TimeBesselianEpochString¶
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class
astropy.time.TimeBesselianEpochString(val1, val2, scale, precision, in_subfmt, out_subfmt, from_jd=False)[source]¶ Bases:
astropy.time.TimeEpochDateStringBesselian Epoch year as string value(s) like ‘B1950.0’
Attributes Summary
Return the cache associated with this instance.
Class property for ctypes library for fast C parsing of string times.
Time scale
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
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
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cache¶ Return the cache associated with this instance.
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epoch_prefix= 'B'¶
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epoch_to_jd= 'epb2jd'¶
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in_subfmt¶
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jd1¶
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jd2¶
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jd2_filled¶
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jd_to_epoch= 'epb'¶
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lib_parse_time¶ Class property for ctypes library for fast C parsing of string times.
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mask¶
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masked¶
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name= 'byear_str'¶
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out_subfmt¶
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scale¶ Time scale
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subfmts= ()¶
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time_struct_dtype¶
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value¶
Methods Documentation
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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.
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get_jds_fast(val1, val2)¶ Use fast C parser to parse time strings in val1 and get jd1, jd2
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get_jds_python(val1, val2)¶ Parse the time strings contained in val1 and get jd1, jd2
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mask_if_needed(value)¶
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parse_string(timestr, subfmts)¶ Read time from a single string, using a set of possible formats.
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set_jds(val1, val2)¶ Parse the time strings contained in val1 and set jd1, jd2
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str_kwargs()¶ Generator that yields a dict of values corresponding to the calendar date and time for the internal JD values.
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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
parentand uses thevalueproperty to compute the output. This is done by temporarily settingself.out_subfmtand 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 thevalueproperty be a simple call toself.to_value().- Parameters
- parentobj
Parent
Timeobject associated with thisTimeFormatobject- 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
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