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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