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ATel #15430; Sean N. Pike (Caltech), Amruta Jaodand (Caltech), R. M. Ludlam (Caltech), John A. Tomsick (SSL/UC Berkeley) on 10 Jun 2022; 06:32 UTCredential Certification: Sean Pike (spike@caltech.edu)
Subjects: X-ray, Neutron Star, Transient
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We would like to clarify that the bolometric flux of (6.5+/-0.5)x10^-9 erg/s/cm^2 which we reported for 1A 1744-361 in Atel #15429 corresponds to the unabsorbed flux.
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