Visit image#

Individual processed and calibrated sky images.

Citation: NSF-DOE Vera C. Rubin Observatory (2025); Legacy Survey of Space and Time Data Preview 1: visit_image dataset type DOI Logo https://doi.org/10.71929/rubin/2570311 [BibTeX]

Access#

The visit images are accessible via the Butler, SIA, and TAP services.

Butler#

  • Dataset type: (‘visit_image’, {band, instrument, day_obs, detector, physical_filter, visit}, ExposureF)

  • Format: FITS

  • Number of Butler datasets: 15,972

SIA and TAP#

Schema: ObsCore table

IVOA calibration level: 2

Dataproduct subtype: lsst.visit_image

Description#

Raw images from the camera undergo processing that includes instrument signature removal (ISR), image calibration (photometric and astrometric), and PSF estimation. The result is a fully calibrated visit image.

Each individual visit image contains data from one of the camera’s detectors.

Processing#

The visit images are the result of Image calibration.

Pixel data#

The visit images have three planes of pixel data.

Image: Sky pixel data in flux units of nJy.

Variance: Uncertainty (noise) in the flux in units of nJy^2.

Mask: An integer bitmask of representative flag values that indicate processing status or issues, similar to the SDSS bitmasks.

Metadata#

The metadata for visit images retrieved from the Butler include information about the observation (e.g., pointing, weather), and the derived PSF, photometric calibration, and WCS.

WCS#

The World Coordinate System objects for visit images are not exactly representable as FITS; the FITS headers have an approximation that is good enough only for visualization. Transformations with the true WCS are currently only possible using LSST Science Pipelines libraries, and those can be easy to misuse. See WCS FITS approximations and misleading interfaces for more information.

Tutorials#

See the 200-level notebook or 200-level portal tutorials demonstrating how to access the visit images.