meta/wcsinfo-1.0.0

World Coordinate System (WCS) Information

Outline

Schema Definitions

This type is an object with the following properties:

  • aperture_name

    stringRequired

    Aperture Name

    Name of the aperture used to specify the transformations between detector pixel, science pixel, and spacecraft V coordinate frames. This information comes from the Science Instrument Aperture File (SIAF) in the Science Operations Center (SOC) Project Reference Database (PRD).

    No length restriction

    Only the following values are valid for this node:

    • WFI01_FULL

    • WFI02_FULL

    • WFI03_FULL

    • WFI04_FULL

    • WFI05_FULL

    • WFI06_FULL

    • WFI07_FULL

    • WFI08_FULL

    • WFI09_FULL

    • WFI10_FULL

    • WFI11_FULL

    • WFI12_FULL

    • WFI13_FULL

    • WFI14_FULL

    • WFI15_FULL

    • WFI16_FULL

    • WFI17_FULL

    • WFI18_FULL

    • WFI_01_FULL

    • WFI_02_FULL

    • WFI_03_FULL

    • WFI_04_FULL

    • WFI_05_FULL

    • WFI_06_FULL

    • WFI_07_FULL

    • WFI_08_FULL

    • WFI_09_FULL

    • WFI_10_FULL

    • WFI_11_FULL

    • WFI_12_FULL

    • WFI_13_FULL

    • WFI_14_FULL

    • WFI_15_FULL

    • WFI_16_FULL

    • WFI_17_FULL

    • WFI_18_FULL

    • WFI_CEN

    • BORESIGHT

    • CGI_CEN

  • v2_ref

    numberRequired

    V2 Reference Position (arcsec)

    Coordinate of the reference pixel position along the telescope V2 axis in units of arcseconds. This information comes from the Science Instrument Aperture File (SIAF) in the Science Operations Center (SOC) Project Reference Database (PRD). The telescope V coordinate system is defined with its origin at the vertex of the primary mirror. The +V1 axis is defined as parallel to the telescope boresight, the +V3 axis is orthogonal to the sunshield, and the +V2 axis completes the right-hand system. See Roman-STScI-000143 “Description of the Roman SIAF and Coordinate Frames” for more information.

  • v3_ref

    numberRequired

    V3 Reference Position (arcsec)

    Coordinate of the reference pixel position along the telescope V3 axis in units of arcseconds. This information comes from the Science Instrument Aperture File (SIAF) in the Science Operations Center (SOC) Project Reference Database (PRD). The telescope V coordinate system is defined with its origin at the vertex of the primary mirror. The +V3 axis is orthogonal to the sunshield. See Roman-STScI-000143 “Description of the Roman SIAF and Coordinate Frames” for more information.

  • vparity

    integerRequired

    Relative Rotation Between the Ideal and Telescope Axes

    Relative sense of rotation between the ideal and telescope coordinate systems. The value may be either 1 or -1. This information comes from the Science Instrument Aperture File (SIAF) in the Science Operations Center (SOC) Project Reference Database (PRD). See documents STScI-JWST-001550 and STScI-Roman-000143 for more information.

    Only the following values are valid for this node:

    • -1

    • 1

  • v3yangle

    numberRequired

    Angle Between the V3 and Ideal Y Axes (deg)

    Angle between the telescope V3 axis and the ideal Y axis in units of degrees. This information comes from the Science Instrument Aperture File (SIAF) in the Science Operations Center (SOC) Project Reference Database (PRD). The telescope V coordinate system is defined with its origin at the vertex of the primary mirror. The +V3 axis is orthogonal to the sunshield. The ideal coordinate system is a geomtric-distortion-corrected reference frame projected onto a tangent plane. See Roman-STScI-000143 “Description of the Roman SIAF and Coordinate Frames” for more information.

  • ra_ref

    numberRequired

    Right Ascension of the Reference Position (deg)

    Right ascension of the reference pixel position on the sky in units of degrees.

  • dec_ref

    numberRequired

    Declination of the Reference Position (deg)

    Declination of the reference pixel position on the sky in units of degrees.

  • roll_ref

    numberRequired

    V3 Position Angle at the Reference Position

    Position angle of the telescope V3 axis at the reference pixel position measured from North to East. The telescope V coordinate system is defined with its origin at the vertex of the primary mirror. The +V3 axis is orthogonal to the sunshield. See Roman-STScI-000143 “Description of the Roman SIAF and Coordinate Frames” for more information.

  • s_region

    stringRequired

    Spatial Extent of the Exposure

    The region of the sky enclosed by the pixel data contained within this file. This is given as a polygon stored as a string with the vertices defined by a list of right ascension and declination pairs in units of degrees.

    No length restriction

Original Schema

%YAML 1.1
---
$schema: asdf://stsci.edu/datamodels/roman/schemas/rad_schema-1.0.0
id: asdf://stsci.edu/datamodels/roman/schemas/meta/wcsinfo-1.0.0

title: World Coordinate System (WCS) Information
type: object
properties:
  aperture_name:
    title: Aperture Name
    description: |
      Name of the aperture used to specify the
      transformations between detector pixel, science pixel, and
      spacecraft V coordinate frames. This information comes from the
      Science Instrument Aperture File (SIAF) in the Science
      Operations Center (SOC) Project Reference Database (PRD).
    type: string
    enum:
      [
        "WFI01_FULL",
        "WFI02_FULL",
        "WFI03_FULL",
        "WFI04_FULL",
        "WFI05_FULL",
        "WFI06_FULL",
        "WFI07_FULL",
        "WFI08_FULL",
        "WFI09_FULL",
        "WFI10_FULL",
        "WFI11_FULL",
        "WFI12_FULL",
        "WFI13_FULL",
        "WFI14_FULL",
        "WFI15_FULL",
        "WFI16_FULL",
        "WFI17_FULL",
        "WFI18_FULL",
        "WFI_01_FULL",
        "WFI_02_FULL",
        "WFI_03_FULL",
        "WFI_04_FULL",
        "WFI_05_FULL",
        "WFI_06_FULL",
        "WFI_07_FULL",
        "WFI_08_FULL",
        "WFI_09_FULL",
        "WFI_10_FULL",
        "WFI_11_FULL",
        "WFI_12_FULL",
        "WFI_13_FULL",
        "WFI_14_FULL",
        "WFI_15_FULL",
        "WFI_16_FULL",
        "WFI_17_FULL",
        "WFI_18_FULL",
        "WFI_CEN",
        "BORESIGHT",
        "CGI_CEN",
      ]
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: nvarchar(20)
      destination: [WFIExposure.aperture_name, GuideWindow.aperture_name]

  v2_ref:
    title: V2 Reference Position (arcsec)
    description: |
      Coordinate of the reference pixel position along the
      telescope V2 axis in units of arcseconds. This information comes
      from the Science Instrument Aperture File (SIAF) in the Science
      Operations Center (SOC) Project Reference Database (PRD). The
      telescope V coordinate system is defined with its origin at the
      vertex of the primary mirror. The +V1 axis is defined as
      parallel to the telescope boresight, the +V3 axis is orthogonal
      to the sunshield, and the +V2 axis completes the right-hand
      system. See Roman-STScI-000143 "Description of the Roman SIAF
      and Coordinate Frames" for more information.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.v2_ref, GuideWindow.v2_ref]
  v3_ref:
    title: V3 Reference Position (arcsec)
    description: |
      Coordinate of the reference pixel position along the
      telescope V3 axis in units of arcseconds. This information comes
      from the Science Instrument Aperture File (SIAF) in the Science
      Operations Center (SOC) Project Reference Database (PRD). The
      telescope V coordinate system is defined with its origin at the
      vertex of the primary mirror. The +V3 axis is orthogonal to the
      sunshield. See Roman-STScI-000143 "Description of the Roman SIAF
      and Coordinate Frames" for more information.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.v3_ref, GuideWindow.v3_ref]
  vparity:
    title: Relative Rotation Between the Ideal and Telescope Axes
    description: |
      Relative sense of rotation between the ideal and
      telescope coordinate systems. The value may be either 1 or -1.
      This information comes from the Science Instrument Aperture File
      (SIAF) in the Science Operations Center (SOC) Project Reference
      Database (PRD). See documents STScI-JWST-001550 and
      STScI-Roman-000143 for more information.
    type: integer
    enum: [-1, 1]
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: smallint
      destination: [WFIExposure.vparity, GuideWindow.vparity]
  v3yangle:
    title: Angle Between the V3 and Ideal Y Axes (deg)
    description: |
      Angle between the telescope V3 axis and the ideal Y
      axis in units of degrees. This information comes from the
      Science Instrument Aperture File (SIAF) in the Science
      Operations Center (SOC) Project Reference Database (PRD). The
      telescope V coordinate system is defined with its origin at the
      vertex of the primary mirror. The +V3 axis is orthogonal to the
      sunshield. The ideal coordinate system is a
      geomtric-distortion-corrected reference frame projected onto a
      tangent plane. See Roman-STScI-000143 "Description of the Roman
      SIAF and Coordinate Frames" for more information.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.v3yangle, GuideWindow.v3yangle]
  ra_ref:
    title: Right Ascension of the Reference Position (deg)
    description: |
      Right ascension of the reference pixel position on the
      sky in units of degrees.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.ra_ref, GuideWindow.ra_ref]
  dec_ref:
    title: Declination of the Reference Position (deg)
    description: |
      Declination of the reference pixel position on the sky
      in units of degrees.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.dec_ref, GuideWindow.dec_ref]
  roll_ref:
    title: V3 Position Angle at the Reference Position
    description: |
      Position angle of the telescope V3 axis at the
      reference pixel position measured from North to East. The
      telescope V coordinate system is defined with its origin at the
      vertex of the primary mirror. The +V3 axis is orthogonal to the
      sunshield. See Roman-STScI-000143 "Description of the Roman SIAF
      and Coordinate Frames" for more information.
    type: number
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: float
      destination: [WFIExposure.roll_ref, GuideWindow.roll_ref]
  s_region:
    title: Spatial Extent of the Exposure
    description: |
      The region of the sky enclosed by the pixel data
      contained within this file. This is given as a polygon stored as
      a string with the vertices defined by a list of right ascension
      and declination pairs in units of degrees.
    type: string
    sdf:
      special_processing: VALUE_REQUIRED
      source:
        origin: TBD
    archive_catalog:
      datatype: nvarchar(max)
      destination: [WFIExposure.s_region, GuideWindow.s_region]
required:
  [
    aperture_name,
    v2_ref,
    v3_ref,
    vparity,
    v3yangle,
    ra_ref,
    dec_ref,
    roll_ref,
    s_region,
  ]