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NOTE: Highlights with a version number in bold represent a change from version 14.0. | ||||||||
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Photometry
| ||||||||
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Engineering ConversionCommon Pipeline | ||||||||
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Photometer Pipeline
|
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NOTE: Highlights with a version number in bold represent a change from version 14.0. | ||||||||
Line: 387 to 388 | ||||||||
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Spectrometer Pipeline
|
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in version 14.x | ||||||||
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| ||||||||
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< < | * HCSS 142.: the gyro-based attitude reconstruction algorithm has been modified in order to in order to allow switching the logic used when estimating the star vector measurement error during the star tracker attitude calculations | |||||||
> > |
| |||||||
Numeric routinesData fitting |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in version 14.x | ||||||||
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> > | * HCSS 142.: the gyro-based attitude reconstruction algorithm has been modified in order to in order to allow switching the logic used when estimating the star vector measurement error during the star tracker attitude calculations | |||||||
Numeric routinesData fitting |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> | ||||||||
Changed: | ||||||||
< < | What's new in HIPE 14 | |||||||
> > | What's new in version 14.x | |||||||
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HIFI | ||||||||
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| ||||||||
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Core system |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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PACS
| ||||||||
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|
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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SPIRE
| ||||||||
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Spectroscopy
|
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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PACS | ||||||||
Changed: | ||||||||
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Deleted: | ||||||||
< < |
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SPIRE
| ||||||||
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Spectroscopy | ||||||||
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---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Calibration | ||||||||
Line: 344 to 343 | ||||||||
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Pipeline | ||||||||
Changed: | ||||||||
< < | * A new task runPacsSpg has been introduced, with which a user can run a full SPG pipeline within HIPE, starting from the level-0 data in an observation context from the HSA, or even from the raw telemetry files when they are available. | |||||||
> > | * A new task runPacsSpg was introduced in 14.0, with which a user can run a full SPG pipeline within HIPE, starting from the level-0 data in an observation context from the HSA, or even from the raw telemetry files when they are available. | |||||||
Photometry
| ||||||||
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| ||||||||
Added: | ||||||||
> > | ||||||||
Spectroscopy | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > | * Interactive pipeline scripts in 14.0, 14.2 | |||||||
| ||||||||
Changed: | ||||||||
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| |||||||
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| |||||||
| ||||||||
Changed: | ||||||||
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Calibration | ||||||||
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Analysis tools | ||||||||
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Spectroscopy
| ||||||||
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> > |
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Product changes | ||||||||
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Spectroscopy | ||||||||
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Documentation | ||||||||
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SPIRE |
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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| |||||||
HIFI | ||||||||
Changed: | ||||||||
< < |
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Numeric routines | ||||||||
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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 --> | |||||||
| ||||||||
Changed: | ||||||||
< < | <!--<br />* Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup <br />--> | |||||||
> > | <-- | |||||||
-- AlvarGarcia - 24 Nov 2014
Editors & Viewers |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
Line: 17 to 17 | ||||||||
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< < |
| |||||||
> > |
| |||||||
HIFI
| ||||||||
Line: 107 to 107 | ||||||||
| ||||||||
Changed: | ||||||||
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Numeric routines |
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---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Core system | ||||||||
Line: 348 to 349 | ||||||||
| ||||||||
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> > |
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Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
Line: 23 to 23 | ||||||||
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SPIRE
|
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---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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| ||||||||
Added: | ||||||||
> > |
| |||||||
PACS
| ||||||||
Line: 215 to 220 | ||||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
HIFI Spectrum ToolboxSpectrum Explorer (HIFI specifics) | ||||||||
Line: 225 to 233 | ||||||||
Baseline Removal
| ||||||||
Added: | ||||||||
> > |
| |||||||
Deconvolution
Spectral Cube creation | ||||||||
Line: 240 to 250 | ||||||||
HiClass export tool | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
DocumentationFor HCSS 14, many figures were refreshed in both manuals (HIFI Data Reduction Guide and HIFI Pipeline Specification). | ||||||||
Line: 253 to 263 | ||||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Spectrometer Pipeline
| ||||||||
Added: | ||||||||
> > |
| |||||||
Interactive Analysis and Tools
| ||||||||
Added: | ||||||||
> > |
| |||||||
Documentation |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
| ||||||||
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 in HIPE 14
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Changed: | ||||||||
< < |
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Analysis tools |
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---|---|---|---|---|---|---|---|---|
<-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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Core
| ||||||||
Changed: | ||||||||
< < |
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| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
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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 in HIPE 14
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
See also the HIPE known issues and the Data products known issues pages for last-minute information on known problems. | ||||||||
Changed: | ||||||||
< < |
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> > |
| |||||||
Highlights | ||||||||
Line: 20 to 20 | ||||||||
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Changed: | ||||||||
< < |
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Changed: | ||||||||
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> > |
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Core system | ||||||||
Line: 79 to 80 | ||||||||
would open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. | ||||||||
Changed: | ||||||||
< < | ![]() | |||||||
> > | ![]() | |||||||
Passing a Jython script as the first argument will still behave as running HIPE in batch mode:
bash> hipe myScript.py arg1 arg2 | ||||||||
Line: 272 to 273 | ||||||||
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
Spectroscopy
| ||||||||
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Spectroscopy | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
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| ||||||||
Line: 333 to 334 | ||||||||
Calibration Products
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
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| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
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Calibration Framework | ||||||||
Line: 362 to 363 | ||||||||
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: | ||||||||
< < | <-- | |||||||
> > | <!--<br />* Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup <br />--> | |||||||
-- AlvarGarcia - 24 Nov 2014
Editors & Viewers |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's new in HIPE 14 | ||||||||
Line: 20 to 20 | ||||||||
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Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
| ||||||||
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 in HIPE 14
| ||||||||
Line: 17 to 17 | ||||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
HIFI
| ||||||||
Line: 96 to 99 | ||||||||
Dataset viewerAstronomical utilities | ||||||||
Deleted: | ||||||||
< < |
| |||||||
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
Numeric routinesData fitting | ||||||||
Line: 361 to 364 | ||||||||
Documentation | ||||||||
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< < | <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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< < | <!--<br />* Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup <br />--> | |||||||
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-- AlvarGarcia - 24 Nov 2014
Editors & Viewers |
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Dataset viewerAstronomical utilities | ||||||||
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HIFI Software Configuration and PropertiesHIFI Calibration | ||||||||
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Opening the observation context instead is also possible, either with the popup menu or by configuring so as the default behaviour, in the Quick Analysis preferences category.
Command line | ||||||||
Changed: | ||||||||
< < | It is now possible to pass arguments to HIPE from the command line, which will be tried to be interpreted as files to be opened with the proper viewers. For example: | |||||||
> > | It is now possible to pass arguments to HIPE from the command line, which will be tried to be interpreted as files to be opened with the proper viewers. For example: | |||||||
bash> hipe myImage.jpg cube.fits resultTable.csvwould open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. ![]() | ||||||||
Changed: | ||||||||
< < | Passing a Jython script as the first argument will still behave as running HIPE in batch mode: | |||||||
> > | Passing a Jython script as the first argument will still behave as running HIPE in batch mode: | |||||||
bash> hipe myScript.py arg1 arg2would not open the HIPE window, but execute the script with the given arguments passed to it. | ||||||||
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What's new in HIPE 14
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See also the HIPE known issues and the Data products known issues pages for last-minute information on known problems. | ||||||||
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Highlights | ||||||||
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Opening the observation context instead is also possible, either with the popup menu or by configuring so as the default behaviour, in the Quick Analysis preferences category.
Command line | ||||||||
Changed: | ||||||||
< < | It is now possible to pass arguments to HIPE from the command line, which will be tried to be interpreted as files to be opened with the proper viewers. For example: | |||||||
> > | It is now possible to pass arguments to HIPE from the command line, which will be tried to be interpreted as files to be opened with the proper viewers. For example: | |||||||
bash> hipe myImage.jpg cube.fits resultTable.csvwould open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. | ||||||||
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< < | ![]() | |||||||
> > | ![]() | |||||||
Added: | ||||||||
> > | Passing a Jython script as the first argument will still behave as running HIPE in batch mode: | |||||||
bash> hipe myScript.py arg1 arg2would not open the HIPE window, but execute the script with the given arguments passed to it. | ||||||||
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What's new in HIPE 14
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Baseline Removal
Deconvolution | ||||||||
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Spectral Cube creationflagToolidentifyLines | ||||||||
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HiClass export tool | ||||||||
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< < | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
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< < | 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.![]() ![]() | |||||||
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< < | <-- | |||||||
> > | <!--<br />* Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup <br />--> | |||||||
-- AlvarGarcia - 24 Nov 2014
Editors & Viewers |
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Product changes | ||||||||
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< < | What's coming up in HIPE 14 | |||||||
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Common PipelinePhotometer Pipeline | ||||||||
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Spectrometer Pipeline
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HIFI Software Configuration and PropertiesHIFI Calibration | ||||||||
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HIFI PipelinehifiPipeline task | ||||||||
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Level 0 PipelineWBS PipelineHRS PipelineLevel 1 PipelineLevel 2 Pipeline | ||||||||
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Level 2.5 Pipeline | ||||||||
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HIFI Products
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HIFI Spectrum ToolboxSpectrum Explorer (HIFI specifics) | ||||||||
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HiClass export tool | ||||||||
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DocumentationFor HCSS 14, many figures were refreshed in both manuals (HIFI Data Reduction Guide and HIFI Pipeline Specification). |
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HRS PipelineLevel 1 PipelineLevel 2 Pipeline | ||||||||
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HIFI PipelinehifiPipeline task | ||||||||
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Level 0 PipelineWBS PipelineHRS Pipeline | ||||||||
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HIFI Spectrum ToolboxSpectrum Explorer (HIFI specifics) | ||||||||
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HIFI Data Processing ToolsStanding Wave Removal | ||||||||
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Baseline Removal | ||||||||
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Deconvolution
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Level 2.5 PipelineHIFI Products | ||||||||
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HIFI Spectrum ToolboxSpectrum Explorer (HIFI specifics) |
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SPIRE
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PACSPipeline | ||||||||
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> > | * A new task runPacsSpg has been introduced, with which a user can run a full SPG pipeline within HIPE, starting from the level-0 data in an observation context from the HSA, or even from the raw telemetry files when they are available. | |||||||
Photometry
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Analysis tools | ||||||||
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Photometry
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Display
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Analysis |
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Documentation | ||||||||
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< < | <!-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
> > | <-- COMMENT BOX CODE - DO NOT EDIT --> | |||||||
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< < | <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 --> | |||||||
> > | <-- | |||||||
-- AlvarGarcia - 24 Nov 2014
Editors & Viewers |
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's coming up in HIPE 14 | ||||||||
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Highlights | ||||||||
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< < | HIPE | |||||||
> > | Core
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PACS | ||||||||
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SPIRE
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< < | <!-- 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 coming up in HIPE 14
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< < | Planned workHIPE * TBD HIFI * TBD PACS * TBD SPIRE * TBD | |||||||
Highlights | ||||||||
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Spectroscopy
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HIFI Data Processing ToolsStanding Wave Removal | ||||||||
Added: | ||||||||
> > |
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Baseline Removal | ||||||||
Added: | ||||||||
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Deconvolution | ||||||||
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Spectral Cube creationflagToolidentifyLines | ||||||||
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HiClass export tool | ||||||||
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CalibrationPhotometrySpectroscopy | ||||||||
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> > |
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Analysis toolsPhotometry
Spectroscopy | ||||||||
Added: | ||||||||
> > |
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Product changesPhotometry
Spectroscopy | ||||||||
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< < |
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DeconvolutionSpectral Cube creationflagTool | ||||||||
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> > | identifyLines
| |||||||
HiClass export tool |
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<-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> What's coming up in HIPE 14 | ||||||||
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would open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. | ||||||||
Changed: | ||||||||
< < | ![]() | |||||||
> > | ![]() | |||||||
Passing a Jython script as the first argument will still behave as running HIPE in batch mode: | ||||||||
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There are interesting enhancements in the Console view with HIPE 14.0:
| ||||||||
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< < |
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PlottingTablePlotterOverPlotter | ||||||||
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Improvement of readability of quality flags in the meta data of products in FITS files. Now one meta data item per quality flag making proper use of parameter values and descriptions. | ||||||||
Changed: | ||||||||
< < | eg.) qflag_PARXXXXX_p <value> ⁄ <description> | |||||||
> > | eg.) qflag_PARXXXXX_p <value> ⁄ <description> | |||||||
Systematic product generation | ||||||||
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PipelinePhotometry
| ||||||||
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< < |
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| |||||||
CalibrationPhotometrySpectroscopy | ||||||||
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Photometry
Spectroscopy | ||||||||
Changed: | ||||||||
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DocumentationSPIRE |
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PACS |
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<-- Google Analytics script BEGIN --> <-- Google Analytics script END --><!-- END OF ANALYTICS CODE --> What's coming up in HIPE 14 | ||||||||
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Improvement of readability of quality flags in the meta data of products in FITS files. Now one meta data item per quality flag making proper use of parameter values and descriptions. eg.) | ||||||||
Changed: | ||||||||
< < | qflag_PARXXXXX_p <value> ⁄ <description> | |||||||
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Systematic product generation | ||||||||
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Quality control | ||||||||
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> > | Reorganization of quality flags as private or public for HCSS, HIFI, PACS and SPIRE Quality Flags. This ensures that only the flags useful for the assessment of the science by the user (the public ones) make its way to the quality summary.All the information from the quality flags remain at the quality product, for internal assessment or history. In the quality report, a new "Ïmpact" column in the "Quality flags" table, after "Concept" and "Value" columns has been added. This new column is an automatically filled column with a brief text describing the possible consequences for science data from the situations that caused that quality flag to be raised. Improvement of readability of quality flags in the meta data of products in FITS files. Now one meta data item per quality flag making proper use of parameter values and descriptions. eg.) qflag_PARXXXXX_p <value> ⁄ <description> | |||||||
Systematic product generationData input-output | ||||||||
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Installer | ||||||||
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> > | The user installer has been reduced by 400-800MB by removing the pointing distortion maps previously included with the data a part of user installation. | |||||||
DocumentationHIFI |
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AnalysisData cubes | ||||||||
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< < | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
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Other functionsSource extraction | ||||||||
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> > | Improved history recording so that it can be added to the sub-products of a context. | |||||||
Quality controlSystematic product generation |
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Recent open files The size of the recently opened files list, which can be accessed through the File menu, is now configurable through preferences. | ||||||||
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> > |
Metadata tables A new option in the popup menu of metadata tables allows copying cell values in other way than with the usual key combinations (Ctrl+C or Cmd+C). Array data viewer The array data viewer shows tooltips over the spinners (above the data table) for informing about the array dimensions. | |||||||
Quick AnalysisThere is a new perspective in HIPE, which is accessible by clicking on the magnifying glass at the top right toolbar, for quickly inspecting scientific data from the Herschel Science Archive. | ||||||||
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Opening the observation context instead is also possible, either with the popup menu or by configuring so as the default behaviour, in the Quick Analysis preferences category.
Command line | ||||||||
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< < | Starting with version 14.0, it is possible to pass arguments to HIPE from the command line, which will try to interpret them as files to be opened with the proper viewers. For example: | |||||||
> > | It is now possible to pass arguments to HIPE from the command line, which will be tried to be interpreted as files to be opened with the proper viewers. For example: | |||||||
bash> hipe myImage.jpg cube.fits resultTable.csvwould open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. |
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bash> hipe myScript.py arg1 arg2would not open the HIPE window, but execute the script with the given arguments passed to it. | ||||||||
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> > | ConsoleThere are interesting enhancements in the Console view with HIPE 14.0:
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PlottingTablePlotterOverPlotter |
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When clicking on an observation, its standalone browse products are opened in the editor area for quick analysis, by means of the image, spectra or cube viewers. Opening the observation context instead is also possible, either with the popup menu or by configuring so as the default behaviour, in the Quick Analysis preferences category. | ||||||||
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> > | Command lineStarting with version 14.0, it is possible to pass arguments to HIPE from the command line, which will try to interpret them as files to be opened with the proper viewers. For example:bash> hipe myImage.jpg cube.fits resultTable.csvwould open HIPE with three viewers: one for the image, a spectrum explorer for the cube, and a dataset viewer for the CSV table. ![]() bash> hipe myScript.py arg1 arg2would not open the HIPE window, but execute the script with the given arguments passed to it. | |||||||
PlottingTablePlotterOverPlotter |
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Core systemHIPE | ||||||||
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> > | Editors & Viewers | |||||||
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> > | Default editor
The default editor for every type of data, which is the one used when double clicking on a variable, is preserved regardless the editors opened through the Open With menu.
The previous behaviour, which is to use the last opened editor as the default, can still be set, by means of a new preference in the Editors & Viewers category.
Recent open files
The size of the recently opened files list, which can be accessed through the File menu, is now configurable through preferences.
Quick AnalysisThere is a new perspective in HIPE, which is accessible by clicking on the magnifying glass at the top right toolbar, for quickly inspecting scientific data from the Herschel Science Archive. Observations can be searched by target name, observation id, operational day or Ra/Dec. When clicking on an observation, its standalone browse products are opened in the editor area for quick analysis, by means of the image, spectra or cube viewers. Opening the observation context instead is also possible, either with the popup menu or by configuring so as the default behaviour, in the Quick Analysis preferences category. | |||||||
PlottingTablePlotterOverPlotter | ||||||||
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What's coming up in HIPE 14
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< < | <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. ![]() ![]() | |||||||
> > | <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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< < | <!-- * Set ALLOWTOPICCHANGE = RegisteredUsersGroup, TWikiAdminGroup --> | |||||||
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Planned work | ||||||||
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HIFI | ||||||||
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PACS | ||||||||
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SPIRE | ||||||||
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Highlights | ||||||||
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Images | ||||||||
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< < | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
> > | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
Display | ||||||||
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Data cubes | ||||||||
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< < | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
> > | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
Display | ||||||||
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Products and datasets | ||||||||
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< < | A new Auxiliary Observation Summary Product which can be retrieved using the tag LATEST_OBSERVATION_SUMMARY_PRODUCT. This product contains one dataset with a summary of information for each observation. Useful methods exist for querying the data as documented here: ObservationSummaryProduct | |||||||
> > | A new Auxiliary Observation Summary Product which can be retrieved using the tag LATEST_OBSERVATION_SUMMARY_PRODUCT. This product contains one dataset with a summary of information for each observation. Useful methods exist for querying the data as documented here: ObservationSummaryProduct | |||||||
Observation context | ||||||||
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< < | A new Calibration Table Product exists under the Auxiliary Context in each Observation Context. This product contains calibration tables data for the given instrument including exactly how the hardware was configured, hard limits, soft limits etc. This provides valuable information for the long term completeness of an observation. Useful methods exist for querying the table data as documented here: SimpleCalTableProduct | |||||||
> > | A new Calibration Table Product exists under the Auxiliary Context in each Observation Context. This product contains calibration tables data for the given instrument including exactly how the hardware was configured, hard limits, soft limits etc. This provides valuable information for the long term completeness of an observation. Useful methods exist for querying the table data as documented here: SimpleCalTableProduct | |||||||
Product Access Layer | ||||||||
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PipelinePhotometry | ||||||||
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Analysis toolsPhotometry | ||||||||
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SpectroscopyProduct changesPhotometry | ||||||||
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Interactive Analysis and ToolsDocumentation | ||||||||
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> > | <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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PACS SPIRE | ||||||||
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SPIRECalibration Products | ||||||||
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Photometer PipelineSpectrometer Pipeline | ||||||||
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PACS |
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HiClass export toolDocumentation | ||||||||
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> > | For HCSS 14, many figures were refreshed in both manuals (HIFI Data Reduction Guide and HIFI Pipeline Specification).
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Source extractionImages | ||||||||
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> > | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
Display | ||||||||
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> > | * Added shortcuts to some of the task directly in the image viewer. | |||||||
AnalysisSpectra | ||||||||
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AnalysisData cubes | ||||||||
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> > | * When requesting the unit, the FITS compatible unit is returned. * The naxis keywords are not longer duplicated in the fits header. * The Wcs ia added to all datasets of the images (like the stddev, ...). | |||||||
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AnalysisHerschel Science Archive |
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Calibration sourcesProducts and datasets | ||||||||
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> > | A new Auxiliary Observation Summary Product which can be retrieved using the tag LATEST_OBSERVATION_SUMMARY_PRODUCT. This product contains one dataset with a summary of information for each observation. Useful methods exist for querying the data as documented here: ObservationSummaryProduct | |||||||
Observation context | ||||||||
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> > | A new Calibration Table Product exists under the Auxiliary Context in each Observation Context. This product contains calibration tables data for the given instrument including exactly how the hardware was configured, hard limits, soft limits etc. This provides valuable information for the long term completeness of an observation. Useful methods exist for querying the table data as documented here: SimpleCalTableProduct | |||||||
Product Access LayerTasks |
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<-- ANALYTICS CODE - DO NOT EDIT --> <-- Google Analytics script BEGIN --> <-- Google Analytics script END --> <-- END OF ANALYTICS CODE --> What's coming up in HIPE 14
Planned workHIPE * TBD HIFI * TBD PACS * TBD SPIRE * TBDHighlightsHIPE 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 -->blog comments powered by Disqus <-- END OF COMMENT BOX CODE --> <--
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