TimeYearDayTime

class astropy.time.TimeYearDayTime(val1, val2, scale, precision, in_subfmt, out_subfmt, from_jd=False)

Bases: TimeISO

Year, day-of-year and time as “YYYY:DOY:HH:MM:SS.sss…”. The day-of-year (DOY) goes from 001 to 365 (366 in leap years). For example, 2000:001:00:00:00.000 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.
fast_parser_pars
in_subfmt
jd1
jd2
jd2_filled
mask
masked
name
out_subfmt
precision
scale	Time scale.
subfmts
value

Methods Summary

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.
mask_if_needed(value)
parse_string(timestr, subfmts)	Read time from a single string, using a set of possible formats.
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, out_subfmt])	Return time representation from internal jd1 and jd2 in specified out_subfmt.

Attributes Documentation

cache

Return the cache associated with this instance.

fast_parser_pars = {'break_allowed': (0, 0, 0, 1, 0, 1, 1), 'delims': (0, 0, 58, 58, 58, 58, 46), 'has_day_of_year': 1, 'starts': (0, -1, 4, 8, 11, 14, 17), 'stops': (3, -1, 7, 10, 13, 16, -1)}

in_subfmt

jd1

jd2

jd2_filled

mask

masked

name = 'yday'

out_subfmt

precision

scale

Time scale.

subfmts = (('date_hms', '%Y:%j:%H:%M:%S', '{year:d}:{yday:03d}:{hour:02d}:{min:02d}:{sec:02d}'), ('date_hm', '%Y:%j:%H:%M', '{year:d}:{yday:03d}:{hour:02d}:{min:02d}'), ('date', '%Y:%j', '{year:d}:{yday:03d}'))

value

Methods Documentation

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.

mask_if_needed(value)

parse_string(timestr, subfmts)

Read time from a single string, using a set of possible formats.

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 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:

parentobject

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