TimeISO¶

class astropy.time.TimeISO(val1, val2, scale, precision, in_subfmt, out_subfmt, from_jd=False)[source]¶

Bases: astropy.time.TimeString

ISO 8601 compliant date-time format “YYYY-MM-DD HH:MM:SS.sss…”. For example, 2000-01-01 00:00:00.000 is midnight on January 1, 2000.

The allowed subformats are:

‘date_hms’: date + hours, mins, secs (and optional fractional secs)
‘date_hm’: date + hours, mins
‘date’: date

Attributes Summary

`cache`	Return the cache associated with this instance.
`in_subfmt`
`jd1`
`jd2`
`jd2_filled`
`mask`
`masked`
`name`
`out_subfmt`
`scale`	Time scale
`subfmts`
`value`

Methods Summary

`format_string`(self, str_fmt, **kwargs)	Write time to a string using a given format.
`mask_if_needed`(self, value)
`parse_string`(self, timestr, subfmts)	Read time from a single string, using a set of possible formats.
`set_jds`(self, val1, val2)	Parse the time strings contained in val1 and set jd1, jd2
`str_kwargs`(self)	Generator that yields a dict of values corresponding to the calendar date and time for the internal JD values.
`to_value`(self[, parent, out_subfmt])	Return time representation from internal jd1 and jd2 in specified `out_subfmt`.

Attributes Documentation

cache¶: Return the cache associated with this instance.

in_subfmt¶

jd1¶

jd2¶

jd2_filled¶

mask¶

masked¶

name = 'iso'¶

out_subfmt¶

scale¶: Time scale

subfmts = (('date_hms', re.compile('(?P<year>\\d\\d\\d\\d)-(?P<mon>\\d{1,2})-(?P<mday>\\d{1,2}) (?P<hour>\\d{1,2}):(?P<min>\\d{1,2}):(?P<sec>\\d{1,2})$'), '{year:d}-{mon:02d}-{day:02d} {hour:02d}:{min:02d}:{sec:02d}'), ('date_hm', re.compile('(?P<year>\\d\\d\\d\\d)-(?P<mon>\\d{1,2})-(?P<mday>\\d{1,2}) (?P<hour>\\d{1,2}):(?P<min>\\d{1,2})$'), '{year:d}-{mon:02d}-{day:02d} {hour:02d}:{min:02d}'), ('date', re.compile('(?P<year>\\d\\d\\d\\d)-(?P<mon>\\d{1,2})-(?P<mday>\\d{1,2})$'), '{year:d}-{mon:02d}-{day:02d}'))¶

value¶

Methods Documentation

format_string(self, 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.

mask_if_needed(self, value)¶

parse_string(self, timestr, subfmts)[source]¶: Read time from a single string, using a set of possible formats.

set_jds(self, val1, val2)¶: Parse the time strings contained in val1 and set jd1, jd2

str_kwargs(self)¶: Generator that yields a dict of values corresponding to the calendar date and time for the internal JD values.

to_value(self, 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 the value property to compute the output. This is done by temporarily setting self.out_subfmt and calling self.value. This is required for legacy Format subclasses prior to astropy 4.0 New code should instead implement the value functionality in to_value() and then make the value property be a simple call to self.to_value().

Parameters

parentobj: Parent Time object associated with this TimeFormat object
out_subfmtstr or None: Output subformt (use existing self.out_subfmt if None)

Returns

valuenumpy.array, numpy.ma.array: Array or masked array of formatted time representation values

Navigation

TimeISO¶