TimeDeltaDatetime

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

Bases: astropy.time.TimeDeltaFormat, astropy.time.TimeUnique

Time delta in datetime.timedelta

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

mask_if_needed(value)

set_jds(val1, val2)

Set internal jd1 and jd2 from val1 and val2.

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.

in_subfmt
jd1
jd2
jd2_filled
mask
masked
name = 'datetime'
out_subfmt
scale

Time scale

subfmts = ()
value

Methods Documentation

mask_if_needed(value)
set_jds(val1, val2)[source]

Set internal jd1 and jd2 from val1 and val2. Must be provided by derived classes.

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
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