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20172022
most citedAPOGEE Net: An expanded spectral model of both low mass and high mass stars

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astro-ph.SR2017

Optical and Near-Infrared Spectra of sigma Orionis Isolated Planetary-mass Objects

M. R. Zapatero Osorio, V. J. S. Béjar, K. Peña Ramírez

We have obtained low-resolution optical (0.7-0.98 micron) and near-infrared (1.11-1.34 micron and 0.8-2.5 micron) spectra of twelve isolated planetary-mass candidates (J = 18.2-19.…