IMAG |
IMAG_2 |
IMAG_4 |
IMAG_8 |
IMAG_9 |
IMAG_4S4 |
IMAG_VGW |
IMAG_VGW2 |
IMAG_VGW4 |
IMAG_VGW8 |
IMAG_VGW9 |
IMAG_VGW4S4 |
IMAG_BL64 |
IMAG_BL128 |
SPEC |
SPEC_2 |
SPEC_4 |
SPEC_ABBA |
SPEC_2S2 |
SPEC_4S4 |
Parameter | Default Value | |
IMAG | IMAG_2, IMAG_4, IMAG_8, IMAG_9 | |
IMAG_VGW | IMAG_VGW2,IMAG_VGW4,IMAG_VGW8,IMAG_VGW9 | |
DATASET_ID | "DS0000" | "DS0000" |
DITH | - | 10.0 |
OBJECT | "OBJECT" | "OBJECT" |
RA | DUMMY | DUMMY |
DEC | DUMMY | DUMMY |
EQUINOX | DUMMY | DUMMY |
PA | (-90.0-2.0*!TSCL.INSROTPA) | (-90.0-2.0*!TSCL.INSROTPA) |
EXPTIME | NOP | NOP |
FILTER | NOP | NOP |
SLITX | NOP | NOP |
SLITY | NOP | NOP |
NSAMPLE | NOP | NOP |
NFRAME | 6 | 6 |
Parameter | Default Value | |
SPEC | SPEC_2, SPEC_4, SPEC_ABBA | |
DATASET_ID | "DS0000" | "DS0000" |
DITH | - | 10.0 |
OBJECT | "OBJECT" | "OBJECT" |
RA | DUMMY | DUMMY |
DEC | DUMMY | DUMMY |
EQUINOX | DUMMY | DUMMY |
PA | DUMMY | (-90.0 - 2.0 * !TSCL.INSROTPA ) |
EXPTIME | NOP | NOP |
FILTER | NOP | NOP |
SLITX | NOP | NOP |
SLITY | NOP | NOP |
NSAMPLE | NOP | NOP |
NFRAME | 3 | 3 |
Parameter | Default Value | |
IMAG_4S4 | SPEC_2S2 | |
IMAG_VGW4S4 | SPEC_4S4 | |
DATASET_ID | "DS0000" | "DS0000" |
DITH | 20.0 | 10.0 |
OBJECT | "OBJECT" | "OBJECT" |
RA | DUMMY | DUMMY |
DEC | DUMMY | DUMMY |
EQUINOX | DUMMY | DUMMY |
PA | (-90.0 - 2.0 * !TSCL.INSROTPA) | (-90.0 - 2.0 * !TSCL.INSROTPA) |
EXPTIME | NOP | NOP |
FILTER | NOP | NOP |
SLITX | NOP | NOP |
SLITY | NOP | NOP |
NSAMPLE | NOP | NOP |
NFRAME | 6 | 3 |
RASEC_SKY | 180.0 | 180.0 |
DECSEC_SKY | 180.0 | 180.0 |
Parameter | Default Value |
IMAG_BL64 | |
IMAG_BL128 | |
DATASET_ID | "DS0000" |
OBJECT | "STANDARD" |
RA | DUMMY |
DEC | DUMMY |
EQUINOX | DUMMY |
PA | DUMMY |
EXPTIME | NOP |
FILTER | NOP |
SLITX | NOP |
SLITY | NOP |
NSAMPLE | DUMMY |
NSTEP | 1 |
The dithering patterns are shown below.
Because the nodding is realized by CCD offset, DITH should be smaller than 20. The dithering patterns are shown below.
Expected to used for extended objects.