TY - ICOMM
T1 - Further observations of GRO J1750-27 (AXJ1749.1-2639) with INTEGRAL
AU - Brandt, S.
AU - Shaw, S.
AU - Hill, A.
AU - Kretschmar, P.
AU - Wijnands, R.
AU - Oosterbroek, T.
AU - Kuulkers, E.
AU - Beckmann, V.
AU - Soldi, S.
AU - Chenevez, J.
AU - Courvoisier, T. J.-L.
AU - Domingo, A.
AU - Ebisawa, K.
AU - Jonker, P.
AU - Markwardt, C.
AU - Paizis, A.
AU - Risquez, D.
AU - Sanchez-Fernandez, C.
PY - 2008/2/28
Y1 - 2008/2/28
N2 - The transient accreting X-ray pulsar GRO J1750-27 (AX J1749.1-2639), which became active end of January 2008 (ATel #1376), has been repeatedly observed by the INTEGRAL Galactic Bulge monitoring program since mid February (ATel #1385) on 11, 20 and 23 Feb. 2008. During the three observations, totalling about 27 ks, the source has remained bright at a roughly constant level with the following flux averaged over the 3 observations: 186+/-9 mCrab (3-10 keV), 319+/-15 mCrab (10-25 keV), 198+/-2 mCrab (18-40 keV), and 20+/-3 mCrab (40-100 keV).
AB - The transient accreting X-ray pulsar GRO J1750-27 (AX J1749.1-2639), which became active end of January 2008 (ATel #1376), has been repeatedly observed by the INTEGRAL Galactic Bulge monitoring program since mid February (ATel #1385) on 11, 20 and 23 Feb. 2008. During the three observations, totalling about 27 ks, the source has remained bright at a roughly constant level with the following flux averaged over the 3 observations: 186+/-9 mCrab (3-10 keV), 319+/-15 mCrab (10-25 keV), 198+/-2 mCrab (18-40 keV), and 20+/-3 mCrab (40-100 keV).
M3 - Net publication - Internet publication
T3 - The Astronomer's telegram
ER -