pypeit.spectrographs.aat_uhrf module
Module for Shane/Kast specific methods.
- class pypeit.spectrographs.aat_uhrf.AATUHRFSpectrograph[source]
Bases:
Spectrograph
Child to handle AAT/UHRF specific code
- allowed_extensions = ['.FTS']
Defines the allowed extensions for the input fits files.
- camera = 'UHRF'
Name of the spectrograph camera or arm. This is used by specdb, so use that naming convention
- check_frame_type(ftype, fitstbl, exprng=None)[source]
Check for frames of the provided type.
- Parameters:
ftype (
str
) – Type of frame to check. Must be a valid frame type; see frame-type Definitions.fitstbl (astropy.table.Table) – The table with the metadata for one or more frames to check.
exprng (
list
, optional) – Range in the allowed exposure time for a frame of typeftype
. Seepypeit.core.framematch.check_frame_exptime()
.
- Returns:
Boolean array with the flags selecting the exposures in
fitstbl
that areftype
type frames.- Return type:
- compound_meta(headarr, meta_key)[source]
Methods to generate metadata requiring interpretation of the header data, instead of simply reading the value of a header card.
- Parameters:
headarr (
list
) – List of astropy.io.fits.Header objects.meta_key (
str
) – Metadata keyword to construct.
- Returns:
Metadata value read from the header(s).
- Return type:
- config_specific_par(scifile, inp_par=None)[source]
Modify the PypeIt parameters to hard-wired values used for specific instrument configurations.
- Parameters:
scifile (
str
) – File to use when determining the configuration and how to adjust the input parameters.inp_par (
ParSet
, optional) – Parameter set used for the full run of PypeIt. If None, usedefault_pypeit_par()
.
- Returns:
The PypeIt parameter set adjusted for configuration specific parameter values.
- Return type:
- configuration_keys()[source]
Return the metadata keys that define a unique instrument configuration.
This list is used by
PypeItMetaData
to identify the unique configurations among the list of frames read for a given reduction.- Returns:
List of keywords of data pulled from file headers and used to constuct the
PypeItMetaData
object.- Return type:
- classmethod default_pypeit_par()[source]
Return the default parameters to use for this instrument.
- Returns:
Parameters required by all of PypeIt methods.
- Return type:
- get_detector_par(det, hdu=None)[source]
Return metadata for the selected detector.
- Parameters:
det (
int
) – 1-indexed detector number.hdu (astropy.io.fits.HDUList, optional) – The open fits file with the raw image of interest. If not provided, frame-dependent parameters are set to a default.
- Returns:
Object with the detector metadata.
- Return type:
- header_name = 'uhrf'
Name of the spectrograph camera or arm from the Header. Usually the INSTRUME card.
- init_meta()[source]
Define how metadata are derived from the spectrograph files.
That is, this associates the PypeIt-specific metadata keywords with the instrument-specific header cards using
meta
.
- name = 'aat_uhrf'
The name of the spectrograph. See Spectrographs for the currently supported spectrographs.
- ndet = 1
Number of detectors for this instrument.
- ql_supported = False
Flag that PypeIt code base has been sufficiently tested with data from this spectrograph in quicklook mode that it is officially supported by the development team.
- supported = True
Flag that PypeIt code base has been sufficiently tested with data from this spectrograph that it is officially supported by the development team.
- telescope = Parameter Value Default Type Callable ---------------------------------------------------------------- name AAT KECK str False longitude 149.06119444444445 None int, float False latitude -31.273361111111104 None int, float False elevation 1149.0000000015516 None int, float False fratio None None int, float False diameter 3.9 None int, float False eff_aperture 12.0 None int, float False
Instance of
TelescopePar
providing telescope-specific metadata.
- url = 'https://aat.anu.edu.au/science/instruments/decomissioned/uhrf/overview'
Reference url