X-Ray Light Curve of GRO J1744-28 observed with RXTE/PCA on day 154 of 1996
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X-ray light curve of GRO J1744-28 observed with RXTE/PCA.
The source was observed from June 2 12:40 to 16:56, 1996 (UT),
which is almost 3 orbits of XTE.
Bin #0 of X-axis corresponds to June 2 12:39:11, 1996.
Bin width of each data is 16 seconds.
This observation was done with 5 PCU's.
This light curve includes background counts of roughly 1600-2400
counts/bin.
XTE detected eight bursts during the observation of GRO J1744-28,
however it is not clear if all of these bursts are from GRO J1744-28.
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Light curves of some bursts with higher time resolution (1-sec and/or 0.125-sec) are also available.
#1: 2nd burst light curve with 1-sec resolution (Download:
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#2: 4th burst light curve with 1-sec resolution (Download:
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#3: 5th burst light curve with 1-sec resolution (Download:
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#4: 6th burst light curve with 1-sec resolution (Download:
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#5: 6th & 7th bursts light curve with 1-sec resolution (Download:
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#6: 8th burst light curve with 1-sec resolution (Download:
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#7: 5th burst light curve with 0.125-sec resolution (Download:
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#8: 6th burst light curve with 0.125-sec resolution (Download:
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#9: 7th burst light curve with 0.125-sec resolution (Download:
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#10: 8th burst light curve with 0.125-sec resolution (Download:
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Power Spectrum of GRO J1744-28 on day 154 (June 2, 1996)
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Power spectrum of GRO J1744-28 observed with RXTE/PCA
on day 154 (June 2, 1996).
This power spectrum is an ensemble average of 78 spectra,
each of which are calculated from 128 seconds continuous data
in 0.125 second bin. X-axis represents wave number (WN).
Frequency of each WN is given as WN/128 (Hz). Peak at WN=274
(2.14Hz) corresponds to the coherent pulsation.
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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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