TWiki
>
Public Web
>
HipeWhatsNew
>
HipeWhatsNew6x
(revision 13) (raw view)
Edit
Attach
Tags:
view all tags
---+ What's New in HIPE 6 | *PDF Version* | [[%SCRIPTURLPATH%/genpdf%SCRIPTSUFFIX%/%WEB%/%TOPIC%?pdforientation=portrait&pdftoclevels=2][Click here]] | %TOC% ---++ Core system The Java Virtual Machine included in Windows and Linux downloads has been updated to version 1.6.0_22. ---+++ HIPE ---+++ Plotting * A small subplot can be put inside a bigger plot. ---++++ !TablePlotter ---++++ !OverPlotter ---++++ Dataset viewer ---+++ Astronomical utilities ---+++ Numeric routines ---++++ Data fitting ---++++ Data interpolation ---++++ Random numbers ---++++ Statistics ---++++ Trend analysis ---++++ Mapping ---++++ Other functions ---+++ Source extraction ---+++ Images ---++++ Display * Major speedup when zooming in on images. Less memory is used when zooming in. * Fixed some memory issues. The display does not longer keep a lot of memory in use. * It is possible to hide or show the panel with the panner and the zoom ---++++ Analysis ---+++ Spectra ---++++ Display ---++++ Analysis ---+++ Data cubes ---++++ Display ---++++ Analysis ---+++ Herschel Science Archive ---+++ Calibration sources ---+++ Products and datasets ---++++ Observation context ---+++ Product Access Layer ---+++ Tasks * Improved documentation * Added descriptions to tasks. All tasks can provide a high level description (shown in tooltips in Task View). * Simplified localStoreWriter task ---+++ 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 ---++++ !NaiveProjectionTask replaces !NearestNeighbourProjectionTask for spectral cube creation Level2 spectral cubes are now generated by !NaiveProjectionTask. !NaiveProjectionTask creates spectral cubes by averaging flux values within each pixel. The execution speed of !NaiveProjectionTask has been greatly improved - a set of high resolution spectra is now processed in approximately 10 seconds. ---++++ !Browse product image for observations Within Hipe, observations with spectral cubes (observations with multiple raster positions or jiggle positions) now display an image summarizing the cubes. The image consists of the median flux values for each pixel of the SLW and SSW unapodized cubes. For observations without spectral cubes (sparse observations, no jiggle), an image showing a plot spectra of the central detectors is displayed. ---++++ New Module: spire_ia_pipeline_spec_util This module contains helper classes used in the SPIRE spectrometer pipelines. ---+++++ !FilterChannelsTask This task removes or retains a list of channels from an SDT, SDI, or SDS. ---+++++ !RemoveOutOfBandTask This task removes out-of-band spectral components from an input SDS. ---+++++ !ObservationLayoutTask This task determines the characteristics of an observation, namely point numbers, jiggle numbers, resolution, and building blocks IDs, and places them into a =SpecObsContents= dataset. ---+++++ !MakeSameOpdsTask This task makes all interferograms in an SDI have an OPD range consistent with the commanded resolution, truncating the data if necessary. ---+++++ !MergeFtsBuildingBlocksTask This task merges multiple SDIs and NHKTs into a single SDI and NHKT. ---+++ Interactive Analysis and Tools ---+++ Documentation <!-- * Set ALLOWTOPICCHANGE = Main.RegisteredUsersGroup, Main.TWikiAdminGroup -->
Edit
|
Attach
|
Watch
|
P
rint version
|
H
istory
:
r49
|
r15
<
r14
<
r13
<
r12
|
B
acklinks
|
V
iew topic
|
Raw edit
|
More topic actions...
Topic revision: r13 - 2011-01-13
-
JavierDiaz
Public
Log In
Public Web
Create New Topic
Index
Search
Changes
Notifications
Statistics
Preferences
Webs
Public
TWiki