Bertsch, D.L., et al. 1989, in Proc. Gamma-Ray Observatory Science Workshop, ed. W.N. Johnson (Greenbelt:NASA), 2-52 Hartman, R. C., et al. 1999, ApJS, 123, 79 Hughes, E.B., et al. 1980, IEEE, Trans. Nucl. Sci., NS-27, 364 Kanbach, G., et al. 1988, Space Sci. Rev., 49, 69 Kanbach, G., et al. 1989, in Proc. Gamma-Ray Observatory Science Workshop, ed. W.N. Johnson (Greenbelt:NASA), 2-1 Thompson, D.J., et al. 1993, ApJS, 86, 629 Thompson, D.J., et al. 1993, ApJ, 415, L13
Observation-Specific Files: Users wanting a quicklook image of the EGRET observation, should examine the EGRET Quicklook (GIF) Map file. For most other users, the standard maps contained in the EGRET Photon Count Map files or the EGRET Intensity Map files will likely be the most suitable data products to examine. Those experienced users desiring to do more detailed screening and/or timing analysis will need to get the EGRET Event List (qvp) file. Most users will not need the EGRET Exposure History (exphst) files. All of these observation-specific files are described in more detail below. The file-naming convention used for them is such that they all contain a 4-digit set of characters that specify the viewing period (usually but not always preceded by the characters 'vp'), e.g., an EGRET Event List file for viewing period 2.0 would have the filename of qvp0020f.fits. Files containing standard maps that have been produced for the standard EGRET energy ranges will further contain a 4-digit set of characters of the form 'g001', 'g002', 'g003', or 'g004' that is used to specify the energy ranges included, e.g.,
Energy Ranges of the Standard Maps Extension Energy ranges of maps in file (MeV) g001 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, and 4000-10000 g002 30-100 and 100-10000 g003 30-300 and 300-1000 g004 30-1000 and 1000-10000EGRET Quicklook (GIF) Map File: This file has a filename of the type vp####.gif, and contains a GIF image of the EGRET intensity map for energies integrated above 100 MeV.
EGRET Photon Counts and Map Files: These files have filenames of the type counts_vp####_g00#.fits and contain the standard EGRET maps of the photon counts for the various standard EGRET energy ranges.
EGRET Exposure Map Files: These files have filenames of the type exposr_vp####_g00#.fits and contain the EGRET instrumental exposure maps for the various standard EGRET energy ranges.
EGRET Intensity Map Files: These files have filenames of the type intens_vp####_g00#.fits and contain the EGRET gamma-ray intensity maps for the various standard EGRET energy ranges.
EGRET Photon List File (EGRET Events File): This file has a filename of the type qvp####f.fits and contains a time-ordered list of all photons detected during the viewing periond. This includes earth albedo photons and wide-angle photons that are not useful for higher-level analysis.
EGRET Exposure History File: This file has a filename of the type exphst_v01p####.fits and contains the exposure history information. This file is used by the EGRET program INTMAP.
EGRET Low-Level Data (Primary Database Files): These files have names like pd_19990511_144958_150037.fits, where the first set of numbers is the year-month-day, the second set is the start time in hours-minutes-seconds UT, and the third set is the end time in hours-minutes-seconds UT, and are FITS versions of the EGRET Primary Database Files that were created by the CGRO Science Support Center. The different kinds of records in the original files have been segregated into different binary table extensions. Within each extension, the records remain time-ordered. The extensions are Gamma_Ray_Event, TASC_Burst_Spectra, Housekeeping, and Microsec_Burst. If no Microsecond Burst records were in the original file, the Microsec_Burst HISTORY header is not written. Since the typical duration of a PD file is several hours, there will be, in general, many such files for a given viewing period.
General Files: There are also available various other general EGRET data products including (i) a set of EGRET Combined Data files that contain composite counts, exposure, and intensity maps covering the entire sky and derived from all viewing periods, Phase 1, Phase 2, etc; (ii) a set of EGRET Diffuse Model Data files that contain an all-sky model of the diffuse gamma-ray emission in the form of FITS maps for the standard EGRET energy ranges; (iii) an EGRET/CGRO Timeline file which contains the valid observation times for each viewing period, and is used by the EGRET programs INTMAP and MAPGEN; and (iv) a set of EGRET calibration files for energy dispersion, point-spread function, and sensitive area.
HEASARC User Hotline.