AGILE detection of a rapid γ-ray flare from the blazar PKS 1510-089 during the GASP-WEBT monitoring

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Table 1:

Observation log and fitting results of *Swift*/XRT observations of PKS 1510-089, with power-law model with $N_{\rm H}$ fixed to Galactic absorption.
Observation	Exposure time	Counts	Flux 0.3-10 keV^a	Photon index	$\chi^{2}_{\rm red}$ (d.o.f.)/C-stat ( $\%$ )^b
date	(s)	(0.2-10 keV)	erg cm^-2 s^-1	$\Gamma$
20-Mar-2008	1961	306	$12.20 _{-1.65}^{+1.65} \times 10^{-12}$	$1.16 \pm 0.16$	0.87 (13)
21-Mar-2008	1966	189	$8.77_{-1.39}^{+1.33} \times 10^{-12}$	$1.53 \pm 0.17$	467 (48.2)^b
22-Mar-2008	1885	261	$9.48 _{-1.14}^{+1.13} \times 10^{-12}$	$1.41 \pm 0.19$	1.34 (11)

^a Unabsorbed flux; ^b cash statistic (C-stat) and percentage of Montecarlo realizations that had statistic < C-stat, performing 10⁴ simulations.

Source LaTeX | All tables | In the text

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