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19982025
most citedThe Science Performance of JWST as Characterized in Commissioning

440 citations · 1.8k across the 44 of their papers we have counts for

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astro-ph2006★ 26 cited

Mid-Infrared Observations of Class I/Flat-Spectrum Systems in Six Nearby Molecular Clouds

Karl E. Haisch, Mary Barsony, Michael E. Ressler +1

We have obtained new mid-infrared observations of 65 Class I/Flat-Spectrum (F.S.) objects in the Perseus, Taurus, Chamaeleon I/II, Rho Ophiuchi, and Serpens dark clouds. We detecte…

astro-ph2005★ 18 cited

A Mid-Infrared Study of the Class 0 Cluster in LDN 1448

J. C. O'Linger, D. M. Cole, M. E. Ressler +1

We present ground-based mid-infrared observations of Class 0 protostars in LDN 1448. Of the five known protostars in this cloud, we detected two, L1448N:A and L1448C, at 12.5, 17.9…

astro-ph2005★ 21 cited

Sub-Arcsecond Mid-Infrared Observations of NGC 6240: Limitations of AGN-Starburst Power Diagnostics

E. Egami, G. Neugebauer, B. T. Soifer +3

In order to examine the relative importance of powerful starbursts and Compton-thick AGNs in NGC 6240, we have obtained mid-infrared images and low-resolution spectra of the galaxy…

astro-ph2005★ 7 cited

A New Large-Well 1024x1024 Si:As Detector for the Mid-Infrare

A. K. Mainzer, J. Hong, M. Stapelbroek +7

We present a description of a new 1024x1024 Si:As array designed for ground-based use from 5 - 28 microns. With a maximum well depth of 5e6 electrons, this device brings large-form…

astro-ph2005★ 48 cited

A Mid-Infrared Imaging Survey of Embedded Young Stellar Objects in the Rho Ophiuchi Cloud Core

Mary Barsony, Michael E. Ressler, Kenneth A. Marsh

Results of a comprehensive, new, ground-based mid-infrared imaging survey of the young stellar population of the Rho Ophiuchi cloud are presented. Data were acquired at the Palomar…

astro-ph2004★ 48 cited

Radial Distribution of Dust Grains Around HR 4796A

Z. Wahhaj, D. W. Koerner, D. E. Backman +4

We present high-dynamic-range images of circumstellar dust around HR 4796A that were obtained with MIRLIN at the Keck II telescope at lambda = 7.9, 10.3, 12.5 and 24.5 um. We also…