activity
20022007
most citedMid-Infrared Spectroscopy of Disks around Classical T Tauri Stars

118 citations · 205 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph200787 cited

Decomposing Dusty Galaxies. I. Multi-Component Spectral Energy Distribution Fitting

J. A. Marshall, T. L. Herter, L. Armus +4

We present a new multi-component spectral energy distribution (SED) decomposition method and use it to analyze the ultraviolet to millimeter wavelength SEDs of a sample of dusty in…

astro-ph2006118 cited

Mid-Infrared Spectroscopy of Disks around Classical T Tauri Stars

W. J. Forrest, B. Sargent, E. Furlan +18

We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between Cornell University and Ball Aerospace Corporation funded by NASA through the Je…

astro-ph2005

Spectroscopic Redshifts to z > 2 for Optically Obscured Sources Discovered with the Spitzer Space Telescope

J. R. Houck, B. T. Soifer, D. Weedman +12

We have surveyed a field covering 9.0 degrees^2 within the NOAO Deep Wide-Field Survey region in Bootes with the Multiband Imaging Photometer on the Spitzer Space Telescope (SST) t…

astro-ph2004

Spitzer-IRS Spectroscopy of the Prototypical Starburst Galaxy NGC7714

B. R. Brandl, D. Devost, S. J. U. Higdon +11

We present observations of the starburst galaxy NGC 7714 with the Infrared Spectrograph IRS on board the Spitzer Space Telescope. The spectra yield a wealth of ionic and molecular…

astro-ph2004

The state of protoplanetary material 10 Myr after stellar formation: circumstellar disks in the TW Hydrae association

K. I. Uchida, N. Calvet, L. Hartmann +17

We have used the Spitzer Infrared Spectrograph to observe seven members of the TW Hya association, the nearest stellar association whose age ( 10 Myr) is similar to the times…

astro-ph2002

Radio-selected Galaxies in Very Rich Clusters at z < 0.25: I. Multi-wavelength Observations and Data Reduction Techniques

G. E. Morrison, F. N. Owen, M. J. Ledlow +4

Radio observations were used to detect the `active' galaxy population within rich clusters of galaxies in a non-biased manner that is not plagued by dust extinction or the K-correc…