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A Method of Correcting Near-Infrared Spectra for Telluric Absorption

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We present a method for correcting near-infrared medium-resolution spectra for telluric absorption. The method makes use of a spectrum of an A0V star, observed near in time and close in airmass to the target object, and a high-resolution model of Vega, to construct a telluric correction spectrum that is free of stellar absorption features. The technique was designed specifically to perform telluric corrections on spectra obtained with SpeX, a 0.8-5.5 micron, medium-resolution cross-dispersed spectrograph at the NASA Infrared Telescope Facility, and uses the fact that for medium resolutions there exist spectral regions uncontaminated by atmospheric absorption lines. However, it is also applicable (in a somewhat modified form) to spectra obtained with other near-infrared spectrographs. An IDL-based code that carries out the procedures is available for downloading via the World Wide Web from the IRTF website.

fields

astro-ph.SR 2

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

Gaia21bja: pre-main sequence star with quasi-periodic bursts

astro-ph.SR · 2026-05-19 · unverdicted · novelty 4.0

Gaia21bja is identified as a pre-main sequence star with quasi-periodic bursts, showing spectral features and a 5.5-6 times higher accretion rate during outbursts that place it in the periodic category of outbursting YSOs.

The Accretion Process on Protostars

astro-ph.SR · 2026-05-13 · unverdicted · novelty 2.0

The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.

citing papers explorer

Showing 2 of 2 citing papers.

  • Gaia21bja: pre-main sequence star with quasi-periodic bursts astro-ph.SR · 2026-05-19 · unverdicted · none · ref 76 · internal anchor

    Gaia21bja is identified as a pre-main sequence star with quasi-periodic bursts, showing spectral features and a 5.5-6 times higher accretion rate during outbursts that place it in the periodic category of outbursting YSOs.

  • The Accretion Process on Protostars astro-ph.SR · 2026-05-13 · unverdicted · none · ref 139 · internal anchor

    The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.