First evidence of a gravitational lensing-induced echo in gamma rays with Fermi LAT

被引:32
作者
Barnacka, A. [1 ,2 ]
Glicenstein, J. -F. [1 ]
Moudden, Y. [1 ]
机构
[1] CEA Saclay, DSM IRFU, F-91191 Gif Sur Yvette, France
[2] Nicolaus Copernicus Astron Ctr, Warsaw, Poland
关键词
gravitational lensing: strong; quasars: individual: PKS 1830-211; methods: data analysis; ALL-SKY SURVEY; RADIO-SOURCE; TIME-DELAY; EINSTEIN RING; PKS1830-211; SELECTION; REDSHIFT;
D O I
10.1051/0004-6361/201016175
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. This article shows the first evidence ever of gravitational lensing phenomena in high energy gamma-rays. This evidence comes from the observation of an echo in the light curve of the distant blazar PKS 1830-211 induced by a gravitational lens system. Methods. Traditional methods for estimating time delays in gravitational lensing systems rely on the cross-correlation of the light curves from individual images. We used the 300 MeV-30 GeV photons detected by the Fermi-LAT instrument. It cannot separate the images of known lenses, so the observed light curve is the superposition of individual image light curves. The Fermi-LAT instrument has the advantage of providing long, evenly spaced, time series with very low photon noise. This allows us to use Fourier transform methods directly. Results. A time delay between the two compact images of PKS 1830-211 has been searched for by both the autocorrelation method and the "double power spectrum" method. The double power spectrum shows a 4.2 sigma proof of a time delay of 27.1 +/- 0.6 days, consistent with others' results.
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