Fh/defaultyamls

ERIS/default.yaml

@@ -0,0 +1,15 @@
+---
+### ERIS package metadata
+alias: PKG
+name: ERIS
+description: NOT YET FUNCTIONAL PLACEHOLDER
+status: concept
+date_modified: 2024-12-12
+changes:
+  - 2024-12-12 (FH) initial creation
+
+packages:
+  - ERIS
+
+yamls:
+  - ERIS.yaml

ERIS/readme.md

@@ -1,18 +1,18 @@
-ERIS at the VLT
-===============
+# ERIS at the VLT
 
 ERIS is a combination of the SPIFFI IFU spectrograph from SINFONI and the NIX JHKLM imager with an AOF compatible WFS
 
-NIX Imager
-----------
+## NIX Imager
+
 * Wavelength: 1-5um (J,H,Ks,Lp,Mp)
 * Pixel scale: Wide 0.027"/pix, Zoom 0.013"/pix
 * FOV: Wide 54", Zoom 27"
 * Filters: J, H, Ks, IB 2.42, IB 2.48, Fe-II, HS 1-0S(1), H2 cont, Br-gamma
 * Detector: (2x2)k H2RG
 * LSS Slit: 12x86 mas
 
-Optics:
+### Optics
+
 * Dichroic to WFS
 * NIX selector mirror (45deg)
 * Entrance window
@@ -24,8 +24,8 @@ Optics:
 * H2RG
 
 
-SPIFFIER IFU
-------------
+## SPIFFIER IFU
+
 * FOV: 0.8", 3.2", 8"
 * Pixel scale: 12.5x25 mas, 50x100mas, 125x250mas
 * IFU: 32 Slices, each 64 pixels wide ?? Really=2048 pix exactly. What is the SINFONI detetor?
@@ -36,11 +36,12 @@ SPIFFIER IFU
 * Detector: H2RG
 * Saturation: 110k e-/DIT/pix
 * Dark: 0.15 e-/s
-* RON: 16e-   
+* RON: 16e-
 * Gain: 2.42 e-/ADU
 
 
-Optics
+### Optics
+
 * 2x Lens collimator
 * Pupil stop
 * Filter wheel

FORS/default.yaml

@@ -0,0 +1,15 @@
+---
+### FORS package metadata
+alias: PKG
+name: FORS
+description: NOT YET FUNCTIONAL PLACEHOLDER
+status: concept
+date_modified: 2024-12-12
+changes:
+  - 2024-12-12 (FH) initial creation
+
+packages:
+  - FORS
+
+yamls:
+  - FORS.yaml

FORS/readme.md

@@ -0,0 +1,50 @@
+# FORS2 at the VLT
+
+Modes: IMG, POL, LSS, Slit-MOS
+Wave-range: 0.33-1.1um
+Pixel-scale: Wide 0.25", Zoom 0.125"
+Binning: 2x2, optionally unbinned.
+FOV: Wide 6.8' (edges vignetted by optics), Zoom 4.25'
+Filters: Nf
+Grisms: Ng
+LSS slits: 9x from 0.3"-2.5"
+MOS arms: 19x
+Slit Mask: <=470 slit cuts
+
+### Detectors
+
+* 2x E2V (2x4)k CCDs @ 15um/pix (good blue sensitivity @ <0.5um)
+* 2x MIT (2x4)k CCDs @ 15um/pix (good red sensitivity @ >0.75um)
+
+### Optics
+
+* Detector Plane: 2 exchangeable 2x CCD mosaics
+* Collimator unit: 2 exchangeable units (Wide or Zoom)
+
+* Polarimeter swing arm:
+  * Quarter wave plate (circular)
+  * Half wave plate (linear)
+* Wheel 1 (Misc)
+  * WOLL_34+13 : Wollaston prism
+  * g_HIGH+115 : Standard g-band filter
+  * GRIS_150I+27 : Grism 150I
+  * GRIS_600RI+19 : Grism 600RI
+  * GRIS_600z+23 : Grism 600z
+  * z_GUNN+78 : Standard z-band filter
+  * GRIS_600V+94 : Grism 600V
+* Wheel 2 (Grisms)
+  * GRIS_1028z+29 : Grism 1028z
+  * GRIS_1400V+18 : Grism 1400V
+  * GRIS_600B+22 : Grism 600B
+  * GRIS_1200B+97 : Grism 1200B
+  * GRIS_1200R+93 : Grism 1200R
+  * GRIS_300I+11 : Grism 300I
+  * GRIS_300V+10 : Grism 300V
+* Wheel 3 (Filters)
+  * u_HIGH+112 : Standard u-band filter
+  * GG435+81 : Order sorting filter GG435
+  * OG590+32 : Order sorting filter OG590
+  * b_HIGH+113 : Standard b-band filter
+  * v_HIGH+114 : Standard v-band filter
+  * R_SPECIAL+76 : Standard R-band filter
+  * I_BESS+77 : Standard I-band filter

HARMONI/readme.md

@@ -0,0 +1 @@
+# HARMONI at the ELT

HAWKI/default.yaml

@@ -1,13 +1,15 @@
+---
 ### default observation parameters needed for a HAWKI simulation
-object : configuration
-alias : OBS
-name : HAWKI_default_configuration
-description : default parameters needed for a HAWKI simulation
+alias: PKG
+name: HAWKI_default_configuration
+description: default parameters needed for a HAWKI simulation
 status: experimental
-date_modified: 2022-02-22
+date_modified: 2024-12-12
 changes:
+  - 2019-08-14 (KL) initial creation
   - 2022-02-22 (MV) formatting
-
+  - 2024-11-19 (FH) add status keywords
+  - 2024-12-12 (FH) restructure default OBS properties, add PKG alias
 
 packages:
   - Paranal
@@ -20,28 +22,26 @@ yamls:
   - HAWKI.yaml
   - HAWKI_H2RG.yaml
 
-properties :
-  filter_name : Ks
-  airmass : 1.2
-  declination : -30
-  hour_angle : 0
-  pupil_angle : 0
-  dit : 60
-  ndit : 1
-
+---
+### default observation parameters needed for a HAWKI simulation
+alias: OBS
+properties:
+  filter_name: Ks
+  airmass: 1.2
+  declination: -30
+  hour_angle: 0
+  pupil_angle: 0
+  dit: 60  # [s]
+  ndit: 1
 
 ---
 ### default simulation parameters needed for a HAWKI simulation
-object : simulation
-alias : SIM
-name : HAWKI_simulation_paramters
-description : RC simulation paramters which need to change for a HAWKI run
-
-properties :
-  random :
-    seed : 9001
-
-  spectral :
-    wave_min : 0.85
-    wave_mid : 1.6
-    wave_max : 2.5
+alias: SIM
+properties:
+  random:
+    seed: 9001
+
+  spectral:
+    wave_min: 0.85  # [um]
+    wave_mid: 1.6   # [um]
+    wave_max: 2.5   # [um]

KMOS/default.yaml

@@ -0,0 +1,15 @@
+---
+### KMOS package metadata
+alias: PKG
+name: KMOS
+description: NOT YET FUNCTIONAL PLACEHOLDER
+status: concept
+date_modified: 2024-12-12
+changes:
+  - 2024-12-12 (FH) initial creation
+
+packages:
+  - KMOS
+
+yamls:
+  - KMOS.yaml

LFOA/default.yaml

@@ -1,45 +1,49 @@
-### default observation parameters needed for a LFOA simulation
-object : configuration
-alias : OBS
-name : LFOA_default_configuration
-description : default parameters needed for a LFOA simulation
+---
+### LFOA package metadata
+alias: PKG
+name: LFOA_default_configuration
+description: default parameters needed for a LFOA simulation
 status: experimental
+date_modified: 2024-12-12
+changes:
+  - 2020-05-18 (KL) initial creation
+  - 2020-05-29 (KL) add LFAO sloan filters
+  - 2024-11-19 (FH) add status keywords
+  - 2024-12-12 (FH) restructure default OBS properties, add PKG alias
 
-packages :
-- LFOA
+packages:
+  - LFOA
 
-yamls :
-- LFOA.yaml
-- LFOA_SBIG.yaml
-
-properties :
-  airmass : 1.2
-  declination : +30
-  hour_angle : 0
-  pupil_angle : 0
-  dit : 60
-  ndit : 1
-  filter_name : V
-  sky :
-    bg_mag : 19.5
-    filter_name : V
+yamls:
+  - LFOA.yaml
+  - LFOA_SBIG.yaml
 
 ---
+### default observation parameters needed for a LFOA simulation
+alias: OBS
+properties:
+  airmass: 1.2
+  declination: +30
+  hour_angle: 0
+  pupil_angle: 0
+  dit: 60  # [s]
+  ndit: 1
+  filter_name: V
+  sky:
+    bg_mag: 19.5
+    filter_name: V
 
+---
 ### default simulation parameters needed for a LFAO simulation
-object : simulation
-alias : SIM
-name : LFAO_simulation_paramters
-description : RC simulation paramters
-
-properties :
-  random :
-    seed : 9001
-
-  spectral :
-    wave_min : 0.3
-    wave_mid : 0.55
-    wave_max : 1.0
-
-  computing :
-    preload_field_of_view : False
+alias: SIM
+properties:
+  random:
+    seed: 9001
+
+  spectral:
+    wave_min: 0.3   # [um]
+    wave_mid: 0.55  # [um]
+    wave_max: 1.0   # [um]
+
+  computing:
+    preload_field_of_view: False

MCIFU/default.yaml

@@ -0,0 +1,15 @@
+---
+### MCIFU package metadata
+alias: PKG
+name: MCIFU
+description: NOT YET FUNCTIONAL PLACEHOLDER
+status: concept
+date_modified: 2024-12-12
+changes:
+  - 2024-12-12 (FH) initial creation
+
+packages:
+  - MCIFU
+
+yamls:
+  - MCIFU.yaml

MCIFU/readme.rst → MCIFU/readme.md

@@ -1,8 +1,6 @@
-Multi-core Integral field unit
-==============================
+# Multi-core Integral field unit
 
-Eckdaten
---------
+## Eckdaten
 
 73 fibres attached to hexagonal lenslets stacked together to form a ring.
 The idea is to have a lenslet every 1.5 lam/D (at 1.3um) to capture the spectrum of different portions of the PSF
@@ -11,5 +9,4 @@ Wavelength range: 1-1.6um
 System throughput: 0.5%
 Resolution ~ 3000
 Detector 2048x2048
-    - currently uses 480x640 chip and mosaicing it around
-
+* currently uses 480x640 chip and mosaicing it around