pypeit.masterframe module¶
Implements the master frame base class.
-
class
pypeit.masterframe.
MasterFrame
(master_type, master_dir=None, master_key=None, file_format='fits', reuse_masters=False)[source]¶ Bases:
object
Base class for all PypeIt calibration master frames.
Main methods of the class are to implement the default paths for the master frames and their I/O methods.
Parameters: - master_type (str) – Master frame type, used when constructing the output file
name. See
file_name
. - master_dir (str or None) – Name of the MasterFrame folder. If None, set to current working directory.
- master_key (str or None) – Root of the MasterFrame names, e.g. ‘A_1_01’. If None, set to ‘master’
- file_format (
str
, optional) – File format for the master frame. Typically ‘fits’ or ‘json’. - reuse_masters (bool, optional) – Reuse already created master files from disk.
-
static
construct_file_name
(master_type, master_key, file_format='fits')[source]¶ Name of the MasterFrame file.
-
file_name
¶ Name of the MasterFrame file.
-
file_path
¶ Full path to MasterFrame file.
-
initialize_header
(hdr=None)[source]¶ Initialize the master frame header.
The function writes information generic to all PypeIt master frame headers with basic information.
Parameters: hdr (astropy.io.fits.Header, optional) – Header object to update with basic summary information. The object is modified in-place and also returned. If None, an empty header is instantiated, edited, and returned. Returns: The initialized (or edited) fits header. Return type: astropy.io.fits.Header
-
load
(ext, ifile=None, return_header=False)[source]¶ Generic master file reader.
This generic reader assumes the file is in fits format.
Parameters: Returns: Returns the image data from each provided extension. If return_header is true, the primary header is also returned. If nothing is loaded, either because
reuse_masters
is False or the file does not exist, everything is returned as None (one per expected extension and one if the header is requested).Return type:
-
static
load_from_file
(filename, ext, return_header=False)[source]¶ Generic static method to read a master file.
Parameters: Returns: Returns the image data from each provided extension. If return_header is true, the primary header is also returned.
Return type:
-
save
(data, extnames, outfile=None, overwrite=True, raw_files=None, steps=None, checksum=True)[source]¶ Base interface for saving master frame image data to a fits file.
Data is always placed in extensions, with the PRIMARY extension only containing the header data. More complicated master frame data models should overload this function.
Parameters: - data (
list
, numpy.ndarray) – One or more data arrays to save. - extnames (
list
,str
) – The names for the data extensions. - outfile (
str
, optional) – Name for the output file. Defaults tofile_path
. - overwrite (
bool
, optional) – Overwrite any existing file. - raw_files (
list
, optional) – List of processed raw files used to construct the master frame. - steps (
list
, optional) – The list of steps executed by the derived class to construct the master frame. - checksum (
bool
, optional) – Passed to astropy.io.fits.HDUList.writeto to add the DATASUM and CHECKSUM keywords fits header(s).
- data (
- master_type (str) – Master frame type, used when constructing the output file
name. See