Fermi Large Area Telescope detection of gravitational lens delayed γ-ray flares from Blazar B0218+357
- Naval Research Lab. (NRL), Washington, DC (United States). Space Science Division
- Stockholm Univ. (Sweden). Dept. of Physics and Dept. of Astronomy; Oskar Klein Centre for Cosmoparticle Physics, Stockholm (Sweden)
- NASA Ames Research Center (ARC), Moffett Field, Mountain View, CA (United States). Space Sciences Division
- Univ. of Cambridge (United Kingdom). Kavli Inst. for Cosmology and Inst. for Astronomy
- Stanford Univ. and SLAC National Accelerator Lab., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
- Stanford Univ., CA (United States). Dept. of Physics
- Agenzia Spaziale Italiana (ASI) Science Data Center, Rome (Italy); National Inst. of Astrophysics- Astronomical Observatory of Rome (Italy)
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD (United States); Univ. of Maryland Baltimore County (UMBC), Baltimore, MD (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Stanford Univ. and SLAC National Accelerator Lab., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Oxford Univ. (United Kingdom). Dept. of Physics
- Praxis Inc., Alexandria, VA (United States)
- Univ. of California, Berkeley, CA (United States). Space Sciences Lab.
- National Inst. of Nuclear Physics, Padova (Italy); Univ. of Padova (Italy). Dept. of Physics and Astronomy
- George Mason Univ., Fairfax, VA (United States). Center for Earth Observing and Space Research
- National Inst. for Astrophysics (INAF), Bologna (Italy). Inst. for Radio Astronomy
- Univ. of Bordeaux (France). Gradignan Bordeaux Center for Nuclear Research
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- National Inst. of Nuclear Physics, Pisa (Italy)
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
We report the first clear γ-ray measurement of a delay between flares from the gravitationally lensed images of a blazar, using data from the Fermi Large Area Telescope (LAT). We detected a delay in B0218+357, a known double-image lensed system, during a period of enhanced γ-ray activity with peak fluxes consistently observed to reach >20-50 × its previous average flux. An auto-correlation function analysis identified a delay in the γ-ray data of 11.46 ± 0.16 days (1σ) that is ~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 γ-ray flares/delayed emissions. In three such ~8-10 day-long sequences within a ~4 month span, considering confusion due to overlapping flaring emission and flux measurement uncertainties, we found flux ratios consistent with ~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 ~3-6 hr implying as well extremely compact γ-ray emitting regions.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Contributing Organization:
- Fermi LAT Collaboration
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1356535
- Journal Information:
- The Astrophysical Journal. Letters, Vol. 782, Issue 2; ISSN 2041-8205
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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