TY - JOUR
T1 - FERMI-LAT OBSERVATIONS of the 2014 MAY-July OUTBURST from 3C 454.3
AU - Britto, Richard J.
AU - Bottacini, Eugenio
AU - Lott, Benoît
AU - Razzaque, Soebur
AU - Buson, Sara
N1 - Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved.
PY - 2016/10/20
Y1 - 2016/10/20
N2 - A prominent outburst of the flat spectrum radio quasar 3C 454.3 was observed in 2014 June with the Fermi Large Area Telescope. This outburst was characterized by a three-stage light-curve pattern - plateau, flare, and post-flare - that occurred from 2014 May to July, in a similar pattern as observed during the exceptional outburst in 2010 November. The highest flux of the outburst reported in this paper occurred during 2014 June 7-29, showing a multiple-peak structure in the light-curves. The average flux in these 22 days was found to be F [E > 100 MeV] = (7.2 ± 0.2) × 10-6 ph cm-2 s-1, with a spectral index, for a simple power law, of Γ = 2.04 ± 0.01. That made this outburst the first γ-ray high state of 3C 454.3 ever to be detected by Fermi with such a hard spectrum over several days. The highest flux was recorded on 2014 June 15, in a 3 hr bin, at MJD 56823.5625, at a level of F [E > 100 MeV] = (17.6 ± 1.9) × 10-6 ph cm-2 s-1. The rise time of one of the short subflares was found to be Tr = 1200 ± 700 s at MJD = 56827, when the flux increased from 4 to 12 × 10-6 ph cm-2 s-1. Several photons above 20 GeV were collected during this outburst, including one at 45 GeV on MJD 56827, constraining the γ-ray emission region to be located close to the outer boundary of the broad-line region, leading to fast flux variability.
AB - A prominent outburst of the flat spectrum radio quasar 3C 454.3 was observed in 2014 June with the Fermi Large Area Telescope. This outburst was characterized by a three-stage light-curve pattern - plateau, flare, and post-flare - that occurred from 2014 May to July, in a similar pattern as observed during the exceptional outburst in 2010 November. The highest flux of the outburst reported in this paper occurred during 2014 June 7-29, showing a multiple-peak structure in the light-curves. The average flux in these 22 days was found to be F [E > 100 MeV] = (7.2 ± 0.2) × 10-6 ph cm-2 s-1, with a spectral index, for a simple power law, of Γ = 2.04 ± 0.01. That made this outburst the first γ-ray high state of 3C 454.3 ever to be detected by Fermi with such a hard spectrum over several days. The highest flux was recorded on 2014 June 15, in a 3 hr bin, at MJD 56823.5625, at a level of F [E > 100 MeV] = (17.6 ± 1.9) × 10-6 ph cm-2 s-1. The rise time of one of the short subflares was found to be Tr = 1200 ± 700 s at MJD = 56827, when the flux increased from 4 to 12 × 10-6 ph cm-2 s-1. Several photons above 20 GeV were collected during this outburst, including one at 45 GeV on MJD 56827, constraining the γ-ray emission region to be located close to the outer boundary of the broad-line region, leading to fast flux variability.
KW - galaxies: active
KW - gamma rays: galaxies
KW - quasars: individual (3C 454.3)
UR - http://www.scopus.com/inward/record.url?scp=84992692370&partnerID=8YFLogxK
U2 - 10.3847/0004-637X/830/2/162
DO - 10.3847/0004-637X/830/2/162
M3 - Article
AN - SCOPUS:84992692370
SN - 0004-637X
VL - 830
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 162
ER -