Source code for sourcefinder.accessors.dataaccessor
import logging
import numpy as np
from math import degrees, sqrt, sin, pi, cos
from dataclasses import dataclass, field
from sourcefinder.utils import is_valid_beam_tuple
from sourcefinder.utility.coordinates import WCS
from sourcefinder.config import ImgConf
from typing import Optional, cast
[docs]
logger = logging.getLogger(__name__)
@dataclass
[docs]
class DataAccessor:
"""Base class for accessors used with
:class:`sourcefinder.image.ImageData`.
Data accessors provide a uniform way for the ImageData class (i.e.,
generic image representation) to access the various ways in which
images may be stored (FITS files, arrays in memory, potentially HDF5,
etc.).
This class cannot be instantiated directly, but should be subclassed
and the abstract properties provided. Note that all abstract
properties are required to provide a valid accessor.
Additional properties may also be provided by subclasses. However,
TraP components are required to degrade gracefully in the absence of
these optional properties.
Attributes
----------
beam : tuple
Restoring beam. Tuple of three floats: semi-major axis (in pixels),
semi-minor axis (pixels), and position angle (radians).
centre_ra : float
Right ascension at the central pixel of the image. Units of J2000
decimal degrees.
centre_decl : float
Declination at the central pixel of the image. Units of J2000
decimal degrees.
data : numpy.ndarray
Two-dimensional numpy.ndarray of floating point pixel values.
freq_bw : float
The frequency bandwidth of this image in Hz.
freq_eff : float
Effective frequency of the image in Hz. That is, the mean frequency
of all the visibility data which comprises this image.
pixelsize : tuple
(x, y) tuple representing the size of a pixel along each axis in
units of degrees.
tau_time : float
Total time on sky in seconds.
taustart_ts : float
Timestamp of the first integration which constitutes part of this
image. MJD in seconds.
url : str
A URL representing the location of the image at the time of
processing.
wcs : :class:`sourcefinder.utility.coordinates.WCS`
An instance of :py:class:`sourcefinder.utility.coordinates.WCS`,
describing the mapping from data pixels to sky-coordinates.
Notes
-----
The class also provides some common functionality: static methods used
for parsing data files, and an 'extract_metadata' function which
provides key info in a simple dict format.
"""
[docs]
beam: Optional[tuple[float, float, float]] = field(default=None)
[docs]
conf: Optional[ImgConf] = field(default=None, repr=False)
def __post_init__(self):
if self.conf is not None:
beam_tuple = (self.conf.bmaj, self.conf.bmin, self.conf.bpa)
if is_valid_beam_tuple(beam_tuple):
deltax, deltay = self.pixelsize
self.beam = DataAccessor.degrees2pixels(
*beam_tuple, deltax, deltay
)
[docs]
def parse_pixelsize(self) -> tuple[float, float]:
"""Parse pixel size.
Returns
-------
deltax : float
Pixel size along the x axis in degrees.
deltay : float
Pixel size along the y axis in degrees.
"""
wcs = self.wcs
# Check that pixels are square
# (Would have to be pretty strange data for this not to be the case)
assert wcs.cunit[0] == wcs.cunit[1]
if wcs.cunit[0] == "deg":
deltax = wcs.cdelt[0]
deltay = wcs.cdelt[1]
elif wcs.cunit[0] == "rad":
deltax = degrees(wcs.cdelt[0])
deltay = degrees(wcs.cdelt[1])
else:
raise ValueError("Unrecognised WCS co-ordinate system")
# NB. What's a reasonable epsilon here?
eps = 1e-7
if abs(abs(deltax) - abs(deltay)) > eps:
raise ValueError(
"Image WCS header suggests non-square pixels."
"This is an untested use case, and may break "
"things - specifically the skyregion tracking "
"but possibly other stuff too."
)
return deltax, deltay
@staticmethod
[docs]
def degrees2pixels(
bmaj, bmin, bpa, deltax, deltay
) -> tuple[float, float, float]:
"""Convert beam in degrees to beam in pixels and radians.
For example, FITS beam parameters are in degrees.
Parameters
----------
bmaj : float
Beam major axis in degrees.
bmin : float
Beam minor axis in degrees.
bpa : float
Beam position angle in degrees.
deltax : float
Pixel size along the x-axis in degrees.
deltay : float
Pixel size along the y-axis in degrees.
Returns
-------
semimaj : float
Beam semi-major axis in pixels.
semimin : float
Beam semi-minor axis in pixels.
theta : float
Beam position angle in radians.
"""
theta = pi * bpa / 180
semimaj = (bmaj / 2.0) * (
sqrt(
(sin(theta) ** 2) / (deltax**2)
+ (cos(theta) ** 2) / (deltay**2)
)
)
semimin = (bmin / 2.0) * (
sqrt(
(cos(theta) ** 2) / (deltax**2)
+ (sin(theta) ** 2) / (deltay**2)
)
)
return semimaj, semimin, theta