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Spectra.md

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Spectra

The Spectra table contains spectra for sources listed in the Sources table. Spectra are stored as strings representing the full URL of the spectrum location. The combination of source, spectrum, regime, observation_date, and reference is expected to be unique. Columns marked with an asterisk (*) may not be empty.

Column Name Description Unit Data Type Key Type
*source Unique identifier for the source String(100) primary and foreign: Sources.source
*spectrum URL of spectrum location String(1000) primary
original_spectrum URL of original spectrum location, if applicable String(1000)
local_spectrum Local path of spectrum String(1000)
*regime Regime of the spectrum, eg Optical, Infrared, etc foreign: Regimes.regime
*telescope Name of telescope String(30) foreign: Telescopes.telescope
*instrument Name of instrument String(30) foreign: Instruments.instrument
*mode Mode of spectrum String(30) foreign: Instruments.mode
*observation_date Observation date DateTime primary
comments Free form comments String(1000)
*reference Primary Reference String(30) primary and foreign: Publications.reference
other_references Other References String(100)

Relevant functions: spectra.ingest_spectrum, spectra.spectrum_plottable, spectra.find_spectra

If the spectrum provided has been modified from the author-provided one, a link to the original spectrum can be provided in the original_spectrum column.

The local_spectrum is meant to store the path to a local copy of the spectrum with an environment variable to define part of the path (so it can be shared among other users). For example: $ASTRODB_SPECTRA/infrared/filename.fits

Notes

  • An accurate observation date is required for a spectrum to be ingested.
  • Data based on data from multiple observation dates has 'Multiple observation dates' indicated in the comments field. One of the dates should be used for the observation_date.
  • Spectra for companions should be associated with individual sources and not grouped with the primary source.