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Chemo-kinematic ages of eccentric-planet-hosting M dwarf stars. Accepted for publication in ApJ
Veyette, M. J., et al. (2017).
A physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs. ApJ, 851, 26
Kesseli, A. Y., et al. (2017).
An Empirical Template Library of Stellar Spectra for a Wide Range of Spectral Classes, Luminosity Classes, and Metallicities Using SDSS BOSS Spectra. ApJS, 230, 16
Veyette, M. J., et al. (2016).
NEWS: the near-infrared Echelle for wideband spectroscopy. Proceedings of the SPIE, 9908, 99086M
Veyette, M. J., Muirhead, P., Mann, A., Allard, F. (2016).
The physical mechanism behind M dwarf metallicity indicators and the role of C and O abundances. ApJ, 828, 95
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The Transit Transmission Spectrum of a Cold Gas Giant Planet. ApJ, 814, 154
Girardi, L. et al. (2015).
TP-AGB stars in M31: Results from PHAT. ASP Conference Series, 497, 413
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Panchromatic Hubble Andromeda Treasury IX: A Photometric Survey of Planetary Nebulae in M31.
ApJ, 792, 121
Muirhead, P. S., Hall, Z. J., & Veyette, M. J. (2014).
HiJaK: the High-resolution J, H and K spectrometer.
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