コード例 #1
0
def _format_obs_history(obs_history, field_ids, save_to_disk=None):
    obs_history = obs_history.loc[obs_history['Field_fieldID'].isin(
        field_ids)].copy()
    # Some unit conversion and column renaming
    obs_history['Ixx_PSF'] = units.fwhm_to_sigma(
        obs_history['finSeeing'].values)**2.0
    obs_history['apFluxErr'] = units.mag_to_flux(
        obs_history['fiveSigmaDepth'].values - 22.5) / 5.0
    obs_history = obs_history.rename(
        {
            'filtSkyBrightness': 'sky',
            'obsHistID': 'ccdVisitId'
        }, axis=1)
    # Only keep columns we'll need
    obs_keep_cols = [
        'ccdVisitId',
        'Field_fieldID',
        'expMJD',
        'Ixx_PSF',
        'apFluxErr',
        'sky',
        'filter',
    ]
    obs_history = obs_history[obs_keep_cols]
    if save_to_disk is not None:
        obs_history.to_csv(save_to_disk, index=False)
    return obs_history
コード例 #2
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def _format_truth_catalog(point_neighbors, save_to_disk=None):
    # Point-source neighbors
    point_neighbors[['ra', 'dec'
                     ]] = units.deg_to_arcsec(point_neighbors[['ra', 'dec']])
    for bp in 'ugrizy':
        point_neighbors['flux_%s' % bp] = units.mag_to_flux(
            point_neighbors[bp].values, to_unit='nMgy')
    if save_to_disk is not None:
        point_neighbors.to_csv(save_to_disk, index=False)
    return point_neighbors
コード例 #3
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def _format_obs_history(obs_history, field, save_to_disk=None):
    """
    Parameters
    ----------
    obs_history : Pandas.DataFrame
    field : Pandas.DataFrame
    save_to_disk : str
    
    Note
    ----
    We use the dithered RA, Dec and express all positions in arcsec.
    
    Returns
    -------
    DataFrame obs_history, formatted with new column conventions and units
    """
    # Join with Field table
    obs_history = pd.merge(obs_history,
                           field,
                           left_on='Field_fieldID',
                           right_on='fieldID')
    # Some unit conversion and column renaming
    # NOTE: OpSim DB defines dithered positions as offset from the field center.
    obs_history['ditheredRA'] = units.deg_to_arcsec(
        obs_history['ditheredRA'].values + obs_history['fieldRA'].values)
    obs_history['ditheredDec'] = units.deg_to_arcsec(
        obs_history['ditheredDec'].values + obs_history['fieldDec'].values)
    obs_history['Ixx_PSF'] = units.fwhm_to_sigma(
        obs_history['finSeeing'].values)**2.0
    obs_history['apFluxErr'] = units.mag_to_flux(
        obs_history['fiveSigmaDepth'].values - 22.5) / 5.0
    obs_history = obs_history.rename(
        {
            'filtSkyBrightness': 'sky',
            'obsHistID': 'ccdVisitId'
        }, axis=1)
    # Only keep columns we'll need
    obs_keep_cols = [
        'ccdVisitId',
        'Field_fieldID',
        'expMJD',
        'ditheredRA',
        'ditheredDec',
        'Ixx_PSF',
        'apFluxErr',
        'sky',
        'filter',
    ]
    obs_history = obs_history[obs_keep_cols]
    obs_history['ccdVisitId'] = obs_history['ccdVisitId'].astype(np.int64)
    if save_to_disk is not None:
        obs_history.to_csv(save_to_disk, index=False)
    return obs_history
コード例 #4
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def _format_extragal_catalog(galaxies, save_to_disk=None):
    # Unit conversion and column renaming
    filters = list('ugrizy')
    galaxies.columns = map(str.lower, galaxies.columns)
    galaxies[['ra',
              'dec']] = units.deg_to_arcsec(galaxies[['ra_true', 'dec_true']])
    galaxies['phi_bulge'] = units.e1e2_to_phi(
        e1=galaxies['ellipticity_1_bulge_true'].values,
        e2=galaxies['ellipticity_2_bulge_true'].values)
    galaxies['phi_disk'] = units.e1e2_to_phi(
        e1=galaxies['ellipticity_1_disk_true'].values,
        e2=galaxies['ellipticity_2_disk_true'].values)
    galaxies['disk_to_total_ratio'] = 1.0 - galaxies['bulge_to_total_ratio_i']
    for bp in 'ugrizy':
        galaxies['flux_%s' % bp] = units.mag_to_flux(
            galaxies['mag_true_%s_lsst' % bp].values, to_unit='nMgy')
        galaxies['flux_disk_%s' % bp] = galaxies[
            'flux_%s' % bp].values * galaxies['disk_to_total_ratio'].values
        galaxies['flux_bulge_%s' % bp] = galaxies[
            'flux_%s' % bp].values * galaxies['bulge_to_total_ratio_i'].values
    for component in ['disk', 'bulge']:
        galaxies['ra_%s' % component] = galaxies['ra'].values
        galaxies['dec_%s' % component] = galaxies['dec'].values
        galaxies['size_circular_%s' % component] = (
            galaxies['size_minor_%s_true' % component].values *
            galaxies['size_%s_true' % component].values)**0.5
        galaxies['e_%s' % component] = galaxies['ellipticity_%s_true' %
                                                component]
    # Only keep columns we'll use
    galaxies_cols_to_keep = ['galaxy_id', 'ra',
                             'dec']  # 'agn', 'sprinkled', 'star']
    galaxies_cols_to_keep += [
        'ra_bulge', 'dec_bulge', 'size_circular_bulge', 'e_bulge', 'phi_bulge'
    ]
    galaxies_cols_to_keep += [
        'ra_disk', 'dec_disk', 'size_circular_disk', 'e_disk', 'phi_disk'
    ]
    galaxies_cols_to_keep += [
        prop + '_' + bp
        for prop, bp in product(['flux_bulge', 'flux_disk'], filters)
    ]
    galaxies = galaxies[galaxies_cols_to_keep]
    if save_to_disk is not None:
        galaxies.to_csv(save_to_disk, index=False)
    return galaxies