Timespan¶
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class
lsst.daf.butler.Timespan(begin: Union[astropy.time.core.Time, lsst.daf.butler.core.timespan._SpecialTimespanBound, None], end: Union[astropy.time.core.Time, lsst.daf.butler.core.timespan._SpecialTimespanBound, None], padInstantaneous: bool = True, _nsec: Optional[Tuple[int, int], None] = None)¶ Bases:
objectA half-open time interval with nanosecond precision.
Parameters: - begin :
astropy.time.Time,Timespan.EMPTY, orNone Minimum timestamp in the interval (inclusive).
Noneindicates that the timespan has no lower bound.Timespan.EMPTYindicates that the timespan contains no times; if this is used as either bound, the other bound is ignored.- end :
astropy.time.Time,SpecialTimespanBound, orNone Maximum timestamp in the interval (exclusive).
Noneindicates that the timespan has no upper bound. As withbegin,Timespan.EMPTYcreates an empty timespan.- padInstantaneous :
bool, optional If
True(default) andbegin == endafter discretization to integer nanoseconds, extendendby one nanosecond to yield a finite-duration timespan. IfFalse,begin == endevaluates to the empty timespan.- _nsec :
tupleofint, optional Integer nanosecond representation, for internal use by
TimespanandTimespanDatabaseRepresentationimplementation only. If provided, all other arguments are are ignored.
Raises: - TypeError
Raised if
beginorendhas a type other thanastropy.time.Time, and is notNoneorTimespan.EMPTY.- ValueError
Raised if
beginorendexceeds the minimum or maximum times supported by this class.
Notes
Timespans are half-open intervals, i.e.
[begin, end).Any timespan with
begin > endafter nanosecond discretization (begin >= endifpadInstantaneousisFalse), or with either bound set toTimespan.EMPTY, is transformed into the empty timespan, with both bounds set toTimespan.EMPTY. The empty timespan is equal to itself, and contained by all other timespans (including itself). It is also disjoint with all timespans (including itself), and hence does not overlap any timespan - this is the only case wherecontainsdoes not implyoverlaps.Finite timespan bounds are represented internally as integer nanoseconds, and hence construction from
astropy.time.Time(which has picosecond accuracy) can involve a loss of precision. This is of course deterministic, so anyastropy.time.Timevalue is always mapped to the exact same timespan bound, but ifpadInstantaneousisTrue, timespans that are empty at full precision (begin > end,begin - end < 1ns) may be finite after discretization. In all other cases, the relationships between full-precision timespans should be preserved even if the values are not.The
astropy.time.Timebounds that can be obtained after construction fromTimespan.beginandTimespan.endare also guaranteed to round-trip exactly when used to construct otherTimespaninstances.Attributes Summary
EMPTYbeginMinimum timestamp in the interval, inclusive. endMaximum timestamp in the interval, exclusive. yaml_tagMethods Summary
contains(other, …)Test if the supplied timespan is within this one. difference(other)Return the one or two timespans that cover the interval(s). fromInstant(time)Construct a timespan that approximates an instant in time. from_json(json_str, universe, registry)Return new class from JSON string. from_simple(simple, universe, registry)Construct a new object from simplified form. from_yaml(loader, node)Convert YAML node into _SpecialTimespanBound. intersection(*args)Return a new Timespanthat is contained by all of the given ones.isEmpty()Test whether selfis the empty timespan (bool).makeEmpty()Construct an empty timespan. overlaps(other, astropy.time.core.Time])Test if the intersection of this Timespan with another is empty. to_json(minimal)Convert this class to JSON form. to_simple(minimal)Return simple python type form suitable for serialization. to_yaml(dumper, timespan)Convert Timespan into YAML format. Attributes Documentation
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EMPTY= 1¶
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begin¶ Minimum timestamp in the interval, inclusive.
If this bound is finite, this is an
astropy.time.Timeinstance. If the timespan is unbounded from below, this isNone. If the timespan is empty, this is the special valueTimespan.EMPTY.
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end¶ Maximum timestamp in the interval, exclusive.
If this bound is finite, this is an
astropy.time.Timeinstance. If the timespan is unbounded from above, this isNone. If the timespan is empty, this is the special valueTimespan.EMPTY.
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yaml_tag= '!lsst.daf.butler.Timespan'¶
Methods Documentation
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contains(other: Union[astropy.time.core.Time, lsst.daf.butler.core.timespan.Timespan]) → bool¶ Test if the supplied timespan is within this one.
Tests whether the intersection of this timespan with another timespan or point is equal to the other one.
Parameters: - other :
Timespanorastropy.time.Time. Timespan or instant in time to relate to
self.
Returns: - overlaps :
bool The result of the contains test.
Notes
If
otheris empty,Trueis always returned. In all other cases,self.contains(other)beingTrueimplies thatself.overlaps(other)is alsoTrue.Testing whether an instantaneous
astropy.time.Timevalue is contained in a timespan is not equivalent to testing a timespan constructed viaTimespan.fromInstant, because Timespan cannot exactly represent zero-duration intervals. In particular,[a, b)contains the timeb, but not the timespan[b, b + 1ns)that would be returned byTimespan.fromInstant(b)`.- other :
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difference(other: lsst.daf.butler.core.timespan.Timespan) → Generator[lsst.daf.butler.core.timespan.Timespan, None, None]¶ Return the one or two timespans that cover the interval(s).
The interval is defined as one that is in
selfbut notother.This is implemented as a generator because the result may be zero, one, or two
Timespanobjects, depending on the relationship between the operands.Parameters: - other :
Timespan Timespan to subtract.
Yields: - other :
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classmethod
fromInstant(time: astropy.time.core.Time) → lsst.daf.butler.core.timespan.Timespan¶ Construct a timespan that approximates an instant in time.
This is done by constructing a minimum-possible (1 ns) duration timespan.
This is equivalent to
Timespan(time, time, padInstantaneous=True), but may be slightly more efficient.Parameters: - time :
astropy.time.Time Time to use for the lower bound.
Returns: - instant :
Timespan A
[time, time + 1ns)timespan.
- time :
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classmethod
from_json(json_str: str, universe: Optional[DimensionUniverse] = None, registry: Optional[Registry] = None) → SupportsSimple¶ Return new class from JSON string.
Converts a JSON string created by
to_jsonand return something of the supplied class.Parameters: - json_str :
str Representation of the dimensions in JSON format as created by
to_json().- universe :
DimensionUniverse, optional The special graph of all known dimensions. Passed directly to
from_simple().- registry :
lsst.daf.butler.Registry, optional Registry to use to convert simple name of a DatasetType to a full
DatasetType. Passed directly tofrom_simple().
Returns: - constructed : Any
Newly-constructed object.
- json_str :
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classmethod
from_simple(simple: List[int], universe: Optional[DimensionUniverse] = None, registry: Optional[Registry] = None) → Timespan¶ Construct a new object from simplified form.
Designed to use the data returned from the
to_simplemethod.Parameters: - simple :
listofint The values returned by
to_simple().- universe :
DimensionUniverse, optional Unused.
- registry :
lsst.daf.butler.Registry, optional Unused.
Returns: - result :
Timespan Newly-constructed object.
- simple :
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classmethod
from_yaml(loader: yaml.loader.SafeLoader, node: yaml.nodes.MappingNode) → Optional[lsst.daf.butler.core.timespan.Timespan, None]¶ Convert YAML node into _SpecialTimespanBound.
Parameters: - loader :
yaml.SafeLoader Instance of YAML loader class.
- node :
yaml.ScalarNode YAML node.
Returns: - value :
Timespan Timespan instance, can be
None.
- loader :
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intersection(*args) → lsst.daf.butler.core.timespan.Timespan¶ Return a new
Timespanthat is contained by all of the given ones.Parameters: - *args
All positional arguments are
Timespaninstances.
Returns: - intersection :
Timespan The intersection timespan.
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classmethod
makeEmpty() → lsst.daf.butler.core.timespan.Timespan¶ Construct an empty timespan.
Returns: - empty :
Timespan A timespan that is contained by all timespans (including itself) and overlaps no other timespans (including itself).
- empty :
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overlaps(other: lsst.daf.butler.core.timespan.Timespan | astropy.time.core.Time[lsst.daf.butler.core.timespan.Timespan, astropy.time.core.Time]) → bool¶ Test if the intersection of this Timespan with another is empty.
Parameters: Returns: - overlaps :
bool The result of the overlap test.
Notes
If either
selforotheris empty, the result is alwaysFalse. In all other cases,self.contains(other)beingTrueimplies thatself.overlaps(other)is alsoTrue.- overlaps :
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to_json(minimal: bool = False) → str¶ Convert this class to JSON form.
The class type is not recorded in the JSON so the JSON decoder must know which class is represented.
Parameters: - minimal :
bool, optional Use minimal serialization. Requires Registry to convert back to a full type.
Returns: - json :
str The class in JSON string format.
- minimal :
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to_simple(minimal: bool = False) → List[int]¶ Return simple python type form suitable for serialization.
Parameters: - minimal :
bool, optional Use minimal serialization. Has no effect on for this class.
Returns: - minimal :
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classmethod
to_yaml(dumper: yaml.dumper.Dumper, timespan: lsst.daf.butler.core.timespan.Timespan) → Any¶ Convert Timespan into YAML format.
This produces a scalar node with a tag “!_SpecialTimespanBound” and value being a name of _SpecialTimespanBound enum.
Parameters: - dumper :
yaml.Dumper YAML dumper instance.
- timespan :
Timespan Data to be converted.
- dumper :
- begin :