ALMA OT Release Notes for Cycle-6 Phase-2 release
The most important changes to the OT since the last release are:
- TP SBs that require multiple sources should now be dealt with properly. The observation time per SB should never exceed ~40 mins and sources will be split into multiple TP SBs if necessary to respect the 40-min limit.
- The calculation of the TP sensitivity goal now includes a factor due to observing the OFF position. Various bugs in the calculation of the SB sensitivity goal have also been fixed.
- Amplitude-calibration SBs are no longer generated except for Bands 5 and 8.
- The decision on whether to schedule a Check Source has been changed such that this is done if either of the min or max angular resolution values in the SB are less than 0.25". This was principally done to ensure that projects that ask for a range of angular resolution will get a Check Source if one might be needed.
- Only the PWV-uncorrected data are written out from the correlator. This halves the data rates compared to previous cycles.
- The check to see if a setup might fail due to being near a band edge is now based on the baseband positions. This is more reliable than the previous spw-based criteria.
- Both the names of SBs and the sources within an SB are now checked to see if illegal characters are present ("sanitisation") which are then either removed or replaced.
- It is no longer possible to place more than one SB in a MOUS, except for CSV projects.
- Bug fix: Long-baseline projects should now have the P2G flag correctly set.
- Bug fix: At Phase 1, Galactic coordinates were not being converted to equatorial for the purposes of calculating the source elevation at transit. This might cause some properties of Galactic projects to change e.g. which configurations and/or arrays are required, sensitivity, etc.
- Bug fix: It was not possible to create a Band-9 mosaic with >100 pointings at Phase 1. This has now been fixed.
ALMA OT Release Notes for Cycle-6 Phase-1 release
Summary list of the key new capabilities, features and improvements.
- As circular polarization will be officially supported for Cycle 6, the user is requested to enter the expected level of circular polarization, for continuum and/or spectral line. As with linear polarization, a limit is enforced below which a validation error will be triggered. New circular-polarization fields have been added to the ASCII input format.
- Band 8 is now a standard mode. This means that it can now be requested for the Stand-alone ACA.
- The IF bandwidth of Band 6 has been increased by 0.5 GHz. This will make it easier to observe CO and 13CO simultaneously.
- Data rates are now calculated for 50 antennas. This is to ensure that the SB will not fail at execution time.
- Projects that require long baselines will use a smaller clustering length (1 degree) as the phase calibrator must be quite close to the science targets.
- There is no longer a separate coordinate system associated with rectangular-field definitions. The source coordinate system will be assumed.
- FITS files in Galactic coordinates are now handled correctly.
- ASCII input format: Source coordinates in decimal degrees will now be recognised as Galactic.
- Investigator details (affiliation, email, etc.) will be updated at submission time (Phase 1 only).
- It is no longer possible to enter a user-defined bandwith that exceeds the bandwidth of the spectral setup.
- There is no longer a text box associated with the time-constraint interface. The box on the TJ node should be used.
- The PI institution and email is no longer shown on the proposal Cover Sheet.
- Bug fix: the lsrk to barycentric correction now works correctly for all velocity definitions. This may mean that existing projects will not validate. If so, the spectral setup should be (slightly) edited.
- Java fix: Mac users may have experienced pop-up windows being hidden - this should now be fixed.
ALMA OT Release Notes for Cycle 5 Phase 2 release
Summary list of the key new capabilities, features and improvements since Cycle 5 Phase I. For the major changes please consult the Proposer's Guide for more details.
- There is no longer a requirement for PIs to generate SBs for their projects when updating/checking them for Phase II. All that is required is any minor changes to Science Goal setups.
- It is now possible to delegate submission of Phase II projects to one of the CoIs
- Some features previously disabled in Phase II, such as use of the visual editors, are now enabled.
- The OT now correctly rotates maps when the source coordinates are in galactic
- Contact scientists can now only open projects assigned to them in a read-only mode
- A number of detailed updates have been made to SB generation for Solar projects.
- There have been several minor updates to general SB generation, in line with current observing practice
ALMA OT Release Notes for Cycle 5
Summary list of the key new capabilities, features and improvements since Cycle 4. For the major changes please consult the Proposer's Guide for more details.
- Major change to the presentation and use of the angular resolution parameters for a Science Goal.
- Band 5 is now available for use.
- Setting up a Science Goal to use 90 degree walsh switching in its spectral setup (for Bands 9 and 10) is now allowed. The User and Proposer's Guide should be consulted for more information about this feature.
- Users are now asked to justify observations knowingly duplicated observations.
- It is now possible to capture information about spectral lines that are expected to be found within the bandwidth of the spectral windows that are setup. This information is made available to the processing pipeline and latere analysis tools
- Overlays of spectral lines are now saved
- Full polarisation is nw supported for Band 4.
- The limit at which a Stand-Alone ACA project is considered a Large Program has been raised to 150 hours.
- A number of small changes that affect time estimates were made: number of/time spent on calibrations, minimum on-source time increased to 5 minutes.
- The "system" option for calibration has been split into two, one allowing for a forced solar-system amplitude calibration.
- It is now possible to select simultaneous observations for a single 12M configuration and the 7M array.
- Small improvements to the Ephemeris loading/viewing
- Sources may now be cloned.
- The speed of Validation (which is part of the submission process) has been improved, especially for Large projects. (Only for multi-core processors.)
- Spectral Averaging default set to 2 for spectral line observations.
- Co-PIs are allowed for VLBI proposals.
- Time constrained observing is now allowed for Stand-Alone ACA.
- Now only the "visual" editors for the spatial and spectral setups are shown.
- Usability improvements to the spectral line picker.
- More spectral lines for new receiver bands.
- C4_013: Bug - Co-PIs are not receiving email confirmations after proposal submission (or resubmission). Fixed.
- C4_009: Bug - A value entered into the minutes field of the 'single visit' time-constrained interface will automatically reset to zero. Time constraints read in via an ASCII file are not affected. Fixed.
- C4_007: Bug - Under certain circumstances, an ATM calibration is being scheduled with every phase-calibrator scan. This will lead to an over-estimate of the time required. Fixed.
- C4_003: Bug - Immediately after starting, the OT GUI can minimize itself such that only the title bar buttons (close, maximize, minimize) are visible. This has been reported on Macs and Ubuntu. The workaround is to just maximize the GUI with the appropriate button. Believe fixed.
- C4_014: Bug - The spectral setup can report the following error: "The spectral window range exceeds the baseband width". Fixed.
- C4_015: Proposal submission may hang for proposals that request many hundreds of sources or pointings. The default maximum allowed memory for the OT has been increased.
ALMA OT Release Notes for Cycle 4 Phase II (Update 2)
Update 2 addresses the following known issues for Cycle 4 Phase II:
- C4_012: OT is ignoring user-specified sensitivity unit when reading project
- Centre frequency in process of being edited is copied across spectral setups
- Frequencies are copied from one spectral spec to another when a frequency edit is not confirmed
- OT not always showing band-edge error
ALMA OT Release Notes for Cycle 4 Phase II (Update 1)
Update 1 addresses the following known issues for Cycle 4 Phase II:
- This update fixes a bug that made it impossible to generate SBs for Solar proposals using mosaics.
ALMA OT Release Notes for Cycle 4 Phase II release
Summary list of the key new capabilities, features and improvements since Cycle 4 Phase I. For the major changes please consult the Proposer's Guide for more details.
- The primary change in this release is to allow Principal Investigators the ability to generate their own Scheduling Blocks from their approved Science Goals.
- It is not possible to generate Scheduling Blocks from descoped Science Goals.
- Principal Investigators may only edit certain fields in a Science Goal, and only within pre-defined margins. PIs are not allowed to edit Scheduling Blocks directly.
- The project file chooser has been enhanced with a history feature to file chooser.
ALMA OT Release Notes for Cycle 4 (Update 2)
Update 2 addresses the following known issues for Cycle 4:
- C4_010: Executive share and validation does not work correctly for SACA Large Programs
- C4_011: Some EA PIs are getting Chilean executive shares
ALMA OT Release Notes for Cycle 4 (Update 1)
Update 1 addresses the following known issues for Cycle 4:
- C4_006: High redshifts can lead to the OT refusing to display the time-estimate dialogue.
- C4_005: In the Technical Justification editor, the achieved RMS over the total bandwidth and over 1/3 of the line width are reported as 0.00
- C4_008: Sources read in from a source list will have their coordinate system set to FK5. This should be ICRS.
ALMA OT Release Notes for Cycle 4
Summary list of the key new capabilities, features and improvements since Cycle 3. For the major changes please consult the Proposer's Guide for more details.
- It is now possible to create a Science Goal that will make use of the ACA only (7m and TP)
- Large programs are now supported.
- It is now possible to create Science Goals to observe Solar phenomena. Choose "Sun" as your Solar System target.
- The creation of VLBI proposals is now supported, in conjunction with the global VLBI mm network.
- Full polarization with spectral line setups is now allowed.
- It is now possible to select a number of sources across the visible sky in one Science Goal, with the same spectral spectral setup and performance parameters.
There is no longer a restriction on the closeness. During Phase II these sources will be separated into clusters for separate Scheduling Block execution.
- "Shadowing" is accounted for in 7m array and compact array sensitivity calculations.
- All ALMA Observations are taken using the ICRS coordindate system, accordingly ICRS is the default for coordinate specification and is recommended. All FK5 (J2000) cooordinates will be treated as if they were ICRS. Galactic is still
supported.
- Previously submitted proposals from the Archive may now be used as the basis for new proposals, even if they have been moved to "Phase II".
- It is no longer possible to override the choice of using or not using the ACA.
- "Standard" proposals are now called "Regular" (to avoid confusion with Standard/non-Standard observing setups) although the ".S" suffix is retained.
- It is now possible to use projects from the Archive as "templates".
- A number of user interface enhancements have been made.
- C1_001: On MacOS cmd-X, cmd-C and cmd-V should now be used for cutting, copying, pasting in text field and text areas within the OT.
- C3_012: It should no longer be the case that the proposal title on proposal node can become that of an open template.
ALMA OT Release Notes for Cycle 3 (Update 1)
Update 1 addresses the following known issues for Cycle 3:
- C3_001: The time shown on the Cover Sheet for "Multiple visit" Science Goals is too high
- C3_002: Copy and paste of a Science Goal followed by an edit of the spectral setup can cause the source line width to change.
- C3_003: The time estimate in brackets is not always that due to the sensitivity, but also includes certain minima.
- C3_004: Time overrides when two 12-m configurations are required cannot be requested.
- C3_005: It is possible to define multiple clusters of pointings using the custom mosaic option.
- C3_006: The polarization non-standard time on the cover sheet is too long.
- C3_007: Changing between Doppler types doesn't always work properly.
- C3_010: Moving to a new Science Goal deselects ACA in the original Science Goal
ALMA OT Release Notes for Cycle 3
Summary list of the key new capabilities, features and improvements since Cycle 2.
- Band 10 is now available for limited use.
- Free choice of TDM frequency for full polarization observations, in Bands 3, 6 and 7.
- Increase in number of antennas: 36 12-m array, 10 7-m array, 2 Total Power array.
- Introduction of non-standard modes.
- New antenna beamsize definition in use.
- Sesame is now used to query source information.
- A Science Goal may now contain multiple sources with rectangular field definitions.
- The Total Power mapping area is automatically calculated for custom mosaics or single pointings.
- Fuller Import/export of pointing positions.
- Absolute positions are now supported for pointing centres.
- The “Point source” button has been removed.
- Source declination is taken into account when determining which array configurations are required.
- Total Power will not be scheduled if the 7-m array can achieve the requested Largest Angular Scale.
- Noise contribution from the image sideband is now explicitly calculated for DSB receivers (Bands 9 and 10).
- Improvements to the time-constrained interface.
- Overhaul of Technical Justification node:
- Better organised
- More information for the user
- Copy and Paste between SGs improved
- The total time for a proposal can be displayed in the main OT GUI - see under "Tool" on the top-level menu bar.
- J2000 coordinate system name changed to "FK5 J2000".
- The target linewidth may only be specified in velocity units, km/s or m/s.
More detailed information on the above can be found in the Science Portal under Documents and Tools.