An atlas of bright star spectra in the near infrared from Cassini-VIMS
arXiv:1511.01670 · doi:10.1088/0067-0049/221/2/30
Abstract
We present the Cassini Atlas Of Stellar Spectra (CAOSS), comprised of near-infrared low-resolution spectra of bright stars recovered from space-based observations by the Cassini spacecraft. The 65 stellar targets in the atlas are predominately M, K and S giants. However it also contains spectra of other bright nearby stars including carbon stars and main sequence stars from A to F. The spectra presented are free of all spectral contamination caused by the Earth's atmosphere, including the detrimental telluric molecular bands which put parts of the near-infrared spectrum out of reach of terrestrial observations. With a single instrument, a spectro-photometric dataset is recovered that spans the near-infrared from 0.8 to 5.1 microns with spectral resolution ranging from R=53.5 to R=325. Spectra have been calibrated into absolute flux units after careful characterisation of the instrumental spectral efficiency. Spectral energy distributions for most stars match closely with literature values. All final data products have been made available online.
10 emulateapj pages, 4 figures, 4 tables. Accepted by ApJS. Full atlas available at http://www.physics.usyd.edu.au/sifa/caoss/
References in corpus (4)
- Near-infrared integral field spectroscopy of the Homunculus nebula around Eta Carinae using Gemini/CIRPASS
- High Angular Resolution Stellar Imaging with Occultations from the Cassini Spacecraft I: Observational Technique
- Infrared spectral properties of M giants
- High Angular Resolution Stellar Imaging with Occultations from the Cassini Spacecraft II: Kronocyclic Tomography
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