"""
Module containing functions to generate astrometric/photometric calibration catalogs
for LMI images
"""
# pylint: disable=duplicate-code
import logging
from mirar.catalog import BaseCatalog, GaiaVizier
from mirar.catalog.vizier import PS1, SkyMapper
from mirar.catalog.vizier.sdss import SDSS, NotInSDSSError, in_sdss
from mirar.data.image_data import Image
from mirar.pipelines.git.config import (
psfex_config_path,
sextractor_photometry_config,
swarp_config_path,
)
from mirar.pipelines.lmi.config.constants import LMI_WIDTH_DEG
from mirar.pipelines.lmi.generator.sources import lmi_skyportal_formatter
from mirar.pipelines.lmi.generator.stacks import label_stack_id
from mirar.pipelines.lmi.generator.target import annotate_target_coordinates
from mirar.processors.astromatic import PSFex, Sextractor, Swarp
from mirar.references import BaseReferenceGenerator, PS1Ref, SDSSRef
logger = logging.getLogger(__name__)
LMI_SEARCH_RADIUS_ARCMIN = LMI_WIDTH_DEG * 60.0 / (2.0**0.5) # Triangle diagonal
LMI_PHOTOMETRIC_MAX_MAG = 22
[docs]
def lmi_astrometric_catalog_generator(_) -> GaiaVizier:
"""
Returns an astrometric catalog for LMI
:param _: Image
:return: Gaia catalog around image
"""
cat = GaiaVizier(
min_mag=10,
max_mag=20,
search_radius_arcmin=LMI_SEARCH_RADIUS_ARCMIN,
filter_name="G",
)
return cat
[docs]
def lmi_photometric_catalog_generator(image: Image) -> BaseCatalog:
"""
Generate a photometric calibration catalog for LMI images
For u band: SDSS if possible, otherwise Skymapper, otherwise fail
For g/r/i/z: use PS1
:param image: Image
:return: catalog at image position
"""
filter_name = image["FILTER"].replace("'", "")
ra, dec = image["CRVAL1"], image["CRVAL2"]
if filter_name in ["u", "U"]:
if in_sdss(ra, dec):
return SDSS(
min_mag=8,
max_mag=LMI_PHOTOMETRIC_MAX_MAG,
search_radius_arcmin=LMI_SEARCH_RADIUS_ARCMIN,
filter_name=filter_name,
)
if dec < 0.0:
return SkyMapper(
min_mag=8,
max_mag=LMI_PHOTOMETRIC_MAX_MAG,
search_radius_arcmin=LMI_SEARCH_RADIUS_ARCMIN,
filter_name=filter_name,
)
err = "U band image is in a field with no reference image."
logger.error(err)
raise NotInSDSSError(err)
return PS1(
min_mag=10,
max_mag=LMI_PHOTOMETRIC_MAX_MAG,
search_radius_arcmin=LMI_SEARCH_RADIUS_ARCMIN,
filter_name=filter_name,
)
[docs]
def lmi_reference_image_generator(image: Image) -> BaseReferenceGenerator:
"""
Get a reference image generator for a LMI image
For u band: SDSS if possible, otherwise fail
For g/r/i/z: use PS1
:param image: image
:return: Reference image generator
"""
filter_name = image["FILTER"].replace("'", "")
logger.debug(f"Filter is {filter_name}")
if filter_name in ["u", "U"]:
if in_sdss(image["CRVAL1"], image["CRVAL2"]):
return SDSSRef(filter_name=filter_name)
err = "U band image is in a field with no reference image."
logger.error(err)
raise NotInSDSSError(err)
logger.debug("Will query reference image from PS1")
return PS1Ref(filter_name=filter_name)
[docs]
def lmi_reference_image_resampler(**kwargs) -> Swarp:
"""
Generates a resampler for reference images
:param kwargs: kwargs
:return: Swarp processor
"""
return Swarp(
swarp_config_path=swarp_config_path, cache=False, subtract_bkg=True, **kwargs
)
[docs]
def lmi_sdss_reference_cat_purifier(catalog, image: Image):
"""
Purify SDSS catalog
:param catalog:
:param image:
:return:
"""
zero_point = image["ZP"]
mags = catalog["MAG_AUTO"] + zero_point
good_sources_mask = mags > 18
return catalog[good_sources_mask]
[docs]
def lmi_reference_psfex(output_sub_dir: str, norm_fits: bool) -> PSFex:
"""
Generates a PSFex processor for reference images
:param output_sub_dir: output sui directory
:param norm_fits: boolean
:return: Sextractor processor
"""
return PSFex(
config_path=psfex_config_path,
output_sub_dir=output_sub_dir,
norm_fits=norm_fits,
)
[docs]
def lmi_zogy_catalogs_purifier(sci_catalog, ref_catalog):
"""
Purify catalogs for ZOGY
"""
good_sci_sources = (
(sci_catalog["FLAGS"] == 0)
& (sci_catalog["SNR_WIN"] > 5)
& (sci_catalog["FWHM_WORLD"] < 4.0 / 3600)
& (sci_catalog["FWHM_WORLD"] > 0.5 / 3600)
& (sci_catalog["SNR_WIN"] < 1000)
)
good_ref_sources = (
(ref_catalog["SNR_WIN"] > 5)
& (ref_catalog["FWHM_WORLD"] < 5.0 / 3600)
& (ref_catalog["FWHM_WORLD"] > 0.5 / 3600)
)
return good_sci_sources, good_ref_sources