Source code for gemini_instruments.bhros.adclass

from astrodata import astro_data_tag, astro_data_descriptor, returns_list, TagSet
from ..gemini import AstroDataGemini
from .. import gmu

[docs]class AstroDataBhros(AstroDataGemini): __keyword_dict = dict(array_section = 'CCDSEC', central_wavelength = 'WAVELENG', overscan_section = 'BIASSEC') @staticmethod def _matches_data(source): return source[0].header.get('INSTRUME', '').upper() == 'BHROS' @astro_data_tag def _tag_instrument(self): return TagSet(set(['BHROS', 'SPECT']), ())
[docs] @astro_data_descriptor def central_wavelength(self, asMicrometers=False, asNanometers=False, asAngstroms=False): """ Returns the central wavelength in meters or the specified units Parameters ---------- asMicrometers : bool If True, return the wavelength in microns asNanometers : bool If True, return the wavelength in nanometers asAngstroms : bool If True, return the wavelength in Angstroms Returns ------- float The central wavelength setting """ unit_arg_list = [asMicrometers, asNanometers, asAngstroms] if unit_arg_list.count(True) == 1: # Just one of the unit arguments was set to True. Return the # central wavelength in these units if asMicrometers: output_units = "micrometers" if asNanometers: output_units = "nanometers" if asAngstroms: output_units = "angstroms" else: # Either none of the unit arguments were set to True or more than # one of the unit arguments was set to True. In either case, # return the central wavelength in the default units of meters. output_units = "meters" # The central_wavelength keyword is in Angstroms keyword = self._keyword_for('central_wavelength') wave_in_angstroms = self.phu.get(keyword, -1) if wave_in_angstroms < 0: return None return gmu.convert_units('angstroms', wave_in_angstroms, output_units)
[docs] @astro_data_descriptor def dec(self): """ Returns the Declination of the center of field in degrees. Since a fiber is used it coincides with the position of the target. For code re-used, use target_dec() if you really want the position of the target rather than the center of the field. Returns ------- float right ascension in degrees """ # using the target_dec descriptor since the WCS is not sky coords return self.target_dec(offset=True, icrs=True)
[docs] @astro_data_descriptor def disperser(self, stripID=False, pretty=False): """ Returns the name of the disperser. This is always 'bHROS' Parameters ---------- stripID : bool Does nothing pretty : bool Does nothing Returns ------- str The name of the disperser """ return 'bHROS'
[docs] @astro_data_descriptor def ra(self): """ Returns the Right Ascension of the center of field in degrees. Since a fiber is used it coincides with the position of the target. For code re-used, use target_ra() if you really want the position of the target rather than the center of the field. Returns ------- float right ascension in degrees """ # using the target_ra descriptor since the WCS is not sky coords return self.target_ra(offset=True, icrs=True)