson, Kari, Fallah Ramazani, Vandad, Reinthal, Riho, Takalo, Leo, Pursimo, Tapio, and Boschin, Walter. A significant hardening and rising shape detected in the MeV/GeV νFν spectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February. United States: N. p., 2016. Web. doi:10.1093/pasj/psw049.
Tanaka, Yasuyuki T., Becerra Gonzalez, Josefa, Itoh, Ryosuke, Finke, Justin D., Inoue, Yoshiyuki, Ojha, Roopesh, Carpenter, Bryce, Lindfors, Elina, Krauß, Felicia, Desiante, Rachele, Shiki, Kensei, Fukazawa, Yasushi, Longo, Francesco, McEnery, Julie E., Buson, Sara, Nilsson, Kari, Fallah Ramazani, Vandad, Reinthal, Riho, Takalo, Leo, Pursimo, Tapio, & Boschin, Walter. A significant hardening and rising shape detected in the MeV/GeV νFν spectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February. United States. https://doi.org/10.1093/pasj/psw049
Tanaka, Yasuyuki T., Becerra Gonzalez, Josefa, Itoh, Ryosuke, Finke, Justin D., Inoue, Yoshiyuki, Ojha, Roopesh, Carpenter, Bryce, Lindfors, Elina, Krauß, Felicia, Desiante, Rachele, Shiki, Kensei, Fukazawa, Yasushi, Longo, Francesco, McEnery, Julie E., Buson, Sara, Nilsson, Kari, Fallah Ramazani, Vandad, Reinthal, Riho, Takalo, Leo, Pursimo, Tapio, and Boschin, Walter. Mon . "A significant hardening and rising shape detected in the MeV/GeV νFν spectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February". United States. https://doi.org/10.1093/pasj/psw049. https://www.osti.gov/servlets/purl/1355691.
@article{osti_1355691,
title = {A significant hardening and rising shape detected in the MeV/GeV νFν spectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 February},
author = {Tanaka, Yasuyuki T. and Becerra Gonzalez, Josefa and Itoh, Ryosuke and Finke, Justin D. and Inoue, Yoshiyuki and Ojha, Roopesh and Carpenter, Bryce and Lindfors, Elina and Krauß, Felicia and Desiante, Rachele and Shiki, Kensei and Fukazawa, Yasushi and Longo, Francesco and McEnery, Julie E. and Buson, Sara and Nilsson, Kari and Fallah Ramazani, Vandad and Reinthal, Riho and Takalo, Leo and Pursimo, Tapio and Boschin, Walter},
abstractNote = {In this paper, we report on Fermi Large Area Telescope (LAT) and multi-wavelength results on the recently discovered very-high-energy (VHE, E > 100 GeV) blazar S4 0954+65 (z = 0.368) during an exceptionally bright optical flare in 2015 February. During the time period (2015 February 13/14, or MJD 57067) when the MAGIC telescope detected VHE γ-ray emission from the source, the Fermi-LAT data indicated a significant spectral hardening at GeV energies, with a power-law photon index of 1.8 ± 0.1—compared with the 3FGL (The Fermi LAT 4-Year Point Source Catalog) value (averaged over four years of observation) of 2.34 ± 0.04. In contrast, Swift X-Ray Telescope data showed a softening of the X-ray spectrum, with a photon index of 1.72 ± 0.08 (compared with 1.38 ± 0.03 averaged during the flare from MJD 57066 to 57077), possibly indicating a modest contribution of synchrotron photons by the highest-energy electrons superposed on the inverse Compton component. Fitting of the quasi-simultaneous (<1 d) broad-band spectrum with a one-zone synchrotron plus inverse-Compton model revealed that GeV/TeV emission could be produced by inverse-Compton scattering of external photons from the dust torus. Finally, we emphasize that a flaring blazar showing high flux of ≳1.0 × 10-6 photons cm-2s-1 (E > 100 MeV) and a hard spectral index of ΓGeV < 2.0 detected by Fermi-LAT on daily timescales is a promising target for TeV follow-up by ground-based Cherenkov telescopes to discover high-redshift blazars, investigate their temporal variability and spectral features in the VHE band, and also constrain the intensity of the extragalactic background light.},
doi = {10.1093/pasj/psw049},
journal = {Publications of the Astronomical Society of Japan},
number = 4,
volume = 68,
place = {United States},
year = {Mon May 23 00:00:00 EDT 2016},
month = {Mon May 23 00:00:00 EDT 2016}
}

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Works referenced in this record:

INSIGHTS INTO THE HIGH-ENERGY γ-RAY EMISSION OF MARKARIAN 501 FROM EXTENSIVE MULTIFREQUENCY OBSERVATIONS IN THE FERMI ERA
journal, January 2011


FERMI LARGE AREA TELESCOPE OBSERVATIONS OF MARKARIAN 421: THE MISSING PIECE OF ITS SPECTRAL ENERGY DISTRIBUTION
journal, July 2011


Gamma-Rays from the Quasar pks 1441+25: Story of an Escape
journal, December 2015


FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG
journal, June 2015

  • Acero, F.; Ackermann, M.; Ajello, M.
  • The Astrophysical Journal Supplement Series, Vol. 218, Issue 2
  • DOI: 10.1088/0067-0049/218/2/23

THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION
journal, October 2012

  • Ackermann, M.; Ajello, M.; Albert, A.
  • The Astrophysical Journal Supplement Series, Vol. 203, Issue 1
  • DOI: 10.1088/0067-0049/203/1/4

The Imprint of the Extragalactic Background Light in the Gamma-Ray Spectra of Blazars
journal, November 2012


Multifrequency Studies of the Peculiar Quasar 4c +21.35 During the 2010 Flaring Activity
journal, April 2014


2FHL: THE SECOND CATALOG OF HARD FERMI -LAT SOURCES
journal, January 2016

  • Ackermann, M.; Ajello, M.; Atwood, W. B.
  • The Astrophysical Journal Supplement Series, Vol. 222, Issue 1
  • DOI: 10.3847/0067-0049/222/1/5

VERY HIGH ENERGY γ -RAYS FROM THE UNIVERSE’S MIDDLE AGE: DETECTION OF THE z = 0.940 BLAZAR PKS 1441+25 WITH MAGIC
journal, December 2015


THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION
journal, May 2009


The Swift X-Ray Telescope
journal, October 2005


The power of blazar jets: The power of blazar jets
journal, February 2008


On the Soft X‐Ray Spectra of γ‐Loud Blazars
journal, May 1997

  • Comastri, Andrea; Fossati, Giovanni; Ghisellini, Gabriele
  • The Astrophysical Journal, Vol. 480, Issue 2
  • DOI: 10.1086/303986

Gamma-Ray Studies of Blazars: Synchro-Compton Analysis of flat Spectrum Radio Quasars
journal, February 2009


Extragalactic background light inferred from AEGIS galaxy-SED-type fractions: EBL from AEGIS galaxy-SED-type fractions
journal, October 2010


Multi-Wavelength Observations of pks 2142–75 During Active and Quiescent Gamma-Ray States
journal, December 2013


Synchrotron Self‐Compton Analysis of TeV X‐Ray‐Selected BL Lacertae Objects
journal, October 2008

  • Finke, Justin D.; Dermer, Charles D.; Böttcher, Markus
  • The Astrophysical Journal, Vol. 686, Issue 1
  • DOI: 10.1086/590900

Modeling the Extragalactic Background Light from Stars and dust
journal, February 2010


The transition between BL Lac objects and flat spectrum radio quasars: FSRQs and BL Lacs
journal, May 2011


General physical properties of bright Fermi blazars: Properties of bright Fermi blazars
journal, November 2009


The power of relativistic jets is larger than the luminosity of their accretion disks
journal, November 2014

  • Ghisellini, G.; Tavecchio, F.; Maraschi, L.
  • Nature, Vol. 515, Issue 7527
  • DOI: 10.1038/nature13856

Extragalactic Background Light from Hierarchical Galaxy Formation: Gamma-Ray Attenuation up to the Epoch of Cosmic Reionization and the First Stars
journal, April 2013

  • Inoue, Yoshiyuki; Inoue, Susumu; Kobayashi, Masakazu A. R.
  • The Astrophysical Journal, Vol. 768, Issue 2
  • DOI: 10.1088/0004-637X/768/2/197

The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
journal, September 2005


FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
journal, February 2009

  • Komatsu, E.; Dunkley, J.; Nolta, M. R.
  • The Astrophysical Journal Supplement Series, Vol. 180, Issue 2
  • DOI: 10.1088/0067-0049/180/2/330

What is the Redshift of the Gamma-Ray bl lac Source s4 0954+65?
journal, November 2015


Optical Spectra of a Complete Sample of Radio Sources. I. The Spectra
journal, November 1996

  • Lawrence, C. R.; Zucker, J. R.; Readhead, A. C. S.
  • The Astrophysical Journal Supplement Series, Vol. 107
  • DOI: 10.1086/192375

Optical spectroscopy and polarization of a new sample of optically bright flat radio spectrum sources
journal, July 1996

  • Marcha, M. J. M.; Browne, I. W. A.; Impey, C. D.
  • Monthly Notices of the Royal Astronomical Society, Vol. 281, Issue 2
  • DOI: 10.1093/mnras/281.2.425

The Likelihood Analysis of EGRET Data
journal, April 1996

  • Mattox, J. R.; Bertsch, D. L.; Chiang, J.
  • The Astrophysical Journal, Vol. 461
  • DOI: 10.1086/177068

EGRET gamma-ray sources: GRO J0744+54 and GRO J0957+65 (= BL Lacertae object 0954+658)
journal, May 1995

  • Mukherjee, R.; Aller, H. D.; Aller, M. F.
  • The Astrophysical Journal, Vol. 445
  • DOI: 10.1086/175685

AGN Dusty Tori. II. Observational Implications of Clumpiness
journal, September 2008

  • Nenkova, Maia; Sirocky, Matthew M.; Nikutta, Robert
  • The Astrophysical Journal, Vol. 685, Issue 1
  • DOI: 10.1086/590483

FERMI LARGE AREA TELESCOPE SECOND SOURCE CATALOG
journal, March 2012

  • Nolan, P. L.; Abdo, A. A.; Ackermann, M.
  • The Astrophysical Journal Supplement Series, Vol. 199, Issue 2
  • DOI: 10.1088/0067-0049/199/2/31

EXPLORING THE BLAZAR ZONE IN HIGH-ENERGY FLARES OF FSRQs
journal, July 2014


Photometric calibration of the Swift ultraviolet/optical telescope: Photometric calibration of the Swift UVOT
journal, December 2007


The Swift Ultra-Violet/Optical Telescope
journal, October 2005

  • Roming, Peter W. A.; Kennedy, Thomas E.; Mason, Keith O.
  • Space Science Reviews, Vol. 120, Issue 3-4
  • DOI: 10.1007/s11214-005-5095-4

Measuring Reddening with Sloan Digital sky Survey Stellar Spectra and Recalibrating sfd
journal, August 2011


Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
journal, June 1998

  • Schlegel, David J.; Finkbeiner, Douglas P.; Davis, Marc
  • The Astrophysical Journal, Vol. 500, Issue 2
  • DOI: 10.1086/305772

On Pair Content and Variability of Subparsec Jets in Quasars
journal, May 2000

  • Sikora, M.; Madejski, G.
  • The Astrophysical Journal, Vol. 534, Issue 1
  • DOI: 10.1086/308756

FERMI LARGE AREA TELESCOPE DETECTION OF BRIGHT γ-RAY OUTBURSTS FROM THE PECULIAR QUASAR 4C +21.35
journal, April 2011


Fermi LARGE AREA TELESCOPE DETECTION OF TWO VERY-HIGH-ENERGY ( E > 100 GeV) γ-RAY PHOTONS FROM THE z = 1.1 BLAZAR PKS 0426–380
journal, October 2013


Unified Schemes for Radio-Loud Active Galactic Nuclei
journal, June 1995

  • Urry, C. Megan; Padovani, Paolo
  • Publications of the Astronomical Society of the Pacific, Vol. 107
  • DOI: 10.1086/133630

Works referencing / citing this record:

Detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state
journal, September 2018


High-energy neutrino flux from individual blazar flares
journal, September 2019

  • Oikonomou, Foteini; Murase, Kohta; Padovani, Paolo
  • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 3
  • DOI: 10.1093/mnras/stz2246

Detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state
text, January 2018

  • Ahnen, M. L.; Ansoldi, S.; Antonelli, L. A.
  • Deutsches Elektronen-Synchrotron, DESY, Hamburg
  • DOI: 10.3204/pubdb-2018-03717

High energy neutrino flux from individual blazar flares
text, January 2019