Source code for rubin_scheduler.utils.healpy_utils

__all__ = (
    "hpid2_ra_dec",
    "ra_dec2_hpid",
    "healbin",
    "_hpid2_ra_dec",
    "_ra_dec2_hpid",
    "_healbin",
    "moc2array",
    "hp_grow_argsort",
)

import warnings

import healpy as hp
import numpy as np


def _hpid2_ra_dec(nside, hpids, **kwargs):
    """
    Correct for healpy being silly and running dec from 0-180.

    Parameters
    ----------
    nside : int
        Must be a value of 2^N.
    hpids : np.array
        Array (or single value) of healpixel IDs.

    Returns
    -------
    ra_ret : float (or np.array)
        RA positions of the input healpixel IDs. In radians.
    dec_ret : float (or np.array)
        Dec positions of the input healpixel IDs. In radians.
    """
    lat, lon = hp.pix2ang(nside, hpids, **kwargs)
    dec_ret = np.pi / 2.0 - lat
    ra_ret = lon

    return ra_ret, dec_ret


[docs] def hpid2_ra_dec(nside, hpids, **kwargs): """ Correct for healpy being silly and running dec from 0-180. Parameters ---------- nside : int Must be a value of 2^N. hpids : np.array Array (or single value) of healpixel IDs. Returns ------- raRet : float (or np.array) RA positions of the input healpixel IDs. In degrees. decRet : float (or np.array) Dec positions of the input healpixel IDs. In degrees. """ ra, dec = _hpid2_ra_dec(nside, hpids, **kwargs) return np.degrees(ra), np.degrees(dec)
def _ra_dec2_hpid(nside, ra, dec, **kwargs): """ Assign ra,dec points to the correct healpixel. Parameters ---------- nside : int Must be a value of 2^N. ra : np.array RA values to assign to healpixels. Radians. dec : np.array Dec values to assign to healpixels. Radians. Returns ------- hpids : np.array Healpixel IDs for the input positions. """ lat = np.pi / 2.0 - dec hpids = hp.ang2pix(nside, lat, ra, **kwargs) return hpids
[docs] def ra_dec2_hpid(nside, ra, dec, **kwargs): """ Assign ra,dec points to the correct healpixel. Parameters ---------- nside : int Must be a value of 2^N. ra : np.array RA values to assign to healpixels. Degrees. dec : np.array Dec values to assign to healpixels. Degrees. Returns ------- hpids : np.array Healpixel IDs for the input positions. """ return _ra_dec2_hpid(nside, np.radians(ra), np.radians(dec), **kwargs)
def _healbin(ra, dec, values, nside=128, reduce_func=np.mean, dtype=float, fill_val=hp.UNSEEN): """ Take arrays of ra's, dec's, and value and bin into healpixels. Like numpy.hexbin but for bins on a sphere. Parameters ---------- ra : np.array RA positions of the data points. Radians. dec : np.array Dec positions of the data points. Radians values : np.array The values at each ra,dec position. nside : int Healpixel nside resolution. Must be a value of 2^N. reduce_func : function (numpy.mean) A function that will return a single value given a subset of `values`. dtype : dtype ('float') Data type of the resulting mask fill_val : float (hp.UNSEEN) Value to fill in with healpixels that have no value. Default is the healpy mask value. Returns ------- map_vals : np.array A numpy array that is a valid Healpixel map. """ hpids = _ra_dec2_hpid(nside, ra, dec) order = np.argsort(hpids) hpids = hpids[order] values = values[order] pixids = np.unique(hpids) left = np.searchsorted(hpids, pixids) right = np.searchsorted(hpids, pixids, side="right") map_vals = np.zeros(hp.nside2npix(nside), dtype=dtype) + fill_val # Wow, I thought histogram would be faster than the loop, but # this has been faster! for i, idx in enumerate(pixids): map_vals[idx] = reduce_func(values[left[i] : right[i]]) # Change any NaNs to fill value map_vals[np.isnan(map_vals)] = fill_val return map_vals
[docs] def healbin(ra, dec, values, nside=128, reduce_func=np.mean, dtype=float, fill_val=hp.UNSEEN): """ Take arrays of ra's, dec's, and value and bin into healpixels. Like numpy.hexbin but for bins on a sphere. Parameters ---------- ra : np.array RA positions of the data points. Degrees. dec : np.array Dec positions of the data points. Degrees. values : np.array The values at each ra,dec position. nside : int Healpixel nside resolution. Must be a value of 2^N. reduce_func : function (numpy.mean) A function that will return a single value given a subset of `values`. dtype : dtype ('float') Data type of the resulting mask fill_val : float (hp.UNSEEN) Value to fill in with healpixels that have no value. Default is the healpy mask value. Returns ------- mapVals : np.array A numpy array that is a valid Healpixel map. """ return _healbin( np.radians(ra), np.radians(dec), values, nside=nside, reduce_func=reduce_func, dtype=dtype, fill_val=fill_val, )
[docs] def moc2array(data, uniq, nside=128, reduce_func=np.sum, density=True, fill_val=0.0): """Convert a Multi-Order Coverage Map to a single nside HEALPix array. Useful for converting maps output by LIGO alerts. Expect that future versions of healpy or astropy will be able to replace this functionality. Note that this is a convienence function that will probably degrade portions of the MOC that are sampled at high resolution. Details of HEALPix Mulit-Order Coverage map: http://ivoa.net/documents/MOC/20190404/PR-MOC-1.1-20190404.pdf Parameters ---------- data : np.array Data values for the MOC map uniq : np.array The UNIQ values for the MOC map nside : int (128) The output map nside reduce_func : function (np.sum) The function to use to combine data into single healpixels. density : bool (True) If True, multiplies data values by pixel area before applying reduce_func, and divides the final array by the output pixel area. Should be True if working on a probability density MOC. fill_val : float (0.) Value to fill empty HEALPixels with. Good choices include 0 (default), hp.UNSEEN, and np.nan. Returns ------- np.array : HEALpy array of nside. Units should be the same as the input map as processed by reduce_func. """ # NUNIQ packing, from page 12 of # http://ivoa.net/documents/MOC/20190404/PR-MOC-1.1-20190404.pdf orders = np.floor(np.log2(uniq / 4) / 2).astype(int) npixs = (uniq - 4 * 4**orders).astype(int) nsides = 2**orders names = ["ra", "dec", "area"] types = [float] * len(names) data_points = np.zeros(data.size, dtype=list(zip(names, types))) for order in np.unique(orders): good = np.where(orders == order) ra, dec = _hpid2_ra_dec(nsides[good][0], npixs[good], nest=True) data_points["ra"][good] = ra data_points["dec"][good] = dec data_points["area"][good] = hp.nside2pixarea(nsides[good][0]) if density: tobin_data = data * data_points["area"] else: tobin_data = data result = _healbin( data_points["ra"], data_points["dec"], tobin_data, nside=nside, reduce_func=reduce_func, fill_val=fill_val, ) if density: good = np.where(result != fill_val) result[good] = result[good] / hp.nside2pixarea(nside) return result
[docs] def hp_grow_argsort(in_map, ignore_nan=True): """Find the maximum of a healpix map, then orders healpixels by selecting the maximum bordering the selected area. Parameters ---------- in_map : np.array A valid HEALpix array ignore_nan : bool (True) If true, ignores values that are NaN Returns ------- ordered_hp : int array The indices that put in_map in the correct order """ nside = hp.npix2nside(np.size(in_map)) npix = np.size(in_map) pix_indx = np.arange(npix) if ignore_nan: not_nan_pix = ~np.isnan(in_map) npix = np.size(in_map[not_nan_pix]) # Check if we have already run with this nside if hasattr(hp_grow_argsort, "nside"): nside_match = nside == hp_grow_argsort.nside else: nside_match = False # If we already have neighbors chached, just use it if nside_match: neighbors = hp_grow_argsort.neighbors_cache else: # Running a new nside, or for the first time, compute # neighbors and set attributes Make a `bool` area to keep # track of which pixels still need to be sorted neighbors = hp.get_all_neighbours(nside, pix_indx).T hp_grow_argsort.neighbors_cache = neighbors hp_grow_argsort.nside = nside valid_neighbors_mask = np.ones(neighbors.shape, dtype=bool) # Sometimes there can be no neighbors in some directions valid_neighbors_mask[np.where(neighbors == -1)] = False ordered_hp = np.zeros(npix, dtype=int) current_max = np.where(in_map == np.nanmax(in_map))[0].min() ordered_hp[0] = current_max # Remove max from valid_neighbors. Can be clever with indexing # so we don't have to do a brute force search of the entire # neghbors array to mask it. # valid_neighbors_mask[np.where(neighbors == current_max)] = False current_neighbors = neighbors[current_max][valid_neighbors_mask[current_max]] sub_indx = np.where(neighbors[current_neighbors] == current_max) valid_neighbors_mask[(current_neighbors[sub_indx[0]], sub_indx[1])] = False for i in np.arange(1, npix): current_neighbors = neighbors[ordered_hp[0:i]][valid_neighbors_mask[ordered_hp[0:i]]] indx = np.where(in_map[current_neighbors] == np.nanmax(in_map[current_neighbors]))[0] if np.size(indx) == 0: # We can't connect to any more pixels warnings.warn("Can not connect to any more pixels.") return ordered_hp[0:i] else: indx = np.min(indx) current_max = current_neighbors[indx] ordered_hp[i] = current_max # current_max is no longer a valid neighbor to consider neighbors_of_current = neighbors[current_max] sub_indx = np.where(neighbors[neighbors_of_current] == current_max) valid_neighbors_mask[(neighbors_of_current[sub_indx[0]], sub_indx[1])] = False return ordered_hp