The BATSE Bright Source Reports are available. These indicate the brightest sources as seen by BATSE only, but occasionally include sources for which light curves are not found at this web site.

Even though some screening is performed of the MOPS histories, there is no determination of systematic errors. Single day averages of the source intensity significantly away from the trend of nearby days should be viewed as suspicious. The same is true for apparent 52-day periods that can appear in the data for two or more cycles. The cyclic behavior in some flux histories is caused by the effect of spacecraft orbital precession on the daily flux analysis. Sometimes the behavior can be removed in the archival histories.

1E 1740-29
2S 1417-624
3C 273
4U 0115+634
4U 1145-619
4U 1543-47
4U 1608-522
4U 1630-47
4U 1700-377
A 0535+262
A 1118-616
Aql X-1
Cen A
Cen X-3
Crab Nebula
Cyg X-1
Cyg X-3
GRO J0422+32
GRO J1008-57
GRO J1655-40
GRO J1719-24 = GRS 1716-249
GRO J1744-28
GRO J1944+26
GRO J2058+42
GRS 0834-430
GRS 1009-45
GRS 1915+105
GS 1354-645
GX 1+4
GX 301-2
GX 339-4
GX 354+0
Her X-1
NGC 4151
Nova Muscae = GRS 1124-63
OAO 1657-415
Sco X-1
Vela X-1
XTE J0421+560 = CI Cam
XTE J1550-564
XTE J1748-288
XTE 1859+226

Please return to the BATSE Occultation Page or the BATSE Home Page or the Gamma Ray Astrophysics Home Page.