The small scale angular anisotropy at 145 GHz as seen by the Atacama Cosmology Telescope
Not Available
Hernandez-Monteagudo, C.
Advertised on:
2
2010
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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The quest for the solar g modesSolar gravity modes (or g modes)—oscillations of the solar interior on which buoyancy acts as the restoring force—have the potential to provide unprecedented inference on the structure and dynamics of the solar core, inference that is not possible with the well-observed acoustic modes (or p modes). The relative high amplitude of the g-modeAppourchaux, T. et al.
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22010 -
The optical counterpart of the new Fermi LAT flaring source J0109+6134 near the Galactic PlaneThe position of the recently discovered transient gamma-ray source J0109+6134 (ATEL #2414) lies within the footprints of the IPHAS (Drew et al. 2005, MNRAS, 362, 753; http://www.iphas.org) and UVEX (Groot et al. 2009, MNRAS, 399, 323) surveys of the northern Galactic plane. Paredes et al. (ATEL #2421) have already suggested an optical counterpartKnigge, C. et al.
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22010 -
The Minor Role of Gas-Rich Major Mergers in the Rise of Intermediate-Mass Early Types at z <= 1We study the evolution of galaxy structure since z ~ 1 to the present. From a Great Observatories Origins Deep Survey South (GOODS-S) multi-band catalog, we define (blue) luminosity- and mass-weighted samples, limited by MB = 1010 M sun, comprising 1122 and 987 galaxies, respectively. We extract early-type (ET; E/S0/Sa) and late-type (LT; Sb-Irr)López-Sanjuan, C. et al.
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22010 -
The Intergalactic Stellar Population from Mergers of Elliptical Galaxies with Dark Matter HalosWe present simulations of dry-merger encounters between pairs of elliptical galaxies with dark matter halos. The aim of these simulations is to study the intergalactic (IG) stellar populations produced in both parabolic and hyperbolic encounters. We model progenitor galaxies with total-to-luminous mass ratios MT /M L= 3 and 11. The initial mass ofGonzález-García, A. Cesar et al.
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22010 -
The huge (but forgotten) population of weak line galaxies in the SDSS: AGN or just retired galaxiesNot AvailableFernandes, R. C.
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22010