LsstTS3Translator

class lsst.obs.lsst.translators.LsstTS3Translator(header, filename=None)

Bases: lsst.obs.lsst.translators.lsst.LsstBaseTranslator

Metadata translator for LSST BNL Test Stand 3 data.

Attributes Summary

DETECTOR_NAME	Fixed name of single sensor.
cameraPolicyFile
detectorMapping
detectorSerials
name	Name of this translation class
supported_instrument
translators

Methods Summary

are_keys_ok(keywords)	Are the supplied keys all present and defined?
can_translate(header[, filename])	Indicate whether this translation class can translate the supplied header.
can_translate_with_options(header, options)	Helper method for can_translate allowing options.
cards_used()	Cards used during metadata extraction.
compute_detector_exposure_id(exposure_id, …)	Compute the detector exposure ID from detector number and exposure ID.
compute_detector_info_from_serial(…)	Helper method to return the detector information from the serial.
compute_detector_num_from_name(…)	Helper method to return the detector number from the name.
compute_exposure_id(dateobs[, seqnum])	Helper method to calculate the TS3 exposure_id.
defined_in_this_class(name)	Report if the specified class attribute is defined specifically in this class.
detector_mapping()	Returns the mapping of full name to detector ID and serial.
detector_serials()	Obtain the mapping of detector serial to detector group, name, and number.
determine_translator(header[, filename])	Determine a translation class by examining the header
is_key_ok(keyword)	Return True if the value associated with the named keyword is present in this header and defined.
is_keyword_defined(header, keyword)	Return True if the value associated with the named keyword is present in the supplied header and defined.
quantity_from_card(keywords, unit[, …])	Calculate a Astropy Quantity from a header card and a unit.
search_paths()	Search paths to use for LSST data when looking for header correction files.
to_altaz_begin()	Telescope boresight azimuth and elevation at start of observation.
to_boresight_airmass()	Airmass of the boresight of the telescope.
to_boresight_rotation_angle()	Angle of the instrument in boresight_rotation_coord frame.
to_boresight_rotation_coord()	Coordinate frame of the instrument rotation angle (options: sky, unknown).
to_dark_time()	Calculate the dark time.
to_datetime_begin()
to_datetime_end()
to_detector_exposure_id()
to_detector_group()
to_detector_name()	Name of the detector within the instrument (might not be unique if there are detector groups).
to_detector_num()
to_detector_serial()	Serial number/string associated with this detector.
to_detector_unique_name()	Return a unique name for the detector.
to_exposure_id()	Generate a unique exposure ID number
to_exposure_time()	Duration of the exposure with shutter open (seconds).
to_instrument()	Calculate the instrument name.
to_location()	Location of the observatory.
to_object()	Object of interest or field name.
to_observation_id()
to_observation_type()
to_physical_filter()	The bandpass filter used for this observation.
to_pressure()	Atmospheric pressure outside the dome.
to_relative_humidity()	Relative humidity outside the dome.
to_science_program()	Calculate the science program information.
to_telescope()	Full name of the telescope.
to_temperature()	Temperature outside the dome.
to_tracking_radec()	Requested RA/Dec to track.
to_visit_id()	Generate a unique exposure ID number
validate_value(value, default[, minimum, …])	Validate the supplied value, returning a new value if out of range

Attributes Documentation

DETECTOR_NAME = 'S00'

Fixed name of single sensor.

cameraPolicyFile = 'policy/ts3.yaml'

detectorMapping = None

detectorSerials = None

name = 'LSST-TS3'

Name of this translation class

supported_instrument = None

translators = {'DECam': <class 'astro_metadata_translator.translators.decam.DecamTranslator'>, 'HSC': <class 'astro_metadata_translator.translators.hsc.HscTranslator'>, 'ImSim': <class 'lsst.obs.lsst.translators.imsim.ImsimTranslator'>, 'LSST-TS3': <class 'lsst.obs.lsst.translators.ts3.LsstTS3Translator'>, 'LSST-TS8': <class 'lsst.obs.lsst.translators.ts8.LsstTS8Translator'>, 'LSST-UCDCam': <class 'lsst.obs.lsst.translators.lsst_ucdcam.LsstUCDCamTranslator'>, 'LSSTAuxTel': <class 'lsst.obs.lsst.translators.auxTel.LsstAuxTelTranslator'>, 'LSSTCam': <class 'lsst.obs.lsst.translators.lsstCam.LsstCamTranslator'>, 'MegaPrime': <class 'astro_metadata_translator.translators.megaprime.MegaPrimeTranslator'>, 'PhoSim': <class 'lsst.obs.lsst.translators.phosim.PhosimTranslator'>, 'SuprimeCam': <class 'astro_metadata_translator.translators.suprimecam.SuprimeCamTranslator'>}

Methods Documentation

are_keys_ok(keywords)

Are the supplied keys all present and defined?

Parameters:

keywords : iterable of str

Keywords to test.

Returns:

all_ok : bool

True if all supplied keys are present and defined.

classmethod can_translate(header, filename=None)

Indicate whether this translation class can translate the supplied header.

There is no usable INSTRUME header in TS3 data. Instead we use the TSTAND header.

Parameters:

header : dict-like

Header to convert to standardized form.

filename : str, optional

Name of file being translated.

Returns:

can : bool

True if the header is recognized by this class. False otherwise.

classmethod can_translate_with_options(header, options, filename=None)

Helper method for can_translate allowing options.

Parameters:

header : dict-like

Header to convert to standardized form.

options : dict

Headers to try to determine whether this header can be translated by this class. If a card is found it will be compared with the expected value and will return that comparison. Each card will be tried in turn until one is found.

filename : str, optional

Name of file being translated.

Returns:

can : bool

True if the header is recognized by this class. False otherwise.

Notes

Intended to be used from within can_translate implementations for specific translators. Is not intended to be called directly from determine_translator.

cards_used()

Cards used during metadata extraction.

Returns:

used : frozenset of str

Cards used when extracting metadata.

static compute_detector_exposure_id(exposure_id, detector_num)

Compute the detector exposure ID from detector number and exposure ID.

This is a helper method to allow code working outside the translator infrastructure to use the same algorithm.

Parameters:

exposure_id : int

Unique exposure ID.

detector_num : int

Detector number.

Returns:

detector_exposure_id : int

The calculated ID.

classmethod compute_detector_info_from_serial(detector_serial)

Helper method to return the detector information from the serial.

Parameters:

detector_serial : str

Detector serial ID.

Returns:

info : tuple of (str, str, int)

Detector group, name, and number.

classmethod compute_detector_num_from_name(detector_group, detector_name)

Helper method to return the detector number from the name.

Parameters:

detector_group : str

Name of the detector grouping. This is generally the raft name.

detector_name : str

Detector name.

Returns:

num : int

Detector number.

static compute_exposure_id(dateobs, seqnum=0)

Helper method to calculate the TS3 exposure_id.

Parameters:

dateobs : str

Date of observation in FITS ISO format.

seqnum : int, unused

Sequence number. Ignored.

Returns:

exposure_id : int

Exposure ID.

classmethod defined_in_this_class(name)

Report if the specified class attribute is defined specifically in this class.

Parameters:

name : str

Name of the attribute to test.

Returns:

in_class : bool

True if there is a attribute of that name defined in this specific subclass. False if the method is not defined in this specific subclass but is defined in a parent class. Returns None if the attribute is not defined anywhere in the class hierarchy (which can happen if translators have typos in their mapping tables).

Notes

Retrieves the attribute associated with the given name. Then looks in all the parent classes to determine whether that attribute comes from a parent class or from the current class. Attributes are compared using id().

classmethod detector_mapping()

Returns the mapping of full name to detector ID and serial.

Returns:

mapping : dict of str:tuple

Returns the mapping of full detector name (group+detector) to detector number and serial.

Raises:

ValueError

Raised if no camera policy file has been registered with this translation class.

Notes

Will construct the mapping if none has previously been constructed.

classmethod detector_serials()

Obtain the mapping of detector serial to detector group, name, and number.

Returns:

info : dict of tuple of (str, str, int)

A dict with the serial numbers as keys and values of detector group, name, and number.

classmethod determine_translator(header, filename=None)

Determine a translation class by examining the header

Parameters:

header : dict-like

Representation of a header.

filename : str, optional

Name of file being translated.

Returns:

translator : MetadataTranslator

Translation class that knows how to extract metadata from the supplied header.

Raises:

ValueError

None of the registered translation classes understood the supplied header.

is_key_ok(keyword)

Return True if the value associated with the named keyword is present in this header and defined.

Parameters:

keyword : str

Keyword to check against header.

Returns:

is_ok : bool

True if the header is present and not-None. False otherwise.

static is_keyword_defined(header, keyword)

Return True if the value associated with the named keyword is present in the supplied header and defined.

Parameters:

header : dict-lik

Header to use as reference.

keyword : str

Keyword to check against header.

Returns:

is_defined : bool

True if the header is present and not-None. False otherwise.

quantity_from_card(keywords, unit, default=None, minimum=None, maximum=None, checker=None)

Calculate a Astropy Quantity from a header card and a unit.

Parameters:

keywords : str or list of str

Keyword to use from header. If a list each keyword will be tried in turn until one matches.

unit : astropy.units.UnitBase

Unit of the item in the header.

default : float, optional

Default value to use if the header value is invalid. Assumed to be in the same units as the value expected in the header. If None, no default value is used.

minimum : float, optional

Minimum possible valid value, optional. If the calculated value is below this value, the default value will be used.

maximum : float, optional

Maximum possible valid value, optional. If the calculated value is above this value, the default value will be used.

checker : function, optional

Callback function to be used by the translator method in case the keyword is not present. Function will be executed as if it is a method of the translator class. Running without raising an exception will allow the default to be used. Should usually raise KeyError.

Returns:

q : astropy.units.Quantity

Quantity representing the header value.

Raises:

KeyError

The supplied header key is not present.

search_paths()

Search paths to use for LSST data when looking for header correction files.

Returns:

path : list

List with a single element containing the full path to the corrections directory within the obs_lsst package.

to_altaz_begin()

Telescope boresight azimuth and elevation at start of observation.

Returns:

translation : astropy.coordinates.AltAz

Translated property.

to_boresight_airmass()

Airmass of the boresight of the telescope.

Returns:

translation : float

Translated property.

to_boresight_rotation_angle()

Angle of the instrument in boresight_rotation_coord frame.

Returns:

translation : astropy.coordinates.Angle

Translated property.

to_boresight_rotation_coord()

Coordinate frame of the instrument rotation angle (options: sky, unknown).

Returns:

translation : str

Translated property.

to_dark_time()

Calculate the dark time.

If a DARKTIME header is not found, the value is assumed to be identical to the exposure time.

Returns:

dark : astropy.units.Quantity

The dark time in seconds.

to_datetime_begin()

to_datetime_end()

to_detector_exposure_id()

to_detector_group()

to_detector_name()

Name of the detector within the instrument (might not be unique if there are detector groups).

Returns:

translation : str

Translated property.

to_detector_num()

to_detector_serial()

Serial number/string associated with this detector.

Returns:

translation : str

Translated value derived from the header.

to_detector_unique_name()

Return a unique name for the detector.

Base class implementation attempts to combine detector_name with detector_group. Group is only used if not None.

Can be over-ridden by specialist translator class.

Returns:

name : str

detector_group``_``detector_name if detector_group is defined, else the detector_name is assumed to be unique. If neither return a valid value an exception is raised.

Raises:

NotImplementedError

Raised if neither detector_name nor detector_group is defined.

to_exposure_id()

Generate a unique exposure ID number

Note that SEQNUM is not unique for a given day in TS3 data so instead we convert the ISO date of observation directly to an integer.

Returns:

exposure_id : int

Unique exposure number.

to_exposure_time()

Duration of the exposure with shutter open (seconds).

Returns:

translation : astropy.units.Quantity

Translated value derived from the header.

to_instrument()

Calculate the instrument name.

Returns:

instrume : str

Name of the test stand.

to_location()

Location of the observatory.

Returns:

translation : astropy.coordinates.EarthLocation

Translated property.

to_object()

Object of interest or field name.

Returns:

translation : str

Translated property.

to_observation_id()

to_observation_type()

to_physical_filter()

The bandpass filter used for this observation.

Returns:

translation : str

Translated value derived from the header.

to_pressure()

Atmospheric pressure outside the dome.

Returns:

translation : astropy.units.Quantity

Translated property.

to_relative_humidity()

Relative humidity outside the dome.

Returns:

translation : float

Translated property.

to_science_program()

Calculate the science program information.

There is no header recording this in TS3 data so instead return the observing day in YYYY-MM-DD format.

Returns:

run : str

Observing day in YYYY-MM-DD format.

to_telescope()

Full name of the telescope.

Returns:

translation : str

Translated property.

to_temperature()

Temperature outside the dome.

Returns:

translation : astropy.units.Quantity

Translated property.

to_tracking_radec()

Requested RA/Dec to track.

Returns:

translation : astropy.coordinates.SkyCoord

Translated property.

to_visit_id()

Generate a unique exposure ID number

Note that SEQNUM is not unique for a given day in TS3 data so instead we convert the ISO date of observation directly to an integer.

Returns:

exposure_id : int

Unique exposure number.

static validate_value(value, default, minimum=None, maximum=None)

Validate the supplied value, returning a new value if out of range

Parameters:

value : float

Value to be validated.

default : float

Default value to use if supplied value is invalid or out of range. Assumed to be in the same units as the value expected in the header.

minimum : float

Minimum possible valid value, optional. If the calculated value is below this value, the default value will be used.

maximum : float

Maximum possible valid value, optional. If the calculated value is above this value, the default value will be used.

Returns:

value : float

Either the supplied value, or a default value.