Source code for panoptes.utils.images.fits

import os
import shutil
import subprocess
from warnings import warn

from astropy import units as u
from astropy.io import fits
from astropy.wcs import WCS
from panoptes.utils import error
from panoptes.utils.logging import logger


[docs]def solve_field(fname, timeout=15, solve_opts=None, *args, **kwargs): """ Plate solves an image. Note: This is a low-level wrapper around the underlying `solve-field` program. See `get_solve_field` for more typical usage and examples. Args: fname(str, required): Filename to solve in .fits extension. timeout(int, optional): Timeout for the solve-field command, defaults to 60 seconds. solve_opts(list, optional): List of options for solve-field. """ solve_field_script = shutil.which('solve-field') if solve_field_script is None: # pragma: no cover raise error.InvalidSystemCommand(f"Can't find solve-field, is astrometry.net installed?") # Add the options for solving the field if solve_opts is not None: options = solve_opts else: # Default options options = [ '--guess-scale', '--cpulimit', str(timeout), '--no-verify', '--crpix-center', '--temp-axy', '--index-xyls', 'none', '--solved', 'none', '--match', 'none', '--rdls', 'none', '--corr', 'none', '--downsample', '4', '--no-plots', ] if 'ra' in kwargs: options.append('--ra') options.append(str(kwargs.get('ra'))) if 'dec' in kwargs: options.append('--dec') options.append(str(kwargs.get('dec'))) if 'radius' in kwargs: options.append('--radius') options.append(str(kwargs.get('radius'))) # Gather all the kwargs that start with `--` and are not already present. logger.debug(f'Adding kwargs: {kwargs!r}') def _modify_opt(opt, val): if isinstance(val, bool): opt_string = str(opt) else: opt_string = f'{opt}={val}' return opt_string options.extend([_modify_opt(opt, val) for opt, val in kwargs.items() if opt.startswith('--') and opt not in options and not isinstance(val, bool)]) cmd = [solve_field_script] + options + [fname] logger.debug(f'Solving with: {cmd}') try: proc = subprocess.Popen(cmd, universal_newlines=True, stdout=subprocess.PIPE, stderr=subprocess.PIPE) except Exception as e: raise error.PanError(f"Problem plate-solving in solve_field: {e!r}") return proc
[docs]def get_solve_field(fname, replace=True, overwrite=True, timeout=30, **kwargs): """Convenience function to wait for `solve_field` to finish. This function merely passes the `fname` of the image to be solved along to `solve_field`, which returns a subprocess.Popen object. This function then waits for that command to complete, populates a dictonary with the EXIF informaiton and returns. This is often more useful than the raw `solve_field` function. Example: >>> from panoptes.utils.images import fits as fits_utils >>> # Get our fits filename. >>> fits_fn = getfixture('unsolved_fits_file') >>> # Perform the solve. >>> solve_info = fits_utils.get_solve_field(fits_fn) >>> # Show solved filename. >>> solve_info['solved_fits_file'] '.../unsolved.fits' >>> # Pass a suggested location. >>> ra = 15.23 >>> dec = 90 >>> radius = 5 # deg >>> solve_info = fits_utils.solve_field(fits_fn, ra=ra, dec=dec, radius=radius) >>> # Pass kwargs to `solve-field` program. >>> solve_kwargs = {'--pnm': '/tmp/awesome.bmp', '--overwrite': True} >>> solve_info = fits_utils.get_solve_field(fits_fn, **solve_kwargs, skip_solved=False) >>> assert os.path.exists('/tmp/awesome.bmp') Args: fname ({str}): Name of FITS file to be solved. replace (bool, optional): Saves the WCS back to the original file, otherwise output base filename with `.new` extension. Default True. overwrite (bool, optional): Clobber file, default True. Required if `replace=True`. timeout (int, optional): The timeout for solving, default 30 seconds. **kwargs ({dict}): Options to pass to `solve_field` should start with `--`. Returns: dict: Keyword information from the solved field. """ skip_solved = kwargs.get('skip_solved', True) out_dict = {} output = None errs = None header = getheader(fname) wcs = WCS(header) # Check for solved file if skip_solved and wcs.is_celestial: logger.info(f"Skipping solved file (use skip_solved=False to solve again): {fname}") out_dict.update(header) out_dict['solved_fits_file'] = fname return out_dict # Set a default radius of 15 if overwrite: kwargs['--overwrite'] = True # Use unpacked version of file. was_compressed = False if fname.endswith('.fz'): logger.debug(f'Uncompressing {fname}') fname = funpack(fname) logger.debug(f'Using {fname} for solving') was_compressed = True logger.debug(f'Solving with: {kwargs!r}') proc = solve_field(fname, **kwargs) try: output, errs = proc.communicate(timeout=timeout) except subprocess.TimeoutExpired: proc.kill() output, errs = proc.communicate() raise error.Timeout(f'Timeout while solving: {output!r} {errs!r}') else: if proc.returncode != 0: logger.debug(f'Returncode: {proc.returncode}') for log in [output, errs]: if log and log > '': logger.debug(f'Output on {fname}: {log}') if proc.returncode == 3: raise error.SolveError(f'solve-field not found: {output}') new_fname = fname.replace('.fits', '.new') if replace: logger.debug(f'Overwriting original {fname}') os.replace(new_fname, fname) else: fname = new_fname try: header = getheader(fname) header.remove('COMMENT', ignore_missing=True, remove_all=True) header.remove('HISTORY', ignore_missing=True, remove_all=True) out_dict.update(header) except OSError: logger.warning(f"Can't read fits header for: {fname}") # Check it was solved. if WCS(header).is_celestial is False: raise error.SolveError('File not properly solved, no WCS header present.') # Remove WCS file. os.remove(fname.replace('.fits', '.wcs')) if was_compressed and replace: logger.debug(f'Compressing plate-solved {fname}') fname = fpack(fname) out_dict['solved_fits_file'] = fname return out_dict
[docs]def get_wcsinfo(fits_fname, **kwargs): """Returns the WCS information for a FITS file. Uses the `wcsinfo` astrometry.net utility script to get the WCS information from a plate-solved file. Args: fits_fname ({str}): Name of a FITS file that contains a WCS. **kwargs: Args that can be passed to wcsinfo. Returns: dict: Output as returned from `wcsinfo`. Raises: error.InvalidCommand: Raised if `wcsinfo` is not found (part of astrometry.net) """ assert os.path.exists(fits_fname), warn(f"No file exists at: {fits_fname}") wcsinfo = shutil.which('wcsinfo') if wcsinfo is None: raise error.InvalidCommand('wcsinfo not found') run_cmd = [wcsinfo, fits_fname] if fits_fname.endswith('.fz'): run_cmd.append('-e') run_cmd.append('1') proc = subprocess.Popen(run_cmd, stdout=subprocess.PIPE, stderr=subprocess.STDOUT, universal_newlines=True) try: output, errs = proc.communicate(timeout=5) except subprocess.TimeoutExpired: # pragma: no cover proc.kill() output, errs = proc.communicate() unit_lookup = { 'crpix0': u.pixel, 'crpix1': u.pixel, 'crval0': u.degree, 'crval1': u.degree, 'cd11': (u.deg / u.pixel), 'cd12': (u.deg / u.pixel), 'cd21': (u.deg / u.pixel), 'cd22': (u.deg / u.pixel), 'imagew': u.pixel, 'imageh': u.pixel, 'pixscale': (u.arcsec / u.pixel), 'orientation': u.degree, 'ra_center': u.degree, 'dec_center': u.degree, 'orientation_center': u.degree, 'ra_center_h': u.hourangle, 'ra_center_m': u.minute, 'ra_center_s': u.second, 'dec_center_d': u.degree, 'dec_center_m': u.minute, 'dec_center_s': u.second, 'fieldarea': (u.degree * u.degree), 'fieldw': u.degree, 'fieldh': u.degree, 'decmin': u.degree, 'decmax': u.degree, 'ramin': u.degree, 'ramax': u.degree, 'ra_min_merc': u.degree, 'ra_max_merc': u.degree, 'dec_min_merc': u.degree, 'dec_max_merc': u.degree, 'merc_diff': u.degree, } wcs_info = {} for line in output.split('\n'): try: k, v = line.split(' ') try: v = float(v) except Exception: pass wcs_info[k] = float(v) * unit_lookup.get(k, 1) except ValueError: pass # print("Error on line: {}".format(line)) wcs_info['wcs_file'] = fits_fname return wcs_info
[docs]def fpack(fits_fname, unpack=False, overwrite=True): """Compress/Decompress a FITS file Uses `fpack` (or `funpack` if `unpack=True`) to compress a FITS file Args: fits_fname ({str}): Name of a FITS file that contains a WCS. unpack ({bool}, optional): file should decompressed instead of compressed, default False. Returns: str: Filename of compressed/decompressed file. """ assert os.path.exists(fits_fname), warn( "No file exists at: {}".format(fits_fname)) if unpack: fpack = shutil.which('funpack') run_cmd = [fpack, '-D', fits_fname] out_file = fits_fname.replace('.fz', '') else: fpack = shutil.which('fpack') run_cmd = [fpack, '-D', '-Y', fits_fname] out_file = fits_fname.replace('.fits', '.fits.fz') if os.path.exists(out_file): if overwrite is False: raise FileExistsError(f'Destination file already exists at location and overwrite=False') else: os.remove(out_file) try: assert fpack is not None except AssertionError: warn("fpack not found (try installing cfitsio). File has not been changed") return fits_fname logger.debug("fpack command: {}".format(run_cmd)) proc = subprocess.Popen(run_cmd, stdout=subprocess.PIPE, stderr=subprocess.STDOUT, universal_newlines=True) try: output, errs = proc.communicate(timeout=5) except subprocess.TimeoutExpired: proc.kill() output, errs = proc.communicate() return out_file
[docs]def funpack(*args, **kwargs): """Unpack a FITS file. Note: This is a thin-wrapper around the ~fpack function with the `unpack=True` option specified. See ~fpack documentation for details. Args: *args: Arguments passed to ~fpack. **kwargs: Keyword arguments passed to ~fpack. Returns: str: Path to uncompressed FITS file. """ return fpack(*args, unpack=True, **kwargs)
[docs]def write_fits(data, header, filename, exposure_event=None, **kwargs): """Write FITS file to requested location. >>> from panoptes.utils.images import fits as fits_utils >>> data = np.random.normal(size=100) >>> header = { 'FILE': 'delete_me', 'TEST': True } >>> filename = str(getfixture('tmpdir').join('temp.fits')) >>> fits_utils.write_fits(data, header, filename) >>> assert os.path.exists(filename) >>> fits_utils.getval(filename, 'FILE') 'delete_me' >>> data2 = fits_utils.getdata(filename) >>> assert np.array_equal(data, data2) Args: data (array_like): The data to be written. header (dict): Dictionary of items to be saved in header. filename (str): Path to filename for output. exposure_event (None|`threading.Event`, optional): A `threading.Event` that can be triggered when the image is written. kwargs (dict): Options that are passed to the `astropy.io.fits.PrimaryHDU.writeto` method. """ if not isinstance(header, fits.Header): header = fits.Header(header) hdu = fits.PrimaryHDU(data, header=header) # Create directories if required. if os.path.dirname(filename): os.makedirs(os.path.dirname(filename), mode=0o775, exist_ok=True) try: hdu.writeto(filename, **kwargs) except OSError as err: logger.error(f'Error writing image to {filename}: {err!r}') else: logger.debug(f'Image written to {filename}') finally: if exposure_event: exposure_event.set()
[docs]def update_observation_headers(file_path, info): """Update FITS headers with items from the Observation status. >>> # Check the headers >>> from panoptes.utils.images import fits as fits_utils >>> fits_fn = getfixture('unsolved_fits_file') >>> # Show original value >>> fits_utils.getval(fits_fn, 'FIELD') 'KIC 8462852' >>> info = {'field_name': 'Tabbys Star'} >>> update_observation_headers(fits_fn, info) >>> # Show new value >>> fits_utils.getval(fits_fn, 'FIELD') 'Tabbys Star' Args: file_path (str): Path to a FITS file. info (dict): The return dict from `pocs.observatory.Observation.status`, which includes basic information about the observation. """ with fits.open(file_path, 'update') as f: hdu = f[0] hdu.header.set('IMAGEID', info.get('image_id', '')) hdu.header.set('SEQID', info.get('sequence_id', '')) hdu.header.set('FIELD', info.get('field_name', '')) hdu.header.set('RA-MNT', info.get('ra_mnt', ''), 'Degrees') hdu.header.set('HA-MNT', info.get('ha_mnt', ''), 'Degrees') hdu.header.set('DEC-MNT', info.get('dec_mnt', ''), 'Degrees') hdu.header.set('EQUINOX', info.get('equinox', 2000.)) # Assume J2000 hdu.header.set('AIRMASS', info.get('airmass', ''), 'Sec(z)') hdu.header.set('FILTER', info.get('filter', '')) hdu.header.set('LAT-OBS', info.get('latitude', ''), 'Degrees') hdu.header.set('LONG-OBS', info.get('longitude', ''), 'Degrees') hdu.header.set('ELEV-OBS', info.get('elevation', ''), 'Meters') hdu.header.set('MOONSEP', info.get('moon_separation', ''), 'Degrees') hdu.header.set('MOONFRAC', info.get('moon_fraction', '')) hdu.header.set('CREATOR', info.get('creator', ''), 'POCS Software version') hdu.header.set('INSTRUME', info.get('camera_uid', ''), 'Camera ID') hdu.header.set('OBSERVER', info.get('observer', ''), 'PANOPTES Unit ID') hdu.header.set('ORIGIN', info.get('origin', '')) hdu.header.set('RA-RATE', info.get('tracking_rate_ra', ''), 'RA Tracking Rate')
[docs]def getdata(fn, *args, **kwargs): """Get the FITS data. Small wrapper around `astropy.io.fits.getdata` to auto-determine the FITS extension. This will return the data associated with the image. >>> fits_fn = getfixture('solved_fits_file') >>> d0 = getdata(fits_fn) >>> d0 array([[2215, 2169, 2200, ..., 2169, 2235, 2168], [2123, 2191, 2133, ..., 2212, 2127, 2217], [2208, 2154, 2209, ..., 2159, 2233, 2187], ..., [2120, 2201, 2120, ..., 2209, 2126, 2195], [2219, 2151, 2199, ..., 2173, 2214, 2166], [2114, 2194, 2122, ..., 2202, 2125, 2204]], dtype=uint16) >>> d1, h1 = getdata(fits_fn, header=True) >>> (d0 == d1).all() True >>> h1['FIELD'] 'KIC 8462852' Args: fn (str): Path to FITS file. *args: Passed to `astropy.io.fits.getdata`. **kwargs: Passed to `astropy.io.fits.getdata`. Returns: `np.ndarray`: The FITS data. """ return fits.getdata(fn, *args, **kwargs)
[docs]def getheader(fn, *args, **kwargs): """Get the FITS header. Small wrapper around `astropy.io.fits.getheader` to auto-determine the FITS extension. This will return the header associated with the image. If you need the compression header information use the astropy module directly. >>> fits_fn = getfixture('tiny_fits_file') >>> os.path.basename(fits_fn) 'tiny.fits' >>> header = getheader(fits_fn) >>> header['IMAGEID'] 'PAN001_XXXXXX_20160909T081152' >>> # Works with fpacked files >>> fits_fn = getfixture('solved_fits_file') >>> os.path.basename(fits_fn) 'solved.fits.fz' >>> header = getheader(fits_fn) >>> header['IMAGEID'] 'PAN001_XXXXXX_20160909T081152' Args: fn (str): Path to FITS file. *args: Passed to `astropy.io.fits.getheader`. **kwargs: Passed to `astropy.io.fits.getheader`. Returns: `astropy.io.fits.header.Header`: The FITS header for the data. """ ext = 0 if fn.endswith('.fz'): ext = 1 return fits.getheader(fn, ext=ext)
[docs]def getwcs(fn, *args, **kwargs): """Get the WCS for the FITS file. Small wrapper around `astropy.wcs.WCS`. >>> from panoptes.utils.images import fits as fits_utils >>> fits_fn = getfixture('solved_fits_file') >>> wcs = fits_utils.getwcs(fits_fn) >>> wcs.is_celestial True >>> fits_fn = getfixture('unsolved_fits_file') >>> wcs = fits_utils.getwcs(fits_fn) >>> wcs.is_celestial False Args: fn (str): Path to FITS file. *args: Passed to `astropy.io.fits.getheader`. **kwargs: Passed to `astropy.io.fits.getheader`. Returns: `astropy.wcs.WCS`: The World Coordinate System information. """ return WCS(getheader(fn, *args, **kwargs), *args, **kwargs)
[docs]def getval(fn, *args, **kwargs): """Get a value from the FITS header. Small wrapper around `astropy.io.fits.getval` to auto-determine the FITS extension. This will return the value from the header associated with the image (not the compression header). If you need the compression header information use the astropy module directly. >>> fits_fn = getfixture('tiny_fits_file') >>> getval(fits_fn, 'IMAGEID') 'PAN001_XXXXXX_20160909T081152' Args: fn (str): Path to FITS file. Returns: str or float: Value from header (with no type conversion). """ ext = 0 if fn.endswith('.fz'): ext = 1 return fits.getval(fn, *args, ext=ext, **kwargs)