LSRKfreq_to_chan(msfile, field, spw, ...[, ...])
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Identifies the channel(s) corresponding to input LSRK frequencies. |
check_image_nterms(fracbw, SNR)
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check_mosaic(vislist, target)
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check_narrow_window_flagging(...)
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check_spectral_gain_gradient(...)
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check_spw_widest_in_bb(selfcal_library, vis, spw)
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checkmask(imagename)
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chi2_spectral_phase_per_soln(per_spw_phase, ...)
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collect_listobs_per_vis(vislist)
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compare_beams(image1, image2)
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create_noise_histogram(imagename)
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create_noise_histogram_plots(N_1, N_2, ...)
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estimate_SNR(imagename[, maskname, verbose, ...])
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estimate_near_field_SNR(imagename[, las, ...])
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evaluate_per_spw_gaintables(...)
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fetch_scan_times_band_aware(vislist, ...)
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fetch_spws(vislist, targets)
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fetch_targets(vislist, telescope)
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find_matching_spw(vis1, spw1, vis2, ...[, ...])
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flag_spectral_lines(vislist, all_targets, ...)
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flagchannels_from_contdotdat(vis, target, ...)
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Generates a string with the list of lines identified by the cont.dat file from the ALMA pipeline, that need to be flagged. |
gaussian_norm(x, mean, sigma)
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get_ALMA_band_string(meanfreq)
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get_SNR_self(selfcal_library, selfcal_plan, ...)
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get_SNR_self_individual(vislist, ...)
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get_SNR_self_update(selfcal_library, ...)
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get_SNR_self_update_old(selfcal_library, ...)
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get_ant_list(vis)
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get_bands(vislist, fields, telescope)
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get_basebands(observed_bands, vis, band, ...)
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get_baseline_dist(vis)
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get_desired_width(meanfreq)
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get_dr_correction(telescope, dirty_peak, ...)
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get_fitspw_dict(vis, target, spwsarray, ...)
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Generates a string with the list of lines identified by the cont.dat file from the ALMA pipeline, that need to be flagged. |
get_flagged_solns_per_ant(gaintable, vis)
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get_flagged_solns_per_ant_from_dict(...)
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get_flagged_solns_per_spw(spwlist, gaintable)
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get_flagging_baseline(gc_dict_list, spwlist)
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get_gaintable_flagging_stats(gc_dict_list, ...)
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get_image_parameters(vislist, telescope, ...)
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get_intflux(imagename, rms[, maskname, ...])
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get_max_uvdist(vislist, bands, ...)
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get_mean_freq(vis, spwsarray)
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get_min_SNR_spw(snr_per_spw)
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get_n_ants(vislist)
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get_nearest_wide_bw_spw(selfcal_library, ...)
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get_phasecenter(vis, field)
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get_reffreq(vislist, field_ids, spwsarray, ...)
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get_sensitivity(vislist, selfcal_library[, ...])
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get_solints_simple(vislist, scantimesdict, ...)
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get_sols_flagged_solns(gaintable)
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get_spw_bandwidth(vis, spwsarray_dict, ...)
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get_spw_chanavg(vis, widtharray, bwarray, ...)
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get_spw_chanwidths(vis, spwarray)
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get_spw_eff_bandwidth(vis, target, vislist, ...)
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get_spw_map(selfcal_library, target, band, ...)
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get_spwnum_refvis(vislist, target, ...[, ...])
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get_telescope(vis)
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get_uv_range(band, band_properties, vislist)
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importdata(vislist, all_targets, telescope)
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is_iterable(obj)
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largest_prime_factor(n)
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make_distance_time_phaseerr_plots(vislist)
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parse_contdotdat(contdotdat_file, target)
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Parses the cont.dat file that includes line emission automatically identified by the ALMA pipeline. |
plot_amp_err(amp_err, snr, gaintable)
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plot_ants_flagging_colored(filename, vis, ...)
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plot_ants_flagging_colored_from_dict(...)
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plot_image(filename, outname[, min_val, ...])
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plot_phase_err(phase_err, snr, gaintable)
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plot_spectral_amp(per_spw_amp, ...)
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plot_spectral_phase(per_spw_phase, ...)
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plot_spectral_phase_per_soln(per_spw_phase, ...)
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plotcals(source)
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rank_refants(vis[, caltable])
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remove_modes(selfcal_plan, vis, start_index)
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sanitize_string(string)
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select_best_gaincal_mode(selfcal_library, ...)
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split_to_selfcal_ms(all_targets, vislist, ...)
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tclean_wrapper(selfcal_library, imagename, band)
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Wrapper for tclean with keywords set to values desired for the Large Program imaging See the CASA 6.1.1 documentation for tclean to get the definitions of all the parameters |
test_truncated_scans(ints_per_solint, ...)
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triage_calibrators(vis, target, ...[, ...])
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unflag_failed_antennas(vis, caltable, ...[, ...])
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usermodel_wrapper(selfcal_library, ...[, ...])
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version()
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version_string()
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zero_out_gc_return_dict(gaincal_return)
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