We present results from our analysis of F160W NICMOS Parallel images. These data cover ~9 sq. arcminutes and reach 3σ depths of H= 24.3 - 25.5 in a 0.6" diameter aperture with integration times of 2,000 to 13,000 seconds. We derive the first deep H band galaxy counts. The slope of the counts for H< 20 is 0.31, consistent with various K-band measurements from the Keck telescopes. The measured number counts vs. magnitude relation is reasonably well fitted with no-evolution models with a low Ω value. The half-light radii of the galaxies declines steeply with apparent magnitude and reaches the NIC3 resolution limit at H=23.5. Deep ground-based VRI imaging of one NICMOS field has revealed an extremely red galaxy with R-H = 6 and H of 18.8. Ou...
We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and...
A photometric redshift analysis of optical and infrared images of the Northern Hubble Deep Field ind...
We present the first results of a survey of random fields with the slitless G141 ($\lambda_c = 1.5\m...
We present results from our analysis of F160W NICMOS Parallel images. These data cover ~9 sq. arcmi...
We present deep galaxy counts and half-light radii from F160W (λ_c=1.6 μm) images obtained with the ...
We present high resolution NICMOS images of random fields obtained in parallel to other HST observat...
We present positions, magnitudes, sizes and morphological classifications for 111 galaxies discovere...
Using the Hubble Ultra Deep Field Near Infrared Camera and Multi-Object Spectrometer (HUDF-NICMOS) U...
We present the first results of a survey of random fields with the slitless G141 (λ_c = 1.5 μm, Δλ =...
We present Keck LRIS spectroscopy along with NICMOS F110W (~J) and F160W (~H) images of the galaxy H...
We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and...
Deep, near-infrared imaging surveys have been motivated by the desire to study the rest-frame optica...
This paper presents initial results and performance levels from the Near Infrared Camera and Multi-O...
We present deep, high angular-resolution HST NICMOS imaging in the Hubble Deep Field South (HDF-S), ...
We present deep, high angular-resolution HST/NICMOS imaging in the Hubble Deep Field South (HDF-S), ...
We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and...
A photometric redshift analysis of optical and infrared images of the Northern Hubble Deep Field ind...
We present the first results of a survey of random fields with the slitless G141 ($\lambda_c = 1.5\m...
We present results from our analysis of F160W NICMOS Parallel images. These data cover ~9 sq. arcmi...
We present deep galaxy counts and half-light radii from F160W (λ_c=1.6 μm) images obtained with the ...
We present high resolution NICMOS images of random fields obtained in parallel to other HST observat...
We present positions, magnitudes, sizes and morphological classifications for 111 galaxies discovere...
Using the Hubble Ultra Deep Field Near Infrared Camera and Multi-Object Spectrometer (HUDF-NICMOS) U...
We present the first results of a survey of random fields with the slitless G141 (λ_c = 1.5 μm, Δλ =...
We present Keck LRIS spectroscopy along with NICMOS F110W (~J) and F160W (~H) images of the galaxy H...
We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and...
Deep, near-infrared imaging surveys have been motivated by the desire to study the rest-frame optica...
This paper presents initial results and performance levels from the Near Infrared Camera and Multi-O...
We present deep, high angular-resolution HST NICMOS imaging in the Hubble Deep Field South (HDF-S), ...
We present deep, high angular-resolution HST/NICMOS imaging in the Hubble Deep Field South (HDF-S), ...
We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and...
A photometric redshift analysis of optical and infrared images of the Northern Hubble Deep Field ind...
We present the first results of a survey of random fields with the slitless G141 ($\lambda_c = 1.5\m...