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The SAURON project - X. The orbital anisotropy of elliptical and lenticular galaxies: revisiting the (V/σ, ɛ) diagram with integral-field stellar kinematics
DOI: 10.1111/j.1365-2966.2007.11963.x Bibcode: 2007MNRAS.379..418C

Krajnović, Davor; Emsellem, Eric; van de Ven, Glenn +11 more

We analyse the orbital distribution of elliptical (E) and lenticular (S0) galaxies using SAURON integral-field stellar kinematics within about one effective (half-light) radius. We construct the anisotropy diagram, which relates the ratio of the ordered and random motion in a galaxy (V/σ) to its observed ellipticity (ɛ), for the 48 E/S0 galaxies f…

2007 Monthly Notices of the Royal Astronomical Society
eHST 514
Star Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law
DOI: 10.1086/522300 Bibcode: 2007ApJ...671..333K

Gordon, Karl D.; Bot, Caroline; Calzetti, Daniela +20 more

We have studied the relationship between the star formation rate (SFR), surface density, and gas surface density in the spiral galaxy M51a (NGC 5194), using multiwavelength data obtained as part of the Spitzer Infrared Nearby Galaxies Survey (SINGS). We introduce a new SFR index based on a linear combination of Hα emission-line and 24 µm con…

2007 The Astrophysical Journal
eHST 508
The Process of Tholin Formation in Titan’s Upper Atmosphere
DOI: 10.1126/science.1139727 Bibcode: 2007Sci...316..870W

Coates, A. J.; Young, D. T.; Waite, J. H. +4 more

Titan’s lower atmosphere has long been known to harbor organic aerosols (tholins) presumed to have been formed from simple molecules, such as methane and nitrogen (CH4 and N2). Up to now, it has been assumed that tholins were formed at altitudes of several hundred kilometers by processes as yet unobserved. Using measurements …

2007 Science
Cassini 501
Strong size evolution of the most massive galaxies since z ∼ 2
DOI: 10.1111/j.1365-2966.2007.12388.x Bibcode: 2007MNRAS.382..109T

Cooper, M. C.; Ellis, Richard S.; Trujillo, Ignacio +3 more

Using the combined capabilities of the large near-infrared Palomar/DEEP-2 survey, and the superb resolution of the Advanced Camera for Surveys HST camera, we explore the size evolution of 831 very massive galaxies (M≥ 1011h-270 M) since z~ 2. We split our sample according to their light conc…

2007 Monthly Notices of the Royal Astronomical Society
eHST 477
Radio Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
DOI: 10.1086/511972 Bibcode: 2007ApJ...658..815S

Stawarz, Łukasz; Sikora, Marek; Lasota, Jean-Pierre

We investigate how the total radio luminosity of AGN-powered radio sources depends on their accretion luminosity and the central black hole mass. Our studies cover about 7 orders of magnitude in accretion luminosity (expressed in Eddington units, i.e., as Eddington ratios) and the full range of AGN black hole masses. We find that AGNs form two dis…

2007 The Astrophysical Journal
eHST 472
The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters without Previous Hubble Space Telescope Photometry
DOI: 10.1086/511979 Bibcode: 2007AJ....133.1658S

Anderson, Jay; Dotter, Aaron; Sarajedini, Ata +10 more

We present the first results of a large Advanced Camera for Surveys (ACS) survey of Galactic globular clusters. This Hubble Space Telescope (HST) Treasury project is designed to obtain photometry with S/N (signal-to-noise ratio) gtrsim10 for main-sequence stars with masses gtrsim0.2 Modot in a sample of globulars using the ACS Wide Fiel…

2007 The Astronomical Journal
eHST 462
COSMOS: Hubble Space Telescope Observations
DOI: 10.1086/516580 Bibcode: 2007ApJS..172...38S

Kneib, J. -P.; Aussel, H.; Daddi, E. +52 more

The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high-resolution imaging. Here we review the characteristics of the HST imaging with the Advanced Camera for Surveys (ACS) and parallel observations with NICMOS and WFPC2. A square field (1.8 deg

2007 The Astrophysical Journal Supplement Series
eHST 462
The lakes of Titan
DOI: 10.1038/nature05438 Bibcode: 2007Natur.445...61S

Lorenz, R. D.; Stiles, B.; Kelleher, K. +35 more

The surface of Saturn's haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface. Initial visible and radar imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing liquids have existed on the surface. Here we provide definitive…

2007 Nature
Cassini 442
The Sloan Digital Sky Survey Quasar Catalog. IV. Fifth Data Release
DOI: 10.1086/518474 Bibcode: 2007AJ....134..102S

Castander, Francisco J.; Brandt, W. N.; Shen, Yue +41 more

We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar Catalog. The catalog contains 77,429 objects; this is an increase of over 30,000 entries since the previous edition. The catalog consists of the objects in the SDSS Fifth Data Release that have luminosities larger than Mi=-22.0 (in a cosmology with H0

2007 The Astronomical Journal
XMM-Newton 428
The Infrared Camera (IRC) for AKARI -- Design and Imaging Performance
DOI: 10.1093/pasj/59.sp2.S401 Bibcode: 2007PASJ...59S.401O

Pearson, C. P.; Ohyama, Y.; Takagi, T. +25 more

The Infrared Camera (IRC) is one of two focal-plane instruments on the AKARI satellite. It is designed for wide-field deep imaging and low-resolution spectroscopy in the near- to mid-infrared (1.8-26.5'

2007 Publications of the Astronomical Society of Japan
AKARI 424