Here is a list of files in sequence.tar. After gunzipping the tar file, unpackage using tar xvf [sequence].tar, for the following list: sequence_gis.expo gis mean exposure map sequence_gis2.arf gis 2 arf file sequence_gis2.evt gis 2 screened events file sequence_gis2.expo gis 2 exposure map sequence_gis2.rmf gis 2 response matrix sequence_gis2_bgd.evt gis 2 events file for the background region sequence_gis2_bgd.pha gis 2 background spectrum file sequence_gis2_bgd.reg ascii background region file sequence_gis2_bgd_hard.evt gis 2 hard-band bgd events file sequence_gis2_randc.reg ascii region file, gis exclusion of bad areas sequence_gis2_sky.img sky image for gis 2 sequence_gis2_src.evt events file for gis 2 source region sequence_gis2_src.pha gis 2 source region spectral file sequence_gis2_src.reg ascii source extraction region file sequence_gis2_src_20.pha gis 2 source region spectral file, binned sequence_gis2_src_hard.evt gis 2 hard -band events file from source region sequence_gis3.arf sequence_gis3.evt sequence_gis3.expo sequence_gis3.rmf sequence_gis3_bgd.evt sequence_gis3_bgd.pha sequence_gis3_bgd.reg sequence_gis3_bgd_hard.evt sequence_gis3_randc.reg sequence_gis3_sky.img sequence_gis3_src.evt sequence_gis3_src.pha sequence_gis3_src.reg sequence_gis3_src_20.pha sequence_gis3_src_hard.evt sequence_gis_bgd_32s.flc combined gis FITS light curve 32s bins from bgd reg sequence_gis_bgd_32s_hard.flc fits light curve hard-band, 32s bins, bgd region sequence_gis_bgd_5760s.flc sequence_gis_sky_expcor.gif gis of exposure-corrected sky image sequence_gis_sky_expcor.img FITS image exp-corrected sky image sequence_gis_sky_sm.img smoothed FITS image exp-corrected sky image sequence_gis_src_128s.flc 128 s bins for FITS light curve from source region sequence_gis_src_32s.flc sequence_gis_src_32s_hard.flc sequence_gis_src_5760s.flc sequence_gis_src_5760s_hard.flc sequence_sis.expo sequence_sis0.arf sequence_sis0.evt sequence_sis0.expo sequence_sis0.rmf sequence_sis0_bgd.evt sequence_sis0_bgd.pha sequence_sis0_bgd.reg sequence_sis0_bgd_hard.evt sequence_sis0_bgd_soft.evt sequence_sis0_bgd_xm1.evt sequence_sis0_bgd_xm2.evt sequence_sis0_bgd_xm3.evt sequence_sis0_sky.img sequence_sis0_src.evt sequence_sis0_src.pha sequence_sis0_src.reg sequence_sis0_src_20.pha sequence_sis0_src_hard.evt sequence_sis0_src_soft.evt sequence_sis0_src_xm1.evt events file from source region in xm1 band/sis0 sequence_sis0_src_xm2.evt sequence_sis0_src_xm3.evt sequence_sis1.arf sequence_sis1.evt sequence_sis1.expo sequence_sis1.rmf sequence_sis1_bgd.evt sequence_sis1_bgd.pha sequence_sis1_bgd.reg sequence_sis1_bgd_hard.evt sequence_sis1_bgd_soft.evt sequence_sis1_bgd_xm1.evt sequence_sis1_bgd_xm2.evt sequence_sis1_bgd_xm3.evt sequence_sis1_sky.img sequence_sis1_src.evt sequence_sis1_src.pha sequence_sis1_src.reg sequence_sis1_src_20.pha sequence_sis1_src_hard.evt sequence_sis1_src_soft.evt sequence_sis1_src_xm1.evt sequence_sis1_src_xm2.evt sequence_sis1_src_xm3.evt sequence_sis_bgd_32s.flc sequence_sis_bgd_32s_hard.flc sequence_sis_bgd_32s_soft.flc sequence_sis_bgd_5760s.flc sequence_sis_sky_expcor.img sequence_sis_sky_sm.img sequence_sis_src_128s.flc sequence_sis_src_32s.flc sequence_sis_src_32s_hard.flc sequence_sis_src_32s_soft.flc sequence_sis_src_5760s.flc sequence_sis_src_5760s_hard.flc sequence_sis_src_5760s_soft.flc sequence_webfit.xcm xcm file for use in xspec, starts the user at the spectral fit on the web page evt, img,rmf,arf,pha,flc files are FITS format reg ,xcm files are ASCII format evt files are events lists, img are images, pha are spectra, flc are light curves, rmf/arf files are photon redistribution and ancilliary matrices for use in spectral fitting "src" means extracted from the source region, "bgd" extracted from the background region, "sky" products are using sky coordinates, hard/soft/xm1/xm2/xm3 are the energy bands (defined elsewhere on our pages), "5760/32/128" etc are the time bins in seconds used in the light curves. sis0/sis1/gis2/gis3 are the instrument designations, simple sis or gis mean the combined (summed or mean) of the two instruments of same type.
Tartarus Feedback:
Responsible Scientists, Jane Turner & Kirpal Nandra
tartarus@olegacy.gsfc.nasa.gov