Suppose that you wish to use the FGS to observe a binary star named Binary01, as well as five reference stars ref1,......,ref5. All stars are in the same FGS field of view, and can therefore be observed in one and the same visit (see Section 6.2.2). Stars ref4 and ref5 have magnitude V=14.6, and all the other targets have 13.0<V<14.0. The targets have a declination of +42 degrees, so that there are 53 minutes of visibility time per orbit (see Table 6.1). To enable the removal of drift and jitter in the post observation analysis of the data, the binary is observed in POS mode several times (twice in our example) and the reference stars are each observed twice. Your desired exposures are listed in Table A.4, and the associated overheads are listed in Table A.5. In Table A.6 you can see how this fits into a total of 1 orbit.
Config |
Mode |
Spectral Element |
Number of Exp |
Time per Exp [min.] |
Notes |
---|---|---|---|---|---|
FGS |
POS |
F583W |
8 |
0.2 |
2 exposures of target Binary01, and 2 exposures for each of the targets ref1, ref2, and ref3 |
FGS |
POS |
F583W |
4 |
0.7 |
2 exposures for each of the targets ref4 and ref5 |
FGS |
TRANS |
F583W |
1 |
13.3 |
20 scans of 40 sec each (see Table 6.8) for Binary01 |
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