Corrections to ATel #15927
ATel #15928; T. Maccarone (TTU), U. Kashyap (TTU), C. O. Heinke (U. Alberta), L. E. Rivera Sandoval (UTRGV), A. Bahramian,(Curtin U.), on behalf of SBS team
on 5 Mar 2023; 23:56 UT
Credential Certification: Tom Maccarone (thomas.maccarone@ttu.edu)
Subjects: X-ray, Binary, Neutron Star, Transient
In ATel #15927, we reported count rates and fluxes of sources without giving uncertainties. Three of these were cases where we clearly noted that the sources were severely piled up, and we emphasize that these should be taken as lower limits. Careful analysis of the spectra will be needed to obtain accurate count rates with uncertainties for these observations.
For the observation made on 2023/02/26 for IGR J17445-2747, we reported a count rate of 0.08 cts/sec. Given that this was obtained from 8 counts, with neglible background, this rate is 0.08+-0.03 cts/sec.
