Erratum: "Dark Matter Decay and Annihilation in the Local Universe: Clues from Fermi" (2011, ApJ, 726, L6)
Not Available
Cuesta, A. J. et al.
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2012
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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EROs in Groth Strip (Hempel+, 2011)We have selected a sample of extremely red galaxies (EROs) from the GOYA Survey (Balcells et al., 2002INGN....6...11B). This is a combined Ks selected catalogue covering the Groth-Westphal strip (~155arcmin2) in four optical bands, U, B, F606W and F814W, as well as J, Ks in the NIR. (2 data files).Hempel, A. et al.
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Dynamical evolution of a bulge in an N-body model of the Milky WayThe detailed dynamical structure of the bulge in the Milky Way is currently under debate. Although kinematics of the bulge stars can be well reproduced by a boxy-bulge, the possible existence of a small embedded classical bulge can not be ruled out. We study the dynamical evolution of a small classical bulge in a model of the Milky Way using a selfSaha, K. et al.
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Dissecting Early-type Dwarf Galaxies into Their Multiple ComponentsEarly-type dwarf galaxies, once believed to be simple systems, have recently been shown to exhibit an intriguing diversity in structure and stellar content. To analyze this further, we started the SMAKCED project (Stellar content, MAss and Kinematics of Cluster Early-type Dwarfs, http://www.smakced.net) and obtained deep H-band images for 101 earlyJanz, J. et al.
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Detection of the γ-Ray Binary LS I +61°303 in a Low-flux State at Very High Energy γ-Rays with the MAGIC Telescopes in 2009We present very high energy (E > 100 GeV) γ-ray observations of the γ-ray binary system LS I +61°303 obtained with the MAGIC stereo system between 2009 October and 2010 January. We detect a 6.3σ γ-ray signal above 400 GeV in the combined data set. The integral flux above an energy of 300 GeV is F(E > 300 GeV) = (1.4 ± 0.3stat ± 0.4syst) × 10-12 cmAleksić, J. et al.
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