# FILTER TURRET SETTING ALIAS LIST |
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2024-10-17 |
by IT |
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ALIAS NAME |
FILTER1 |
FILTER2 |
FILTER3 |
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# Imaging |
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#
BB Filters etc |
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DEF_DARK |
NOP |
NOP |
BP |
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DEF_IMY |
Y |
CSLM |
HOLE |
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DEF_IMJ |
J |
CSLM |
HOLE |
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DEF_IMH |
H |
CSLM |
HOLE |
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DEF_IMKS |
KS |
CSLM |
HOLE |
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DEF_IMK |
STD_K |
CSLM |
HOLE |
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# MB filters |
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DEF_IMMBK3 |
HOLE |
CSLM |
MBK3 |
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DEF_IMMBK4 |
HOLE |
CSLM |
MBK4 |
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# NB filters |
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DEF_IMNB119 |
NB119 |
CSLM |
HOLE |
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DEF_IMFE2 |
FE2 |
CSLM |
HOLE |
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DEF_IMNB1550 |
HOLE |
NB1550 |
HOLE |
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DEF_IMNB1657 |
HOLE |
NB1657 |
HOLE |
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DEF_IMH2 |
H2 |
CSLM |
HOLE |
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DEF_IMBRG |
BRG |
CSLM |
HOLE |
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DEF_IMNB2071 |
HOLE |
NB2071 |
HOLE |
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DEF_IMNB2083 |
HOLE |
NB2083 |
HOLE |
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DEF_IMNB2095 |
HOLE |
NB2095 |
HOLE |
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DEF_IMCO |
CO |
CSLM |
HOLE |
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DEF_IMNB2315 |
HOLE |
NB2315 |
HOLE |
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# Pupil Viewer
(Engineering Purpose) |
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DEF_PV |
HOLE |
CSL |
PV |
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* Note: ND
filter and K-cont filter were retired in 2020. ND filter is still available
on request. Contact the SA at least ~1 yr before use. |
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# Spectroscopy |
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Coverage(um)*1 |
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DEF_HK500 |
HOLE |
OC_HK |
HK500 |
1.3 - 2.3 |
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DEF_HK500LONG |
OC1_3 |
CSLM |
HK500 |
1.3 - 2.5: w
more thermal BG. |
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DEF_HK500KS |
KS |
CSLM |
HK500 |
2.0 - 2.3: less
thermal BK than HK500K |
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DEF_ZJ500 |
HOLE |
OC_ZJ |
ZJ500 |
0.9 - 1.78 |
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DEF_ZJ500HOLE |
HOLE |
CSLM |
ZJ500 |
0.9 - (but 2nd
order contaminates beyond 1.8um) |
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DEF_VPH_Y |
HOLE |
CSLM |
VPH_Y |
0.9 - 1.15:
longer side determined by detector edge. |
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DEF_LS_J |
HOLE |
OC_ZJ |
LS_J |
1.09 - 1.39 (determined by detector edges) |
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DEF_LS_H |
HOLE |
OC_HK |
LS_H |
1.43 -1.82 (determined by detector edges) |
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DEF_VPH_K |
HOLE |
OC_HK |
VPH_K |
1.8 - 2.3:
shorter side defined by detector edge. Less thermal BG. |
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DEF_VPH_KLONG |
OC1_3 |
CSLM |
VPH_K |
1.8 - 2.5:
shorter side defined by detector edge. |
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DEF_VPH_KS |
KS |
CSLM |
VPH_K |
2.0 - 2.3 |
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DEF_VB_K |
HOLE |
OC_HK |
VB_K |
1.8 - 2.3:
shorter side defined by detector edge. Less thermal BG. |
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DEF_VB_KLONG |
OC1_3 |
CSLM |
VB_K |
1.8 - 2.5:
shorter side defined by detector edge. |
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DEF_VB_KS |
KS |
CSLM |
VB_K |
2.0 - 2.3 |
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* Note 1: the
values are defined by filters. The actual spectra may be cut off by detector
edges. |
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* Note 2: R1300
was retired in 2020 due to microcrack issue. |
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* Note 3: VPH_J
& VPH_H Grisms were replaced to LS_J and LS_H, respectively, in
2020. |
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* Note 4: You
may also use NB/MB filters with grisms. Ask SA if necessary. |
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### Special Setting for Ch1-Ch2
Independent Filter/Grisms: upper=ch1 lower=ch2 ### |
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# Ch1 = Imaging
for Monitor, Ch2 = Spectroscopy |
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DEF_HK500WIN1 |
H2 |
CSLM |
HOLE |
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HOLE |
OC_HK |
HK500 |
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DEF_HK500LONGWIN1 |
H2 |
CSLM |
HOLE |
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OC1_3 |
CSLM |
HK500 |
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DEF_ZJ500WIN1 |
NB119 |
CSLM |
HOLE |
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HOLE |
OC_ZJ |
ZJ500 |
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DEF_ZJ500HOLEWIN1 |
NB119 |
CSLM |
HOLE |
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HOLE |
CSLM |
ZJ500 |
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DEF_VPH_YWIN1 |
Y |
CSLM |
HOLE |
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HOLE |
CSLM |
VPH_Y |
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DEF_VPH_KWIN1 |
H2 |
CSLM |
HOLE |
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HOLE |
OC_HK |
VPH_K |
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DEF_VPH_KLONGWIN1 |
H2 |
CSLM |
HOLE |
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OC1_3 |
CSLM |
VPH_K |
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DEF_LS_J_WIN1 |
NB119 |
OC_ZJ |
HOLE |
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HOLE |
OC_ZJ |
LS_J |
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DEF_LS_H_WIN1 |
FE2 |
CSLM |
HOLE |
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HOLE |
OC_HK |
LS_H |
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DEF_VB_KWIN1 |
H2 |
CSLM |
HOLE |
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HOLE |
OC_HK |
VB_K |
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DEF_VB_KLONGNWIN1 |
H2 |
CSLM |
HOLE |
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HOLE |
OC_HK |
VB_K |
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* NOTE: When
you take dome flats, add "B" at the end of the definition part. It
will put blank plate (cover) to the imaging channel to protect detector. |
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# Ch2 = Imaging
for Monitor, Ch1 = Spectroscopy |
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DEF_HK500WIN2 |
HOLE |
OC_HK |
HK500 |
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H2 |
CSLM |
HOLE |
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DEF_HK500LONGWIN2 |
OC1_3 |
CSLM |
HK500 |
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H2 |
CSLM |
HOLE |
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DEF_ZJ500WIN2 |
HOLE |
OC_ZJ |
ZJ500 |
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NB119 |
CSLM |
HOLE |
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DEF_ZJ500HOLEWIN2 |
HOLE |
CSLM |
ZJ500 |
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NB119 |
CSLM |
HOLE |
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DEF_VPH_YWIN2 |
HOLE |
CSLM |
VPH_Y |
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Y |
CSLM |
HOLE |
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DEF_VPH_KWIN2 |
HOLE |
OC_HK |
VPH_K |
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H2 |
CSLM |
HOLE |
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DEF_VPH_KLONGWIN2 |
OC1_3 |
CSLM |
VPH_K |
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H2 |
CSLM |
HOLE |
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DEF_LS_J_WIN2 |
HOLE |
OC_ZJ |
LS_J |
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NB119 |
OC_ZJ |
HOLE |
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DEF_LS_H_WIN2 |
HOLE |
OC_HK |
LS_H |
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FE2 |
CSLM |
HOLE |
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DEF_VB_KWIN2 |
HOLE |
OC_HL |
VB_K |
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H2 |
CSLM |
HOLE |
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DEF_VB_KLONGNWIN2 |
OC1_3 |
CSLM |
VB_K |
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H2 |
CSLM |
HOLE |
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* NOTE: When
you take dome flats, add "B" at the end of the definition part. It
will put blank plate (cover) to the imaging channel to protect detector. |
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Update History: |
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2016-10-10:
Default order-sorting filter for VPHJ is changed from OC_ZJ to HOLE+CSL. This
mode has been effective since the October observations. |
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2016-11-15:
The alias for VPH filters has changed to keep their consistency with grism
name. e.g., DEF_VPHJ --> DEF_VPH_J etc. |
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2016-11-15:
TheNB filters used with the VPH_H grism with the window imaging has changed
from Fe2 to NB119, as the sky for Fe2 is too bright. |
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2020-06-30:
VPH-Y and R1300 Grisms were retired in 2020. Instead, LS_J and LS_H Grisms
were installed in 2020. All the related aliases were updated. |
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2020-09-17: The
filter for LS_J has changed from CSLM to OC_ZJ to suppress the ghost. |
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2023-2-5: VPH-Y
is back, VPH-J/H are removed. A confusion on VPH_HK and VPH_K are cleared
now. |
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2023-02-05: The
retirement of K-cont and ND were reflected to the table. |
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2024-03-05:
removed remaining VPHJ/H part. Editted VPH_K part following the change of the
definition. Added VB_K-related definition. Removed th BP-adding definition
and put the note for it. |
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