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Swift-XRT products for GRB 150402A — Source 3

RA/Dec (J2000) = 11h 35m 10.62s, +40° 50′ 39.6″ +/- 3.0 (radius, 90%)

Back to list of objects in this field.

This is the probable afterglow because:

Light curve	Spectrum

We expect ~0.00×10⁺⁰ serendipitous objects at least as bright as this source in this tiled dataset, based on the logN-logS distribution of Mateos et al. (2008) [More details]

Source details

Peak XRT count rate	1.5 (±0.9) ×10^-3 ct s^-1
Mean XRT count rate	1.1 (±0.5) ×10^-3 ct s^-1
RASS upper limit	0.04 ct s^-1
Fading?	No