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STIS Instrument Handbook for Cycle 24 |
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Our current estimates of the overheads on STIS exposures are summarized in Table 9.1 and Table 9.2. All numbers given are approximate and rounded up to the nearest half minute; they do not differentiate in detail the overheads for different STIS modes and configurations. These overhead times are to be used (in conjunction with the actual exposure times and the HST Primer) to estimate the total number of orbits for your proposal. After your HST proposal is accepted, you will be asked to submit a Phase II proposal to support scheduling of your approved observations. At that time you will be presented with actual, up-to-date overheads by the scheduling software. Allowing sufficient time for overheads in your Phase I proposal is important; additional time to cover unplanned overheads will not be granted later.
- In subsequent contiguous orbits you must include the overhead for the guide-star reacquisition (5 minutes). If you are observing in the Continuous Viewing Zone (see the HST Primer), no guide-star reacquisitions are required.
- All STIS spectroscopic exposures that use a slit (long slit or echelle slit) will need to include a target acquisition exposure to place the target in the slit (see Section 8.2). As discussed in Section 8.3, for the narrower slits you may also need to perform a peakup exposure to center the target in the slit.
For V ≤ 21 point sources, 6 minutes.
For diffuse acqs, add 0.2 в checkbox2 seconds to the nominal 6 minutes.
5.01 8.02 1.03 5.04 8.05 For CR-SPLIT=n, each exposure has a 1 minute overhead, so there will be (n – 1) minutes of extra overhead. If small CCD subarrays are used, the overhead per exposure decreases to 20 seconds.