AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst

S. Vercellone, P. Romano, G. Piano, V. Vittorini, I. Donnarumma, P. Munar-Adrover, C. M. Raiteri, M. Villata, F. Verrecchia, F. Lucarelli, C. Pittori, A. Bulgarelli, V. Fioretti, M. Tavani, J. A. Acosta-Pulido, I. Agudo, A. A. Arkharov, U. Bach, R. Bachev, G. A. BormanM. S. Butuzova, M. I. Carnerero, C. Casadio, G. Damljanovic, F. D'Ammando, A. Di Paola, V. T. Doroshenko, N. V. Efimova, Sh. A. Ehgamberdiev, M. Giroletti, J. L. Gomez, T. S. Grishina, E. Jarvela, S. A. Klimanov, E. N. Kopatskaya, O. M. Kurtanidze, A. Lahteenmaki, V. M. Larionov, L. V. Larionova, B. Mihov, D. O. Mirzaqulov, S. N. Molina, D. A. Morozova, S. V. Nazarov, M. Orienti, S. Righini, S. S. Savchenko, E. Semkov, L. Slavcheva-Mihova, A. Strigachev, M. Tornikoski, Yu. V. Troitskaya, O. Vince, P. W. Cattaneo, S. Colafrancesco, F. Longo, A. Morselli, F. Paoletti, N. Parmiggiani

Результат исследований: Научные публикации в периодических изданияхстатья

3 Цитирования (Scopus)

Выдержка

Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), gamma-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc.

Aims. 4C +71.07 has been detected in outburst twice by the AGILE gamma-ray satellite during the period from the end of October to mid-November 2015, when it reached a gamma-ray flux of the order of F(E > 100 MeV) = (1.2 +/- 0.3) x 10(-6) photons cm (2) s(-1) and F(E > 100 MeV) = (3.1 +/- 0.6) x 10(-6) photons cm(-2) s(-1), respectively, allowing us to investigate the properties of the jet and the emission region.

Methods. We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and gamma-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites.

Results. The spectral energy distribution of the second gamma-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 x 10(47) erg s(-1).

Conclusions. During the most prominent gamma-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future gamma-ray satellites such as e-ASTROGAM.

Язык оригиналаАнглийский
Номер статьиA82
Число страниц8
ЖурналASTRONOMY & ASTROPHYSICS
Том621
DOI
СостояниеОпубликовано - 1 янв 2019

Предметные области Scopus

  • Астрономия и астрофизика
  • Космические науки и планетоведение

Цитировать

Vercellone, S. ; Romano, P. ; Piano, G. ; Vittorini, V. ; Donnarumma, I. ; Munar-Adrover, P. ; Raiteri, C. M. ; Villata, M. ; Verrecchia, F. ; Lucarelli, F. ; Pittori, C. ; Bulgarelli, A. ; Fioretti, V. ; Tavani, M. ; Acosta-Pulido, J. A. ; Agudo, I. ; Arkharov, A. A. ; Bach, U. ; Bachev, R. ; Borman, G. A. ; Butuzova, M. S. ; Carnerero, M. I. ; Casadio, C. ; Damljanovic, G. ; D'Ammando, F. ; Di Paola, A. ; Doroshenko, V. T. ; Efimova, N. V. ; Ehgamberdiev, Sh. A. ; Giroletti, M. ; Gomez, J. L. ; Grishina, T. S. ; Jarvela, E. ; Klimanov, S. A. ; Kopatskaya, E. N. ; Kurtanidze, O. M. ; Lahteenmaki, A. ; Larionov, V. M. ; Larionova, L. V. ; Mihov, B. ; Mirzaqulov, D. O. ; Molina, S. N. ; Morozova, D. A. ; Nazarov, S. V. ; Orienti, M. ; Righini, S. ; Savchenko, S. S. ; Semkov, E. ; Slavcheva-Mihova, L. ; Strigachev, A. ; Tornikoski, M. ; Troitskaya, Yu. V. ; Vince, O. ; Cattaneo, P. W. ; Colafrancesco, S. ; Longo, F. ; Morselli, A. ; Paoletti, F. ; Parmiggiani, N. / AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst. В: ASTRONOMY & ASTROPHYSICS. 2019 ; Том 621.
@article{736c7a5c00be49e5a088dec94f3269a5,
title = "AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst",
abstract = "Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), gamma-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc.Aims. 4C +71.07 has been detected in outburst twice by the AGILE gamma-ray satellite during the period from the end of October to mid-November 2015, when it reached a gamma-ray flux of the order of F(E > 100 MeV) = (1.2 +/- 0.3) x 10(-6) photons cm (2) s(-1) and F(E > 100 MeV) = (3.1 +/- 0.6) x 10(-6) photons cm(-2) s(-1), respectively, allowing us to investigate the properties of the jet and the emission region.Methods. We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and gamma-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites.Results. The spectral energy distribution of the second gamma-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 x 10(47) erg s(-1).Conclusions. During the most prominent gamma-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future gamma-ray satellites such as e-ASTROGAM.",
keywords = "acceleration of particles, radiation mechanisms: non-thermal, relativistic processes, quasars: supermassive black holes, quasars: individual: 4C+71.07, gamma rays: galaxies, PHOTON IMAGING CAMERA, GAMMA-RAY FLARE, XMM-NEWTON, FIELDS, POWER, Quasars: Supermassive black holes, Quasars: Individual: 4C +71.07, Relativistic processes, Radiation mechanisms: non-thermal, Gamma rays: Galaxies, Acceleration of particles",
author = "S. Vercellone and P. Romano and G. Piano and V. Vittorini and I. Donnarumma and P. Munar-Adrover and Raiteri, {C. M.} and M. Villata and F. Verrecchia and F. Lucarelli and C. Pittori and A. Bulgarelli and V. Fioretti and M. Tavani and Acosta-Pulido, {J. A.} and I. Agudo and Arkharov, {A. A.} and U. Bach and R. Bachev and Borman, {G. A.} and Butuzova, {M. S.} and Carnerero, {M. I.} and C. Casadio and G. Damljanovic and F. D'Ammando and {Di Paola}, A. and Doroshenko, {V. T.} and Efimova, {N. V.} and Ehgamberdiev, {Sh. A.} and M. Giroletti and Gomez, {J. L.} and Grishina, {T. S.} and E. Jarvela and Klimanov, {S. A.} and Kopatskaya, {E. N.} and Kurtanidze, {O. M.} and A. Lahteenmaki and Larionov, {V. M.} and Larionova, {L. V.} and B. Mihov and Mirzaqulov, {D. O.} and Molina, {S. N.} and Morozova, {D. A.} and Nazarov, {S. V.} and M. Orienti and S. Righini and Savchenko, {S. S.} and E. Semkov and L. Slavcheva-Mihova and A. Strigachev and M. Tornikoski and Troitskaya, {Yu. V.} and O. Vince and Cattaneo, {P. W.} and S. Colafrancesco and F. Longo and A. Morselli and F. Paoletti and N. Parmiggiani",
year = "2019",
month = "1",
day = "1",
doi = "10.1051/0004-6361/201732532",
language = "Английский",
volume = "621",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",

}

Vercellone, S, Romano, P, Piano, G, Vittorini, V, Donnarumma, I, Munar-Adrover, P, Raiteri, CM, Villata, M, Verrecchia, F, Lucarelli, F, Pittori, C, Bulgarelli, A, Fioretti, V, Tavani, M, Acosta-Pulido, JA, Agudo, I, Arkharov, AA, Bach, U, Bachev, R, Borman, GA, Butuzova, MS, Carnerero, MI, Casadio, C, Damljanovic, G, D'Ammando, F, Di Paola, A, Doroshenko, VT, Efimova, NV, Ehgamberdiev, SA, Giroletti, M, Gomez, JL, Grishina, TS, Jarvela, E, Klimanov, SA, Kopatskaya, EN, Kurtanidze, OM, Lahteenmaki, A, Larionov, VM, Larionova, LV, Mihov, B, Mirzaqulov, DO, Molina, SN, Morozova, DA, Nazarov, SV, Orienti, M, Righini, S, Savchenko, SS, Semkov, E, Slavcheva-Mihova, L, Strigachev, A, Tornikoski, M, Troitskaya, YV, Vince, O, Cattaneo, PW, Colafrancesco, S, Longo, F, Morselli, A, Paoletti, F & Parmiggiani, N 2019, 'AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst', ASTRONOMY & ASTROPHYSICS, том. 621, A82. https://doi.org/10.1051/0004-6361/201732532, https://doi.org/10.1051/0004-6361/201732532

AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst. / Vercellone, S.; Romano, P.; Piano, G.; Vittorini, V.; Donnarumma, I.; Munar-Adrover, P.; Raiteri, C. M.; Villata, M.; Verrecchia, F.; Lucarelli, F.; Pittori, C.; Bulgarelli, A.; Fioretti, V.; Tavani, M.; Acosta-Pulido, J. A.; Agudo, I.; Arkharov, A. A.; Bach, U.; Bachev, R.; Borman, G. A.; Butuzova, M. S.; Carnerero, M. I.; Casadio, C.; Damljanovic, G.; D'Ammando, F.; Di Paola, A.; Doroshenko, V. T.; Efimova, N. V.; Ehgamberdiev, Sh. A.; Giroletti, M.; Gomez, J. L.; Grishina, T. S.; Jarvela, E.; Klimanov, S. A.; Kopatskaya, E. N.; Kurtanidze, O. M.; Lahteenmaki, A.; Larionov, V. M.; Larionova, L. V.; Mihov, B.; Mirzaqulov, D. O.; Molina, S. N.; Morozova, D. A.; Nazarov, S. V.; Orienti, M.; Righini, S.; Savchenko, S. S.; Semkov, E.; Slavcheva-Mihova, L.; Strigachev, A.; Tornikoski, M.; Troitskaya, Yu. V.; Vince, O.; Cattaneo, P. W.; Colafrancesco, S.; Longo, F.; Morselli, A.; Paoletti, F.; Parmiggiani, N.

В: ASTRONOMY & ASTROPHYSICS, Том 621, A82, 01.01.2019.

Результат исследований: Научные публикации в периодических изданияхстатья

TY - JOUR

T1 - AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C+71.07 in outburst

AU - Vercellone, S.

AU - Romano, P.

AU - Piano, G.

AU - Vittorini, V.

AU - Donnarumma, I.

AU - Munar-Adrover, P.

AU - Raiteri, C. M.

AU - Villata, M.

AU - Verrecchia, F.

AU - Lucarelli, F.

AU - Pittori, C.

AU - Bulgarelli, A.

AU - Fioretti, V.

AU - Tavani, M.

AU - Acosta-Pulido, J. A.

AU - Agudo, I.

AU - Arkharov, A. A.

AU - Bach, U.

AU - Bachev, R.

AU - Borman, G. A.

AU - Butuzova, M. S.

AU - Carnerero, M. I.

AU - Casadio, C.

AU - Damljanovic, G.

AU - D'Ammando, F.

AU - Di Paola, A.

AU - Doroshenko, V. T.

AU - Efimova, N. V.

AU - Ehgamberdiev, Sh. A.

AU - Giroletti, M.

AU - Gomez, J. L.

AU - Grishina, T. S.

AU - Jarvela, E.

AU - Klimanov, S. A.

AU - Kopatskaya, E. N.

AU - Kurtanidze, O. M.

AU - Lahteenmaki, A.

AU - Larionov, V. M.

AU - Larionova, L. V.

AU - Mihov, B.

AU - Mirzaqulov, D. O.

AU - Molina, S. N.

AU - Morozova, D. A.

AU - Nazarov, S. V.

AU - Orienti, M.

AU - Righini, S.

AU - Savchenko, S. S.

AU - Semkov, E.

AU - Slavcheva-Mihova, L.

AU - Strigachev, A.

AU - Tornikoski, M.

AU - Troitskaya, Yu. V.

AU - Vince, O.

AU - Cattaneo, P. W.

AU - Colafrancesco, S.

AU - Longo, F.

AU - Morselli, A.

AU - Paoletti, F.

AU - Parmiggiani, N.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), gamma-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc.Aims. 4C +71.07 has been detected in outburst twice by the AGILE gamma-ray satellite during the period from the end of October to mid-November 2015, when it reached a gamma-ray flux of the order of F(E > 100 MeV) = (1.2 +/- 0.3) x 10(-6) photons cm (2) s(-1) and F(E > 100 MeV) = (3.1 +/- 0.6) x 10(-6) photons cm(-2) s(-1), respectively, allowing us to investigate the properties of the jet and the emission region.Methods. We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and gamma-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites.Results. The spectral energy distribution of the second gamma-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 x 10(47) erg s(-1).Conclusions. During the most prominent gamma-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future gamma-ray satellites such as e-ASTROGAM.

AB - Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), gamma-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc.Aims. 4C +71.07 has been detected in outburst twice by the AGILE gamma-ray satellite during the period from the end of October to mid-November 2015, when it reached a gamma-ray flux of the order of F(E > 100 MeV) = (1.2 +/- 0.3) x 10(-6) photons cm (2) s(-1) and F(E > 100 MeV) = (3.1 +/- 0.6) x 10(-6) photons cm(-2) s(-1), respectively, allowing us to investigate the properties of the jet and the emission region.Methods. We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and gamma-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites.Results. The spectral energy distribution of the second gamma-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 x 10(47) erg s(-1).Conclusions. During the most prominent gamma-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future gamma-ray satellites such as e-ASTROGAM.

KW - acceleration of particles

KW - radiation mechanisms: non-thermal

KW - relativistic processes

KW - quasars: supermassive black holes

KW - quasars: individual: 4C+71.07

KW - gamma rays: galaxies

KW - PHOTON IMAGING CAMERA

KW - GAMMA-RAY FLARE

KW - XMM-NEWTON

KW - FIELDS

KW - POWER

KW - Quasars: Supermassive black holes

KW - Quasars: Individual: 4C +71.07

KW - Relativistic processes

KW - Radiation mechanisms: non-thermal

KW - Gamma rays: Galaxies

KW - Acceleration of particles

UR - http://www.scopus.com/inward/record.url?scp=85060380182&partnerID=8YFLogxK

UR - https://www.aanda.org/10.1051/0004-6361/201732532

UR - http://www.mendeley.com/research/agile-ifermii-iswifti-gaspwebt-multiwavelength-observations-highredshift-blazar-4c-7107-outburst

U2 - 10.1051/0004-6361/201732532

DO - 10.1051/0004-6361/201732532

M3 - статья

VL - 621

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

M1 - A82

ER -