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LSSTApplications
18.0.0+106,18.0.0+50,19.0.0,19.0.0+1,19.0.0+10,19.0.0+11,19.0.0+13,19.0.0+17,19.0.0+2,19.0.0-1-g20d9b18+6,19.0.0-1-g425ff20,19.0.0-1-g5549ca4,19.0.0-1-g580fafe+6,19.0.0-1-g6fe20d0+1,19.0.0-1-g7011481+9,19.0.0-1-g8c57eb9+6,19.0.0-1-gb5175dc+11,19.0.0-1-gdc0e4a7+9,19.0.0-1-ge272bc4+6,19.0.0-1-ge3aa853,19.0.0-10-g448f008b,19.0.0-12-g6990b2c,19.0.0-2-g0d9f9cd+11,19.0.0-2-g3d9e4fb2+11,19.0.0-2-g5037de4,19.0.0-2-gb96a1c4+3,19.0.0-2-gd955cfd+15,19.0.0-3-g2d13df8,19.0.0-3-g6f3c7dc,19.0.0-4-g725f80e+11,19.0.0-4-ga671dab3b+1,19.0.0-4-gad373c5+3,19.0.0-5-ga2acb9c+2,19.0.0-5-gfe96e6c+2,w.2020.01
LSSTDataManagementBasePackage
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Align SkyFrames using the offset coordinate system? (bool)
This attribute is a boolean value which controls how a SkyFrame behaves when it is used (by Frame::findFrame or Frame::convert) as a template to match another (target) SkyFrame. It determines the coordinate system in which the two SkyFrames are aligned if a match occurs.
If the template and target SkyFrames both have defined offset coordinate systems (i.e. the SkyRefIs attribute is set to either "Origin" or " Pole"), and they both have a non-zero value for AlignOffset, then alignment occurs within the offset coordinate systems (that is, a UnitMap will always be used to align the two SkyFrames). If either the template or target SkyFrame has zero (the default value) for AlignOffset, or if either SkyFrame has SkyRefIs set to "Ignored", then alignment occurring within the coordinate system specified by the AlignSystem attribute.
Format celestal coordinates as times? (bool)
This attribute specifies the default style of formatting to be used (e.g. by astFormat) for the celestial coordinate values described by a SkyFrame. It takes a separate boolean value for each SkyFrame axis so that, for instance, the setting "AsTime(2)=0" specifies the default formatting style for celestial latitude values.
If the AsTime attribute for a SkyFrame axis is zero, then coordinates on that axis will be formatted as angles by default (using degrees, minutes and seconds), otherwise they will be formatted as times (using hours, minutes and seconds).
The default value of AsTime is chosen according to the sky coordinate system being represented, as determined by the SkyFrame's System attribute. This ensures, for example, that right ascension values will be formatted as times by default, following normal conventions.
Epoch of the mean equinox. (double)
This attribute is used to qualify those celestial coordinate systems described by a SkyFrame which are notionally based on the ecliptic (the plane of the Earth's orbit around the Sun) and/or the Earth's equator.
Both of these planes are in motion and their positions are difficult to specify precisely. In practice, therefore, a model ecliptic and/or equator are used instead. These, together with the point on the sky that defines the coordinate origin (the intersection of the two planes termed the "mean equinox") move with time according to some model which removes the more rapid fluctuations. The SkyFrame class supports both the FK4 and FK5 models.
The position of a fixed source expressed in any of these coordinate systems will appear to change with time due to movement of the coordinate system itself (rather than motion of the source). Such coordinate systems must therefore be qualified by a moment in time (the "epoch of the mean equinox" or "equinox" for short) which allows the position of the model coordinate system on the sky to be determined. This is the role of the Equinox attribute.
The Equinox attribute is stored as a Modified Julian Date, but when setting or getting its value you may use the same formats as for the Epoch attribute (q.v.).
The default Equinox value is B1950.0 (Besselian) for the old FK4-based coordinate systems (see the System attribute) and J2000.0 (Julian) for all others.
Is the specified celestial axis a latitude axis? (bool, read only)
This is a read-only boolean attribute that indicates the nature of the specified axis. The attribute has a non-zero value if the specified axis is a celestial latitude axis (Declination, Galactic latitude, etc), and is zero otherwise.
Is the specified celestial axis a longitude axis? (bool, read only)
This is a read-only boolean attribute that indicates the nature of the specified axis. The attribute has a non-zero value if the specified axis is a celestial longitude axis (Right Ascension, Galactic longitude, etc), and is zero otherwise.
Index of the latitude axis. (int, read only)
This read-only attribute gives the index (1 or 2) of the latitude axis within the SkyFrame (taking into account any current axis permutations).
Index of the longitude axis. (int, read only)
This read-only attribute gives the index (1 or 2) of the longitude axis within the SkyFrame (taking into account any current axis permutations).
Display negative longitude values? (bool)
This attribute is a boolean value which controls how longitude values are normalized for display by astNorm.
If the NegLon attribute is zero, then normalized longitude values will be in the range zero to 2.pi. If NegLon is non-zero, then normalized longitude values will be in the range -pi to pi.
The default value depends on the current value of the SkyRefIs attribute, If SkyRefIs has a value of "Origin", then the default for NegLon is one, otherwise the default is zero.
Sky projection description. (string)
This attribute provides a place to store a description of the type of sky projection used when a SkyFrame is attached to a 2-dimensional object, such as an image or plotting surface. For example, typical values might be "orthographic", "Hammer-Aitoff" or "cylindrical equal area".
The Projection value is purely descriptive and does not affect the celestial coordinate system represented by the SkyFrame in any way. If it is set to a non-blank string, the description provided may be used when forming the default value for the SkyFrame's Title attribute (so that typically it will appear in graphical output, for instance). The default value is an empty string.
Position defining the offset coordinate system. (double)
This attribute allows a SkyFrame to represent offsets, rather than absolute axis values, within the coordinate system specified by the System attribute. If supplied, SkyRef should be set to hold the longitude and latitude of a point within the coordinate system specified by the System attribute. The coordinate system represented by the SkyFrame will then be rotated in order to put the specified position at either the pole or the origin of the new coordinate system (as indicated by the SkyRefIs attribute). The orientation of the modified coordinate system is then controlled using the SkyRefP attribute.
If an integer axis index is included in the attribute name (e.g. "SkyRef(1)") then the attribute value should be supplied as a single floating point axis value, in radians, when setting a value for the attribute, and will be returned in the same form when getting the value of the attribute. In this case the integer axis index should be "1" or "2" (the values to use for longitude and latitude axes are given by the LonAxis and LatAxis attributes).
If no axis index is included in the attribute name (e.g. "SkyRef") then the attribute value should be supplied as a character string containing two formatted axis values (an axis 1 value followed by a comma, followed by an axis 2 value). The same form will be used when getting the value of the attribute.
The default values for SkyRef are zero longitude and zero latitude.
The offset coordinate system within a SkyFrame should normally be considered as a superficial "re-badging" of the axes of the coordinate system specified by the System attribute - it merely provides an alternative numerical "label" for each position in the System coordinate system. The SkyFrame retains full knowledge of the celestial coordinate system on which the offset coordinate system is based (given by the System attribute). For instance, the SkyFrame retains knowledge of the way that one celestial coordinate system may "drift" with respect to another over time. Normally, if you attempt to align two SkyFrames (e.g. using Frame::convert or Frame::findFrame), the effect of any offset coordinate system defined in either SkyFrame will be removed, resulting in alignment being performed in the celestial coordinate system given by the AlignSystem attribute. However, by setting the AlignOffset attribute ot a non-zero value, it is possible to change this behaviour so that the effect of the offset coordinate system is not removed when aligning two SkyFrames.
Selects the nature of the offset coordinate system. (string)
This attribute controls how the values supplied for the SkyRef and SkyRefP attributes are used. These three attributes together allow a SkyFrame to represent offsets relative to some specified origin or pole within the coordinate system specified by the System attribute, rather than absolute axis values. SkyRefIs can take one of the case-insensitive values "Origin", "Pole" or "Ignored".
If SkyRefIs is set to "Origin", then the coordinate system represented by the SkyFrame is modified to put the origin of longitude and latitude at the position specified by the SkyRef attribute.
If SkyRefIs is set to "Pole", then the coordinate system represented by the SkyFrame is modified to put the north pole at the position specified by the SkyRef attribute.
If SkyRefIs is set to "Ignored" (the default), then any value set for the SkyRef attribute is ignored, and the SkyFrame represents the coordinate system specified by the System attribute directly without any rotation.
Position on primary meridian of offset coordinate system. (double)
This attribute is used to control the orientation of the offset coordinate system defined by attributes SkyRef and SkyRefIs. If used, it should be set to hold the longitude and latitude of a point within the coordinate system specified by the System attribute. The offset coordinate system represented by the SkyFrame will then be rotated in order to put the position supplied for SkyRefP on the zero longitude meridian. This rotation is about an axis from the centre of the celestial sphere to the point specified by the SkyRef attribute. The default value for SkyRefP is usually the north pole (that is, a latitude of +90 degrees in the coordinate system specified by the System attribute). The exception to this is if the SkyRef attribute is itself set to either the north or south pole. In these cases the default for SkyRefP is the origin (that is, a (0,0) in the coordinate system specified by the System attribute).
If an integer axis index is included in the attribute name (e.g. "SkyRefP(1)") then the attribute value should be supplied as a single floating point axis value, in radians, when setting a value for the attribute, and will be returned in the same form when getting the value of the attribute. In this case the integer axis index should be "1" or "2" (the values to use for longitude and latitude axes are given by the LonAxis and LatAxis attributes).
If no axis index is included in the attribute name (e.g. "SkyRefP") then the attribute value should be supplied as a character string containing two formatted axis values (an axis 1 value followed by a comma, followed by an axis 2 value). The same form will be used when getting the value of the attribute.
The smallest significant shift in sky coordinates. (double)
This attribute indicates the accuracy of the axis values that will be represented by the SkyFrame. If the arc-distance between two positions within the SkyFrame is smaller than the value of SkyTol, then the two positions will (for the puposes indicated below) be considered to be co-incident.
This value is used only when constructing the Mapping between two different SkyFrames (for instance, when calling Frame::convert or Frame::findFrame). If the transformation between the two SkyFrames causes positions to shift by less than SkyTol arc-seconds, then the transformation is replaced by a UnitMap. This could in certain circumatances allow major simplifications to be made to the transformation between any pixel grids associated with the two SkyFrames (for instance, if each SkyFrame is part of the WCS FrameSet associated with an image).
A common case is when two SkyFrames use the FK5 system, but have slightly different Epoch values. If the AlignSystem attribute has its default value of "ICRS", then the transformation between the two SkyFrames will include a very small rotation (FK5 rotates with respect to ICRS as a rate of about 0.0005 arc-seconds per year). In most circumstances such a small rotation is insignificant. Setting SkyTol to some suitably small non-zero value will cause this rotation to be ignored, allowing much simpler transformations to be used.
The test to determine the shift introduced by transforming between the two SkyFrames is performed by transforming a set of 14 position spread evenly over the whole sky. The largest shift produced at any of these 14 positions is compared to the value of SkyTol.
The SkyTol value is in units of arc-seconds, and the default value is 0.001.
1.8.13