# Licensed under a 3-clause BSD style license - see LICENSE.rst
"""Catalog utility functions / classes."""
from __future__ import absolute_import, division, print_function, unicode_literals
import numpy as np
from astropy.coordinates import Angle, SkyCoord
__all__ = [
"coordinate_iau_format",
"ra_iau_format",
"dec_iau_format",
"skycoord_from_table",
"select_sky_box",
"select_sky_circle",
]
def _ra_iau_format_scalar(ra, digits):
"""Format a single Right Ascension."""
# Note that Python string formatting always rounds the last digit,
# but the IAU spec requires to truncate instead.
# That's why integers with the correct digits are computed and formatted
# instead of formatting floats directly
ra_h = int(ra.hms[0])
ra_m = int(ra.hms[1])
ra_s = ra.hms[2]
if digits == 2: # format: HH
ra_str = "{0:02d}".format(ra_h)
elif digits == 3: # format: HHh
ra_str = "{0:03d}".format(int(10 * ra.hour))
elif digits == 4: # format: HHMM
ra_str = "{0:02d}{1:02d}".format(ra_h, ra_m)
elif digits == 5: # format : HHMM.m
ra_str = "{0:02d}{1:02d}.{2:01d}".format(ra_h, ra_m, int(ra_s / 6))
elif digits == 6: # format: HHMMSS
ra_str = "{0:02d}{1:02d}{2:02d}".format(ra_h, ra_m, int(ra_s))
else: # format: HHMMSS.s
SS = int(ra_s)
s_digits = digits - 6
s = int(10 ** s_digits * (ra_s - SS))
fmt = "{0:02d}{1:02d}{2:02d}.{3:0" + str(s_digits) + "d}"
ra_str = fmt.format(ra_h, ra_m, SS, s)
return ra_str
def _dec_iau_format_scalar(dec, digits):
"""Format a single declination."""
# Note that Python string formatting always rounds the last digit,
# but the IAU spec requires to truncate instead.
# That's why integers with the correct digits are computed and formatted
# instead of formatting floats directly
dec_sign = "+" if dec.deg >= 0 else "-"
dec_d = int(abs(dec.dms[0]))
dec_m = int(abs(dec.dms[1]))
dec_s = abs(dec.dms[2])
if digits == 2: # format: +DD
dec_str = "{}{:02d}".format(dec_sign, dec_d)
elif digits == 3: # format: +DDd
dec_str = "{:+04d}".format(int(10 * dec.deg))
elif digits == 4: # format : +DDMM
dec_str = "{}{:02d}{:02d}".format(dec_sign, dec_d, dec_m)
elif digits == 5: # format: +DDMM.m
dec_str = "{}{:02d}{:02d}.{:01d}".format(dec_sign, dec_d, dec_m, int(dec_s / 6))
elif digits == 6: # format: +DDMMSS
dec_str = "{}{:02d}{:02d}.{:02d}".format(dec_sign, dec_d, dec_m, int(dec_s))
else: # format: +DDMMSS.s
SS = int(dec_s)
s_digits = digits - 6
s = int(10 ** s_digits * (dec_s - SS))
fmt = "{}{:02d}{:02d}{:02d}.{:0" + str(s_digits) + "d}"
dec_str = fmt.format(dec_sign, dec_d, dec_m, SS, s)
return dec_str
[docs]def skycoord_from_table(table):
"""Make `~astropy.coordinates.SkyCoord` from lon, lat columns in `~astropy.table.Table`.
This is a convenience function similar to `~astropy.coordinates.SkyCoord.guess_from_table`,
but with the column names we usually use.
TODO: I'm not sure if it's a good idea to use this because it's not always clear
which positions are taken.
"""
try:
keys = table.colnames
except AttributeError:
keys = table.keys()
if set(["RAJ2000", "DEJ2000"]).issubset(keys):
lon, lat, frame = "RAJ2000", "DEJ2000", "icrs"
elif set(["RA", "DEC"]).issubset(keys):
lon, lat, frame = "RA", "DEC", "icrs"
elif set(["GLON", "GLAT"]).issubset(keys):
lon, lat, frame = "GLON", "GLAT", "galactic"
elif set(["glon", "glat"]).issubset(keys):
lon, lat, frame = "glon", "glat", "galactic"
else:
raise KeyError("No column GLON / GLAT or RA / DEC or RAJ2000 / DEJ2000 found.")
unit = table[lon].unit.to_string() if table[lon].unit else "deg"
skycoord = SkyCoord(table[lon], table[lat], unit=unit, frame=frame)
return skycoord
[docs]def select_sky_box(table, lon_lim, lat_lim, frame="icrs", inverted=False):
"""Select sky positions in a box.
This function can be applied e.g. to event lists of source catalogs
or observation tables.
Note: if useful we can add a function that returns the mask
or indices instead of applying the selection directly
Parameters
----------
table : `~astropy.table.Table`
Table with sky coordinate columns.
lon_lim, lat_lim : `~astropy.coordinates.Angle`
Box limits (each should be a min, max tuple).
frame : str, optional
Frame in which to apply the box cut.
Built-in Astropy coordinate frames are supported, e.g.
'icrs', 'fk5' or 'galactic'.
inverted : bool, optional
Invert selection: keep all entries outside the selected region.
Returns
-------
table : `~astropy.table.Table`
Copy of input table with box cut applied.
Examples
--------
>>> selected_obs_table = select_sky_box(obs_table,
... lon_lim=Angle([150, 300], 'deg'),
... lat_lim=Angle([-50, 0], 'deg'),
... frame='icrs')
"""
skycoord = skycoord_from_table(table)
skycoord = skycoord.transform_to(frame)
lon = skycoord.data.lon
lat = skycoord.data.lat
# SkyCoord automatically wraps lon angles at 360 deg, so in case
# the lon range is wrapped at 180 deg, lon angles must be wrapped
# also at 180 deg for the comparison to work
if any(l < Angle(0., "deg") for l in lon_lim):
lon = lon.wrap_at(Angle(180, "deg"))
lon_mask = (lon_lim[0] <= lon) & (lon < lon_lim[1])
lat_mask = (lat_lim[0] <= lat) & (lat < lat_lim[1])
mask = lon_mask & lat_mask
if inverted:
mask = np.invert(mask)
return table[mask]
[docs]def select_sky_circle(table, lon_cen, lat_cen, radius, frame="icrs", inverted=False):
"""Select sky positions in a circle.
This function can be applied e.g. to event lists of source catalogs
or observation tables.
Note: if useful we can add a function that returns the mask
or indices instead of applying the selection directly
Parameters
----------
table : `~astropy.table.Table`
Table with sky coordinate columns.
lon_cen, lat_cen : `~astropy.coordinates.Angle`
Circle center.
radius : `~astropy.coordinates.Angle`
Circle radius.
frame : str, optional
Frame in which to apply the box cut.
Built-in Astropy coordinate frames are supported, e.g.
'icrs', 'fk5' or 'galactic'.
inverted : bool, optional
Invert selection: keep all entries outside the selected region.
Returns
-------
table : `~astropy.table.Table`
Copy of input table with circle cut applied.
Examples
--------
>>> selected_obs_table = select_sky_circle(obs_table,
... lon=Angle(0, 'deg'),
... lat=Angle(0, 'deg'),
... radius=Angle(5, 'deg'),
... frame='galactic')
"""
skycoord = skycoord_from_table(table)
skycoord = skycoord.transform_to(frame)
# no need to wrap lon angleshere, since the SkyCoord separation
# method takes care of it
center = SkyCoord(lon_cen, lat_cen, frame=frame)
ang_distance = skycoord.separation(center)
mask = ang_distance < radius
if inverted:
mask = np.invert(mask)
return table[mask]