`lofarSun.cli.pyms_utils`

command line tools to process the lofar solar data

by Peijin Zhang version 0.1 2022-5-23 00:24:52: Initial version

Module Contents

`info_print`(header, content)
`human_format`(number)
`get_obs_info_from_ms`(fname)	get observation information from ms
`get_t_from_ms`(fname)	get time information from ms
`get_freq_from_ms`(fname)
`ms_datetime_to_index`(fname, t[, t_format])	convert datetime to index
`ms_index_to_datetime`(fname, idx)
`cook_wsclean_cmd`(fname[, mode, multiscale, weight, ...])
`pyms_overview_main`()
`pyms_datetime_to_index_main`()
`pyms_cook_wsclean_cmd_main`()
`pyms_index_to_datetime_main`()
`pyms_psf_fit_peak_gauss_main`()

class lofarSun.cli.pyms_utils.bcolors

lofarSun.cli.pyms_utils.get_obs_info_from_ms(fname)

get observation information from ms

Parameters:: fname (string) – measurement set name
Returns:: list of antenna name int : number of baselines string : telescope name
Return type:: list

lofarSun.cli.pyms_utils.get_t_from_ms(fname)

get time information from ms

lofarSun.cli.pyms_utils.ms_datetime_to_index(fname, t, t_format='%H:%M:%S.%f')

convert datetime to index

Parameters:

Returns:

index

Return type:

int

lofarSun.cli.pyms_utils.cook_wsclean_cmd(fname, mode='default', multiscale=True, weight='briggs 0', mgain=0.8, thresholding='-auto-mask 3 -auto-threshold 0.3', len_baseline_eff=35000, FOV=10000, scale_factor=4.3, circbeam=True, niter=1200, pol='I', data_col='CORRECTED_DATA', misc='', name='', interval=[-1, -1], intervals_out=-1)