Source code for pyuvdata.uvdata.miriad

# -*- mode: python; coding: utf-8 -*-
# Copyright (c) 2018 Radio Astronomy Software Group
# Licensed under the 2-clause BSD License

"""Class for reading and writing Miriad files."""
import os
import shutil
import numpy as np
import itertools
import warnings
from astropy import constants as const
from astropy.coordinates import Angle, SkyCoord

from .uvdata import UVData
from .. import telescopes as uvtel
from .. import utils as uvutils

__all__ = ["Miriad"]


[docs]class Miriad(UVData): """ Defines a Miriad-specific subclass of UVData for reading and writing Miriad files. This class should not be interacted with directly, instead use the read and write_miriad methods on the UVData class. """ def _pol_to_ind(self, pol): if self.polarization_array is None: raise ValueError( "Can't index polarization {p} because " "polarization_array is not set".format(p=pol) ) pol_ind = np.argwhere(self.polarization_array == pol) if len(pol_ind) != 1: raise ValueError( "multiple matches for pol={pol} in " "polarization_array".format(pol=pol) ) return pol_ind def _load_miriad_variables(self, uv): """ Load miriad variables from an aipy.miriad UV descriptor onto self. Parameters ---------- uv : aipy.miriad.UV aipy object to load variables from. Returns ------- default_miriad_variables : list of str list of default miriad variables other_miriad_variables: list of str list of other miriad variables extra_miriad_variables: list of str list of extra, non-standard variables """ # list of miriad variables always read # NB: this includes variables in try/except (i.e. not all variables are # necessarily present in the miriad file) default_miriad_variables = [ "nchan", "npol", "inttime", "sdf", "source", "telescop", "latitud", "longitu", "altitude", "history", "visunits", "instrume", "dut1", "gst0", "rdate", "timesys", "xorient", "cnt", "ra", "dec", "lst", "pol", "nants", "antnames", "nblts", "ntimes", "nbls", "sfreq", "epoch", "antpos", "antnums", "degpdy", "antdiam", "phsframe", "xorient", "bltorder", ] # list of miriad variables not read, but also not interesting # NB: nspect (I think) is number of spectral windows, will want one day # NB: xyphase & xyamp are "On-line X Y phase/amplitude measurements" # which we may want in a calibration object some day # NB: systemp, xtsys & ytsys are "System temperatures of the antenna/X/Y feed" # which we may want in a calibration object some day # NB: freqs, leakage and bandpass may be part of a calibration object some day other_miriad_variables = [ "nspect", "obsdec", "vsource", "ischan", "restfreq", "nschan", "corr", "freq", "freqs", "leakage", "bandpass", "tscale", "coord", "veldop", "time", "obsra", "operator", "version", "axismax", "axisrms", "xyphase", "xyamp", "systemp", "xtsys", "ytsys", "baseline", "obspa", "antaz", "antel", "axisoff", "cable", "dazim", "delev", "jyperka", "phaselo1", "phaselo2", "phasem1", "themt", "wfreq", "wwidth", "wsystemp", "wcorr", ] extra_miriad_variables = [] for variable in uv.variables(): if ( variable not in default_miriad_variables and variable not in other_miriad_variables ): extra_miriad_variables.append(variable) miriad_header_data = { "Nfreqs": "nchan", "Nspws": "nspect", "Npols": "npol", "channel_width": "sdf", # in Ghz! "object_name": "source", "telescope_name": "telescop", } for item in miriad_header_data: if isinstance(uv[miriad_header_data[item]], str): header_value = uv[miriad_header_data[item]].replace("\x00", "") else: header_value = uv[miriad_header_data[item]] setattr(self, item, header_value) # Do the units and potential sign conversion for channel_width self.channel_width = np.abs(self.channel_width * 1e9) # change from GHz to Hz # Deal with the spectral axis now if self.Nspws > 1: self._set_flex_spw() # Channel widths are described per spw, just need to expand it out to be # for each frequency channel. self.channel_width = ( np.concatenate( tuple( np.abs(chan_width) + np.zeros(nchan) for (chan_width, nchan) in zip(uv["sdf"] * 1e9, uv["nschan"]) ) ) .flatten() .astype(np.float64) ) # Now setup frequency array # TODO: Spw axis to be collapsed in future release self.freq_array = np.reshape( np.concatenate( tuple( chan_width * np.arange(nchan) + sfreq for (chan_width, nchan, sfreq) in zip( uv["sdf"] * 1e9, uv["nschan"], uv["sfreq"] * 1e9 ) ) ) .flatten() .astype(np.float64), (1, -1), ) # TODO: Fix this to capture unsorted spectra self.flex_spw_id_array = np.concatenate( tuple( idx + np.zeros(nchan, dtype=int) for (idx, nchan) in zip(range(self.Nspws), uv["nschan"]) ) ) else: self.freq_array = np.reshape( np.arange(self.Nfreqs) * self.channel_width + uv["sfreq"] * 1e9, (1, -1) ) self.channel_width = np.float64(self.channel_width) self.spw_array = np.arange(self.Nspws) self.history = uv["history"] if not uvutils._check_history_version(self.history, self.pyuvdata_version_str): self.history += self.pyuvdata_version_str # check for pyuvdata variables that are not recognized miriad variables if "visunits" in uv.vartable.keys(): self.vis_units = uv["visunits"].replace("\x00", "") else: self.vis_units = "uncalib" # assume no calibration if "instrume" in uv.vartable.keys(): self.instrument = uv["instrume"].replace("\x00", "") else: self.instrument = self.telescope_name # set instrument = telescope if "dut1" in uv.vartable.keys(): self.dut1 = uv["dut1"] if "degpdy" in uv.vartable.keys(): self.earth_omega = uv["degpdy"] if "gst0" in uv.vartable.keys(): self.gst0 = uv["gst0"] if "rdate" in uv.vartable.keys(): self.rdate = uv["rdate"].replace("\x00", "") if "timesys" in uv.vartable.keys(): self.timesys = uv["timesys"].replace("\x00", "") if "xorient" in uv.vartable.keys(): self.x_orientation = uv["xorient"].replace("\x00", "") if "bltorder" in uv.vartable.keys(): blt_order_str = uv["bltorder"].replace("\x00", "") self.blt_order = tuple(blt_order_str.split(", ")) if self.blt_order == ("bda",): self._blt_order.form = (1,) return default_miriad_variables, other_miriad_variables, extra_miriad_variables def _load_telescope_coords(self, uv, correct_lat_lon=True): """ Load telescope lat, lon, alt coordinates from aipy.miriad UV descriptor. Parameters ---------- uv : aipy.miriad.UV aipy object to load lat, lon, alt coordinates from. correct_lat_lon : bool Option to update the latitude and longitude from the known_telescopes list if the altitude is missing. """ # check if telescope name is present if self.telescope_name is None: self._load_miriad_variables(uv) latitude = uv["latitud"] # in units of radians longitude = uv["longitu"] # Catch a weird case where where sometimes long is wrapped like RA (0 -> 2pi # instead of -pi -> pi) if longitude > np.pi: longitude -= 2 * np.pi try: altitude = uv["altitude"] self.telescope_location_lat_lon_alt = (latitude, longitude, altitude) except (KeyError): # get info from known telescopes. # Check to make sure the lat/lon values match reasonably well telescope_obj = uvtel.get_telescope(self.telescope_name) if telescope_obj is not False: tol = 2 * np.pi * 1e-3 / (60.0 * 60.0 * 24.0) # 1mas in radians lat_close = np.isclose( telescope_obj.telescope_location_lat_lon_alt[0], latitude, rtol=0, atol=tol, ) lon_close = np.isclose( telescope_obj.telescope_location_lat_lon_alt[1], longitude, rtol=0, atol=tol, ) if correct_lat_lon: self.telescope_location_lat_lon_alt = ( telescope_obj.telescope_location_lat_lon_alt ) else: self.telescope_location_lat_lon_alt = ( latitude, longitude, telescope_obj.telescope_location_lat_lon_alt[2], ) if lat_close and lon_close: if correct_lat_lon: warnings.warn( "Altitude is not present in Miriad file, " "using known location values for " "{telescope_name}.".format( telescope_name=telescope_obj.telescope_name ) ) else: warnings.warn( "Altitude is not present in Miriad file, " "using known location altitude value " "for {telescope_name} and lat/lon from " "file.".format(telescope_name=telescope_obj.telescope_name) ) else: warn_string = "Altitude is not present in file " if not lat_close and not lon_close: warn_string = ( warn_string + "and latitude and longitude values do not match values " ) else: if not lat_close: warn_string = ( warn_string + "and latitude value does not match value " ) else: warn_string = ( warn_string + "and longitude value does not match value " ) if correct_lat_lon: warn_string = ( warn_string + "for {telescope_name} in known " "telescopes. Using values from known " "telescopes.".format( telescope_name=telescope_obj.telescope_name ) ) warnings.warn(warn_string) else: warn_string = ( warn_string + "for {telescope_name} in known " "telescopes. Using altitude value from known " "telescopes and lat/lon from " "file.".format(telescope_name=telescope_obj.telescope_name) ) warnings.warn(warn_string) else: warnings.warn( "Altitude is not present in Miriad file, and " "telescope {telescope_name} is not in " "known_telescopes. Telescope location will be " "set using antenna positions.".format( telescope_name=self.telescope_name ) ) def _load_antpos(self, uv, sorted_unique_ants=None, correct_lat_lon=True): """ Load antennas and their positions from a Miriad UV descriptor. Parameters ---------- uv : aipy.miriad.UV aipy object to antennas and positions from. sorted_unique_ants : list of ints, optional List of unique antennas. correct_lat_lon : bool Option to update the latitude and longitude from the known_telescopes list if the altitude is missing. """ # check if telescope coords exist if self.telescope_location_lat_lon_alt is None: self._load_telescope_coords(uv, correct_lat_lon=correct_lat_lon) latitude = uv["latitud"] # in units of radians longitude = uv["longitu"] # Miriad has no way to keep track of antenna numbers, so the antenna # numbers are simply the index for each antenna in any array that # describes antenna attributes (e.g. antpos for the antenna_postions). # Therefore on write, nants (which gives the size of the antpos array) # needs to be increased to be the max value of antenna_numbers+1 and the # antpos array needs to be inflated with zeros at locations where we # don't have antenna information. These inflations need to be undone at # read. If the file was written by pyuvdata, then the variable antnums # will be present and we can use it, otherwise we need to test for zeros # in the antpos array and/or antennas with no visibilities. try: # The antnums variable will only exist if the file was written with # pyuvdata. # For some reason Miriad doesn't handle an array of integers properly, # so we convert to floats on write and back here self.antenna_numbers = uv["antnums"].astype(int) self.Nants_telescope = len(self.antenna_numbers) except (KeyError): self.antenna_numbers = None self.Nants_telescope = None nants = uv["nants"] try: # Miriad stores antpos values in units of ns, pyuvdata uses meters. antpos = uv["antpos"].reshape(3, nants).T * const.c.to("m/ns").value # first figure out what are good antenna positions so we can only # use the non-zero ones to evaluate position information antpos_length = np.sqrt(np.sum(np.abs(antpos) ** 2, axis=1)) good_antpos = np.where(antpos_length > 0)[0] mean_antpos_length = np.mean(antpos_length[good_antpos]) if mean_antpos_length > 6.35e6 and mean_antpos_length < 6.39e6: absolute_positions = True else: absolute_positions = False # Miriad stores antpos values in a rotated ECEF coordinate system # where the x-axis goes through the local meridan. Need to convert # these positions back to standard ECEF and if they are absolute # positions, subtract off the telescope position to make them # relative to the array center. ecef_antpos = uvutils.ECEF_from_rotECEF(antpos, longitude) if self.telescope_location is not None: if absolute_positions: rel_ecef_antpos = ecef_antpos - self.telescope_location # maintain zeros because they mark missing data rel_ecef_antpos[np.where(antpos_length == 0)[0]] = ecef_antpos[ np.where(antpos_length == 0)[0] ] else: rel_ecef_antpos = ecef_antpos else: self.telescope_location = np.mean(ecef_antpos[good_antpos, :], axis=0) valid_location = self._telescope_location.check_acceptability()[0] # check to see if this could be a valid telescope_location if valid_location: mean_lat, mean_lon, mean_alt = self.telescope_location_lat_lon_alt tol = 2 * np.pi / (60.0 * 60.0 * 24.0) # 1 arcsecond in radians mean_lat_close = np.isclose(mean_lat, latitude, rtol=0, atol=tol) mean_lon_close = np.isclose(mean_lon, longitude, rtol=0, atol=tol) if mean_lat_close and mean_lon_close: # this looks like a valid telescope_location, and the # mean antenna lat & lon values are close. Set the # telescope_location using the file lat/lons and the mean alt. # Then subtract it off of the antenna positions warnings.warn( "Telescope location is not set, but antenna " "positions are present. Mean antenna latitude and " "longitude values match file values, so " "telescope_position will be set using the " "mean of the antenna altitudes" ) self.telescope_location_lat_lon_alt = ( latitude, longitude, mean_alt, ) rel_ecef_antpos = ecef_antpos - self.telescope_location else: # this looks like a valid telescope_location, but the # mean antenna lat & lon values are not close. Set the # telescope_location using the file lat/lons at sea level. # Then subtract it off of the antenna positions self.telescope_location_lat_lon_alt = (latitude, longitude, 0) warn_string = ( "Telescope location is set at sealevel at " "the file lat/lon coordinates. Antenna " "positions are present, but the mean " "antenna " ) rel_ecef_antpos = ecef_antpos - self.telescope_location if not mean_lat_close and not mean_lon_close: warn_string += ( "latitude and longitude values do not " "match file values so they are not used " "for altiude." ) elif not mean_lat_close: warn_string += ( "latitude value does not " "match file values so they are not used " "for altiude." ) else: warn_string += ( "longitude value does not " "match file values so they are not used " "for altiude." ) warnings.warn(warn_string) else: # This does not give a valid telescope_location. Instead # calculate it from the file lat/lon and sea level for altiude self.telescope_location_lat_lon_alt = (latitude, longitude, 0) warn_string = ( "Telescope location is set at sealevel at " "the file lat/lon coordinates. Antenna " "positions are present, but the mean " "antenna " ) warn_string += ( "position does not give a " "telescope_location on the surface of the " "earth." ) if absolute_positions: rel_ecef_antpos = ecef_antpos - self.telescope_location else: warn_string += ( " Antenna positions do not appear to be " "on the surface of the earth and will be treated " "as relative." ) rel_ecef_antpos = ecef_antpos warnings.warn(warn_string) if self.Nants_telescope is not None: # in this case there is an antnums variable # (meaning that the file was written with pyuvdata), so we'll use it if nants == self.Nants_telescope: # no inflation, so just use the positions self.antenna_positions = rel_ecef_antpos else: # there is some inflation, just use the ones that appear in antnums self.antenna_positions = np.zeros( (self.Nants_telescope, 3), dtype=antpos.dtype ) for ai, num in enumerate(self.antenna_numbers): self.antenna_positions[ai, :] = rel_ecef_antpos[num, :] else: # there is no antnums variable (meaning that this file was not # written by pyuvdata), so we test for antennas with non-zero # positions and/or that appear in the visibility data # (meaning that they have entries in ant_1_array or ant_2_array) antpos_length = np.sqrt(np.sum(np.abs(antpos) ** 2, axis=1)) good_antpos = np.where(antpos_length > 0)[0] # take the union of the antennas with good positions (good_antpos) # and the antennas that have visisbilities (sorted_unique_ants) # if there are antennas with visibilities but zeroed positions # we issue a warning below if sorted_unique_ants is not None: ants_use = set(good_antpos).union(sorted_unique_ants) else: ants_use = set(good_antpos) # ants_use are the antennas we'll keep track of in the UVData # object, so they dictate Nants_telescope self.Nants_telescope = len(ants_use) self.antenna_numbers = np.array(list(ants_use)) self.antenna_positions = np.zeros( (self.Nants_telescope, 3), dtype=rel_ecef_antpos.dtype ) for ai, num in enumerate(self.antenna_numbers): if antpos_length[num] == 0: warnings.warn( "antenna number {n} has visibilities " "associated with it, but it has a position" " of (0,0,0)".format(n=num) ) else: # leave bad locations as zeros to make them obvious self.antenna_positions[ai, :] = rel_ecef_antpos[num, :] except (KeyError): # there is no antpos variable warnings.warn("Antenna positions are not present in the file.") self.antenna_positions = None if self.antenna_numbers is None: # there are no antenna_numbers or antenna_positions, so just use # the antennas present in the visibilities # (Nants_data will therefore match Nants_telescope) if sorted_unique_ants is not None: self.antenna_numbers = np.array(sorted_unique_ants) self.Nants_telescope = len(self.antenna_numbers) # antenna names is a foreign concept in miriad but required in other formats. try: # Here we deal with the way pyuvdata tacks it on to keep the # name information if we have it: # make it into one long comma-separated string ant_name_var = uv["antnames"] ant_name_str = ant_name_var.replace("\x00", "") ant_name_list = ant_name_str[1:-1].split(", ") self.antenna_names = ant_name_list except (KeyError): self.antenna_names = self.antenna_numbers.astype(str).tolist() # check for antenna diameters try: self.antenna_diameters = uv["antdiam"] except (KeyError): # backwards compatibility for when keyword was 'diameter' try: self.antenna_diameters = uv["diameter"] # if we find it, we need to remove it from extra_keywords to # keep from writing it out self.extra_keywords.pop("diameter") except (KeyError): pass if self.antenna_diameters is not None: self.antenna_diameters = self.antenna_diameters * np.ones( self.Nants_telescope, dtype=np.float64 ) def _read_miriad_metadata(self, uv, correct_lat_lon=True): """ Read in metadata (parameter info) but not data from a miriad file. Parameters ---------- uv : aipy.miriad.UV aipy object to load metadata from. correct_lat_lon : bool Option to update the latitude and longitude from the known_telescopes list if the altitude is missing. Returns ------- default_miriad_variables : list of str list of default miriad variables other_miriad_variables: list of str list of other miriad variables extra_miriad_variables: list of str list of extra, non-standard variables check_variables: dict dict of extra miriad variables to add to extra_keywords parameter. """ # load miriad variables ( default_miriad_variables, other_miriad_variables, extra_miriad_variables, ) = self._load_miriad_variables(uv) # dict of extra variables check_variables = {} for extra_variable in extra_miriad_variables: check_variables[extra_variable] = uv[extra_variable] # keep all single valued extra_variables as extra_keywords for key in check_variables.keys(): if type(check_variables[key]) == str: value = check_variables[key].replace("\x00", "") # check for booleans encoded as strings if value == "True": value = True elif value == "False": value = False self.extra_keywords[key] = value else: self.extra_keywords[key] = check_variables[key] # Check for items in itemtable to put into extra_keywords # These will end up as variables in written files, but is internally consistent. for key in uv.items(): # A few items that are not needed, we read elsewhere, or is not supported # when downselecting, so we don't read here. if ( key not in ["vartable", "history", "obstype"] and key not in other_miriad_variables ): if type(uv[key]) == str: value = uv[key].replace("\x00", "") value = uv[key].replace("\x01", "") if value == "True": value = True elif value == "False": value = False self.extra_keywords[key] = value else: self.extra_keywords[key] = uv[key] # load telescope coords self._load_telescope_coords(uv, correct_lat_lon=correct_lat_lon) # load antenna positions self._load_antpos(uv) return ( default_miriad_variables, other_miriad_variables, extra_miriad_variables, check_variables, )
[docs] def read_miriad( self, filepath, antenna_nums=None, ant_str=None, bls=None, polarizations=None, time_range=None, read_data=True, phase_type=None, correct_lat_lon=True, background_lsts=True, run_check=True, check_extra=True, run_check_acceptability=True, strict_uvw_antpos_check=False, calc_lst=True, fix_old_proj=False, fix_use_ant_pos=True, ): """ Read in data from a miriad file. Parameters ---------- filepath : str The miriad root directory to read from. antenna_nums : array_like of int, optional The antennas numbers to read into the object. bls : list of tuple, optional A list of antenna number tuples (e.g. [(0, 1), (3, 2)]) or a list of baseline 3-tuples (e.g. [(0, 1, 'xx'), (2, 3, 'yy')]) specifying baselines to include when reading data into the object. For length-2 tuples, the ordering of the numbers within the tuple does not matter. For length-3 tuples, the polarization string is in the order of the two antennas. If length-3 tuples are provided, `polarizations` must be None. ant_str : str, optional A string containing information about what antenna numbers and polarizations to include when reading data into the object. Can be 'auto', 'cross', 'all', or combinations of antenna numbers and polarizations (e.g. '1', '1_2', '1x_2y'). See tutorial for more examples of valid strings and the behavior of different forms for ant_str. If '1x_2y,2y_3y' is passed, both polarizations 'xy' and 'yy' will be kept for both baselines (1, 2) and (2, 3) to return a valid pyuvdata object. An ant_str cannot be passed in addition to any of `antenna_nums`, `bls` or `polarizations` parameters, if it is a ValueError will be raised. polarizations : array_like of int or str, optional List of polarization integers or strings to read-in. e.g. ['xx', 'yy', ...] time_range : list of float, optional len-2 list containing min and max range of times in Julian Date to include when reading data into the object. e.g. [2458115.20, 2458115.40] read_data : bool Read in the uvws, times, visibility and flag data. If set to False, only the metadata that can be read quickly (without reading the data) will be read in. For Miriad, some of the normally required metadata are not fast to read in (e.g. uvws, times) so will not be read in if this keyword is False. Therefore, setting read_data to False results in an incompletely defined object (check will not pass). phase_type : str, optional Option to specify the phasing status of the data. Options are 'drift', 'phased' or None. 'drift' means the data are zenith drift data, 'phased' means the data are phased to a single RA/Dec. Default is None meaning it will be guessed at based on the file contents. correct_lat_lon : bool Option to update the latitude and longitude from the known_telescopes list if the altitude is missing. background_lsts : bool When set to True, the lst_array is calculated in a background thread. run_check : bool Option to check for the existence and proper shapes of parameters after after reading in the file (the default is True, meaning the check will be run). Ignored if read_data is False. check_extra : bool Option to check optional parameters as well as required ones (the default is True, meaning the optional parameters will be checked). Ignored if read_data is False. run_check_acceptability : bool Option to check acceptable range of the values of parameters after reading in the file (the default is True, meaning the acceptable range check will be done). Ignored if read_data is False. strict_uvw_antpos_check : bool Option to raise an error rather than a warning if the check that uvws match antenna positions does not pass. calc_lst : bool Recalculate the LST values that are present within the file, useful in cases where the "online" calculate values have precision or value errors. Default is True. fix_old_proj : bool Applies a fix to uvw-coordinates and phasing, assuming that the old `phase` method was used prior to writing the data, which had errors of the order of one part in 1e4 - 1e5. See the phasing memo for more details. fix_use_ant_pos : bool If setting `fix_old_proj` to True, use the antenna positions to derive the correct uvw-coordinates rather than using the baseline vectors. Default is True. Raises ------ IOError If root file directory doesn't exist. ValueError If incompatible select keywords are set (e.g. `ant_str` with other antenna selectors, `times` and `time_range`) or select keywords exclude all data or if keywords are set to the wrong type. If the data are multi source or have multiple spectral windows. If the metadata are not internally consistent. """ from . import aipy_extracts if not os.path.exists(filepath): raise IOError(filepath + " not found") uv = aipy_extracts.UV(filepath) # load metadata ( default_miriad_variables, other_miriad_variables, extra_miriad_variables, check_variables, ) = self._read_miriad_metadata(uv, correct_lat_lon=correct_lat_lon) # update filename attribute basename = filepath.rstrip("/") self.filename = [os.path.basename(basename)] self._filename.form = (1,) if not read_data: # don't read in the data. This means the object is incomplete, # but that may not matter for many purposes. return history_update_string = " Downselected to specific " n_selects = 0 # select on ant_str if provided if ant_str is not None: # type check if not isinstance(ant_str, (str, np.str_)): raise ValueError("ant_str must be a string") if antenna_nums is not None or bls is not None: raise ValueError("Cannot provide ant_str with antenna_nums or bls") aipy_extracts.uv_selector(uv, ant_str) if ant_str != "all": history_update_string += "antenna pairs" n_selects += 1 # select on antenna_nums and/or bls using aipy_extracts.uv_selector if antenna_nums is not None or bls is not None: antpair_str = "" if antenna_nums is not None: # type check err_msg = "antenna_nums must be a list of antenna number integers" if not isinstance(antenna_nums, (np.ndarray, list)): raise ValueError(err_msg) if not isinstance(antenna_nums[0], (int, np.integer)): raise ValueError(err_msg) # get all possible combinations antpairs = list( itertools.combinations_with_replacement(antenna_nums, 2) ) # convert antenna numbers to string form required by # aipy_extracts.uv_selector antpair_str_list = ["_".join([str(a) for a in ap]) for ap in antpairs] history_update_string += "antennas" n_selects += 1 if bls is not None: if isinstance(bls, tuple) and (len(bls) == 2 or len(bls) == 3): bls = [bls] if not all(isinstance(item, tuple) for item in bls): raise ValueError( "bls must be a list of tuples of antenna numbers " "(optionally with polarization)." ) if all(len(item) == 2 for item in bls): if not all( [isinstance(item[0], (int, np.integer,)) for item in bls] + [isinstance(item[1], (int, np.integer,)) for item in bls] ): raise ValueError( "bls must be a list of tuples of antenna numbers " "(optionally with polarization)." ) elif all(len(item) == 3 for item in bls): if polarizations is not None: raise ValueError( "Cannot provide length-3 tuples and also specify " "polarizations." ) if not all(isinstance(item[2], str) for item in bls): raise ValueError( "The third element in each bl must be a polarization string" ) else: raise ValueError("bls tuples must be all length-2 or all length-3") bl_str_list = [] bl_pols = set() for bl in bls: if bl[0] <= bl[1]: bl_str_list.append(str(bl[0]) + "_" + str(bl[1])) if len(bl) == 3: bl_pols.add(bl[2]) else: bl_str_list.append(str(bl[1]) + "_" + str(bl[0])) if len(bl) == 3: bl_pols.add(uvutils.conj_pol(bl[2])) if n_selects > 0: # combine antpair_str_list and bl_str_list with an intersection antpair_str_list = list( set(antpair_str_list).intersection(bl_str_list) ) else: antpair_str_list = bl_str_list if len(bl_pols) > 0: polarizations = list(bl_pols) if n_selects > 0: history_update_string += ", baselines" else: history_update_string += "baselines" n_selects += 1 # convert antenna pair list to string form required by # aipy_extracts.uv_selector antpair_str += ",".join(antpair_str_list) aipy_extracts.uv_selector(uv, antpair_str) # select on time range if time_range is not None: # type check err_msg = ( "time_range must be a len-2 list of Julian Date floats, " "Ex: [2458115.2, 2458115.6]" ) if not isinstance(time_range, (list, np.ndarray)): raise ValueError(err_msg) if len(time_range) != 2: raise ValueError(err_msg) if not np.array( [isinstance(t, (float, np.floating, np.float64)) for t in time_range] ).all(): raise ValueError(err_msg) # UVData.time_array marks center of integration, while Miriad # 'time' marks beginning # assume time_range refers to the center of the integrations, # so subtract 1/2 an integration before using with miriad select time_range_use = np.array(time_range) - uv["inttime"] / (24 * 3600.0) / 2 uv.select("time", time_range_use[0], time_range_use[1], include=True) if n_selects > 0: history_update_string += ", times" else: history_update_string += "times" n_selects += 1 # select on polarizations if polarizations is not None: # type check err_msg = ( "pols must be a list of polarization strings or ints, " "Ex: ['xx', ...] or [-5, ...]" ) if not isinstance(polarizations, (list, np.ndarray)): raise ValueError(err_msg) if not np.array( [isinstance(p, (str, np.str_, int, np.integer)) for p in polarizations] ).all(): raise ValueError(err_msg) # convert to pol integer if string polarizations = [ p if isinstance(p, (int, np.integer)) else uvutils.polstr2num(p, x_orientation=self.x_orientation) for p in polarizations ] # iterate through all possible pols and reject if not in pols pol_list = [] for p in np.arange(-8, 5): if p not in polarizations: uv.select("polarization", p, p, include=False) else: pol_list.append(p) # check not empty if len(pol_list) == 0: raise ValueError("No polarizations in data matched input") if n_selects > 0: history_update_string += ", polarizations" else: history_update_string += "polarizations" n_selects += 1 history_update_string += " using pyuvdata." if n_selects > 0: self.history += history_update_string data_accumulator = {} pol_list = [] app_ra = None app_dec = None frame_pa = None epoch = None sou_dict = {} Nphase = 0 record_epoch = "epoch" in uv.vartable.keys() record_app = ("obsra" in uv.vartable.keys()) and ( "obsdec" in uv.vartable.keys() ) record_pa = "obspa" in uv.vartable.keys() # dra_list - Stubbing out for later # ddec_list - Stubbing out for later for (uvw, t, (i, j)), d, f in uv.all_data(raw=True): # control for the case of only a single spw not showing up in # the dimension # Note that the (i, j) tuple is calculated from a baseline number in # _miriad (see miriad_wrap.h). The i, j values are also adjusted by _miriad # to start at 0 rather than 1. # N.B. (Karto): So the below is right, but for the wrong reasons. The data # array return is of length nchan, which encompasses the total number of # channels in all spectral windows, where 'ischan' and 'nschan' demark the # starting positions and length of the individual windows. I don't think # this array should ever _not_ be 1D, but the below does cast the shape of # the data array correctly so that the vestigial spw-axis is preserved. At # some point, the below will need to be fixed -- I'm keeping this here so # that I can skip reading through the MIRIAD programmers guide yet again. if len(d.shape) == 1: d.shape = (1,) + d.shape if np.size(d) != self.Nfreqs: raise ValueError("Number of channels in spectrum has changed!") try: cnt = uv["cnt"] except (KeyError): cnt = np.ones(d.shape, dtype=np.float64) ra = uv["ra"] dec = uv["dec"] if record_epoch: epoch = uv["epoch"] if record_app: app_ra = uv["obsra"] app_dec = uv["obsdec"] if record_pa: frame_pa = uv["obspa"] # LST is pulled from the file here, atlhough as some PAPER/early HERA # data calculated LST from pyephem (which is inconsistent w/ astropy # to the order of ~5 seconds), these values can be recalculated by # setting `calc_lst=True` when calling read_miriad. lst = uv["lst"] inttime = uv["inttime"] try: sou_id = sou_dict[uv["source"]] except KeyError: sou_dict[uv["source"]] = Nphase sou_id = Nphase Nphase += 1 try: # TODO: Gotta clean this up at some point - there are going to be # addition things to stick into the metadata accumulator, and accessing # those values by index number will likely make it more difficult to # maintain/expand the code in the future. data_accumulator[uv["pol"]].append( [ uvw, # Entry 0 t, # Entry 1 i, # Entry 2 j, # Entry 3 d, # Entry 4 f, # Entry 5 cnt, # Entry 6 ra, # Entry 7 dec, # Entry 8 inttime, # Entry 9 sou_id, # Entry 10 epoch, # Entry 11 app_ra, # Entry 12 app_dec, # Entry 13 frame_pa, # Entry 14 lst, # Entry 15 ] ) except (KeyError): data_accumulator[uv["pol"]] = [ [ uvw, # Entry 0 t, # Entry 1 i, # Entry 2 j, # Entry 3 d, # Entry 4 f, # Entry 5 cnt, # Entry 6 ra, # Entry 7 dec, # Entry 8 inttime, # Entry 9 sou_id, # Entry 10 epoch, # Entry 11 app_ra, # Entry 12 app_dec, # Entry 13 frame_pa, # Entry 14 lst, # Entry 15 ] ] pol_list.append(uv["pol"]) # NB: flag types in miriad are usually ints if len(list(data_accumulator.keys())) == 0: raise ValueError( "No data is present, probably as a result of " "select on read that excludes all the data" ) for pol, data in data_accumulator.items(): # make array "object" dtype because underlying array may be ragged data_accumulator[pol] = np.array(data, dtype="object") self.polarization_array = np.array(pol_list) if polarizations is None: # A select on read would make the header npols not match the pols # in the data if len(self.polarization_array) != self.Npols: warnings.warn( "npols={npols} but found {n} pols in data file".format( npols=self.Npols, n=len(self.polarization_array) ) ) self.Npols = len(pol_list) # makes a data_array (and flag_array) of zeroes to be filled in by # data values # any missing data will have zeros # use set to get the unique list of all times ever listed in the file # iterate over polarizations and all spectra (bls and times) in two # nested loops, then flatten into a single vector, then set # then list again. times = list( set(np.concatenate([[k[1] for k in d] for d in data_accumulator.values()])) ) times = np.sort(times) ant_i_unique = list( set(np.concatenate([[k[2] for k in d] for d in data_accumulator.values()])) ) ant_j_unique = list( set(np.concatenate([[k[3] for k in d] for d in data_accumulator.values()])) ) sorted_unique_ants = sorted(set(ant_i_unique + ant_j_unique)) ant_i_unique = np.array(ant_i_unique) ant_j_unique = np.array(ant_j_unique) # Determine maximum digits needed to distinguish different values if sorted_unique_ants[-1] > 0: ndig_ant = np.ceil(np.log10(sorted_unique_ants[-1])).astype(int) + 1 else: ndig_ant = 1 # Be excessive in precision because we use the floating point values as # dictionary keys later prec_t = -2 * np.floor(np.log10(self._time_array.tols[-1])).astype(int) ndig_t = np.ceil(np.log10(times[-1])).astype(int) + prec_t + 2 blts = [] for d in data_accumulator.values(): for k in d: blt = [ "{1:.{0}f}".format(prec_t, k[1]).zfill(ndig_t), str(k[2]).zfill(ndig_ant), str(k[3]).zfill(ndig_ant), str(k[9]).zfill(ndig_t), ] blt = "_".join(blt) blts.append(blt) unique_blts = np.unique(np.array(blts)) reverse_inds = dict(zip(unique_blts, range(len(unique_blts)))) self.Nants_data = len(sorted_unique_ants) # load antennas and antenna positions using sorted unique ants list self._load_antpos(uv, sorted_unique_ants=sorted_unique_ants) # form up a grid which indexes time and baselines along the 'long' # axis of the visdata array tij_grid = np.array([list(map(float, x.split("_"))) for x in unique_blts]) t_grid, ant_i_grid, ant_j_grid, int_grid = tij_grid.T # set the data sizes if ( antenna_nums is None and bls is None and ant_str is None and time_range is None ): try: self.Nblts = uv["nblts"] if self.Nblts != len(t_grid): warnings.warn( "Nblts does not match the number of unique blts in the data" ) self.Nblts = len(t_grid) except (KeyError): self.Nblts = len(t_grid) else: # The select on read will make the header nblts not match the # number of unique blts self.Nblts = len(t_grid) if time_range is None: try: self.Ntimes = uv["ntimes"] if self.Ntimes != len(times): warnings.warn( "Ntimes does not match the number of unique times in the data" ) self.Ntimes = len(times) except (KeyError): self.Ntimes = len(times) else: # The select on read will make the header ntimes not match the # number of unique times self.Ntimes = len(times) # UVData.time_array marks center of integration, while Miriad 'time' # marks beginning # also, int_grid is in units of seconds, so we need to convert to days self.time_array = t_grid + int_grid / (24 * 3600.0) / 2 self.integration_time = np.asarray(int_grid, dtype=np.float64) self.ant_1_array = ant_i_grid.astype(int) self.ant_2_array = ant_j_grid.astype(int) self.baseline_array = self.antnums_to_baseline( ant_i_grid.astype(int), ant_j_grid.astype(int) ) if antenna_nums is None and bls is None and ant_str is None: try: self.Nbls = uv["nbls"] if self.Nbls != len(np.unique(self.baseline_array)): warnings.warn( "Nbls does not match the number of unique baselines in the data" ) self.Nbls = len(np.unique(self.baseline_array)) except (KeyError): self.Nbls = len(np.unique(self.baseline_array)) else: # The select on read will make the header nbls not match the # number of unique bls self.Nbls = len(np.unique(self.baseline_array)) # slot the data into a grid # TODO: Spw axis to be collapsed in future release self.data_array = np.zeros( (self.Nblts, 1, self.Nfreqs, self.Npols), dtype=np.complex64 ) self.flag_array = np.ones(self.data_array.shape, dtype=np.bool_) self.uvw_array = np.zeros((self.Nblts, 3)) # NOTE: Using our lst calculator, which uses astropy, # instead of _miriad values which come from pyephem. # The differences are of order 5 seconds. proc = None if (self.telescope_location is not None) and calc_lst: proc = self.set_lsts_from_time_array(background=background_lsts) self.nsample_array = np.ones(self.data_array.shape, dtype=np.float64) # Temporary arrays to hold polarization axis, which will be collapsed ra_pol_list = np.zeros((self.Nblts, self.Npols)) dec_pol_list = np.zeros((self.Nblts, self.Npols)) uvw_pol_list = np.zeros((self.Nblts, 3, self.Npols)) sou_id_pol_list = np.zeros((self.Nblts, self.Npols), dtype=int) epoch_pol_list = np.zeros((self.Nblts, self.Npols)) app_ra_pol_list = np.zeros((self.Nblts, self.Npols)) app_dec_pol_list = np.zeros((self.Nblts, self.Npols)) frame_pa_pol_list = np.zeros((self.Nblts, self.Npols)) lst_pol_list = np.zeros((self.Nblts, self.Npols)) c_ns = const.c.to("m/ns").value for pol, data in data_accumulator.items(): pol_ind = self._pol_to_ind(pol) for ind, d in enumerate(data): blt = [ "{1:.{0}f}".format(prec_t, d[1]).zfill(ndig_t), str(d[2]).zfill(ndig_ant), str(d[3]).zfill(ndig_ant), str(d[9]).zfill(ndig_t), ] blt = "_".join(blt) blt_index = reverse_inds[blt] self.data_array[blt_index, :, :, pol_ind] = d[4] self.flag_array[blt_index, :, :, pol_ind] = d[5] self.nsample_array[blt_index, :, :, pol_ind] = d[6] # because there are uvws/ra/dec for each pol, and one pol may not # have that visibility, we collapse along the polarization # axis but avoid any missing visbilities uvw = d[0] * c_ns uvw.shape = (1, 3) uvw_pol_list[blt_index, :, pol_ind] = uvw ra_pol_list[blt_index, pol_ind] = d[7] dec_pol_list[blt_index, pol_ind] = d[8] sou_id_pol_list[blt_index, pol_ind] = d[10] epoch_pol_list[blt_index, pol_ind] = d[11] app_ra_pol_list[blt_index, pol_ind] = d[12] app_dec_pol_list[blt_index, pol_ind] = d[13] frame_pa_pol_list[blt_index, pol_ind] = d[14] lst_pol_list[blt_index, pol_ind] = d[15] # Collapse pol axis for ra_list, dec_list, and uvw_list ra_list = np.zeros(self.Nblts) dec_list = np.zeros(self.Nblts) sou_id_list = np.zeros(self.Nblts) epoch_list = np.zeros(self.Nblts) app_ra_list = np.zeros(self.Nblts) app_dec_list = np.zeros(self.Nblts) frame_pa_list = np.zeros(self.Nblts) lst_list = np.zeros(self.Nblts) for blt_index in range(self.Nblts): test = ~np.all(self.flag_array[blt_index, :, :, :], axis=(0, 1)) good_pol = np.where(test)[0] if len(good_pol) == 0: # No good pols for this blt. Fill with first one. good_pol = np.array([0]) if len(good_pol) == 1: # Only one good pol, use it self.uvw_array[blt_index, :] = uvw_pol_list[blt_index, :, good_pol] ra_list[blt_index] = ra_pol_list[blt_index, good_pol] dec_list[blt_index] = dec_pol_list[blt_index, good_pol] sou_id_list[blt_index] = sou_id_pol_list[blt_index, good_pol] epoch_list[blt_index] = epoch_pol_list[blt_index, good_pol] app_ra_list[blt_index] = app_ra_pol_list[blt_index, good_pol] app_dec_list[blt_index] = app_dec_pol_list[blt_index, good_pol] frame_pa_list[blt_index] = frame_pa_pol_list[blt_index, good_pol] lst_list[blt_index] = lst_pol_list[blt_index, good_pol] else: # Multiple good pols, check for consistency. pyuvdata does not # support pol-dependent uvw, ra, or dec. if np.any(np.diff(uvw_pol_list[blt_index, :, good_pol], axis=0)): raise ValueError("uvw values are different by polarization.") else: self.uvw_array[blt_index, :] = uvw_pol_list[ blt_index, :, good_pol[0] ] check_list = [ra_pol_list, dec_pol_list, sou_id_pol_list, lst_pol_list] assign_list = [ra_list, dec_list, sou_id_list, lst_list] check_names = ["ra", "dec", "source id", "lst"] if record_epoch: check_list.append(epoch_pol_list) assign_list.append(epoch_list) check_names.append("epoch") if record_app: check_list.extend([app_ra_pol_list, app_dec_pol_list]) assign_list.extend([app_ra_list, app_dec_list]) check_names.extend(["obsra", "obsdec"]) if record_pa: check_list.append(frame_pa_pol_list) assign_list.append(frame_pa_list) check_names.append("obspa") for item, name in zip(check_list, check_names): if np.any(np.diff(item[blt_index, good_pol])): raise ValueError( "%s values are different by polarization." % name ) for item, target in zip(check_list, assign_list): target[blt_index] = item[blt_index, good_pol[0]] # get unflagged blts # If we have a 1-baseline, single integration data set, set single_ra and # single_time to be true, otherwise evaluate the arrays blt_good = np.where(~np.all(self.flag_array, axis=(1, 2, 3))) single_ra = ( True if (len(blt_good[0]) == 1) else (np.isclose(np.mean(np.diff(ra_list[blt_good])), 0.0)) ) single_time = ( True if (len(blt_good[0]) == 1) else (np.isclose(np.mean(np.diff(self.time_array[blt_good])), 0.0)) ) # first check to see if the phase_type was specified. if phase_type is not None: if phase_type == "phased": self._set_phased() if Nphase > 1: self._set_multi_phase_center() elif phase_type == "drift": self._set_drift() else: raise ValueError( "The phase_type was not recognized. " 'Set the phase_type to "drift" or "phased" to ' "reflect the phasing status of the data" ) else: # check if ra is constant throughout file OR if there are multiple sources # listed; if the obs meets either of those conditions, then assume that the # file is tracking, and if not, assume that the file is drift scanning, # checking if there's only one unflagged time if not single_time: if single_ra or (Nphase > 1): self._set_phased() if Nphase > 1: self._set_multi_phase_center() else: self._set_drift() else: # if there's only one time, checking for consistent RAs doesn't work. # instead check for the presence of an epoch variable, which isn't # really a good option, but at least it prevents crashes. if "epoch" in uv.vartable.keys(): self._set_phased() else: self._set_drift() if proc is not None: proc.join() if (self.telescope_location is None) or not calc_lst: # The float below is the number of sidereal days per solar day, and the # formula below adjusts for the fact that in MIRIAD, the lst is for the # start of the integration, as opposed to pyuvdata, which evaluates these # values at the midpoint of the integration. self.lst_array = lst_list + ( np.pi * 1.002737909350795 * self.integration_time / (24.0 * 3600.0) ) if record_app and (self.phase_type == "phased"): self.phase_center_app_ra = app_ra_list self.phase_center_app_dec = app_dec_list if record_pa: self.phase_center_frame_pa = frame_pa_list if self.multi_phase_center: # This presupposes that the data are already phased self.phase_center_ra = 0.0 # This isn't used for mutli-phase-ctr data self.phase_center_dec = 0.0 # This isn't used for mutli-phase-ctr data # The concept of an epoch is kinda weird in mutli-phase-ctr datasets, b/c # different sources are allowed to have different epochs. Just set it to # the median value for now. Eventually, I think this should be used as the # "if your format forces me to use FK5, here's the epoch" value. Note that # MIRIAD, AIPS, and (I think) CASA tasks assume the coordinates are given # in FK5 format (well, unless epoch <= 1984, in which case MIRIAD assumes # in semi-Orwellian fashion that you _really_ wanted FK4/Bessel-Newcomb). self.phase_center_epoch = 2000.0 self.phase_center_frame = "icrs" self.phase_center_id_array = sou_id_list.astype(int) # Here is where we should package up sources for name in sou_dict.keys(): select_mask = sou_id_list == sou_dict[name] epoch_val = np.median(epoch_list[select_mask]) self._add_phase_center( name, "sidereal", cat_lon=np.median(ra_list[select_mask]), cat_lat=np.median(dec_list[select_mask]), cat_frame="fk4" if (epoch_val < 1984.0) else "fk5", cat_epoch=epoch_val, cat_id=sou_dict[name], info_source="file", ) elif self.phase_type == "phased": # check that the RA values do not vary if not single_ra: raise ValueError( 'phase_type is "phased" but the RA values are varying.' ) self.phase_center_ra = float(ra_list[0]) self.phase_center_dec = float(dec_list[0]) self.phase_center_epoch = uv["epoch"] if "phsframe" not in uv.vartable.keys(): self.phase_center_frame = "fk4" if (uv["epoch"] < 1984.0) else "fk5" else: self.phase_center_frame = uv["phsframe"].replace("\x00", "") else: # check that the RA values are not constant (if more than one time present) if single_ra and not single_time: raise ValueError( 'phase_type is "drift" but the RA values are constant.' ) # use skycoord to simplify calculating sky separations. # Note, this should be done in the TEE frame, which isn't supported # by astropy. Frame doesn't really matter, though, because this is just # geometrical, so use icrs. pointing_coords = SkyCoord( ra=ra_list, dec=dec_list, unit="radian", frame="icrs" ) zenith_coord = SkyCoord( ra=self.lst_array, dec=self.telescope_location_lat_lon_alt[0], unit="radian", frame="icrs", ) separation_angles = pointing_coords.separation(zenith_coord) acceptable_offset = Angle("1d") if np.max(separation_angles.rad) > acceptable_offset.rad: warnings.warn( "drift RA, Dec is off from lst, latitude by more than {}, " "so it appears that it is not a zenith drift scan. " 'Setting phase_type to "drift" for now'.format(acceptable_offset) ) self._set_drift() # close out now that we're done uv.close() if not (record_app and record_pa) and (self.phase_type == "phased"): # At this point, if we are missing information about the sky position of the # source, we want to fill it in now. If we have the apparent coords, but are # only missing the frame position angles (common given that obspa is not a # standard keyword), then we can _just_ fill those in. self._set_app_coords_helper(pa_only=record_app) try: self.set_telescope_params() except ValueError as ve: warnings.warn(str(ve)) # if blt_order is defined, reorder data to match that order # this is required because the data are ordered by (time, baseline) on the read if self.blt_order is not None: if len(list(self.blt_order)) == 2: order, minor_order = self.blt_order else: order = self.blt_order[0] minor_order = None self.reorder_blts(order=order, minor_order=minor_order) # If the data set was recorded using the old phasing method, fix that now. if fix_old_proj and (self.phase_type == "phased"): if not self.multi_phase_center: self.fix_phase(use_ant_pos=fix_use_ant_pos) else: warnings.warn( "Cannot fix the phases of multi phase center datasets, as they " "were not supported when the old phasing method was used, and " "thus, there is no need to correct the data." ) # check if object has all required uv_properties set if run_check: self.check( check_extra=check_extra, run_check_acceptability=run_check_acceptability, strict_uvw_antpos_check=strict_uvw_antpos_check, allow_flip_conj=True, )
[docs] def write_miriad( self, filepath, clobber=False, run_check=True, check_extra=True, run_check_acceptability=True, strict_uvw_antpos_check=False, no_antnums=False, calc_lst=False, ): """ Write the data to a miriad file. Parameters ---------- filename : str The miriad root directory to write to. clobber : bool Option to overwrite the filename if the file already exists. run_check : bool Option to check for the existence and proper shapes of parameters after before writing the file (the default is True, meaning the check will be run). check_extra : bool Option to check optional parameters as well as required ones (the default is True, meaning the optional parameters will be checked). run_check_acceptability : bool Option to check acceptable range of the values of parameters before writing the file (the default is True, meaning the acceptable range check will be done). strict_uvw_antpos_check : bool Option to raise an error rather than a warning if the check that uvws match antenna positions does not pass. no_antnums : bool Option to not write the antnums variable to the file. Should only be used for testing purposes. calc_lst : bool Recalculate the LST values upon writing the file. This is done to perform higher-precision accounting for the difference in MIRAD timestamps vs pyuvdata (the former marks the beginning of an integration, the latter marks the midpoint). Default is False, which instead uses a simple formula for correcting the LSTs, expected to be accurate to approximately 0.1 ┬Ásec precision. Raises ------ ValueError If the frequencies are not evenly spaced or are separated by more than their channel width. TypeError If any entry in extra_keywords is not a single string or number. """ from . import aipy_extracts # change time_array and lst_array to mark beginning of integration, # per Miriad format miriad_time_array = self.time_array - self.integration_time / (24 * 3600.0) / 2 if (self.telescope_location is not None) and calc_lst: latitude, longitude, altitude = self.telescope_location_lat_lon_alt_degrees miriad_lsts = uvutils.get_lst_for_time( miriad_time_array, latitude, longitude, altitude ) else: # The long float below is the number of sidereal days per day. The below # equation should be accurate to _much_ better than 1 ┬Ásec. miriad_lsts = self.lst_array - ( np.pi * 1.002737909350795 * self.integration_time / (24.0 * 3600.0) ) # Miriad requires j>i which we call ant1<ant2 self.conjugate_bls(convention="ant1<ant2") if run_check: self.check( check_extra=check_extra, run_check_acceptability=run_check_acceptability, check_freq_spacing=True, strict_uvw_antpos_check=strict_uvw_antpos_check, ) if os.path.exists(filepath): if clobber: print("File exists: clobbering") shutil.rmtree(filepath) else: raise IOError("File exists: skipping") uv = aipy_extracts.UV(filepath, status="new") # initialize header variables uv._wrhd("obstype", "mixed-auto-cross") # avoid inserting extra \n. if not self.history[-1] == "\n": self.history += "\n" uv._wrhd("history", self.history) # recognized miriad variables uv.add_var("nchan", "i") uv["nchan"] = self.Nfreqs uv.add_var("npol", "i") uv["npol"] = self.Npols ##################################################### # Frequency information here uv.add_var("nspect", "i") uv["nspect"] = self.Nspws if self.future_array_shapes: freq_array_use = self.freq_array else: freq_array_use = self.freq_array[0, :] if self.flex_spw: win_start_pos = np.insert( np.where(self.flex_spw_id_array[1:] != self.flex_spw_id_array[:-1])[0] + 1, 0, 0, ).astype(int) uv.add_var("ischan", "i") # Starting chan of window uv["ischan"] = win_start_pos + 1 # Miriad is 1-based indexed uv.add_var("nschan", "i") # Number of chan per window uv["nschan"] = np.diff(np.append(win_start_pos, self.Nfreqs)) uv.add_var("sfreq", "d") # Freq of first channel of the window, Hz -> GHz uv["sfreq"] = (freq_array_use[win_start_pos] / 1e9).astype(np.double) # Need the array direction here since channel_width is always supposed # to be > 0, but channels can be in descending freq order freq_dir = np.sign( freq_array_use[np.append(win_start_pos[1:] - 1, self.Nfreqs - 1)] - freq_array_use[win_start_pos] ) uv.add_var("sdf", "d") # Channel width, Hz -> GHz uv["sdf"] = self.channel_width[win_start_pos] * freq_dir / 1e9 else: uv.add_var("ischan", "i") # Starting chan of window uv["ischan"] = 1 # Miriad is 1-based indexed uv.add_var("nschan", "i") # Number of chan per window uv["nschan"] = self.Nfreqs # Need the array direction here since channel_width is always supposed # to be > 0, but channels can be in decending freq order freq_dir = np.sign(np.diff(freq_array_use[([0, -1])])) uv.add_var("sfreq", "d") # Freq of first channel of the window, in GHz uv["sfreq"] = (freq_array_use[0] / 1e9).astype(np.double) # Hz -> GHz uv.add_var("sdf", "d") # Channel width, in GHz # we've already run the check_freq_spacing, so channel widths are the # same to our tolerances uv["sdf"] = np.median(self.channel_width) * freq_dir / 1e9 # Hz -> GHz # NB: restfreq should go in here at some point ##################################################### if not self.multi_phase_center: uv.add_var("source", "a") uv["source"] = self.object_name uv.add_var("telescop", "a") uv["telescop"] = self.telescope_name uv.add_var("latitud", "d") uv["latitud"] = self.telescope_location_lat_lon_alt[0].astype(np.double) uv.add_var("longitu", "d") uv["longitu"] = self.telescope_location_lat_lon_alt[1].astype(np.double) uv.add_var("nants", "i") if self.antenna_diameters is not None: if not np.allclose(self.antenna_diameters, self.antenna_diameters[0]): warnings.warn( "Antenna diameters are not uniform, but miriad only" "supports a single diameter. Skipping." ) else: uv.add_var("antdiam", "d") uv["antdiam"] = float(self.antenna_diameters[0]) # Miriad has no way to keep track of antenna numbers, so the antenna # numbers are simply the index for each antenna in any array that # describes antenna attributes (e.g. antpos for the antenna_postions). # Therefore on write, nants (which gives the size of the antpos array) # needs to be increased to be the max value of antenna_numbers+1 and the # antpos array needs to be inflated with zeros at locations where we # don't have antenna information. These inflations need to be undone at # read. If the file was written by pyuvdata, then the variable antnums # will be present and we can use it, otherwise we need to test for zeros # in the antpos array and/or antennas with no visibilities. nants = np.max(self.antenna_numbers) + 1 uv["nants"] = nants if self.antenna_positions is not None: # Miriad wants antenna_positions to be in absolute coordinates # (not relative to array center) in a rotated ECEF frame where the # x-axis goes through the local meridian. rel_ecef_antpos = np.zeros((nants, 3), dtype=self.antenna_positions.dtype) for ai, num in enumerate(self.antenna_numbers): rel_ecef_antpos[num, :] = self.antenna_positions[ai, :] # find zeros so antpos can be zeroed there too antpos_length = np.sqrt(np.sum(np.abs(rel_ecef_antpos) ** 2, axis=1)) ecef_antpos = rel_ecef_antpos + self.telescope_location longitude = self.telescope_location_lat_lon_alt[1] antpos = uvutils.rotECEF_from_ECEF(ecef_antpos, longitude) # zero out bad locations (these are checked on read) antpos[np.where(antpos_length == 0), :] = [0, 0, 0] uv.add_var("antpos", "d") # Miriad stores antpos values in units of ns, pyuvdata uses meters. uv["antpos"] = (antpos.T.flatten() / const.c.to("m/ns").value).astype( np.double ) if self.phase_type == "phased": if self.phase_center_epoch is not None: uv.add_var("epoch", "r") uv["epoch"] = self.phase_center_epoch if self.phase_center_frame is not None: uv.add_var("phsframe", "a") uv["phsframe"] = self.phase_center_frame # required pyuvdata variables that are not recognized miriad variables uv.add_var("ntimes", "i") uv["ntimes"] = self.Ntimes uv.add_var("nbls", "i") uv["nbls"] = self.Nbls uv.add_var("nblts", "i") uv["nblts"] = self.Nblts uv.add_var("visunits", "a") uv["visunits"] = self.vis_units uv.add_var("instrume", "a") uv["instrume"] = self.instrument uv.add_var("altitude", "d") uv["altitude"] = self.telescope_location_lat_lon_alt[2].astype(np.double) # optional pyuvdata variables that are not recognized miriad variables if self.dut1 is not None: uv.add_var("dut1", "d") uv["dut1"] = self.dut1 if self.earth_omega is not None: uv.add_var("degpdy", "d") uv["degpdy"] = self.earth_omega if self.gst0 is not None: uv.add_var("gst0", "d") uv["gst0"] = self.gst0 if self.rdate is not None: uv.add_var("rdate", "a") uv["rdate"] = self.rdate if self.timesys is not None: uv.add_var("timesys", "a") uv["timesys"] = self.timesys if self.x_orientation is not None: uv.add_var("xorient", "a") uv["xorient"] = self.x_orientation if self.blt_order is not None: blt_order_str = ", ".join(self.blt_order) uv.add_var("bltorder", "a") uv["bltorder"] = blt_order_str # other extra keywords # set up dictionaries to map common python types to miriad types # NB: arrays/lists/dicts could potentially be written as strings or 1D # vectors. This is not supported at present! # NB: complex numbers *should* be supportable, but are not currently # supported due to unexplained errors in _miriad and/or its underlying libraries numpy_types = { np.int8: int, np.int16: int, np.int32: int, np.int64: int, np.uint8: int, np.uint16: int, np.uint32: int, np.uint64: int, np.float16: float, np.float32: float, np.float64: float, np.float128: float, } types = { str: "a", int: "i", float: "d", bool: "a", # booleans are stored as strings and changed back on read } for key, value in self.extra_keywords.items(): if isinstance(value, tuple(numpy_types.keys())): if numpy_types[type(value)] == int: value = int(value) elif numpy_types[type(value)] == float: value = float(value) elif type(value) == bool: value = str(value) elif type(value) not in types.keys(): raise TypeError( "Extra keyword {keyword} is of {keytype}. " "Only strings and real numbers are " "supported in miriad.".format(keyword=key, keytype=type(value)) ) if len(str(key)) > 8: warnings.warn( "key {key} in extra_keywords is longer than 8 " "characters. It will be truncated to 8 as required " "by the miriad file format.".format(key=key) ) uvkeyname = str(key)[:8] # name must be string, max 8 letters typestring = types[type(value)] uv.add_var(uvkeyname, typestring) uv[uvkeyname] = value if not no_antnums: # Add in the antenna_numbers so we have them if we read this file back in. # For some reason Miriad doesn't handle an array of integers properly, # so convert to floats here and integers on read. uv.add_var("antnums", "d") uv["antnums"] = self.antenna_numbers.astype(np.float64) # antenna names is a foreign concept in miriad but required in other formats. # Miriad can't handle arrays of strings, so we make it into one long # comma-separated string and convert back on read. ant_name_str = "[" + ", ".join(self.antenna_names) + "]" uv.add_var("antnames", "a") uv["antnames"] = ant_name_str # variables that can get updated with every visibility uv.add_var("pol", "i") uv.add_var("lst", "d") uv.add_var("cnt", "d") if self.multi_phase_center: uv.add_var("source", "a") name_dict = { self.phase_center_catalog[key]["cat_id"]: key for key in self.phase_center_catalog.keys() } uv.add_var("ra", "d") uv.add_var("dec", "d") uv.add_var("inttime", "d") app_record = False if ( self.phase_center_app_ra is not None and self.phase_center_app_dec is not None and self.phase_center_frame_pa is not None ): app_record = True uv.add_var("obsra", "d") uv.add_var("obsdec", "d") uv.add_var("obspa", "d") # Non-standard MIRIAD keyword # write data c_ns = const.c.to("m/ns").value for viscnt, blt in enumerate(self.data_array): uvw = (self.uvw_array[viscnt] / c_ns).astype(np.double) t = miriad_time_array[viscnt] i = self.ant_1_array[viscnt] j = self.ant_2_array[viscnt] uv["lst"] = miriad_lsts[viscnt].astype(np.double) uv["inttime"] = self.integration_time[viscnt].astype(np.double) if self.phase_type == "phased": if self.multi_phase_center: cat_name = name_dict[self.phase_center_id_array[viscnt]] uv["source"] = cat_name uv["ra"] = self.phase_center_catalog[cat_name]["cat_lon"] uv["dec"] = self.phase_center_catalog[cat_name]["cat_lat"] else: uv["ra"] = self.phase_center_ra uv["dec"] = self.phase_center_dec if app_record: uv["obsra"] = self.phase_center_app_ra[viscnt] uv["obsdec"] = self.phase_center_app_dec[viscnt] uv["obspa"] = self.phase_center_frame_pa[viscnt] elif self.phase_type == "drift": uv["ra"] = miriad_lsts[viscnt].astype(np.double) uv["dec"] = self.telescope_location_lat_lon_alt[0].astype(np.double) for polcnt, pol in enumerate(self.polarization_array): uv["pol"] = pol.astype(np.int64) if self.future_array_shapes: uv["cnt"] = self.nsample_array[viscnt, :, polcnt].astype(np.double) else: uv["cnt"] = self.nsample_array[viscnt, 0, :, polcnt].astype( np.double ) if self.future_array_shapes: data = self.data_array[viscnt, :, polcnt] flags = self.flag_array[viscnt, :, polcnt] else: data = self.data_array[viscnt, 0, :, polcnt] flags = self.flag_array[viscnt, 0, :, polcnt] # Using an assert here because it should be guaranteed by an earlier # method call. assert j >= i, ( "Miriad requires ant1<ant2 which should be " "guaranteed by prior conjugate_bls call" ) preamble = (uvw, t, (i, j)) uv.write(preamble, data, flags) # close out now that we're done uv.close() return