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Light Curve of GRS 1739-278 on day 131 (May 10, 1996)
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X-ray light curve of GRS 1739-278 observed with RXTE/PCA.
Goodtime of the observation was May 10 07:30-07:55, 1996 (UT).
This light curve covers from 07:36:47 to 07:53:50.
Bin width of each data is 1 second.
Due to the cold temperature problem, observation was performed
with 3 PCU's.
This light curve includes background counts of 60-90 counts/sec.
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PostScript File
Light Curve of GRS 1739-278 on day 133 (May 12, 1996)
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X-ray light curve of GRS 1739-278 observed with RXTE/PCA.
Goodtime of the observation was May 12 03:22-03:42, 1996 (UT).
This light curve covers from 03:21:35 to 03:42:39.
Bin width of each data is 16 seconds.
Due to the cold temperature problem, observation was performed
with 3 PCU's.
This light curve includes background counts of 960-1440 counts/sec.
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Download : Ascii Dump,
GIF file,
PostScript File
Light Curve of GRS 1739-278 on day 134 (May 13, 1996)
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X-ray light curve of GRS 1739-278 observed with RXTE/PCA.
Goodtime of the observation was May 13 17:13 to 17:50, 1996 (UT).
This light curve covers from 17:11:59 to 17:51:59.
Bin width of each data is 16 seconds.
Due to the cold temperature problem, observation was performed
with 3 PCU's.
This light curve includes background counts of 960-1440 counts/sec.
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Download : Ascii Dump,
GIF file,
PostScript File
Light Curve of GRS 1739-278 on day 135 (May 14, 1996)
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X-ray light curve of GRS 1739-278 observed with RXTE/PCA.
Goodtime of the observation was May 14 13:57-14:47, 1996 (UT).
This light curve covers from 13:55:43 to 14:46:54.
Bin width of each data is 1 seconds.
Due to the cold temperature problem, observation was performed
with 3 PCU's.
This light curve includes background counts of 60-90 counts/sec.
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Download : Ascii Dump,
GIF file,
PostScript File
Light Curve of GRS 1739-278 on day 138 (May 14, 1996)
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X-ray light curve of GRS 1739-278 observed with RXTE/PCA.
Goodtime of the observation was May 17 12:23-13:22, 1996 (UT).
This light curve covers from 12:20:15 to 13:24:15.
Bin width of each data is 16 seconds.
Due to the cold temperature problem, observation was performed
with 3 PCU's.
This light curve includes background counts of 960-1440 counts/sec.
A sharp peak at the beginning of the observation is a source detected
during slew to GRS 1739-278.
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Download : Ascii Dump,
GIF file,
PostScript File
For questions about scheduling of RXTE observations please send email to
xteplan@athena.gsfc.nasa.gov
If you have other questions about RXTE, please send email to one of our
help desks.
Responsible NASA Official:
Phil Newman
Web Curator:
Robin Corbet
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