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19962025
most citedTEXES: A Sensitive High-Resolution Grating Spectrograph for the Mid-Infrared

254 citations · 925 across the 13 of their papers we have counts for

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astro-ph2006★ 221 cited

Characterizing Young Brown Dwarfs using Low Resolution Near-IR Spectra

K. N. Allers, D. T. Jaffe, K. L. Luhman +7

We present near-infrared (1.0-2.4 micron) spectra confirming the youth and cool effective temperatures of 6 brown dwarfs and low mass stars with circumstellar disks toward the Cham…

astro-ph2006★ 113 cited

Young, Low-Mass Brown Dwarfs with Mid-Infrared Excesses

K. N. Allers, J. E. Kessler-Silacci, L. A. Cieza +1

We have combined new I, J, H, and Ks imaging of portions of the Chamaeleon II, Lupus I, and Ophiuchus star-forming clouds with 3.6 to 24 micron imaging from the Spitzer Legacy Prog…

astro-ph2003★ 44 cited

Stellar Properties of Pre-Main Sequence Stars from High Resolution Near-IR Spectra

G. W. Doppmann, D. T. Jaffe, R. J. White

We present high resolution (R=50,000) spectra at 2.2 um of 16 young stars in the rho Ophiuchi dark cloud. Photospheric features are detected in the spectra of 11 of these sources,…

astro-ph2001★ 254 cited

TEXES: A Sensitive High-Resolution Grating Spectrograph for the Mid-Infrared

J. H. Lacy, M. J. Richter, T. K. Greathouse +2

We discuss the design and performance of TEXES, the Texas Echelon Cross Echelle Spectrograph. TEXES is a mid-infrared (5-25 um) spectrograph with several operating modes: high-reso…

astro-ph1999★ 53 cited

Low Velocity Ionized Winds from Regions Around Young O Stars

D. T. Jaffe, J. Martin-Pintado

We have observed seven ultracompact HII regions in hydrogen recombination lines in the millimeter band. Toward four of these regions, there is a high velocity (full width to half m…

astro-ph1996★ 20 cited

Molecular Hydrogen Emission from the Inner 400 Parsecs of the Galaxy

Soojong Pak, D. T. Jaffe, L. D. Keller

We have mapped the H_2 v=1-0 S(1) (λ=2.1215 \micron) emission line along a 400 pc long strip and in a 50 pc region in the Galactic center. There is H_2 emission throughout the surv…