User profiles for D. T. Jaffe
Daniel T JaffeUniversity of Texas at Austin Verified email at astro.as.utexas.edu Cited by 9190 |
Performance of NIRCam on JWST in flight
The Near Infrared Camera for the James Webb Space Telescope (JWST) is delivering the
imagery that astronomers have hoped for ever since JWST was proposed back in the 1990s. …
imagery that astronomers have hoped for ever since JWST was proposed back in the 1990s. …
Sustaining a family dynasty: Key issues facing complex multigenerational business‐and investment‐owning families
DT Jaffe, SH Lane - Family Business Review, 2004 - Wiley Online Library
As a business family moves from the second to the third, fourth, and succeeding generations,
and seeks to maintain shared family control of its often highly diversified financial and …
and seeks to maintain shared family control of its often highly diversified financial and …
[HTML][HTML] Aperture synthesis observations of the circumnuclear ring in the Galactic center
…, R Genzel, MCH Wright, DT Jaffe… - … Journal, Part 1 …, 1987 - adsabs.harvard.edu
… GENZEL,' MCH WRIGHT,3 DT JAFFE,' J. STUTZKI,' AND AI HARRIS' … heterodyne
spectrometer (Harris, Jaffe, and Genzel 1986). The … DT JAFFE: Department ofAstronomy …
spectrometer (Harris, Jaffe, and Genzel 1986). The … DT JAFFE: Department ofAstronomy …
TEXES: A sensitive high‐resolution grating spectrograph for the mid‐infrared
…, MJ Richter, TK Greathouse, DT Jaffe… - Publications of the …, 2002 - iopscience.iop.org
We discuss the design and performance of TEXES, the Texas Echelon Cross Echelle
Spectrograph. TEXES is a mid‐infrared (5–25 μm) spectrograph with several operating modes: …
Spectrograph. TEXES is a mid‐infrared (5–25 μm) spectrograph with several operating modes: …
Characterizing young brown dwarfs using low-resolution near-infrared spectra
We present near-infrared (1.0-2.4 μm) spectra confirming the youth and cool temperatures of
six brown dwarfs and low-mass stars with circumstellar disks toward the Chamaeleon II and …
six brown dwarfs and low-mass stars with circumstellar disks toward the Chamaeleon II and …
[HTML][HTML] Submillimeter and far-infrared line observations of M17 SW-A clumpy molecular cloud penetrated by ultraviolet radiation
…, R Genzel, AI Harris, DT Jaffe… - … Journal, Part 1 …, 1988 - adsabs.harvard.edu
Millimeter, submillimeter, and far-IR spectroscopic observations of the M17 SW star formation
region are reported. Strong forbidden C II 158 micron and CO J= 7-6 line emission arises …
region are reported. Strong forbidden C II 158 micron and CO J= 7-6 line emission arises …
The healthy company: Research paradigms for personal and organizational health.
DT Jaffe - 1995 - psycnet.apa.org
examines the organizational factors that support individual health and organizational
effectiveness/the question arises of whether the arrangements that companies have developed to …
effectiveness/the question arises of whether the arrangements that companies have developed to …
Zodiacal Exoplanets in Time (ZEIT). III. A Short-period Planet Orbiting a Pre-main-sequence Star in the Upper Scorpius OB Association
We confirm and characterize a close-in (${P} _ {{\rm {orb}}} $= 5.425 days), super-Neptune
sized (${5.04} _ {-0.37}^{+ 0.34} $${R} _ {\oplus} $) planet transiting K2-33 (2MASS …
sized (${5.04} _ {-0.37}^{+ 0.34} $${R} _ {\oplus} $) planet transiting K2-33 (2MASS …
Zodiacal exoplanets in time (ZEIT). I. A Neptune-sized planet orbiting an M4. 5 dwarf in the Hyades Star Cluster
Studying the properties of young planetary systems can shed light on how the dynamics
and structure of planets evolve during their most formative years. Recent K2 observations of …
and structure of planets evolve during their most formative years. Recent K2 observations of …
Dense gas and star formation: Characteristics of cloud cores associated with water masers
We have observed 150 regions of massive star formation, selected originally by the presence
of an H 2 O maser, in the J= 5→ 4, 3→ 2, and 2→ 1 transitions of CS, and 49 regions in the …
of an H 2 O maser, in the J= 5→ 4, 3→ 2, and 2→ 1 transitions of CS, and 49 regions in the …