rosalia.utils

Functions

MJysr_to_jyarcsec2(flux_mjy_sr)
angular_distance(ra1, dec1, ra2, dec2)	Einsum version of the angular separation function by Astropy einsum_angular_distance_harversine v1: October 17, 2024 - Fastest version compared against numba, or astropy.
check_file_integrity(filenames)
check_fits_integrity(input)
check_number_of_extensions(input_name, ...)
circle_around_position(ra, dec, radius[, ...])
circular_hist(ax, x[, bins, density, ...])	Produce a circular histogram of angles on ax.
convert_ASDF_to_FITS(asdf_list, output)
create_angle_mask(xsize, ysize, q, theta[, ...])
create_custom_wcs(crpix, crval, cdelt[, ...])
create_dummy_exposure(telescope, instrument, ...)
create_dummy_image_with_wcs(ra_cen, dec_cen, ...)
create_radial_mask(xsize, ysize[, q, theta, ...])
delta_angular_separation(ra, dec)
detect_sci_extensions(input_name)
divide_array_in_chunks(array, chunk_size)
download_file(url[, verbose])	Downloads the file described as an url address.
ds9tomask(fname, nx, ny, outname)
erwinspacing(minimum, number[, rate, mode])
execute_cmd(cmd[, verbose])	Executes a shell command line.
exposure_inspector(input_name[, verbose, lite])	exposure_inspector: Inspects and returns critical information about the contents of an exposure telescope. :param input_name: Exposure file to be inspected. It can be a string with the name of the file, a list of files, or a pattern with *. :type input_name: str, list :return: Exposure identity - A dictionary with critical information about the exposure, including pointing (right ascension and declination), position angle, telescope, instrument, detector, filter, and a WCS (Astropy and GWCS). :rtype: dict, pd.DataFrame.
exposure_inspector_asdf(input_name[, ...])
exposure_inspector_fits(input_name[, ...])
exposure_inspector_single(input_name[, ...])	Inspects and returns critical information about the contents of a telescope exposure, stored as a FITS or ADSF file.
find_SCA_EXTNAME(EXTNAME)
find_max_angular_size_of_image(wcs[, ...])	Returns the maximum angular extension of an image.
find_nearest_index(array, value)
find_subposition_EXTNAME(EXTNAME)
flambda_to_fnu(flambda, wavelength)
fnu_to_flambda(fnu, wavelength)
generate_image_interpolator(data[, x, y])
get_astropywcs_info_from_sciexts(filename, ...)
get_data_and_wcs(input_name, ext)	Opens a fits file and returns the data and wcs at a certain extension.
get_keys_from_header(fits_list, index[, ext])
get_parameters_list(fits_list, index[, ext])
get_pixscale(fits_name, ext)
great_circle_ra_dec_shift(theta, phi)	Estimates the new coordinates (ra2, dec2) after moving an angular distance theta (radial direction) in the phi direction (0 deg, North, counterclockwise) along a Great Circle from the Equator (ra=0, dec=0) Adapted from Great Circle navigation: https://en.wikipedia.org/wiki/Great-circle_navigation
hp_resol2nside(resolution)	This program converts a resolution in degrees to the nside parameter of healpix.
interpolate_location_in_fits(fits_name, ext, ...)	This program interpolates the value of a FITS file at the location of the input coordinates (ra, dec).
load_dict(input_name[, verbose])	Load a python object using pickle.
make_ds9_region(ra, dec[, output])
make_profile(image[, radial_mask, ext, ...])
mask_sources(file_name, ext)
measure_maglim(mu_sky, instrument, ...[, ...])	Measure the limiting magnitude of an image given the sky background level, the instrument, filter, telescope and exposure time.
modify_keyword_hdr(input_name, ext, keyword, ...)
position_angle(ra1, dec1, ra2, dec2)	Einsum version of the position angle function by Astropy einsum_angular_distance_harversine v1: October 17, 2024
radec_to_xy(ra, dec, fits_name, ext)
read_ds9reg(fname)
reproject_roman_wfi_fits(input_name, ...)
run_basic_astrodrizzle(file_name)
run_basic_noisechisel(file_name, ext)
run_swarp(pattern, outname[, scale, ...])	run_swarp: This program runs SWARP on the input pattern of files, and generates a mosaic with the output name specified in outname. The pattern can be a string with the name of the file, a list of files, or a pattern with *. The output mosaic will be saved as outname, and if scale is different from 1, a scaled version of the mosaic will be saved as outname with the suffix "_scaled.fits". .
save_dict(dictionary, input_name[, verbose])	Save a python object using pickle.
save_fits(array, name[, header, extname, ...])
separation_and_position_angle(ra1, dec1, ...)	Einsum version of the angular separation function by Astropy einsum_angular_distance_harversine v1: October 17, 2024 - Fastest version compared against numba, or astropy.
sphere_dist(ra1, dec1, ra2, dec2)	A faster separation calculator than astropy solution.
thetaphi_2_radec(theta, phi)
write_parameters_list(fits_list, index, value)
xy_to_radec(x, y, fits_name, ext)