Minor Planet Observations [809 European Southern Observatory, La Silla]
Not Available
Elst, E. W. et al.
Advertised on:
9
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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Minor Planet Observations [304 Las Campanas Observatory]Not AvailableBenecchi, S. et al.
Advertised on:
92010 -
Mid-IR galaxy morphology from S4G (Buta+,The goals of the S4G project are described by Sheth et al. (2010, submitted). (1 data file).Buta, R. J. et al.
Advertised on:
92010 -
Mid-infrared Galaxy Morphology from the Spitzer Survey of Stellar Structure in Galaxies (S4G): The Imprint of the De Vaucouleurs Revised Hubble-Sandage Classification System at 3.6 μmSpitzer Space Telescope Infrared Array Camera imaging provides an opportunity to study all known morphological types of galaxies in the mid-IR at a depth significantly better than ground-based near-infrared and optical images. The goal of this study is to examine the imprint of the de Vaucouleurs classification volume in the 3.6 μm band, which isButa, Ronald J. et al.
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92010 -
Metal-line emission from the warm-hot intergalactic medium - I. Soft X-raysEmission lines from metals offer one of the most promising ways to detect the elusive warm-hot intergalactic medium (WHIM; 105 T 107K), which is thought to contain a substantial fraction of the baryons in the low-redshift Universe. We present predictions for the soft X-ray line emission from the WHIM using a subset of cosmological simulationsBertone, Serena et al.
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92010 -
MAXI J1659-152 is a BH candidateWe report on a pointed RXTE/PCA observation of the transient source MAXI J1659-152 (Atel #2873,#2874,#2875,#2877,#2880 GCN #11296,#11299, #11307 - initially referred to as GRB 100925A). The observation started on 28th September 2010 at 00:51:10 UT, for a total integration time of ~ 16 ks. We find strong variability in the X-ray light curve (averageKalamkar, M. et al.
Advertised on:
92010