Search Publications

The Nitrogen Chemistry of Titan's Upper Atmosphere Revealed
DOI: 10.1086/507467 Bibcode: 2006ApJ...647L.175V

Yelle, R. V.; Vuitton, V.; Anicich, V. G.

Titan's atmosphere is unique because dissociation of N2 and CH4, the primary atmospheric constituents, provides the H, C, and N atoms necessary for the synthesis of complex organic molecules. The first steps in the synthesis of organic molecules occur in the upper atmosphere where energetic photons and electrons dissociate N<…

2006 The Astrophysical Journal
Cassini 178
Cepheid Distances to SNe Ia Host Galaxies Based on a Revised Photometric Zero Point of the HST WFPC2 and New PL Relations and Metallicity Corrections
DOI: 10.1086/503800 Bibcode: 2006ApJS..165..108S

Saha, A.; Tammann, G. A.; Thim, F. +2 more

With this paper we continue the preparation for a forthcoming summary report of our experiment with the HST to determine the Hubble constant using Type Ia supernovae as standard candles. Two problems are addressed. (1) We examine the need for, and determine the value of, the corrections to the apparent magnitudes of our program Cepheids in the 11 …

2006 The Astrophysical Journal Supplement Series
eHST 178
The unprecedented optical outburst of the quasar 3C 454.3. The WEBT campaign of 2004-2005
DOI: 10.1051/0004-6361:20064817 Bibcode: 2006A&A...453..817V

Lee, C. -U.; Lähteenmäki, A.; Umana, G. +85 more

Context: .The radio quasar 3C 454.3 underwent an exceptional optical outburst lasting more than 1 year and culminating in spring 2005. The maximum brightness detected was R=12.0, which represents the most luminous quasar state thus far observed (MB ∼ -31.4).
Aims: .In order to follow the emission behaviour of the …

2006 Astronomy and Astrophysics
INTEGRAL 178
The X-ray nuclei of intermediate-redshift radio sources
DOI: 10.1111/j.1365-2966.2006.10615.x Bibcode: 2006MNRAS.370.1893H

Hardcastle, M. J.; Croston, J. H.; Evans, D. A.

We present a Chandra and XMM-Newton spectral analysis of the nuclei of the radio galaxies and radio-loud quasars from the 3CRR sample in the redshift range 0.1 < z < 0.5. In the range of radio luminosity sampled by these objects, mostly Fanaroff-Riley type IIs (FR IIs), it has been clear for some time that a population of radio galaxies [low…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 177
A Survey of Galaxy Kinematics to z~1 in the TKRS/GOODS-N Field. I. Rotation and Dispersion Properties
DOI: 10.1086/508921 Bibcode: 2006ApJ...653.1027W

Weiner, Benjamin J.; Faber, S. M.; Willmer, Christopher N. A. +7 more

We present kinematic measurements of a large sample of galaxies from the Team Keck Redshift Survey in the GOODS-N field. We measure line-of-sight velocity dispersions from integrated emission for 1089 galaxies with median redshift 0.637 and spatially resolved kinematics for a subsample of 380 galaxies. This is the largest sample of galaxies to z~1…

2006 The Astrophysical Journal
eHST 176
3D spectroscopy with VLT/GIRAFFE. I. The true Tully Fisher relationship at z ∼ 0.6
DOI: 10.1051/0004-6361:20054217 Bibcode: 2006A&A...455..107F

Flores, H.; Hammer, F.; Puech, M. +2 more

A precise derivation of the evolution of the Tully Fisher is crucial to understand the interplay between dark matter and baryonic matter in cosmological models, using 15 deployable integral field units of FLAMES/GIRAFFE at VLT, we have recovered the velocity fields of 35 galaxies at intermediate redshift (0.4 < z < 0.75). This facility is ab…

2006 Astronomy and Astrophysics
eHST 176
Cosmic Evolution of Black Holes and Spheroids. I. The MBH-σ Relation at z = 0.36
DOI: 10.1086/504586 Bibcode: 2006ApJ...645..900W

Treu, Tommaso; Malkan, Matthew A.; Blandford, Roger D. +1 more

We test the evolution of the correlation between black hole mass and bulge velocity dispersion (MBH-σ), using a carefully selected sample of 14 Seyfert 1 galaxies at z=0.36+/-0.01. We measure velocity dispersion from stellar absorption lines around Mg b (5175 Å) and Fe (5270 Å) using high-S/N Keck spectra and estimate black hole mass fr…

2006 The Astrophysical Journal
eHST 175
Anisotropic Turbulent Spectra in the Terrestrial Magnetosheath as Seen by the Cluster Spacecraft
DOI: 10.1103/PhysRevLett.96.075002 Bibcode: 2006PhRvL..96g5002S

Balogh, A.; Belmont, G.; Sahraoui, F. +3 more

Here we report the first three-dimensional spatial spectrum of the low frequency magnetic turbulence obtained from the four Cluster spacecraft in the terrestrial magnetosheath close to the magnetopause. We show that the turbulence is compressible and dominated by mirror structures, its energy is injected at a large scale kρ∼0.3 (l∼2000 km) via a m…

2006 Physical Review Letters
Cluster 175
The Large-Scale and Small-Scale Clustering of Lyman Break Galaxies at 3.5<=z<=5.5 from the GOODS Survey
DOI: 10.1086/500387 Bibcode: 2006ApJ...642...63L

Ouchi, Masami; Dickinson, Mark; Ferguson, Henry C. +4 more

We report on the angular correlation function of Lyman break galaxies (LBGs) at z~4 and 5 from deep samples obtained from the Great Observatories Deep Origins Survey (GOODS). As for LBGs at z~3, the shape of w(θ) of the GOODS LBGs is well approximated by a power law with a slope β~0.6 at angular separation θ>=10". The clustering strength of the…

2006 The Astrophysical Journal
eHST 175
The Rest-Frame Far-Ultraviolet Morphologies of Star-forming Galaxies at z ~ 1.5 and 4
DOI: 10.1086/497950 Bibcode: 2006ApJ...636..592L

Ferguson, Henry C.; Giavalisco, Mauro; Lotz, Jennifer M. +2 more

We apply a new approach to quantifying galaxy morphology and identifying galaxy mergers to the rest-frame far-ultraviolet images of 82 z~4 Lyman break galaxies (LBGs) and 55 1.2<z<1.8 emission-line galaxies in the GOODS and Ultra Deep Field survey. We compare the distributions of the Gini coefficient (G), the second-order moment of the brigh…

2006 The Astrophysical Journal
eHST 172