Knowledgebase
- What is the tested capability of ALMA for bandpass calibration precision?
- How will high time resolution observations be handled with ALMA?
- What bands, frequencies, or wavelength ranges are available?
- Do I still need a statement on the potential for publicity for my ALMA Proposal?
- May I request an extension to my observing program's proprietary period?
- What are the restrictions on multiple spectral setups within a single science goal?
- Can I set up monitoring observations with the OT?
- How do I change which sideband my spectral windows are placed in?
- How do I set up a mosaic in the OT?
- Can I load a proposal from a previous cycle into the OT and submit it as a new proposal?
- May I make changes to my project after the proposal review process?
- What is the meaning of the code of an ALMA proposal?
- Why have I not received email notification for some or all of my Proposals?
- What is dual-anonymous peer review and how do I adhere to it?
- What is distributed peer review process and how does it work?
- How can I update Cycle 0 absolute fluxes to the Butler-JPL-Horizons 2012 model standards?
- Will re-reduction improve the Cycle 0 data products provided by the archive?
- Why are data binned (averaged) by task cvel so noisy?
- Why are flux scaling and restoring beam calculations in the task clean incorrect?
- The OT instantly fails to startup (commonly EA-ARC issue, with 32-bit JAVA)
- How can I query the calibrator database that ALMA uses?
- As PI of an ALMA proposal, how can I give others access to the data during the proprietary period?
- Why can't I download my data?
- What Calibration and Imaging products will be delivered to me?
- Under what conditions can I request the raw data of my observing program be delivered before quality assurance is completed?
- Where can I find data reduction tutorials and recipes using CASA?
- Can I reduce ALMA data in software packages other than CASA, and is there support for that?
- Does the feathering process for Solar observations differ from that for other observations?
- What Calibration and Imaging products will be delivered to me?
- What changes were made to the PSF beam fitting algorithm in CASA 6?
- To which category should I submit a proposal on distant galaxies: "cosmology/high-z" or "Galaxies/Nuclei"?
- What pwv should I use in my CASA simulations to prepare an ALMA proposal?
- Does the sensitivity calculator account for shadowing?
- Where can I find the configuration files for CASA simulation?
- What is meant by imaging dynamic range?