| タイトル | Fermi-LAT Detection of Gravitational Lens Delayed Gamma-Ray Flares from Blazar B0218+357 |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150008355 |
| 著者（英） | Chekhtman, A.; Amin, M. A.; Smith, A. W.; Chiang, J.; Thompson, D. J.; Blandford, R. D.; Ciprini, S.; Giroletti, M.; Bulmash, D.; Wood, D. L.; Ajello, M.; Larsson, S.; Cheung, C. C.; Falco, E. E.; Perkins, J. S.; Grove, J. E.; Wood, K. S.; Lott, B.; Ohja, R.; Orienti, M.; Corbet, R. D. H.; Scargle, J. D.; D'Ammando, F.; Bastieri, D.; Razzano, M.; Marshall, P. J. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2014-01-02 |
| 言語 | eng |
| 内容記述 | Using data from the Fermi Large Area Telescope (LAT), we report the first clear gamma-ray measurement of a delay between flares from the gravitationally lensed images of a blazar. The delay was detected in B0218+357, a known double-image lensed system, during a period of enhanced gamma-ray activity with peak fluxes consistently observed to reach greater than 20-50 times its previous average flux. An auto-correlation function analysis identified a delay in the gamma-ray data of 11.46 plus or minus 0.16 days (1 sigma) that is approximately 1 day greater than previous radio measurements. Considering that it is beyond the capabilities of the LAT to spatially resolve the two images, we nevertheless decomposed individual sequences of superposing gamma-ray flares/delayed emissions. In three such approximately 8-10 day-long sequences within an approximately 4-month span, considering confusion due to overlapping flaring emission and flux measurement uncertainties, we found flux ratios consistent with approximately 1, thus systematically smaller than those from radio observations. During the first, best-defined flare, the delayed emission was detailed with a Fermi pointing, and we observed flux doubling timescales of approximately 3-6 hours implying as well extremely compact gamma-ray emitting regions. |
| NASA分類 | Astronomy; Astrophysics |
| レポートNO | GSFC-E-DAA-TN21851 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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