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The Bright gamma-ray Flare of 3C 279 in 2015 June : AGILE Detection and Multifrequency Follow-up Observations. / Pittori, C.; Lucarelli, F.; Verrecchia, F.; Raiteri, C. M.; Villata, M.; Vittorini, V.; Tavani, M.; Puccetti, S.; Perri, M.; Donnarumma, I.; Vercellone, S.; Acosta-Pulido, J. A.; Bachev, R.; Benitez, E.; Borman, G. A.; Carnerero, M. I.; Carosati, D.; Chen, W. P.; Ehgamberdiev, Sh. A.; Goded, A.; Grishina, T. S.; Hiriart, D.; Hsiao, H. Y.; Jorstad, S. G.; Kimeridze, G. N.; Kopatskaya, E. N.; Kurtanidze, O. M.; Kurtanidze, S. O.; Larionov, V. M.; Larionova, L. V.; Marscher, A. P.; Mirzaqulov, D. O.; Morozova, D. A.; Nilsson, K.; Samal, M. R.; Sigua, L. A.; Spassov, B.; Strigachev, A.; Takalo, L. O.; Antonelli, L. A.; Bulgarelli, A.; Cattaneo, P.; Colafrancesco, S.; Giommi, P.; Longo, F.; Morselli, A.; Paoletti, F.

In: Astrophysical Journal, Vol. 856, No. 2, 99, 01.04.2018.

Research output: Contribution to journalArticlepeer-review

Harvard

Pittori, C, Lucarelli, F, Verrecchia, F, Raiteri, CM, Villata, M, Vittorini, V, Tavani, M, Puccetti, S, Perri, M, Donnarumma, I, Vercellone, S, Acosta-Pulido, JA, Bachev, R, Benitez, E, Borman, GA, Carnerero, MI, Carosati, D, Chen, WP, Ehgamberdiev, SA, Goded, A, Grishina, TS, Hiriart, D, Hsiao, HY, Jorstad, SG, Kimeridze, GN, Kopatskaya, EN, Kurtanidze, OM, Kurtanidze, SO, Larionov, VM, Larionova, LV, Marscher, AP, Mirzaqulov, DO, Morozova, DA, Nilsson, K, Samal, MR, Sigua, LA, Spassov, B, Strigachev, A, Takalo, LO, Antonelli, LA, Bulgarelli, A, Cattaneo, P, Colafrancesco, S, Giommi, P, Longo, F, Morselli, A & Paoletti, F 2018, 'The Bright gamma-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations', Astrophysical Journal, vol. 856, no. 2, 99. https://doi.org/10.3847/1538-4357/aab1f9

APA

Pittori, C., Lucarelli, F., Verrecchia, F., Raiteri, C. M., Villata, M., Vittorini, V., Tavani, M., Puccetti, S., Perri, M., Donnarumma, I., Vercellone, S., Acosta-Pulido, J. A., Bachev, R., Benitez, E., Borman, G. A., Carnerero, M. I., Carosati, D., Chen, W. P., Ehgamberdiev, S. A., ... Paoletti, F. (2018). The Bright gamma-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations. Astrophysical Journal, 856(2), [99]. https://doi.org/10.3847/1538-4357/aab1f9

Vancouver

Pittori C, Lucarelli F, Verrecchia F, Raiteri CM, Villata M, Vittorini V et al. The Bright gamma-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations. Astrophysical Journal. 2018 Apr 1;856(2). 99. https://doi.org/10.3847/1538-4357/aab1f9

Author

Pittori, C. ; Lucarelli, F. ; Verrecchia, F. ; Raiteri, C. M. ; Villata, M. ; Vittorini, V. ; Tavani, M. ; Puccetti, S. ; Perri, M. ; Donnarumma, I. ; Vercellone, S. ; Acosta-Pulido, J. A. ; Bachev, R. ; Benitez, E. ; Borman, G. A. ; Carnerero, M. I. ; Carosati, D. ; Chen, W. P. ; Ehgamberdiev, Sh. A. ; Goded, A. ; Grishina, T. S. ; Hiriart, D. ; Hsiao, H. Y. ; Jorstad, S. G. ; Kimeridze, G. N. ; Kopatskaya, E. N. ; Kurtanidze, O. M. ; Kurtanidze, S. O. ; Larionov, V. M. ; Larionova, L. V. ; Marscher, A. P. ; Mirzaqulov, D. O. ; Morozova, D. A. ; Nilsson, K. ; Samal, M. R. ; Sigua, L. A. ; Spassov, B. ; Strigachev, A. ; Takalo, L. O. ; Antonelli, L. A. ; Bulgarelli, A. ; Cattaneo, P. ; Colafrancesco, S. ; Giommi, P. ; Longo, F. ; Morselli, A. ; Paoletti, F. / The Bright gamma-ray Flare of 3C 279 in 2015 June : AGILE Detection and Multifrequency Follow-up Observations. In: Astrophysical Journal. 2018 ; Vol. 856, No. 2.

BibTeX

@article{34b45c7cace448328e92c1d9159328b6,
title = "The Bright gamma-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations",
abstract = "We report the AGILE detection and the results of the multifrequency follow-up observations of a bright.-ray flare of the blazar 3C 279 in 2015 June. We use AGILE and Fermi gamma-ray data, together with Swift X-ray andoptical-ultraviolet data, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the.-ray flare. The.-ray flaring data, compared with as yet unpublished simultaneous optical data that will allow constraints on the big blue bump disk luminosity, show very high Compton dominance values of similar to 100, with the ratio of.-ray to optical emission rising by a factor of three in a few hours. The multiwavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the 2015 June flare are also compared with already published data and nonsimultaneous historical 3C 279 archival data.",
keywords = "galaxies: active, gamma rays: galaxies, polarization, quasars: individual (3C 279), radiation mechanisms: non-thermal, X-rays: general, BLAZARS, WEBT, TELESCOPE, RADIATION, EMISSION, 3C-279, VARIABILITY, CAMPAIGN, QUASARS, MISSION",
author = "C. Pittori and F. Lucarelli and F. Verrecchia and Raiteri, {C. M.} and M. Villata and V. Vittorini and M. Tavani and S. Puccetti and M. Perri and I. Donnarumma and S. Vercellone and Acosta-Pulido, {J. A.} and R. Bachev and E. Benitez and Borman, {G. A.} and Carnerero, {M. I.} and D. Carosati and Chen, {W. P.} and Ehgamberdiev, {Sh. A.} and A. Goded and Grishina, {T. S.} and D. Hiriart and Hsiao, {H. Y.} and Jorstad, {S. G.} and Kimeridze, {G. N.} and Kopatskaya, {E. N.} and Kurtanidze, {O. M.} and Kurtanidze, {S. O.} and Larionov, {V. M.} and Larionova, {L. V.} and Marscher, {A. P.} and Mirzaqulov, {D. O.} and Morozova, {D. A.} and K. Nilsson and Samal, {M. R.} and Sigua, {L. A.} and B. Spassov and A. Strigachev and Takalo, {L. O.} and Antonelli, {L. A.} and A. Bulgarelli and P. Cattaneo and S. Colafrancesco and P. Giommi and F. Longo and A. Morselli and F. Paoletti",
year = "2018",
month = apr,
day = "1",
doi = "10.3847/1538-4357/aab1f9",
language = "Английский",
volume = "856",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "2",

}

RIS

TY - JOUR

T1 - The Bright gamma-ray Flare of 3C 279 in 2015 June

T2 - AGILE Detection and Multifrequency Follow-up Observations

AU - Pittori, C.

AU - Lucarelli, F.

AU - Verrecchia, F.

AU - Raiteri, C. M.

AU - Villata, M.

AU - Vittorini, V.

AU - Tavani, M.

AU - Puccetti, S.

AU - Perri, M.

AU - Donnarumma, I.

AU - Vercellone, S.

AU - Acosta-Pulido, J. A.

AU - Bachev, R.

AU - Benitez, E.

AU - Borman, G. A.

AU - Carnerero, M. I.

AU - Carosati, D.

AU - Chen, W. P.

AU - Ehgamberdiev, Sh. A.

AU - Goded, A.

AU - Grishina, T. S.

AU - Hiriart, D.

AU - Hsiao, H. Y.

AU - Jorstad, S. G.

AU - Kimeridze, G. N.

AU - Kopatskaya, E. N.

AU - Kurtanidze, O. M.

AU - Kurtanidze, S. O.

AU - Larionov, V. M.

AU - Larionova, L. V.

AU - Marscher, A. P.

AU - Mirzaqulov, D. O.

AU - Morozova, D. A.

AU - Nilsson, K.

AU - Samal, M. R.

AU - Sigua, L. A.

AU - Spassov, B.

AU - Strigachev, A.

AU - Takalo, L. O.

AU - Antonelli, L. A.

AU - Bulgarelli, A.

AU - Cattaneo, P.

AU - Colafrancesco, S.

AU - Giommi, P.

AU - Longo, F.

AU - Morselli, A.

AU - Paoletti, F.

PY - 2018/4/1

Y1 - 2018/4/1

N2 - We report the AGILE detection and the results of the multifrequency follow-up observations of a bright.-ray flare of the blazar 3C 279 in 2015 June. We use AGILE and Fermi gamma-ray data, together with Swift X-ray andoptical-ultraviolet data, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the.-ray flare. The.-ray flaring data, compared with as yet unpublished simultaneous optical data that will allow constraints on the big blue bump disk luminosity, show very high Compton dominance values of similar to 100, with the ratio of.-ray to optical emission rising by a factor of three in a few hours. The multiwavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the 2015 June flare are also compared with already published data and nonsimultaneous historical 3C 279 archival data.

AB - We report the AGILE detection and the results of the multifrequency follow-up observations of a bright.-ray flare of the blazar 3C 279 in 2015 June. We use AGILE and Fermi gamma-ray data, together with Swift X-ray andoptical-ultraviolet data, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the.-ray flare. The.-ray flaring data, compared with as yet unpublished simultaneous optical data that will allow constraints on the big blue bump disk luminosity, show very high Compton dominance values of similar to 100, with the ratio of.-ray to optical emission rising by a factor of three in a few hours. The multiwavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the 2015 June flare are also compared with already published data and nonsimultaneous historical 3C 279 archival data.

KW - galaxies: active

KW - gamma rays: galaxies

KW - polarization

KW - quasars: individual (3C 279)

KW - radiation mechanisms: non-thermal

KW - X-rays: general

KW - BLAZARS

KW - WEBT

KW - TELESCOPE

KW - RADIATION

KW - EMISSION

KW - 3C-279

KW - VARIABILITY

KW - CAMPAIGN

KW - QUASARS

KW - MISSION

UR - http://www.scopus.com/inward/record.url?scp=85045547537&partnerID=8YFLogxK

UR - http://arxiv.org/abs/1803.07529

UR - http://www.mendeley.com/research/bright-gammaray-flare-3c-279-june-2015-agile-detection-multifrequency-followup-observations

U2 - 10.3847/1538-4357/aab1f9

DO - 10.3847/1538-4357/aab1f9

M3 - статья

VL - 856

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 99

ER -

ID: 26389448