Near-infrared Spectral Characterization of Solar-type Stars in the Northern Hemisphere
Collin D. Lewin, Ellen S. Howell, Ronald J. Vervack Jr, Yanga R., Fern\'andez, Christopher Magri, Sean E. Marshall, Jenna L. Crowell, Mary L., Hinkle

TL;DR
This study characterizes 184 solar-analog stars in the near-infrared range (0.8-4.2 microns) to improve calibration standards for solar system observations, identifying 145 reliable analogs suitable for calibration purposes.
Contribution
It provides a comprehensive near-infrared spectral catalog of solar-analog stars, including classification into reliable, usable, and unsuitable categories, expanding calibration options beyond visible wavelengths.
Findings
145 stars classified as reliable solar analogs
18 stars deemed unsuitable for calibration
Most reliable analogs are consistent from 2.5 to 4.2 microns
Abstract
Although solar-analog stars have been studied extensively over the past few decades, most of these studies have focused on visible wavelengths, especially those identifying solar-analog stars to be used as calibration tools for observations. As a result, there is a dearth of well-characterized solar analogs for observations in the near-infrared, a wavelength range important for studying solar system objects. We present 184 stars selected based on solar-like spectral type and V-J and V-K colors whose spectra we have observed in the 0.8-4.2 micron range for calibrating our asteroid observations. Each star has been classified into one of three ranks based on spectral resemblance to vetted solar analogs. Of our set of 184 stars, we report 145 as reliable solar-analog stars, 21 as solar analogs usable after spectral corrections with low-order polynomial fitting, and 18 as unsuitable for use…
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