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The eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-III
- S. Alam, F. D. Albareti, Key Laboratory of Optical Astronomy
- Physics
- 5 January 2015
The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical…
THEM-σ ANDM-LRELATIONS IN GALACTIC BULGES, AND DETERMINATIONS OF THEIR INTRINSIC SCATTER
- K. Gultekin, D. Richstone, Universit'e libre de Bruxelles
- PhysicsThe Astrophysical Journal
- 27 March 2009
We derive improved versions of the relations between supermassive black hole mass (M BH) and host-galaxy bulge velocity dispersion (σ) and luminosity (L; the M-σ and M-L relations), based on 49 M BH…
Critical transitions in nature and society
- Anthony J. Dellureficio, N. Packard, California
- HistoryChoice Reviews Online
- 1 November 2009
“voluntary animal motion” interested physicians, scholars, and philosophers throughout history for a variety of purposes such as relating “voluntary motion” to the soul and understanding medical…
The AKARI/IRC mid-infrared all-sky survey
- D. Ishihara, T. Onaka, Sony Co. Ltd.
- Physics
- 1 March 2010
Context. AKARI is the first Japanese astronomical satellite dedicated to infrared astronomy. One of the main purposes of AKARI is the all-sky survey performed with six infrared bands between 9 μ m…
KEPLER'S FIRST ROCKY PLANET: KEPLER-10b*
- N. Batalha, W. Borucki, High Altitude Observatory
- Physics, Geology
- 3 February 2011
NASA's Kepler Mission uses transit photometry to determine the frequency of Earth-size planets in or near the habitable zone of Sun-like stars. The mission reached a milestone toward meeting that…
PLANETARY CANDIDATES OBSERVED BY KEPLER. III. ANALYSIS OF THE FIRST 16 MONTHS OF DATA
- N. Batalha, J. Rowe, Georgia State University
- Physics, Geology
- 27 February 2012
New transiting planet candidates are identified in 16 months (2009 May-2010 September) of data from the Kepler spacecraft. Nearly 5000 periodic transit-like signals are vetted against astrophysical…
CANDELS: The Progenitors of Compact Quiescent Galaxies at z ~ 2
We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to track the evolution of structure and activity of massive (M > 1010 M ?) galaxies at redshifts z =…
High-Velocity Clouds: Building Blocks of the Local Group
- L. Blitz, D. Spergel, Leiden University
- Physics
- 20 March 1998
We suggest that the high-velocity clouds (HVCs) are large clouds, with typical diameters of 25 kpc, containing 3×107 M☉ of neutral gas and 3×108 M☉ of dark matter, falling onto the Local Group;…
Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array
- A. Lidz, O. Zahn, M. McQuinn, M. Zaldarriaga, Lars Hernquist Harvard-CfA, Berkeley
- Physics
- 27 November 2007
We forecast the sensitivity with which the Murchison Widefield Array (MWA) can measure the 21 cm power spectrum of cosmic hydrogen. The MWA is sensitive to roughly a decade in scale (wavenumbers of…
Galaxy Zoo: the dependence of morphology and colour on environment
- S. Bamford, R. Nichol, Fingerprint Digital Media
- Physics
- 16 May 2008
We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 105 objects from Galaxy Zoo, the largest sample of visually classified morphologies…
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