Search Publications

The Hubble Higher z Supernova Search: Supernovae to z ~ 1.6 and Constraints on Type Ia Progenitor Models
DOI: 10.1086/422901 Bibcode: 2004ApJ...613..200S

Dickinson, Mark; Giavalisco, Mauro; Ravindranath, Swara +33 more

We present results from the Hubble Higher z Supernova Search, the first space-based open field survey for supernovae (SNe). In cooperation with the Great Observatories Origins Deep Survey, we have used the Hubble Space Telescope with the Advanced Camera for Surveys to cover ~300 arcmin2 in the area of the Chandra Deep Field South and th…

2004 The Astrophysical Journal
eHST 286
The star formation rate of the Universe at z~ 6 from the Hubble Ultra-Deep Field
DOI: 10.1111/j.1365-2966.2004.08326.x Bibcode: 2004MNRAS.355..374B

Bunker, Andrew J.; McMahon, Richard G.; Ellis, Richard S. +1 more

We determine the abundance of i'-band dropouts in the recently released HST/ACS Hubble Ultra-Deep Field (UDF). Because the majority of these sources are likely to be z~ 6 galaxies whose flux decrement between the F775W i'-band and F850LP z'-band arises from Lyman-α absorption, the number of detected candidates provides a valuable upper limit to th…

2004 Monthly Notices of the Royal Astronomical Society
eHST 285
The ACS Virgo Cluster Survey. I. Introduction to the Survey
DOI: 10.1086/421490 Bibcode: 2004ApJS..153..223C

Jordán, Andrés; Tonry, John L.; Côté, Patrick +7 more

The Virgo Cluster is the dominant mass concentration in the Local Supercluster and the largest collection of elliptical and lenticular galaxies in the nearby universe. In this paper, we present an introduction to the ACS Virgo Cluster Survey: a program to image, in the F475W and F850LP bandpasses (~Sloan g and z), 100 early-type galaxies in the Vi…

2004 The Astrophysical Journal Supplement Series
eHST 284
Nearby stars of the Galactic disk and halo. III.
DOI: 10.1002/asna.200310173 Bibcode: 2004AN....325....3F

Fuhrmann, K.

High-resolution spectroscopic observations of about 150 nearby stars or star systems are presented and discussed. The study of these and another 100 objects of the previous papers of this series implies that the Galaxy became reality 13 or 14 Gyr ago with the implementation of a massive, rotationally-supported population of thick-disk stars. The v…

2004 Astronomische Nachrichten
Hipparcos 284
Kinetic parameters of interstellar neutral helium. Review of results obtained during one solar cycle with the Ulysses/GAS-instrument
DOI: 10.1051/0004-6361:20035956 Bibcode: 2004A&A...426..835W

Witte, M.

The GAS-instrument onboard the space probe Ulysses is designed to measure the local angular distribution of the flow of interstellar neutral He-atoms within ≈3 AU distance from the sun. It allows to infer the kinetic parameters (velocity vector, temperature and density) of these particles outside the heliosphere (``at infinity''). During three obs…

2004 Astronomy and Astrophysics
Ulysses 283
Cosmic Variance in the Great Observatories Origins Deep Survey
DOI: 10.1086/378628 Bibcode: 2004ApJ...600L.171S

Ferguson, Henry C.; Giavalisco, Mauro; Somerville, Rachel S. +3 more

Cosmic variance is the uncertainty in observational estimates of the volume density of extragalactic objects such as galaxies or quasars arising from the underlying large-scale density fluctuations. This is often a significant source of uncertainty, especially in deep galaxy surveys, which tend to cover relatively small areas. We present estimates…

2004 The Astrophysical Journal
eHST 282
The Team Keck Treasury Redshift Survey of the GOODS-North Field
DOI: 10.1086/420999 Bibcode: 2004AJ....127.3121W

Davis, Marc; Capak, Peter; Faber, S. M. +19 more

We report the results of an extensive imaging and spectroscopic survey in the Great Observatories Origins Deep Survey (GOODS)-North field completed using DEIMOS on the Keck II telescope. Observations of 2018 targets in a magnitude-limited sample of 2911 objects to RAB=24.4 yield secure redshifts for a sample of 1440 galaxies and active …

2004 The Astronomical Journal
eHST 281
Coronal Magnetic Field Measurements
DOI: 10.1086/425217 Bibcode: 2004ApJ...613L.177L

Lin, H.; Kuhn, J. R.; Coulter, R.

A long-standing solar problem has been to measure the coronal magnetic field. We believe it determines the coronal structure and dynamics from the upper chromosphere out into the heliospheric environment. It is only recently that Zeeman splitting observations of infrared coronal emission lines have been successfully used to deduce the coronal magn…

2004 The Astrophysical Journal
SOHO 280
The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter
DOI: 10.1086/382146 Bibcode: 2004ApJ...604...88S

Smith, Graham P.; Treu, Tommaso; Ellis, Richard S. +1 more

We have undertaken a spectroscopic survey of gravitational arcs in a carefully chosen sample of six clusters, each containing a dominant brightest cluster galaxy. We use these systems to study the relative distributions of dark and baryonic material in the central regions. Three clusters present both radial and tangential arcs and provide particul…

2004 The Astrophysical Journal
eHST 279
Spatial scale of high-speed flows in the plasma sheet observed by Cluster
DOI: 10.1029/2004GL019558 Bibcode: 2004GeoRL..31.9804N

Balogh, A.; Zhang, T. L.; Klecker, B. +9 more

Spatial gradients of high-speed flows in the midtail plasma sheet are determined using multipoint observations from the Cluster spacecraft along the ``dawn-dusk'' direction (perpendicular to the main flow and in the plane of the tail current sheet) and along the north-south direction. If we take the average or median of the spatial gradients and a…

2004 Geophysical Research Letters
Cluster 277