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EXOLOG - EXOSAT Observation Log |
HEASARC Archive |
Taylor B.G. et al., 1981 Sp. Sci. Rev., Vol. 30, p. 479. White N.E. and Peacock A.P. 1988, X-ray Astronomy with EXOSAT, [eds. N.E. White and R. Pallivicini], Memoria S. A. It., p. 59.
Name
The `name` parameter gives the target name. This name usually corresponds to
the target name as specified by the original observer. If a source has been
observed by different observers it may be entered under two or more names. It
is recommended that any search by `name` always be followed by a search on
the found coordinates.
RA
The Right Ascension of the EXOSAT pointing.
Dec
The Declination of the EXOSAT pointing.
LII
The Galactic Longitude of the EXOSAT pointing.
BII
The Galactic Latitude of the EXOSAT pointing.
Time
The `time` of the observation refers to the start time. Times are accurate to
the nearest second.
End_Time
The end time of the observation. The units and use of this parameter are the
same as those for `time`.
Sequence_Number
The number of the observation, in chronological order from the beginning of
the mission.
Target_Number
target number
Observer
The principal investigator for the observation.
Observer_Code
observer code
Proposal_Code
proposal code
Proposal_Type
A code was assigned to each EXOSAT proposal that approximately defined the
class of object to be observed. The codes are as follows:
AGN - active galactic nuclei EXG - other kinds of galaxies CLU - clusters of galaxies HLX - high luminosity galactic sources LLX - low luminosity galactic sources SNR - supernova remnants OPS - operational activities CAL - calibration DEE - deep field MIS - miscellaneous PV - performance verification TOO - target of opportunity
Instrument
For each observation there is one entry per instrument. The `instrument`
parameter gives the name of the instrument. It can be `LE1`, `LE2`, `ME` or
`GSPC`. The two LE telescopes are treated as separate instruments because the
filters and other instrument modes can be different.
OBC_Modes
The OBC modes define on-board computer programs that were running during the
observation. Each program has a short name, e.g., HTR3. More details about
these programs can be found in the EXOSAT FOT handbook, available from the
EXOSAT Observatory. The programs depend on the instrument as follows:
LE: O = old DIRECT N = new DIRECT without spatial filter D = new DIRECT with diamond filter R = new DIRECT with rectangular filter ME: T3 = HTR3 in full sub-mode P1 = PULS (old version) P2 = PULS2 (new version, with background spectrum) E5 = HER5 EH = HER3 or HER4 (data per half array) EQ = HER3 or HER4 (data per quadrant) ED = HER3 or HER4 (data per detector) E2 = HER2 D2 = MDIR2 (new direct) I7 = HER7 T4 = HTR4 I6 = HER6 T3 = HTR3 OPT T5 = HTR5 GSPC: 0 = old DIRECT N = new DIRECT H = HEBL2 or HEBL4
Payload_Status
This is a code that gives information concerning the instrument modes for each
observation. The code depends on the instrument as follows:
LE Filters: LE detector: P = PPL C = CMA with filter 4 = 4000 Lexan G = CMA with grating A = Al/Pa P = PSD 3 = 3000 Lexan B = Boron The orientation of the ME array halves: 1 = half 1 offset for part of the period 2 = half 2 offset for part of the period C = coaligned for part of the period. The number, as a hexadecimal digit, of ME high voltages on. If all 16 detectors are turned on then no character is given. (The argon and xenon layers are treated here as separate detectors). The GSPC gain used: 1 = gain 1.0 2 = gain 2.0 + = non standard gain, probably 0.5.
Channel_Compression
The number of channels combined by the OBC; e.g., 1 means
full resolution, and 4 means the summing of every 4 adjacent channels.
Channel_Selection
The ME PHA channel selection and compression:
spectra intensity channels ------- ------------------ 0 = all channels A = one argon, no xenon 1 = argon 4-67 or 5-68, no xenon B = two argon, no xenon 2 = argon 4-67 and xenon 138-201 C = one argon, one xenon 3 = argon 4-67 and xenon 132-195 D = four argon (HER7) 4 = argon 4-35 and no xenon E = 4 ranges, with one or 5 = argon 0-63 and no xenon more xenon 6 = argon 0-127 and no xenon X = one or two xenon, no ? = a non standard selection argon
Argon_Integration_Time
The accumulation time in seconds of the spectral data for the ME argon
data.
Xenon_Integration_Time
The accumulation time in seconds of the spectral data for the ME xenon data.
Intensity_Sample_Interva
intensity sample interval, sec
FOT_Name
for archive request submission
FOT_Start
for archive request submission
FOT_End
for archive request submission
FOT_Time_1
for archive request submission
FOT_Time_2
for archive request submission
FOT_Time_3
for archive request submission
Multiple_FOT_Flag
for archive request submission
Footnotes
footnotes