Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelpCy20/ch12_acs5.html
Дата изменения: Thu May 31 18:26:09 2012 Дата индексирования: Mon Apr 11 17:43:31 2016 Кодировка: Поисковые слова: reflection nebula |
Space Telescope Science Institute |
Cycle 20 Phase II Proposal Instructions |
11.4.1 Spectral Elements for WFC
Allowed Configurations Hα Hα ramp Hα ramp Hα ramp 1) The polarizers must be used with another spectral element. This is required to maintain focus. The UV polarizers (POL0UV, POL60UV, POL120UV) must be used with a spectral element on wheel 2 except for: POL0V, POL60V, POL120V, and any inner or outer ramp filter segment (see Table 11.4). The visible polarizers (POL0V, POL60V, POL120V) must be used with a spectral element on wheel 1 except for: F850LP, F892N, POL0UV, POL60UV, and POL120UV.Only a subset of possible combinations of spectral elements are permitted. In the following tables, an "S" indicates combinations that are supported. Combinations marked with "O" are permitted ONLY for Mode = ACQ exposures and are intended for use with bright targets.Table 11.3: Permitted WFC filter combinations for Mode = ACCUM
Table 11.4: Wavelength Ranges for the WFCRamp Filters
Minimum Wavelength (е) Maximum Wavelength (е) WFC FOV location 11.4.4 Spectral Elements for ACS/SBC
MgF2 CaF2 BaF2 Ly-α CaF2 PRISM LiF2 PRISM11.4.5 Allowed Combinations of Aperture, Spectral Element & Readout
full frame2
F = normal WFC filters and G800L
S = small elements (polarizers and F892N)
I = inner ramp filter segments
M = middle ramp filter segments
O = outer ramp filter segments
A subarray fixed by STScI will apply to WFC, WFC1, WFC2 when a small
spectral element (polarizer of F892N) is selected.