activity
19982017
most citedNICMOS Imaging of Infrared-Luminous Galaxies

361 citations · 1k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2017★ 102 cited

SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6

K. P. Olsen, T. R. Greve, D. Narayanan +4

Of the almost 40 star forming galaxies at z>~5 (not counting QSOs) observed in [CII] to date, nearly half are either very faint in [CII], or not detected at all, and fall well belo…

astro-ph.CO2015★ 48 cited

The Reionization of Carbon

K. Finlator, R. Thompson, S. Huang +3

Observations suggest that CII was more abundant than CIV in the intergalactic medium towards the end of the hydrogen reionization epoch. This transition provides a unique opportuni…

astro-ph2005★ 49 cited

Distant red galaxies in the Hubble Ultra Deep Field

S. Toft, P. van Dokkum, M. Franx +4

We take advantage of the Hubble Ultra Deep Field (UDF) data to study the restframe optical and ultra violet (UV) morphologies of the novel population of Distant Red Galaxies (DRGs)…

astro-ph2005★ 179 cited

The near-infrared size-luminosity relations for Herbig Ae/Be disks

J. D. Monnier, R. Millan-Gabet, R. Billmeier +31

We report the results of a sensitive K-band survey of Herbig Ae/Be disk sizes using the 85-m baseline Keck Interferometer. Targets were chosen to span the maximum range of stellar…

astro-ph2001★ 108 cited

High-resolution Near-Infrared Images and Models of the Circumstellar Disk in HH 30

A. S. Cotera, B. A. Whitney, E. Young +6

We present Hubble Space Telescope (HST) Near-Infrared Camera and Multi-object Spectrometer (NICMOS) observations of the reflection nebulosity associated with the T Tauri star HH 30…

astro-ph2000★ 11 cited

A Multivariate Analysis of Galaxies in the Hubble Deep Field North

Michael R. Corbin, Andrea Urban, Elizabeth Stobie +2

We use the ultraviolet and optical WFPC2 and near-infrared NICMOS images of the Hubble Deep Field North to measure and statistically compare an array of parameters for over 250 of…