TimeFITS#
- class astropy.time.TimeFITS(val1, val2, scale, precision, in_subfmt, out_subfmt, from_jd=False)[source]#
Bases:
TimeString
FITS format: “[±Y]YYYY-MM-DD[THH:MM:SS[.sss]]”.
ISOT but can give signed five-digit year (mostly for negative years);
The allowed subformats are:
‘date_hms’: date + hours, mins, secs (and optional fractional secs)
‘date’: date
‘longdate_hms’: as ‘date_hms’, but with signed 5-digit year
‘longdate’: as ‘date’, but with signed 5-digit year
See Rots et al., 2015, A&A 574:A36 (arXiv:1409.7583).
Attributes Summary
Time scale.
Convert times to strings, using signed 5 digit if necessary.
Methods Summary
fill_value
(subfmt)Return a value corresponding to J2000 (2000-01-01 12:00:00) in this format.
format_string
(str_fmt, **kwargs)Write time to a string using a given format.
get_jds_fast
(val1, val2)Use fast C parser to parse time strings in val1 and get jd1, jd2.
get_jds_python
(val1, val2)Parse the time strings contained in val1 and get jd1, jd2.
parse_string
(timestr, subfmts)Read time and deprecated scale if present.
set_jds
(val1, val2)Parse the time strings contained in val1 and set jd1, jd2.
Generator that yields a dict of values corresponding to the calendar date and time for the internal JD values.
to_value
([parent, out_subfmt])Return time representation from internal jd1 and jd2 in specified
out_subfmt
.Attributes Documentation
- in_subfmt#
- jd1#
- jd2#
- name = 'fits'#
- out_subfmt#
- precision#
- scale#
Time scale.
- subfmts = (('date_hms', re.compile('(?P<year>\\d{4})-(?P<mon>\\d\\d)-(?P<mday>\\d\\d)T(?P<hour>\\d\\d):(?P<min>\\d\\d):(?P<sec>\\d\\d(\\.\\d*)?)(\\((?P<scale>\\w+)(\\((?P<realization>\\w+)\\))?\\))?$'), '{year:04d}-{mon:02d}-{day:02d}T{hour:02d}:{min:02d}:{sec:02d}'), ('date', re.compile('(?P<year>\\d{4})-(?P<mon>\\d\\d)-(?P<mday>\\d\\d)(\\((?P<scale>\\w+)(\\((?P<realization>\\w+)\\))?\\))?$'), '{year:04d}-{mon:02d}-{day:02d}'), ('longdate_hms', re.compile('(?P<year>[+-]\\d{5})-(?P<mon>\\d\\d)-(?P<mday>\\d\\d)T(?P<hour>\\d\\d):(?P<min>\\d\\d):(?P<sec>\\d\\d(\\.\\d*)?)(\\((?P<scale>\\w+)(\\((?P<realization>\\w+)\\))?\\))?$'), '{year:+06d}-{mon:02d}-{day:02d}T{hour:02d}:{min:02d}:{sec:02d}'), ('longdate', re.compile('(?P<year>[+-]\\d{5})-(?P<mon>\\d\\d)-(?P<mday>\\d\\d)(\\((?P<scale>\\w+)(\\((?P<realization>\\w+)\\))?\\))?$'), '{year:+06d}-{mon:02d}-{day:02d}'))#
- value#
Convert times to strings, using signed 5 digit if necessary.
Methods Documentation
- classmethod fill_value(subfmt)#
Return a value corresponding to J2000 (2000-01-01 12:00:00) in this format.
This is used as a fill value for masked arrays to ensure that any ERFA operations on the masked array will not fail due to the masked value.
- format_string(str_fmt, **kwargs)#
Write time to a string using a given format.
By default, just interprets str_fmt as a format string, but subclasses can add to this.
- get_jds_fast(val1, val2)#
Use fast C parser to parse time strings in val1 and get jd1, jd2.
- get_jds_python(val1, val2)#
Parse the time strings contained in val1 and get jd1, jd2.
- set_jds(val1, val2)#
Parse the time strings contained in val1 and set jd1, jd2.
- str_kwargs()#
Generator that yields a dict of values corresponding to the calendar date and time for the internal JD values.
- to_value(parent=None, out_subfmt=None)#
Return time representation from internal jd1 and jd2 in specified
out_subfmt
.This is the base method that ignores
parent
and uses thevalue
property to compute the output. This is done by temporarily settingself.out_subfmt
and callingself.value
. This is required for legacy Format subclasses prior to astropy 4.0 New code should instead implement the value functionality into_value()
and then make thevalue
property be a simple call toself.to_value()
.- Parameters:
- Returns:
- value
numpy.array
,numpy.ma.array
Array or masked array of formatted time representation values
- value