add parameter info

Author: SpheMakh

cultcargo/tigger-convert.yml

@@ -20,53 +20,79 @@ cabs:
         policies:
           positional: yes
       force:
+        info: Overwrite output
         dtype: bool
         default: yes
       type:
+        info: Input model type
         dtype: str
         choices: [Tigger, ASCII, BBS, NEWSTAR, AIPSCC, APSCCFITS, Gaul, auto]
         default: auto
+      output-type:
+        info: Output model type
+        choices: [Tigger, ASCII, BBS, NEWSTAR, AIPSCC, APSCCFITS, Gaul, auto]
+        default: auto
       append:
-        dtype: File
+        info: Append another model to input model. May be given multiple times.
+        dtype: List[File]
+        policies:
+          repeat: repeat
       append-type:
+        info: Append model type
         dtype: str
         choices: [Tigger, ASCII, BBS, NEWSTAR, AIPSCC, APSCCFITS, Gaul, auto]
         default: auto
       format:
+        info: Input format, for ASCII or BBS tables. For BBS tables, the default format is specified in the file header.
         dtype: str
       append-format:
+        info: Append model format
         dtype: str
       output-format:
+        info: Output model format
         dtype: str
       app-to-int:
+        info: Treat fluxes as apparent, and rescale them into intrinsic using the     supplied primary beam model (see --primary-beam option).
         dtype: bool
       int-to-app:
+        info: Treat fluxes as intrinsic, and rescale them into apparent using the     supplied primary beam model (see --primary-beam option).
         dtype: bool
       primary-beam:
+        info: "Apply a primary beam expression to estimate apparent fluxes. Any valid Python expression using the variables 'r' and 'fq' is accepted. Use 'refresh' to re-estimate fluxes using the current expression. Example (for the WSRT-like 25m dish PB): cos(min(65*fq*1e-9*r,1.0881))**6"
         dtype: str
       fits-l-axis:
+        info: CTYPE for L axis in the FITS PB file. Note that our internal L points East (increasing RA), if the FITS beam axis points the opposite way, prefix the CTYPE with a '-'' character
         dtype: str
         default: X
       fits-m-axis:
+        info: CTYPE for M axis in the FITS PB file. Note that our internal M points North (increasing Dec), if the FITS beam axis points the opposite way, prefix the CTYPE with a '-'' character
         dtype: str
         default: Y
       beam-clip:
+        info: when using a FITS beam, clip (power) beam gains at this level to keep intrinsic source fluxes from blowing up. Sources below this beamgain will be tagged 'nobeam'.
         dtype: float
         default: 0.001
       beam-spi:
+        info: perform a spectral index fit to each source based on a frequency dependent FITS beam, requires --primary-beam option to be used with a FITS file. Apply this spectral index to LSM sources. Must supply a bandwidth (in MHz) (centred on --beam-freq) over which the beam spi is estimated.
         dtype: float
       beam-diag:
+        info: Use diagonal Jones terms only for beam mode
         dtype: bool
       pa-from-ms:
-        dtype: MS
+        info: Rotate the primary beam pattern through a range of parallactic angles as given by the MS and field ID (default 0) and take the average over time. This is more accurate than --pa-range.
+        dtype: str
+        metavar: "MS1[:FIELD1],MS2:[FIELD2],..."
       pa:
+        info: Rotate the primary beam pattern through a parallactic angle (in degrees)
         dtype: float
       pa-range:
+        info: Rotate the primary beam pattern through a range of parallactic angles (in degrees) and use the average value over PA
         dtype: str
       linear-pol:
+        info: Use XY basis correlations for beam filenames and Mueller matrices. Default is RL
         dtype: bool
-        default: yes
       center:
+        info: Override coordinates of the nominal field center specified in the input model.
         dtype: str
     outputs:
       output-model: