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SPIRE
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Interactive Analysis and Tools | ||||||||
Changed: | ||||||||
< < | Using the final, legacy URLs, to the calibration tree and some auxiliary files (e.g. Planck all sky maps) in the interactive useful scripts. | |||||||
> > |
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PhotometrySpectroscopy
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> > |
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Product changesPhotometry | ||||||||
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Documentation
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SPIRE |
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Core
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Added: | ||||||||
> > |
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HIFI
| ||||||||
Added: | ||||||||
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| ||||||||
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CalibrationPhotometry | ||||||||
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Core
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< < |
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HIFI
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SPIRE | ||||||||
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PipelinePhotometrySpectroscopy | ||||||||
Added: | ||||||||
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CalibrationPhotometry | ||||||||
Added: | ||||||||
> > |
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SpectroscopyAnalysis toolsPhotometrySpectroscopy | ||||||||
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> > |
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Product changesPhotometrySpectroscopyDocumentation | ||||||||
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SPIRE | ||||||||
Changed: | ||||||||
< < | Calibration Products | |||||||
> > | The following are the only changes or new addtions in HIPE v15 for SPIRE: | |||||||
Changed: | ||||||||
< < | Calibration FrameworkPreprocessingEngineering ConversionCommon Pipeline | |||||||
> > | Interactive Analysis and Tools | |||||||
Changed: | ||||||||
< < | Photometer Pipeline | |||||||
> > | Using the final, legacy URLs, to the calibration tree and some auxiliary files (e.g. Planck all sky maps) in the interactive useful scripts. | |||||||
Changed: | ||||||||
< < | Spectrometer Pipeline | |||||||
> > | Documentation | |||||||
Changed: | ||||||||
< < | Interactive Analysis and Tools | |||||||
> > | Final updates in SPIRE Data reduction Guide. | |||||||
Deleted: | ||||||||
< < | Documentation | |||||||
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> > | <-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> | |||||||
What's New for HIPE 15.x
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Documentation | ||||||||
Changed: | ||||||||
< < | <!-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
> > | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
Changed: | ||||||||
< < | <script type="text/javascript"><br /> var disqus_shortname = 'herscheltwiki'; // required: replace example with your forum shortname<br /><br /> (function() {<br /> var dsq = document.createElement('script'); dsq.type = 'text/javascript'; dsq.async = true;<br /> dsq.src = 'http://' + disqus_shortname + '.disqus.com/embed.js';<br /> (document.getElementsByTagName('head')[0] || document.getElementsByTagName('body')[0]).appendChild(dsq);<br /> })();<br /></script> <noscript>Please enable JavaScript to view the comments powered by Disqus.![]() ![]() | |||||||
> > | blog comments powered by Disqus![]() <-- END OF COMMENT BOX CODE --> | |||||||
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Data input-output | ||||||||
Changed: | ||||||||
< < | The FitsArchive task has been upgraded in order to re-organise keywords in the products FITS headers in a much more structured fashion. Keywords will not be grouped and ordered according to categories, in the same spirit as what was done e.g. for products from the Hubble Space Telescope or Spitzer. The following snapshots illustrate this re-structuration for the first part of a given FITS header in one HIFI product. The left image shows the product header as of 14.1.0. The right image shows the product header that would be obtained by saving with the FitsArchive task under 15. | |||||||
> > | The FitsArchive task has been upgraded in order to re-organise keywords in the products FITS headers in a much more structured fashion. Keywords will not be grouped and ordered according to categories, in the same spirit as what was done e.g. for products from the Hubble Space Telescope or Spitzer. The following snapshots illustrate this re-structuration for the first part of a given FITS header in one HIFI product. The top image shows the product header as of 14.1.0. The bottom image shows the product header that would be obtained by saving with the FitsArchive task under 15. | |||||||
Changed: | ||||||||
< < | ![]() ![]() | |||||||
> > | ![]() ![]() | |||||||
Virtual ObservatoryInstaller |
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Astronomical utilities | ||||||||
Added: | ||||||||
> > | A new script named Astrometry Thermoelastic Drift Correction has been incorporated to the General Useful Scripts category. This is aimed at estimating astrometry shifts induced by thermoelastic drifts. These appear when an observation is performed at 'warm' attitude conditions (Star Tracker 2 temperature > -15 C). The script calculates the average temperature of STR2 sensors during the mid-point of the observation and, if that is > -15 C, it uses an established STR2-Z-axis offset correlation function to get the Z-axis offset and derive RA and DEC offsets. Two possible outputs are provided.
| |||||||
Numeric routinesData fittingData interpolation | ||||||||
Line: 97 to 101 | ||||||||
Observation contextProduct Access Layer | ||||||||
Deleted: | ||||||||
< < | Useful ScriptsA new script named Astrometry Thermoelastic Drift Correction has been incorporated to the General Useful Scripts category. This is aimed at estimating astrometry shifts induced by thermoelastic drifts. These appear when an observation is performed at 'warm' attitude conditions (Star Tracker 2 temperature > -15 C). The script calculates the average temperature of STR2 sensors during the mid-point of the observation and, if that is > -15 C, it uses an established STR2-Z-axis offset correlation function to get the Z-axis offset and derive RA and DEC offsets. Two possible outputs are provided.
| |||||||
Tasks
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Changed: | ||||||||
< < | <-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> | |||||||
> > | <!-- ANALYTICS CODE - DO NOT EDIT --><-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> | |||||||
What's New for HIPE 15.x
| ||||||||
Line: 14 to 14 | ||||||||
Core
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
HIFI | ||||||||
Changed: | ||||||||
< < |
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> > |
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Changed: | ||||||||
< < |
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> > |
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PACS SPIRE | ||||||||
Line: 75 to 75 | ||||||||
Analysis | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
Data cubesDisplay | ||||||||
Line: 87 to 87 | ||||||||
Analysis | ||||||||
Changed: | ||||||||
< < | Spectrum task extract is much faster when applied on spectral cubes than in previous versions. | |||||||
> > | Spectrum task extract is much faster when applied on spectral cubes than in previous versions. | |||||||
Herschel Science Archive | ||||||||
Line: 99 to 99 | ||||||||
Product Access LayerUseful Scripts | ||||||||
Added: | ||||||||
> > | A new script named Astrometry Thermoelastic Drift Correction has been incorporated to the General Useful Scripts category. This is aimed at estimating astrometry shifts induced by thermoelastic drifts. These appear when an observation is performed at 'warm' attitude conditions (Star Tracker 2 temperature > -15 C). The script calculates the average temperature of STR2 sensors during the mid-point of the observation and, if that is > -15 C, it uses an established STR2-Z-axis offset correlation function to get the Z-axis offset and derive RA and DEC offsets. Two possible outputs are provided.
| |||||||
Tasks
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
Changed: | ||||||||
< < | ||||||||
> > | ||||||||
p = Product() openVariable("p") # already available with previous versions of HIPE openVariable(p) # also available since HIPE 15.0 | ||||||||
Line: 226 to 229 | ||||||||
Documentation | ||||||||
Changed: | ||||||||
< < | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
> > | <!-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
Changed: | ||||||||
< < | blog comments powered by Disqus![]() <-- END OF COMMENT BOX CODE --> | |||||||
> > | <script type="text/javascript"><br /> var disqus_shortname = 'herscheltwiki'; // required: replace example with your forum shortname<br /><br /> (function() {<br /> var dsq = document.createElement('script'); dsq.type = 'text/javascript'; dsq.async = true;<br /> dsq.src = 'http://' + disqus_shortname + '.disqus.com/embed.js';<br /> (document.getElementsByTagName('head')[0] || document.getElementsByTagName('body')[0]).appendChild(dsq);<br /> })();<br /></script> <noscript>Please enable JavaScript to view the comments powered by Disqus.![]() ![]() | |||||||
| ||||||||
Changed: | ||||||||
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> > | <!--<br /> * Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup <br />--> | |||||||
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Spectrum task extract is much faster when applied on spectral cubes than in previous versions. | ||||||||
Changed: | ||||||||
< < | Useful ScriptsHerschel Science Archive | |||||||
> > | Herschel Science Archive | |||||||
Calibration sources | ||||||||
Line: 98 to 97 | ||||||||
Observation contextProduct Access Layer | ||||||||
Added: | ||||||||
> > | Useful Scripts | |||||||
Tasks |
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Documentation | ||||||||||||||||||||||
Added: | ||||||||||||||||||||||
> > | External librariesHIPE uses a rich set of external libraries, of which the following have been upgraded:
| |||||||||||||||||||||
HIFIHIFI Software Configuration and Properties |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
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Changed: | ||||||||
< < | <!-- ANALYTICS CODE - DO NOT EDIT --><-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> | |||||||
> > | <-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> | |||||||
What's New for HIPE 15.x
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< < |
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PACS SPIRE | ||||||||
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Documentation | ||||||||
Changed: | ||||||||
< < | <!-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
> > | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
Changed: | ||||||||
< < | <script type="text/javascript"> var disqus_shortname = 'herscheltwiki'; // required: replace example with your forum shortname (function() { var dsq = document.createElement('script'); dsq.type = 'text/javascript'; dsq.async = true; dsq.src = 'http://' + disqus_shortname + '.disqus.com/embed.js'; (document.getElementsByTagName('head')[0] || document.getElementsByTagName('body')[0]).appendChild(dsq); })(); </script> <noscript>Please enable JavaScript to view the comments powered by Disqus. ![]() ![]() | |||||||
> > | blog comments powered by Disqus![]() <-- END OF COMMENT BOX CODE --> | |||||||
| ||||||||
Changed: | ||||||||
< < | <!-- * Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup --> | |||||||
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> > |
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Console | ||||||||
Line: 61 to 62 | ||||||||
Source extractionImages | ||||||||
Added: | ||||||||
> > |
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DisplayAnalysis | ||||||||
Line: 110 to 112 | ||||||||
openVariable("p") # already available with previous versions of HIPE openVariable(p) # also available since HIPE 15.0 | ||||||||
Added: | ||||||||
> > |
archive = FitsArchive() | |||||||
Quality controlSystematic product generation |
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SpectraDisplay | ||||||||
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> > |
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Analysis | ||||||||
Added: | ||||||||
> > |
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Data cubesDisplay | ||||||||
Added: | ||||||||
> > |
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Analysis | ||||||||
Added: | ||||||||
> > |
Spectrum task extract is much faster when applied on spectral cubes than in previous versions. | |||||||
Useful ScriptsHerschel Science Archive | ||||||||
Line: 83 to 99 | ||||||||
Tasks | ||||||||
Added: | ||||||||
> > |
| |||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
p = Product() openVariable("p") # already available with previous versions of HIPE | ||||||||
Changed: | ||||||||
< < | openVariable(p) # also available since HIPE 15.0 | |||||||
> > | openVariable(p) # also available since HIPE 15.0 | |||||||
Quality control |
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HIPE | ||||||||
Added: | ||||||||
> > | Editors & Viewers
ConsoleImproved auto-completion mechanism.Plug-ins
| |||||||
PlottingTablePlotterOverPlotter | ||||||||
Deleted: | ||||||||
< < | Dataset viewer | |||||||
Astronomical utilities | ||||||||
Line: 69 to 83 | ||||||||
Tasks | ||||||||
Added: | ||||||||
> > |
p = Product() openVariable("p") # already available with previous versions of HIPE openVariable(p) # also available since HIPE 15.0 | |||||||
Quality controlSystematic product generation |
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Changed: | ||||||||
< < | <-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> | |||||||
> > | <!-- ANALYTICS CODE - DO NOT EDIT --><-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> | |||||||
What's New for HIPE 15.x
| ||||||||
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Changed: | ||||||||
< < | ||||||||
> > | ||||||||
HighlightsCore
| ||||||||
Added: | ||||||||
> > |
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HIFI
| ||||||||
Line: 58 to 57 | ||||||||
Data cubesDisplayAnalysis | ||||||||
Changed: | ||||||||
< < | ||||||||
> > | Useful Scripts | |||||||
Herschel Science ArchiveCalibration sources | ||||||||
Line: 165 to 164 | ||||||||
Documentation | ||||||||
Changed: | ||||||||
< < | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
> > | <!-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
Changed: | ||||||||
< < |
blog comments powered by Disqus![]() <-- END OF COMMENT BOX CODE --> | |||||||
> > | <script type="text/javascript"> var disqus_shortname = 'herscheltwiki'; // required: replace example with your forum shortname (function() { var dsq = document.createElement('script'); dsq.type = 'text/javascript'; dsq.async = true; dsq.src = 'http://' + disqus_shortname + '.disqus.com/embed.js'; (document.getElementsByTagName('head')[0] || document.getElementsByTagName('body')[0]).appendChild(dsq); })(); </script> <noscript>Please enable JavaScript to view the comments powered by Disqus. ![]() ![]() | |||||||
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Changed: | ||||||||
< < | <--
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> > | <!-- * Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup --> | |||||||
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> | ||||||||
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HighlightsCore | ||||||||
Changed: | ||||||||
< < | ||||||||
> > |
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HIFI | ||||||||
Changed: | ||||||||
< < |
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> > |
| |||||||
| ||||||||
Line: 76 to 76 | ||||||||
Data input-output | ||||||||
Added: | ||||||||
> > | The FitsArchive task has been upgraded in order to re-organise keywords in the products FITS headers in a much more structured fashion. Keywords will not be grouped and ordered according to categories, in the same spirit as what was done e.g. for products from the Hubble Space Telescope or Spitzer. The following snapshots illustrate this re-structuration for the first part of a given FITS header in one HIFI product. The left image shows the product header as of 14.1.0. The right image shows the product header that would be obtained by saving with the FitsArchive task under 15.
![]() ![]() | |||||||
Virtual ObservatoryInstaller | ||||||||
Line: 185 to 188 | ||||||||
-->
| ||||||||
Added: | ||||||||
> > |
|
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---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> | ||||||||
Line: 104 to 104 | ||||||||
Spectrum tasks (HIFI specifics)The task mkRms has been improved in order to better handle line masking when computing the statistics in spectra containing spectral lines. This will lead to very slight differences with the noise estimates reported in the pipeline products from 14.1. | ||||||||
Added: | ||||||||
> > | On top of that, the task convertK2Jy has been upgraded so that it can take as source model an input file in the form of an image. This allows more complex and ad hoc source filling factor estimate in case the Gaussian or Disk approximation are not appropriate. See the Data Reduction Guide and task URM for more details. | |||||||
HIFI Data Processing ToolsStanding Wave RemovalBaseline Removal | ||||||||
Line: 112 to 114 | ||||||||
flagToolidentifyLinesCatalog | ||||||||
Changed: | ||||||||
< < | See also examples in the task URM![]() | |||||||
> > | See also examples in the task URM. | |||||||
HiClass export toolThe useful script explaining how to export HIFI data into Class with the hiClass task (SaveObsContextToClass.py) has been removed in 15. This is because HIFI FITS files as processed by HIPE 12 and later can now be directly read by Class, if one uses a Gildas installation later than October 2015 - see the following Manual. For HCSS products older than HIPE 12, we recommend to either use more recent products, or fall back on the hiClass export, using the documentation of the task as provided in its URM![]() |
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> | ||||||||
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Added: | ||||||||
> > |
| |||||||
PACS SPIRE | ||||||||
Line: 102 to 103 | ||||||||
Spectrum Explorer (HIFI specifics)Spectrum tasks (HIFI specifics) | ||||||||
Changed: | ||||||||
< < | TBS | |||||||
> > | The task mkRms has been improved in order to better handle line masking when computing the statistics in spectra containing spectral lines. This will lead to very slight differences with the noise estimates reported in the pipeline products from 14.1. | |||||||
HIFI Data Processing ToolsStanding Wave RemovalBaseline Removal |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> | ||||||||
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Core HIFI | ||||||||
Changed: | ||||||||
< < | ||||||||
> > |
| |||||||
PACS SPIRE | ||||||||
Line: 100 to 102 | ||||||||
Spectrum Explorer (HIFI specifics)Spectrum tasks (HIFI specifics) | ||||||||
Added: | ||||||||
> > | TBS | |||||||
HIFI Data Processing ToolsStanding Wave RemovalBaseline RemovalDeconvolutionSpectral Cube creationflagTool | ||||||||
Added: | ||||||||
> > | identifyLinesCatalog | |||||||
Added: | ||||||||
> > | See also examples in the task URM![]() | |||||||
HiClass export tool | ||||||||
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> > | The useful script explaining how to export HIFI data into Class with the hiClass task (SaveObsContextToClass.py) has been removed in 15. This is because HIFI FITS files as processed by HIPE 12 and later can now be directly read by Class, if one uses a Gildas installation later than October 2015 - see the following Manual. For HCSS products older than HIPE 12, we recommend to either use more recent products, or fall back on the hiClass export, using the documentation of the task as provided in its URM![]() | |||||||
Documentation | ||||||||
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> > | Update of DRG and some URMs | |||||||
PACSPipeline |
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> > | <-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's New for HIPE 15.x | |||||||
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HighlightsCore HIFI PACS SPIRECore systemHIPEPlottingTablePlotterOverPlotterDataset viewerAstronomical utilitiesNumeric routinesData fittingData interpolationRandom numbersStatisticsTrend analysisMappingOther functionsSource extractionImagesDisplayAnalysisSpectraDisplayAnalysisData cubesDisplayAnalysisHerschel Science ArchiveCalibration sourcesProducts and datasetsObservation contextProduct Access LayerTasksQuality controlSystematic product generationData input-outputVirtual ObservatoryInstallerDocumentationHIFIHIFI Software Configuration and PropertiesHIFI CalibrationHIFI PipelinehifiPipeline taskLevel 0 PipelineWBS PipelineHRS PipelineLevel 1 PipelineLevel 2 PipelineLevel 2.5 PipelineHIFI ProductsHIFI Spectrum ToolboxSpectrum Explorer (HIFI specifics)Spectrum tasks (HIFI specifics)HIFI Data Processing ToolsStanding Wave RemovalBaseline RemovalDeconvolutionSpectral Cube creationflagToolHiClass export toolDocumentationPACSPipelinePhotometrySpectroscopyCalibrationPhotometrySpectroscopyAnalysis toolsPhotometrySpectroscopyProduct changesPhotometrySpectroscopyDocumentationSPIRECalibration ProductsCalibration FrameworkPreprocessingEngineering ConversionCommon PipelinePhotometer PipelineSpectrometer PipelineInteractive Analysis and ToolsDocumentation<-- COMMENT BOX CODE - DO NOT EDIT --> ![]() <-- END OF COMMENT BOX CODE --> <--
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