TimeFormat#

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

Bases: object

Base class for time representations.

Parameters:
val1numpy ndarray, list, number, str, or bytes

Values to initialize the time or times. Bytes are decoded as ascii. Quantities with time units are allowed for formats where the interpretation is unambiguous.

val2numpy ndarray, list, or number; optional

Value(s) to initialize the time or times. Only used for numerical input, to help preserve precision.

scalestr

Time scale of input value(s)

precisionint

Precision for seconds as floating point

in_subfmtstr

Select subformat for inputting string times

out_subfmtstr

Select subformat for outputting string times

from_jdbool

If true then val1, val2 are jd1, jd2

Attributes Summary

Methods Summary

fill_value(subfmt)

Return a value corresponding to J2000 (2000-01-01 12:00:00) in this format.

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

in_subfmt#
jd1#
jd2#
out_subfmt#
precision#
scale#

Time scale.

subfmts = ()#
value#

Methods Documentation

classmethod fill_value(subfmt)[source]#

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.

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)[source]#

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