|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Astronomical utilities
RadialVelocity task and utility class renamed to RadialV and now using the proper Doppler sign convention. | |
> > |
Numeric routines | |
Wavelet transform
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
- If the Monospaced font is not really monospaced, HIPE proposes an alternate font.
| | RadialVelocity task and utility class renamed to RadialV and now using the proper Doppler sign convention.
Images | |
-
- A count-down progress bar.
Calibration sources | | The Calibrators view allows access to the database of calibration sources at ESAC, used by HSC calibration scientists. It contains spectra of planets, asteroids, and fixed targets. The data can be viewed in the usual HIPE viewers for spectra and images, and manipulated using Jython commands.
| | There is now a detailed outline shown in the Outline view when a task is selected in the Tasks view. This allows inspection of the structure of a task without the need to either use the Console view or open its GUI in the Editor view.
Data input-output | | We have also added a few pre-set applications (Topcat, Aladin and VOSpec) to the Send To menu. This menu is accessible by right-clicking on a variable. The pre-set applications are visible, even if the application in question is not running and/or HIPE is not connected to the VO. Using these pre-set is transparent to the user: When sending a variable, the application will be automatically started first and the data will be sent.
Documentation | | HIFI
HIFI Pipeline | | Level 1 Pipeline
Level 2 Pipeline | |
< < | HIFI Products | > > | HIFI Products | | | |
< < | HIFI Spectrum Toolbox | > > | HIFI Spectrum Toolbox | | Spectrum Explorer (HIFI specifics)
Spectrum tasks (HIFI specifics)
--> | |
- Obsid now exported again to CLASS header
PACS | |
- The API has new methods for showing differences between two calibration trees and for verifying that expected metadata is present and correct.
Common Pipeline |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
- Indent and unindent buttons added to the toolbar.
- If the Monospaced font is not really monospaced, HIPE proposes an alternate font.
| |
> > | | |
Astronomical utilities
RadialVelocity task and utility class renamed to RadialV and now using the proper Doppler sign convention. | |
> > |
| |
Images
Display | |
-
- Fit parameters are written to file.
- A count-down progress bar.
| |
> > | | |
Calibration sources | |
The Calibrators view allows access to the database of calibration sources at ESAC, used by HSC calibration scientists. It contains spectra of planets, asteroids, and fixed targets. The data can be viewed in the usual HIPE viewers for spectra and images, and manipulated using Jython commands. | |
> > | | |
Product Access Layer | |
There is now a detailed outline shown in the Outline view when a task is selected in the Tasks view. This allows inspection of the structure of a task without the need to either use the Console view or open its GUI in the Editor view. | |
> > | | |
Data input-output
-
simpleFitsReader and simpleFitsWriter now also support reading/writting datasets (not just products).
| |
We have also added a few pre-set applications (Topcat, Aladin and VOSpec) to the Send To menu. This menu is accessible by right-clicking on a variable. The pre-set applications are visible, even if the application in question is not running and/or HIPE is not connected to the VO. Using these pre-set is transparent to the user: When sending a variable, the application will be automatically started first and the data will be sent. | |
> > | | |
Documentation | |
-
- Replaced some hardcoded references with hyperlinks.
- Updates to Chapter 5 and Chapter 11 for Level 2.5 products.
| |
< < | Plug-ins | > > | Plug-ins | |
It is now possible for plug-in authors to publish new versions of plug-ins, which will be automatically picked up by existing users of the plug-in. If a new version of a plug-in is found by HIPE, and the author has indicated that the update is compatible with the user's version of HIPE, then HIPE will ask the user if the plug-in should be updated. The update mechanism is automatic, though HIPE must be restarted for the changes to be completed. | |
HIFI | |
> > | | |
HIFI Pipeline
- doPipelineConfiguration now passes changes to the level 2 pipeline. To use this task, pass an HTP to the GUI (doPipelineConfiguration), modify the pipeline steps as required. Press accept (default name of output is out) then pass this new configuration to the pipeline task:
obs_new = hifiPipeline(obs=obs, params=out, save=False) | |
> > | | |
HIFI Data Processing Tools
Standing Wave Removal | |
- doDeconvolution now produces a result even if deconvolution fails. In this case an error message is given
- doDeconvolution now read flags from USB, rather than LSB. Channel flags have always been read from the USB so this change makes it easier for you to pass flagged data to the task
| |
> > | | |
HiClass export tool
- Obsid now exported again to CLASS header
| |
> > | | |
PACS | |
-
- The trees available in the archive can be listed.
- The API has new methods for showing differences between two calibration trees and for verifying that expected metadata is present and correct.
| |
> > | | |
Common Pipeline
- The
AssociateSkyPositionTask now creates a new table "avgVelocity" in photometer level1 scanmap products. The table contains two columns: "sampleTime" (TAI) and "avgVelocity" (deg/sec)
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Virtual Observatory | |
> > | The VO external tools have been made accessible from the Tools menu.
We have also added a few pre-set applications (Topcat, Aladin and VOSpec) to the Send To menu. This menu is accessible by right-clicking on a variable. The pre-set applications are visible, even if the application in question is not running and/or HIPE is not connected to the VO. Using these pre-set is transparent to the user: When sending a variable, the application will be automatically started first and the data will be sent. | | Installer
Documentation | |
-
- Replaced some hardcoded references with hyperlinks.
- Updates to Chapter 5 and Chapter 11 for Level 2.5 products.
| |
> > | Plug-ins
It is now possible for plug-in authors to publish new versions of plug-ins, which will be automatically picked up by existing users of the plug-in. If a new version of a plug-in is found by HIPE, and the author has indicated that the update is compatible with the user's version of HIPE, then HIPE will ask the user if the plug-in should be updated. The update mechanism is automatic, though HIPE must be restarted for the changes to be completed.
| | HIFI
HIFI Software Configuration and Properties |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7
| |
< < | | > > | | |
Core system | |
History | |
< < |
- Detailed error can be opened by double-click in the history table.
| > > |
- Detailed error information can be opened with a double click in the Trace column of the History view.
| |
Status bar
- Progress bar shows the current line number of the executing script.
| |
< < |
- The garbage collector can be run with the button located at the right side of the memory bar.
| > > |
- New bin-shaped button to the right of the memory bar, at the bottom of the HIPE window, to run the garbage collector and free memory manually.
| |
Generic viewers
Dataset viewer | |
< < |
- Multiple cells can be selected and copied in the TableDataset viewer.
| > > |
- Multiple cells can be selected and copied in the TableDataset viewer.
| |
Jython editor | |
< < |
- Find/Replace dialog enhanced. It can show now whitespace characters.
| > > |
- Find/Replace dialog enhanced. It can now show now whitespace characters.
| |
- Autoindentation of Jython code improved.
- Indent and unindent buttons added to the toolbar.
- If the Monospaced font is not really monospaced, HIPE proposes an alternate font.
| | OverPlotter
Astronomical utilities | |
< < | RadialVelocity task and util class renamed to RadialV and now use the proper Doppler sign convention. | > > | RadialVelocity task and utility class renamed to RadialV and now using the proper Doppler sign convention. | | Numeric routines
Data fitting
Data interpolation | | Other functions
Source extraction | |
< < |
- Various internal changes have been made to the Source Extractor tasks, but no changes to the functionality.
| |
Images
Display
- Adapted the popup menu to make it possible to work with axes, add a compass and add a scale.
- Display now returns the commands done using the popup menu to the HIPE console. This makes it very easy to reconstruct an image plot from within a script.
- When dragging source positions to an image, the circles are locked. When dragging contours to an image, the contours are also locked.
| |
< < |
- Added method addArcSecs to add a line of a number of arcseconds to the image.
| > > |
- Added method
addArcSecs to add a line of a given length in arcseconds to an image.
| |
- When using the opacity slider with a cube, the next image is used as the underlying image, not the next layer of the cube anymore.
Analysis | |
< < |
- You can now load all monochrome or indexed gif files using importRgbImageTask
| > > |
- You can now load all monochrome or indexed gif files using
importRgbImageTask .
| |
Spectra
Display | |
-
- sf.doFit( ) or sf.doGlobalFit( )
- sf.saveFitParametersAsASCII(fileName) # writes parameters of all models to fileName
- m.toASCII(dirName) # writes parameters to dirName/[modelname].txt
| |
< < |
- The SpectrumFitterGUI has, in the export TAB, also the possibility to export fit parameters to file.
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, the user can select from:
| > > |
- The SpectrumFitterGUI has, in the export TAB, also the possibility to export fit parameters to file.
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, you can select from:
| |
-
- Instrument specific initial model.
| |
< < | | > > |
-
- User specific initial models - you can specify the models.
- Addition to SpectrumFitterGUI, MultiTAB:
| |
-
- Some information on what will happen.
- Fit parameters are written to file.
- A count-down progress bar.
| |
Calibration sources | |
< < | We have integrated the Calibration Source Database into HIPE. There is a Calibrators View on the Workbench (you may have to reset the perspective for it to appear). | > > | Integrated the Calibration Source Database into HIPE. There is a Calibrators view in the Work Bench perspective, next to the Navigator view. You may have to reset the perspective for it to appear. | | | |
< < | The Calibrators View allows access to the database with calibration sources at ESAC, that is used by HSC calibration scientists. It contains spectra of planets, asteroids, and fixed targets. The data can be viewed in the usual HIPE viewers for spectra and images, and manipulated using Jython commands. | > > | The Calibrators view allows access to the database of calibration sources at ESAC, used by HSC calibration scientists. It contains spectra of planets, asteroids, and fixed targets. The data can be viewed in the usual HIPE viewers for spectra and images, and manipulated using Jython commands. | |
Products and datasets
Observation context | | Tasks
The default Task GUI has been improved with the following upgrades: | |
< < |
- Parameter error detection (red X) also checks the
validator of the parameter
- A new
Help button gives easy direct access to the URM description of the task
- White space in layout moved to the lower part of the panel
- Editors based on text fields now require half the width
| > > |
- Parameter error detection (red X) also checks the
validator of the parameter.
- A new
Help button gives easy direct access to the URM description of the task.
- White space in layout moved to the lower part of the panel.
- Editors based on text fields now require half the width.
| |
- Labels of parameters have now a maximum size to reserve space for the editors.
| |
< < |
- Support for grouping inputs in multiple Tabs. For tasks that have inputs related to different aspects or simply a lot of them, they can be presented in several tabs.
There is now a detailed outline shown in the Outline View when a task is selected in the Task View. This allows inspection of the structure of a task without the need to either use the Console or open its GUI in the Editor . Also, the system is undergoing a review of task compliancy (naming, documentation, tooltips ...) that will make all tasks self-explanatory (ongoing for HIPE 8). | > > |
- Support for grouping inputs in multiple tabs. For tasks that have inputs related to different aspects or simply a lot of them, they can be presented in several tabs.
| | | |
> > | There is now a detailed outline shown in the Outline view when a task is selected in the Tasks view. This allows inspection of the structure of a task without the need to either use the Console view or open its GUI in the Editor view. | |
Quality control
Systematic product generation
Data input-output | |
< < |
-
simpleFitsReader and simpleFitsWriter now also support reading/writting Datasets (not just Products ).
- The
Export View now shows the tags associated with each Observation version.
- The
localStoreWriter task now allows to add a tag to the saved product.
- Now, when you use the contextual menu to save a product variable you will use the
Save to Pool tool instead of the localStoreWriter task.
-
localStoreWriter and localStoreCopier now use a better integrated GUI to select-create a pool.
| > > |
-
simpleFitsReader and simpleFitsWriter now also support reading/writting datasets (not just products).
- The Export view now shows the tags associated with each observation version.
- The
localStoreWriter task now allows to add a tag to the saved product.
-
localStoreWriter and localStoreCopier now use a better integrated GUI to select and create a pool.
| |
- File filters for file dialogs are now self-explanatory (accepted extensions ...).
| |
< < |
- The
clear task now has a simplified syntax to delete all variables (clear() without any parameter, will delete all).
| > > |
- The
clear task now has a simplified syntax to delete all variables (clear() , without any parameter, will delete all variables).
| |
Virtual Observatory | |
Documentation | |
> > |
- Replaced the Read Me First document with the Welcome documentation page, and by a linked page listing the available manuals.
- In the welcome page, added links to a YouTube channel
of tutorials and a Twitter channel of tips.
- Completely revised text and screenshots of the Quick Start Guide.
- Data Analysis Guide
- Scripting and Data Mining guide
- HIPE Owner's Guide
- Frequently Asked Questions
- Products Definitions Document
- Replaced some hardcoded references with hyperlinks.
- Updates to Chapter 5 and Chapter 11 for Level 2.5 products.
| | HIFI
HIFI Software Configuration and Properties |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
HIPE | |
< < | Jython editor
- Find/Replace dialog enhanced. It now can show whitespace characters.
- Autoindentation of Jython improved.
- Indent and unindent buttons added to the toolbar.
| | Console
- Incremental search (Ctrl+I) available.
- Console help text enhanced.
| |
< < |
- New internal commands
!clear , !help and !history added.
| > > |
- New internal commands
!clear , !help and !history .
| |
History
- Detailed error can be opened by double-click in the history table.
| |
< < | Jobs control | > > | Status bar | |
- Progress bar shows the current line number of the executing script.
| |
> > |
- The garbage collector can be run with the button located at the right side of the memory bar.
Generic viewers
Dataset viewer
- Multiple cells can be selected and copied in the TableDataset viewer.
Jython editor
- Find/Replace dialog enhanced. It can show now whitespace characters.
- Autoindentation of Jython code improved.
- Indent and unindent buttons added to the toolbar.
- If the Monospaced font is not really monospaced, HIPE proposes an alternate font.
| |
Plotting
TablePlotter
OverPlotter | |
< < | Dataset viewer | |
Astronomical utilities
RadialVelocity task and util class renamed to RadialV and now use the proper Doppler sign convention. |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
HIFI Data Processing Tools
Standing Wave Removal | |
< < |
- averscan option has been removed as it was found not to work well
| > > |
- new default doplot=2 option opens no more than 2 fitHifiFringe plot windows at the time and allows for inspection before processing next spectrum
- averscan option fitHifiFringe has been removed as standing wave characteristics vary too much between scans
- fitHifiFringe now shows up as applicable task to both HTPs and ObsContexts
| |
Baseline Removal | |
< < |
- The htpcopy option has been removed
| > > |
- New non-stop option in interactive mode of fitBaseline allows automatic processing of remaining spectra
- The htpcopy option of fitBaseline has been removed as modified HTPs are now properly displayed in SpectrumExplorer
| |
Deconvolution
- doDeconvolution now produces a result even if deconvolution fails. In this case an error message is given
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | HIPE> print c.photometer
| |
< < |
New calibration files containing the actual 'best' calibration data for MadMap :
PCalPhotometer_InvnttBL_FM_v4.fits
PCalPhotometer_InvnttBS_FM_v4.fits
PCalPhotometer_InvnttRed_FM_v4.fits
| > > | MadMap
New calibration files containing the actual 'best' calibration data for MadMap :
PCalPhotometer_InvnttBL_FM_v4.fits
PCalPhotometer_InvnttBS_FM_v4.fits
PCalPhotometer_InvnttRed_FM_v4.fits
| | You need to update your local calibration tree Menu to activate it (Menu -> Tools -> PACS_CAL -> run Updater).
You may check by printing the calibration tree :
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | This shall have very minor impact on the coordinates, but correct reverse order of uplink.
Spectroscopy | |
> > |
- All level-2 tasks now do an internal loop over line ID. They behave now the same as the level-0/1 tasks: If you do not select a particular line/range before then the level-2 tasks just process all lines/ranges. As a consequence the level-2 products have changed a bit:
- We no longer have a list context for each line ID within another list context: All slices of a level-2 product are now stored in a single list context. This is much more practical when selecting slices based on arbitrary criteria.
- The pacsSliceContext task now contains all the rules in the ipipe scripts as default rules: Also, it slices by line ID, raster column, raster line, nodding position, nod cycle number, is out of field and band. The rules in the scripts are also now optional and merely for information.
- The interactive pipeline scripts (ipipe) are now tested in the nightly tester
- The interactive pipeline scripts (ipipe) are moved in the build from the directory scripts/pacs/spg/pipeline/ipipe/spec to scripts/pacs/scripts/ipipe/spec since they had to be moved to the package pacs_scripts
| |
Calibration
Photometry | |
Spectroscopy | |
< < | | > > |
- Wrong coordinates in Spectrometer results: update of spec spatial cal file
- Improvements in wavelength calibration scatter for spectral pixels in band B2B -> wavelength calibration file updated
| | Analysis tools
Slicing
- Saving intermediate data on machines with low memory is now done more clever: The slices are only saved to the temporary pool when the memory usage is more than 75% and the sliced product contains more than one slice.
| |
Also, since these keywords are now always consistent with the BlockTable and Status contents they can and should be used for slice selection. The new task pacsSelectSlices does this meta-keyword based selection. It has the same interface as the selectSlices Python function. | |
< < |
- The wavelength grid is now also stored in a list context
| |
-
- All level-2 tasks now do an internal loop over line ID. They behave now the same as the level-0/1 tasks: If you do not select a particular line/range before then the level-2 tasks just process all lines/ranges. As a consequence the level-2 products have changed a bit:
- The wavelength grid is now also stored in a list context, since one needs to pass several ranges from task to task.
- We no longer have a list context for each line ID within another list context: All slices of a level-2 product are now stored in a single list context. This is much more practical when selecting slices based on arbitrary criteria.
| |
< < | | > > |
- Status item "GratingCycle" and "IndexInCycle" is now created for unchopped modes
| | Documentation |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Pipeline
Photometry | |
> > | Improvements for SSO scan maps
Assuming the object move linear a linear interpolation between start and end position is done. This method provides 'smoother' coordinates especially for point source.
Old behavior :
frames = correctRaDec4Sso(frames, horizonsProduct=horizonsProduct, timeOffset=timeOffset, orbitEphem=orbitEphem)
frames = correctRaDec4Sso(frames, horizonsProduct=horizonsProduct, timeOffset=timeOffset, linear=1, orbitEphem=orbitEphem)
New implementation :
frames = correctRaDec4Sso(frames, horizonsProduct=horizonsProduct, timeOffset=timeOffset, linear=0, orbitEphem=orbitEphem)
Aberration correction
Change the oder applying SIAM and Aberration correction in photAddInstantPointing and specAddInstantPointing .
This shall have very minor impact on the coordinates, but correct reverse order of uplink. | | Spectroscopy
Calibration
Photometry | |
> > | Flux calibration
The photometer flux calibration has changed (new response calibration file "FM, 6").
Absolute fluxes of point-sources will change by less than 5%, extended sources will change by 10-20%.
Aperture photometry of point-sources requires from now on the application of
new aperture correction factors, taking into account that there is still significant flux
beyond 60 arcsec.
These new correction factors (together with the old ones) are stored in:
PCalPhotometer_ApertureCorrection_FM_v2.fits and can be retrieved via the new task
photApertureCorrectionPointSource to be applied after annularSkyAperturePhotometry .
See also the update of PACS ipipe script Menu -> Pipeline -> PACS -> Photometer -> Copped point source -> standard pipeline -> L3_pointSourceAperturePhotometry.py
You need to update your local calibration tree Menu to activate it (Menu -> Tools -> PACS_CAL -> run Updater).
You may check by printing the calibration tree :
HIPE> c=getCalTree()
HIPE> print c.photometer
New calibration files containing the actual 'best' calibration data for MadMap :
PCalPhotometer_InvnttBL_FM_v4.fits
PCalPhotometer_InvnttBS_FM_v4.fits
PCalPhotometer_InvnttRed_FM_v4.fits
You need to update your local calibration tree Menu to activate it (Menu -> Tools -> PACS_CAL -> run Updater).
You may check by printing the calibration tree :
HIPE> c=getCalTree()
HIPE> print c.photometer
| | Spectroscopy
Analysis tools | |
> > | Slicing
- Saving intermediate data on machines with low memory is now done more clever: The slices are only saved to the temporary pool when the memory usage is more than 75% and the sliced product contains more than one slice.
- The temporary pools of HIPE are now written under a directory 'null value' which is created where you start HIPE ( HcssSpr:12911
). Workaround: Set the following property in your user.props file:
hcss.ia.pg.temporalpoolparent = ${user.home}/.hcss/lstore
These temporary pools are called tmp_product_sink_NNNNN | | Photometry | |
> > |
- A new Mask Array Viewer displays Masks with their correct size (also the timeline).
- Add start time of last cooler recycling to meta data of products A new calibration product was introduced : CoolerRecyclingTimes
- A convenience tool times = extractCoolerRecTimes(obs, calTree) returns the last cooler recycling of an observation
- This file will be updated on a regular base
| | Spectroscopy | |
> > |
- Map2signalCubeTask gets an additional shortcut: m2sc (besides map2signalCube)
- Spectrum Explorer : New extension panel to edit masks is now fully working
- Spectrum Explorer : Performance improvements
| |
Product changes | |
> > |
- calTree version is now in meta data of products
| | Photometry
Spectroscopy | |
> > |
- Frames and PacsCube meta data is made consistent for every product change (like select or join)
- Additional meta keywords added: onOffSource, minWave, maxWave, nodCycle, lineId
- All masks which are not excluded in rebinning are propagated from PacsCube to PacsRebinnedCube. They can be obtained with the getFlag() method which returns a Flag dataset, which is similar to a PACS mask.
- We have now two more sliced products: SlicedPacsCube? and SlicedPacsRebinnedCube?. SlicedPacsCube? offers the same functionality as SlicedFrames?, but SlicedPacsRebinnedCube? has limited functionality, since it does not have a blocktable. Add, remove and replace work, but selection should be done with the pacsSelectSlices task.
Each slice is described by the following slice info meta keywords (recognizable by description prefix "SLICE_INFO:"):
Keyword |
Values |
Description |
lineId |
0..N |
Numerical ID of a distinct wavelength range (usually a line scan) |
lineDescription |
string |
Which spectral line has been observed (or tells that it is a range scan) |
nodPosition |
A/B |
Nodding position |
nodCycleNum |
1..N |
Nodding cycle number |
isOffPosition |
false/true |
Is it an off position according to the IsOutOfField status? |
onOffSource |
0,1,2 |
Based on new ONSOURCE/OFFSOURCE Status keywords: 0 = not science, 1 = on-source, 2 = off-source |
rasterId |
N M |
first value: raster column, second value: raster line |
calBlock |
false/true |
Belongs to slice to a calibration block? |
minWave |
float |
Minimum wavelength of range |
maxWave |
float |
Maximum wavelength of range |
aotMode |
string |
AOT mode |
Also, since these keywords are now always consistent with the BlockTable and Status contents they can and should be used for slice selection. The new task pacsSelectSlices does this meta-keyword based selection. It has the same interface as the selectSlices Python function.
- The wavelength grid is now also stored in a list context
- All level-2 tasks now do an internal loop over line ID. They behave now the same as the level-0/1 tasks: If you do not select a particular line/range before then the level-2 tasks just process all lines/ranges. As a consequence the level-2 products have changed a bit:
- The wavelength grid is now also stored in a list context, since one needs to pass several ranges from task to task.
- We no longer have a list context for each line ID within another list context: All slices of a level-2 product are now stored in a single list context. This is much more practical when selecting slices based on arbitrary criteria.
| |
Documentation | |
> > | | |
SPIRE |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
HIPE | |
> > | Jython editor
- Find/Replace dialog enhanced. It now can show whitespace characters.
- Autoindentation of Jython improved.
- Indent and unindent buttons added to the toolbar.
Console
- Incremental search (Ctrl+I) available.
- Console help text enhanced.
- New internal commands
!clear , !help and !history added.
History
- Detailed error can be opened by double-click in the history table.
Jobs control
- Progress bar shows the current line number of the executing script.
| | Plotting
TablePlotter
OverPlotter |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Changes to existing Tasks
-
WaveletDeglitcherTask now offers the option to make the number of corrected samples dependent on the glitch size by setting the optionReconstruction parameter to "adaptative" or "adaptativeLinear".
-
SpecFluxConversionTask no longer automatically removes non-seeing channels. One must now use FilterChannelsTask to remove these channels from SpectrometerDetectorSpectrum products.
| |
> > |
-
SpecFluxConversionTask now precedes SpecTelescopeCorrectionTask in the Standard pipelines.
-
SpecTelescopeCorrectionTask now, by default, subtracts only a model of the Herschel telescope and not the model multiplied by the RSRF for Telescope (Sky) port.
| |
Level 1 to Level 2
New Tasks |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Level 0.5 to Level 1
Changes to existing Tasks
-
WaveletDeglitcherTask now offers the option to make the number of corrected samples dependent on the glitch size by setting the optionReconstruction parameter to "adaptative" or "adaptativeLinear".
| |
< < |
-
SpecFluxConversionTask no longer automatically removes non-seeing channels. One must now use FilterChannelsTask to remove these channels from SpectrometerDetectorSpectrum products.
| > > |
-
SpecFluxConversionTask no longer automatically removes non-seeing channels. One must now use FilterChannelsTask to remove these channels from SpectrometerDetectorSpectrum products.
| |
Level 1 to Level 2
New Tasks | |
Changes to existing Tasks
-
NaiveProjectionTask now creates a spectral cube containing error instead of weight.
| |
< < |
-
AverageSpectraTask no longer provides functionality to remove out-of-band spectral samples. One must use RemoveOutOfBandTask instead.
-
AverageSpectraTask no longer provides functionality to reject outlier from the average computation.
| > > |
-
AverageSpectraTask no longer provides functionality to remove out-of-band spectral samples. One must use RemoveOutOfBandTask instead.
-
AverageSpectraTask no longer provides functionality to reject outlier from the average computation.
| |
Interactive Analysis and Tools
- New task
DestriperTask to iteratively remove the relative offsets between Level-1 detector timelines of the same detector array, and thus removing the stripes in the Level-2 map. Signal timelines are re-sampled from a preliminary naive map and subtracted from the original timelines. The resulting offset functions are modeled as polynomials with default degree (n=0) and subtracted. A new naive map is generated from the new difference of original signal and polynomial for the next iteration. The bright source threshold is used to suppress the influence of strong spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
- The mosaicing of maps from overlapping observations in a proposal is now fully functional (this is actually available from 6.1).
Spectrometer Pipeline | |
< < |
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
- New task
GriddingProjectionTask for spectral cube creation. Given SpirePreprocessedCube input, GriddingProjectionTask outputs a spectral cube. It uses HIFI's GriddingTask to perform the mapping.
-
NaiveProjectionTask now outputs a spectral cube containing error instead of weight.
-
WaveletDeglitcherTask offers the option to make the number of corrected samples dependent on the glitch size by setting the "optionReconstruction" parameter to 'adaptative' or 'adaptativeLinear'.
-
AverageSpectraTask no longer provides remove out of band data functionality. Use RemoveOutOfBandTask to remove out of band data from SpectrometerDetectorSpectrum products.
-
AverageSpectraTask no longer provides outlier rejection functionality.
-
SpecFluxConversionTask no longer filters channels. Use FilterChannelsTask to filter channels from SpectrometerDetectorSpectrum products.
| > > | Level 0 to Level 0.5
No changes.
Level 0.5 to Level 1
Changes to existing Tasks
-
WaveletDeglitcherTask now offers the option to make the number of corrected samples dependent on the glitch size by setting the optionReconstruction parameter to "adaptative" or "adaptativeLinear".
-
SpecFluxConversionTask no longer automatically removes non-seeing channels. One must now use FilterChannelsTask to remove these channels from SpectrometerDetectorSpectrum products.
Level 1 to Level 2
New Tasks
-
SpireProduct2SimpleSpectrumTask to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
-
GriddingProjectionTask for spectral cube creation. Given SpirePreprocessedCube input, GriddingProjectionTask produces a spectral cube output. This task uses HIFI's GriddingTask .
Changes to existing Tasks
-
NaiveProjectionTask now creates a spectral cube containing error instead of weight.
-
AverageSpectraTask no longer provides functionality to remove out-of-band spectral samples. One must use RemoveOutOfBandTask instead.
-
AverageSpectraTask no longer provides functionality to reject outlier from the average computation.
| |
Interactive Analysis and Tools
- New task
DestriperTask to iteratively remove the relative offsets between Level-1 detector timelines of the same detector array, and thus removing the stripes in the Level-2 map. Signal timelines are re-sampled from a preliminary naive map and subtracted from the original timelines. The resulting offset functions are modeled as polynomials with default degree (n=0) and subtracted. A new naive map is generated from the new difference of original signal and polynomial for the next iteration. The bright source threshold is used to suppress the influence of strong spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Other functions
Source extraction | |
> > |
- Various internal changes have been made to the Source Extractor tasks, but no changes to the functionality.
| |
Images
Display | |
Interactive Analysis and Tools
- New task
DestriperTask to iteratively remove the relative offsets between Level-1 detector timelines of the same detector array, and thus removing the stripes in the Level-2 map. Signal timelines are re-sampled from a preliminary naive map and subtracted from the original timelines. The resulting offset functions are modeled as polynomials with default degree (n=0) and subtracted. A new naive map is generated from the new difference of original signal and polynomial for the next iteration. The bright source threshold is used to suppress the influence of strong spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
| |
> > |
- New tasks
BaselineRemovalMedianTask and BaselineRemovalPolynomialTask operate on SPIRE Level-1 data to remove a baseline from the data. This is necessary due to the residual baseline that remains in the Level-1 data, which can produce stripes in the map if not removed. For each bolometer, the signal timeline is taken, either for each scan line separately, or for the whole observation as one long timeline. Then either the median value is subtracted (BaselineRemovalMedianTask), or a polynomial is fit to the data and subtracted. These tasks can be thought of as a "lite" version of the DestriperTask : they are simpler and faster, but for some observations containing a lot of structure (such as Galactic cirrus), there will be significant improvement if the DestriperTask is used.
| |
Documentation
- Pipeline Specification Manual: Entries on spectroscopy have been reviewed, examples have been validated.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
-
SpecFluxConversionTask no longer filters channels. Use FilterChannelsTask to filter channels from SpectrometerDetectorSpectrum products.
Interactive Analysis and Tools | |
< < |
- New task
DestriperTask to remove the offset from Level-1 data and thus remove the stripes in the Level-2 map. The offset is modeled as a polynomial with default degree (n=0). The bright source threshold is used to eliminate the spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
| > > |
- New task
DestriperTask to iteratively remove the relative offsets between Level-1 detector timelines of the same detector array, and thus removing the stripes in the Level-2 map. Signal timelines are re-sampled from a preliminary naive map and subtracted from the original timelines. The resulting offset functions are modeled as polynomials with default degree (n=0) and subtracted. A new naive map is generated from the new difference of original signal and polynomial for the next iteration. The bright source threshold is used to suppress the influence of strong spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
| |
Documentation
- Pipeline Specification Manual: Entries on spectroscopy have been reviewed, examples have been validated.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
-
SpecFluxConversionTask no longer filters channels. Use FilterChannelsTask to filter channels from SpectrometerDetectorSpectrum products.
Interactive Analysis and Tools | |
> > |
- New task
DestriperTask to remove the offset from Level-1 data and thus remove the stripes in the Level-2 map. The offset is modeled as a polynomial with default degree (n=0). The bright source threshold is used to eliminate the spikes in the data. The primary output is a SpireListContext containing updated PointedPhotTimelines. The additional outputs are a SimpleImage map, the convergence ratio, Tod etc.
| |
Documentation
- Pipeline Specification Manual: Entries on spectroscopy have been reviewed, examples have been validated.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Product Access Layer | |
> > |
- The HTTP pool now supports digest as well as basic authentication.
| | Tasks
The default Task GUI has been improved with the following upgrades: | |
Calibration Products
- Spectrometer calibration products for nominal detector settings have been updated to make use of in-flight bolometer model parameters.
| |
> > |
- An updated TempDriftCorr product allows a new algorithm in the Signal Jump Detector module to be used (nominal mode only).
| |
Calibration Framework | |
< < | The spireCal task has new features and modified behaviour: | > > |
- The
spireCal task has new features and modified behaviour:
| |
- It will look for a calibration tree in a local pool by default. The default is the one that was last saved if applicable; otherwise the default for the HIPE version.
- It will only download from the HSA if explicitly requested via the
calTree parameter.
- Optionally the tree can be saved to a local pool. In this case that one will become the default.
| |
> > |
-
- The trees available in the archive can be listed.
- The API has new methods for showing differences between two calibration trees and for verifying that expected metadata is present and correct.
| |
Preprocessing | |
Photometer Pipeline
- The
LpfResponseCorrectionTask now accepts a new optional, boolean input parameter "doMirrorSignal". Setting this parameter to true, the task will perform the correction, by mirroring the signal time-lines in the y-axis. The effect of this is to avoid any edge-ringing, resulting from the default correction method when applied to timelines with a large slope. The draw-back of the new method is that it can double the processing time of the Task, however, not to a detrimental effect to single observation processing (It will definitely be noticeable when processing a large number of observations).
| |
> > |
- The mosaicing of maps from overlapping observations in a proposal is now fully functional (this is actually available from 6.1).
| |
Spectrometer Pipeline
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Dataset viewer
Astronomical utilities | |
< < | | > > | RadialVelocity task and util class renamed to RadialV and now use the proper Doppler sign convention. | | Numeric routines
Data fitting
Data interpolation | |
Tasks | |
> > | The default Task GUI has been improved with the following upgrades:
- Parameter error detection (red X) also checks the
validator of the parameter
- A new
Help button gives easy direct access to the URM description of the task
- White space in layout moved to the lower part of the panel
- Editors based on text fields now require half the width
- Labels of parameters have now a maximum size to reserve space for the editors.
- Support for grouping inputs in multiple Tabs. For tasks that have inputs related to different aspects or simply a lot of them, they can be presented in several tabs.
There is now a detailed outline shown in the Outline View when a task is selected in the Task View. This allows inspection of the structure of a task without the need to either use the Console or open its GUI in the Editor . Also, the system is undergoing a review of task compliancy (naming, documentation, tooltips ...) that will make all tasks self-explanatory (ongoing for HIPE 8).
| | Quality control
Systematic product generation
Data input-output | |
> > |
-
simpleFitsReader and simpleFitsWriter now also support reading/writting Datasets (not just Products ).
- The
Export View now shows the tags associated with each Observation version.
- The
localStoreWriter task now allows to add a tag to the saved product.
- Now, when you use the contextual menu to save a product variable you will use the
Save to Pool tool instead of the localStoreWriter task.
-
localStoreWriter and localStoreCopier now use a better integrated GUI to select-create a pool.
- File filters for file dialogs are now self-explanatory (accepted extensions ...).
- The
clear task now has a simplified syntax to delete all variables (clear() without any parameter, will delete all).
| |
Virtual Observatory |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | SPIRE
Calibration Products | |
> > |
- Spectrometer calibration products for nominal detector settings have been updated to make use of in-flight bolometer model parameters.
| |
Calibration Framework | |
-
- scanVelocityLimits: Double1d([lowerVelocityLimit, upperVelocityLimit]), in arcsec/sec, defining a range of scan Velocities. Signal samples with angular velocity outside this range will have their NON_NOMINAL_VELOCITY mask set. Setting this parameter, parameter "scanVelocityTolerance" will be ignored. Setting any velocity limit to a negative value, the task will ignore the scanVelocityLimits parameter and revert to using "scanVelocityTolerance".
Photometer Pipeline | |
< < |
- The
LpfResponseCorrectionTask now accepts a new optional, boolean input parameter "doMirrorSignal". Setting this parameter to true, the task will berform the correction, by mirroring the signal time-lines in the y-axis. The effect of this is to avoid any edge-ringing, resulting from the default correction method when applied to timelines with a large slope. The draw-back of the new method is that it can double the processing time of the Task, however, not to a detrimental effect to single observation processing (It will definately be noticeable when processing a large number of observations).
| > > |
- The
LpfResponseCorrectionTask now accepts a new optional, boolean input parameter "doMirrorSignal". Setting this parameter to true, the task will perform the correction, by mirroring the signal time-lines in the y-axis. The effect of this is to avoid any edge-ringing, resulting from the default correction method when applied to timelines with a large slope. The draw-back of the new method is that it can double the processing time of the Task, however, not to a detrimental effect to single observation processing (It will definitely be noticeable when processing a large number of observations).
| |
Spectrometer Pipeline
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
- New task
GriddingProjectionTask for spectral cube creation. Given SpirePreprocessedCube input, GriddingProjectionTask outputs a spectral cube. It uses HIFI's GriddingTask to perform the mapping.
-
NaiveProjectionTask now outputs a spectral cube containing error instead of weight.
| |
> > |
-
WaveletDeglitcherTask offers the option to make the number of corrected samples dependent on the glitch size by setting the "optionReconstruction" parameter to 'adaptative' or 'adaptativeLinear'.
| |
-
AverageSpectraTask no longer provides remove out of band data functionality. Use RemoveOutOfBandTask to remove out of band data from SpectrometerDetectorSpectrum products.
-
AverageSpectraTask no longer provides outlier rejection functionality.
-
SpecFluxConversionTask no longer filters channels. Use FilterChannelsTask to filter channels from SpectrometerDetectorSpectrum products.
| | Interactive Analysis and Tools
Documentation | |
< < | Change. | > > |
- Pipeline Specification Manual: Entries on spectroscopy have been reviewed, examples have been validated.
| |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
- New task
GriddingProjectionTask for spectral cube creation. Given SpirePreprocessedCube input, GriddingProjectionTask outputs a spectral cube. It uses HIFI's GriddingTask to perform the mapping.
-
NaiveProjectionTask now outputs a spectral cube containing error instead of weight.
| |
> > |
-
AverageSpectraTask no longer provides remove out of band data functionality. Use RemoveOutOfBandTask to remove out of band data from SpectrometerDetectorSpectrum products.
-
AverageSpectraTask no longer provides outlier rejection functionality.
-
SpecFluxConversionTask no longer filters channels. Use FilterChannelsTask to filter channels from SpectrometerDetectorSpectrum products.
| |
Interactive Analysis and Tools |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Calibration sources | |
> > | We have integrated the Calibration Source Database into HIPE. There is a Calibrators View on the Workbench (you may have to reset the perspective for it to appear).
The Calibrators View allows access to the database with calibration sources at ESAC, that is used by HSC calibration scientists. It contains spectra of planets, asteroids, and fixed targets. The data can be viewed in the usual HIPE viewers for spectra and images, and manipulated using Jython commands. | | Products and datasets
Observation context |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
-
- scanVelocityLimits: Double1d([lowerVelocityLimit, upperVelocityLimit]), in arcsec/sec, defining a range of scan Velocities. Signal samples with angular velocity outside this range will have their NON_NOMINAL_VELOCITY mask set. Setting this parameter, parameter "scanVelocityTolerance" will be ignored. Setting any velocity limit to a negative value, the task will ignore the scanVelocityLimits parameter and revert to using "scanVelocityTolerance".
Photometer Pipeline | |
> > |
- The
LpfResponseCorrectionTask now accepts a new optional, boolean input parameter "doMirrorSignal". Setting this parameter to true, the task will berform the correction, by mirroring the signal time-lines in the y-axis. The effect of this is to avoid any edge-ringing, resulting from the default correction method when applied to timelines with a large slope. The draw-back of the new method is that it can double the processing time of the Task, however, not to a detrimental effect to single observation processing (It will definately be noticeable when processing a large number of observations).
| |
Spectrometer Pipeline
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Spectrometer Pipeline
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
| |
> > |
- New task
GriddingProjectionTask for spectral cube creation. Given SpirePreprocessedCube input, GriddingProjectionTask outputs a spectral cube. It uses HIFI's GriddingTask to perform the mapping.
-
NaiveProjectionTask now outputs a spectral cube containing error instead of weight.
| |
Interactive Analysis and Tools |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Calibration Framework | |
> > | The spireCal task has new features and modified behaviour:
- It will look for a calibration tree in a local pool by default. The default is the one that was last saved if applicable; otherwise the default for the HIPE version.
- It will only download from the HSA if explicitly requested via the
calTree parameter.
- Optionally the tree can be saved to a local pool. In this case that one will become the default.
| | Preprocessing
Engineering Conversion |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Spectra
Display
Analysis | |
< < |
- Addition to SpectrumFitter: create ASCII file with fit parameters (not yet in SpectrumFitterGUI). Use:
| > > |
- Addition to SpectrumFitter: create ASCII file with fit parameters. Use in the command line:
| |
-
- sf = SpectrumFitter(...)
- ...
- m = sf.addModel(...)
| |
-
- sf.doFit( ) or sf.doGlobalFit( )
- sf.saveFitParametersAsASCII(fileName) # writes parameters of all models to fileName
- m.toASCII(dirName) # writes parameters to dirName/[modelname].txt
| |
< < |
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, a poly and gauss will be fitted, if switched off, nothing.
| > > |
- The SpectrumFitterGUI has, in the export TAB, also the possibility to export fit parameters to file.
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, the user can select from:
- Instrument specific initial model.
- User specific initial models - the user can specify the models.
- Addition to SpectrumFitterGUI, MultiTAB:
- Some information on what will happen.
- Fit parameters are written to file.
- A count-down progress bar.
| |
Data cubes
Display |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Engineering Conversion
Common Pipeline | |
> > |
- The
AssociateSkyPositionTask now creates a new table "avgVelocity" in photometer level1 scanmap products. The table contains two columns: "sampleTime" (TAI) and "avgVelocity" (deg/sec)
- The
AssociateSkyPositionTask now now accepts two new optional parameters:
- scanVelocityTolerance: double value, in arcsec/sec, defining the scan velocity tolerance relative the the mode's expected scan velocity. Signal samples outside this range will have their NON_NOMINAL_VELOCITY mask set. (default: 1.0"/sec)
- scanVelocityLimits: Double1d([lowerVelocityLimit, upperVelocityLimit]), in arcsec/sec, defining a range of scan Velocities. Signal samples with angular velocity outside this range will have their NON_NOMINAL_VELOCITY mask set. Setting this parameter, parameter "scanVelocityTolerance" will be ignored. Setting any velocity limit to a negative value, the task will ignore the scanVelocityLimits parameter and revert to using "scanVelocityTolerance".
| |
Photometer Pipeline
Spectrometer Pipeline | |
> > |
- New task
SpireProduct2SimpleSpectrumTask , to convert SPIRE Level-1 and Level-2 data to SimpleSpectrum products
| |
Interactive Analysis and Tools |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Spectra
Display
Analysis | |
< < |
- Addition to SpectrumFitter: create ASCII file with fit parameters (not yet in SFGUI). Use:
| > > |
- Addition to SpectrumFitter: create ASCII file with fit parameters (not yet in SpectrumFitterGUI). Use:
| |
-
- ...
- m = sf.addModel(...)
- ...
- sf.doFit( ) or sf.doGlobalFit( )
- sf.saveFitParametersAsASCII(fileName) # writes parameters of all models to fileName
- m.toASCII(dirName) # writes parameters to dirName/[modelname].txt
| |
< < |
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, a poly and gauss will be fitted, if switched off, nothing.
| > > |
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, a poly and gauss will be fitted, if switched off, nothing.
| |
Data cubes
Display | | HIFI Calibration
HIFI Pipeline | |
> > |
- doPipelineConfiguration now passes changes to the level 2 pipeline. To use this task, pass an HTP to the GUI (doPipelineConfiguration), modify the pipeline steps as required. Press accept (default name of output is out) then pass this new configuration to the pipeline task:
obs_new = hifiPipeline(obs=obs, params=out, save=False) | | hifiPipeline task
Level 0 Pipeline
WBS Pipeline | |
HIFI Data Processing Tools
Standing Wave Removal | |
> > |
- averscan option has been removed as it was found not to work well
| | Baseline Removal | |
> > |
- The htpcopy option has been removed
| | Deconvolution | |
> > |
- doDeconvolution now produces a result even if deconvolution fails. In this case an error message is given
- doDeconvolution now read flags from USB, rather than LSB. Channel flags have always been read from the USB so this change makes it easier for you to pass flagged data to the task
| | Spectral Cube creation
HiClass export tool | |
> > |
- Obsid now exported again to CLASS header
| |
Documentation |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Spectra
Display
Analysis | |
> > |
- Addition to SpectrumFitter: create ASCII file with fit parameters (not yet in SFGUI). Use:
- sf = SpectrumFitter(...)
- ...
- m = sf.addModel(...)
- ...
- sf.doFit( ) or sf.doGlobalFit( )
- sf.saveFitParametersAsASCII(fileName) # writes parameters of all models to fileName
- m.toASCII(dirName) # writes parameters to dirName/[modelname].txt
- Addition to SpectrumFitterGUI: user preference for initial models. If switched on, a poly and gauss will be fitted, if switched off, nothing.
| |
Data cubes
Display |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Interactive Analysis and Tools
Documentation | |
> > | Change. | |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Interactive Analysis and Tools
Documentation
\ No newline at end of file | |
> > |
<--
--> | | \ No newline at end of file |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Images
Display
- Adapted the popup menu to make it possible to work with axes, add a compass and add a scale.
| |
> > |
- Display now returns the commands done using the popup menu to the HIPE console. This makes it very easy to reconstruct an image plot from within a script.
| |
- When dragging source positions to an image, the circles are locked. When dragging contours to an image, the contours are also locked.
- Added method addArcSecs to add a line of a number of arcseconds to the image.
- When using the opacity slider with a cube, the next image is used as the underlying image, not the next layer of the cube anymore.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Images
Display | |
> > |
- Adapted the popup menu to make it possible to work with axes, add a compass and add a scale.
| |
- When dragging source positions to an image, the circles are locked. When dragging contours to an image, the contours are also locked.
- Added method addArcSecs to add a line of a number of arcseconds to the image.
- When using the opacity slider with a cube, the next image is used as the underlying image, not the next layer of the cube anymore.
|
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | | Display
- When dragging source positions to an image, the circles are locked. When dragging contours to an image, the contours are also locked.
- Added method addArcSecs to add a line of a number of arcseconds to the image.
| |
> > |
- When using the opacity slider with a cube, the next image is used as the underlying image, not the next layer of the cube anymore.
| | Analysis | |
> > |
- You can now load all monochrome or indexed gif files using importRgbImageTask
| |
Spectra
Display |
|
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7 | |
Images
Display | |
> > |
- When dragging source positions to an image, the circles are locked. When dragging contours to an image, the contours are also locked.
- Added method addArcSecs to add a line of a number of arcseconds to the image.
| | Analysis
Spectra |
|
> > |
META TOPICPARENT |
name="HipeWhatsNew" |
What's New in HIPE 7
Core system
HIPE
Plotting
TablePlotter
OverPlotter
Dataset viewer
Astronomical utilities
Numeric routines
Data fitting
Data interpolation
Random numbers
Statistics
Trend analysis
Mapping
Other functions
Source extraction
Images
Display
Analysis
Spectra
Display
Analysis
Data cubes
Display
Analysis
Herschel Science Archive
Calibration sources
Products and datasets
Observation context
Product Access Layer
Tasks
Quality control
Systematic product generation
Data input-output
Virtual Observatory
Installer
Documentation
HIFI
HIFI Software Configuration and Properties
HIFI Calibration
HIFI Pipeline
hifiPipeline task
Level 0 Pipeline
WBS Pipeline
HRS Pipeline
Level 1 Pipeline
Level 2 Pipeline
HIFI Products
HIFI Spectrum Toolbox
Spectrum Explorer (HIFI specifics)
Spectrum tasks (HIFI specifics)
HIFI Data Processing Tools
Standing Wave Removal
Baseline Removal
Deconvolution
Spectral Cube creation
HiClass export tool
Documentation
PACS
Pipeline
Photometry
Spectroscopy
Calibration
Photometry
Spectroscopy
Analysis tools
Photometry
Spectroscopy
Product changes
Photometry
Spectroscopy
Documentation
SPIRE
Calibration Products
Calibration Framework
Preprocessing
Engineering Conversion
Common Pipeline
Photometer Pipeline
Spectrometer Pipeline
Interactive Analysis and Tools
Documentation |
|
|
|