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Project Charter

Long Description

This project deals with the ingest of FITS data cubes, catalogs, and spectra, and providing access to the products from the archive.  For details of the ALFALFA project see the project web page.

The Arecibo Legacy Fast ALFA (ALFALFA) survey is a completed, blind extragalactic HI survey exploiting Arecibo's superior sensitivity, angular resolution and digital technology to conduct a census of the local HI universe over a cosmologically significant volume. ALFALFA has detected more than 30,000 extragalactic HI line sources out to z~0.06, and its catalog will be especially useful in synergy with wide area surveys conducted at other wavelengths.  The data collection is of great interest to the radio community and NRAO users.  NRAO will partner with the ALFALFA team to ingest and serve their valuable products to the community.

ALFALFA has produced over 7400 dual polarization data cubes, an ASCII catalog of over 30,000 extragalactic detections, and HI line spectra.

ALFALFA is a completed program.  All data products were processed through IDL.   The ALFALFA project will provide the data cubes in FITS format.

From the SRDP perspective, the set of all ALFALFA data products is a collection.

Publications

The main catalog paper by Haynes et al. (2018).

The long and continually growing list of ALFALFA publications.

ALFALFA Data Products

1. Spectral Data Cubes, Spectral Weights, Continuum Maps, Continuum Weights

Data cube option 1 (Everything in one file - a primary header and three image headers)

    Number of files:  ~7500 data cubes

Data cube option 2 (Spectral cube and three ancillary products - spectral weights, continuum maps, and continuum weights)

    Number of files:  ~7500 x 4 (spectral cubes, spectral weights, continuum maps. continuum weights) = ~30,000 FITS files

Dimensions of the data

    Spectral data cubes and weights:   2 polarizations  x  1024 frequency channels   x 144 RA pixels   x 144 Decl. pixels

    Continuum maps and weights:   2 polarizations x 144 RA pixels   x 144 Decl. pixels

Volume of data (< 10 TB)


2. Extragalactic Catalog

The catalog description, an ASCII text file, or a CSV text file.   Data volume ~ 5 Megabytes.


3. HI Spectra

Each detection has a single FITS file with a binary table extension, containing the X-Y points of the spectrum and associated metadata.  Number: ~30,000 FITS files.  Total volume: ~ 1 Gigabyte.

Archive Access to ALFALFA Data Products

The modalities for discovery and filtering of ALFALFA data sets in the Archive

End user manipulation

Th expectation is that a user would search for a position on the sky, or via a galaxy name (NED resolver, etc.).     For instance, if one searches on the position 12h20m00s, +09d00m00s, four data cubes, each with three additional ancillary products, would be returned (16 totals hits, total volume would be ~ 1.6 GB). 

Put readthedocs here...

Stakeholders

Brian Kent, NRAO, Project Sponsor and Technical Expert

Jeff Kern, NRAO, Project Sponsor

Martha Haynes, Cornell, ALFALFA PI and Technical Expert

Others?

Prerequisites

The ALFALFA project will provide to NRAO the FITS spectral data cubes and ancillary products, data cube index,  extragalactic catalog, and HI spectra FITS files.

Examples will be provided to the SSA team for comments on header metadata keywords, to ease archive ingestion.

Requirements

Must haves:

  • Ingest of ALFALFA spectral data cubes and for each cube, three ancillary spectral products (spectral weights, continuum maps, continuum weights)
  • Ingest of the ALFALFA extragalactic catalog
  • Ingest of the ALFALFA spectral line profiles
  • Harvest and persistence of relevant generic and collection specific metadata.
  • Ability to filter on Collection in observation view (both: "must be in" and "must not be in" semantics) in Archive Interface
  • Ability to search on position, data cube name, or object (Cone Search)

Should haves:

  • Search hits should return the data cubes, and any catalog entries and spectra within the search parameters.

Could haves:

  • Search on frequency range?



Implementation Plan

Risk Assessment

The ALFALFA data represent a low-risk, completed, and mature dataset that will be useful to the astronomical community.  The data are not going to be remade or regridded, and will be ingested into the archive only one time.

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