RXTE Helpdesk/FAQ RXTE What's New HEASARC Site Map


RXTE TOO observations of GRS 1915+105 on day 152 of 1996

Light Curve of GRS 1915+105 on day 152 (May 31)

GRS1915_d152_16s_lc image: X-ray light curve of GRS 1915+105 observed with RXTE/PCA. Bin width of each data is 16 second.
X-ray light curve of GRS 1915+105 observed with RXTE/PCA. Observation was done from May 31 11:25 to 16:55, 1996 (UT). Bin width of each data is 16 second and the bin #0 and #880 of X-axis correspond to May 31 11:20:31 and 15:15:11, respectively. This light curve includes background counts of 1600-2400 counts/bin.
Download : Ascii Dump, GIF file, PostScript File


Light Curve of GRS 1915+105 on day 152 (May 31)

X-ray light curves of GRS 1915+105 on day 152 with finer time resolution. This light curve covers from 14:56:15 to 15:13:18. This light curve includes background counts of 100-150 counts/sec.
GRS1915_d152_1sec_lc image: X-ray light curves of GRS 1915+105 on day 152 with finer time resolution.
Download : Ascii Dump, GIF file, PostScript File


Power Spectrum of GRS 1915+105 on day 152 (May 31)
GRS1915_d152_power image: Power spectrum of GRS1915+105 observed with RXTE/PCA.
Power spectrum of GRS1915+105 observed with RXTE/PCA on day 152 (May 31, 1996). This power spectrum is an ensemble average of 60 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).
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.

This page is maintained by the RXTE SOF and was last modified on Wednesday, 24-Aug-2022 11:10:26 EDT.

Responsible NASA Official: Phil Newman
Web Curator: Robin Corbet

Privacy Policy and Important Notices.