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Evolution of the Solar Activity over Time and Effects on Planetary Atmospheres. I. High-Energy Irradiances (1-1700 Å)
DOI: 10.1086/427977 Bibcode: 2005ApJ...622..680R

Güdel, Manuel; Guinan, Edward F.; Audard, Marc +1 more

We report on the results of the Sun in Time multiwavelength program (X-rays to UV) of solar analogs with ages covering ~0.1-7 Gyr. The chief science goals are to study the solar magnetic dynamo and to determine the radiative and magnetic properties of the Sun during its evolution across the main sequence. The present paper focuses on the latter go…

2005 The Astrophysical Journal
IUE eHST 688
Resolved Massive Star Clusters in the Milky Way and Its Satellites: Brightness Profiles and a Catalog of Fundamental Parameters
DOI: 10.1086/497429 Bibcode: 2005ApJS..161..304M

van der Marel, Roeland P.; McLaughlin, Dean E.

We present a database of structural and dynamical properties for 153 spatially resolved star clusters in the Milky Way, the Large and Small Magellanic Clouds, and the Fornax dwarf spheroidal. This database complements and extends others in the literature, such as those of Harris and Mackey & Gilmore. Our cluster sample comprises 50 ``young mas…

2005 The Astrophysical Journal Supplement Series
eHST 631
Luminosity-dependent evolution of soft X-ray selected AGN. New Chandra and XMM-Newton surveys
DOI: 10.1051/0004-6361:20042134 Bibcode: 2005A&A...441..417H

Hasinger, G.; Schmidt, M.; Miyaji, T.

We present new results on the cosmological evolution of unabsorbed (type-1) active galactic nuclei (AGN) selected in the soft (0.5-2 keV) X-ray band. From a variety of ROSAT, XMM-Newton and Chandra surveys we selected a total of ~1000 AGN with an unprecedented spectroscopic and photometric optical/NIR identification completeness. For the first tim…

2005 Astronomy and Astrophysics
XMM-Newton 609
Star counts in the Galaxy. Simulating from very deep to very shallow photometric surveys with the TRILEGAL code
DOI: 10.1051/0004-6361:20042352 Bibcode: 2005A&A...436..895G

Hatziminaoglou, E.; Girardi, L.; Groenewegen, M. A. T. +1 more

We describe TRILEGAL, a new populations synthesis code for simulating the stellar photometry of any Galaxy field. The code attempts to improve upon several technical aspects of star count models, by: dealing with very complete input libraries of evolutionary tracks; using a stellar spectral library to simulate the photometry in virtually any broad…

2005 Astronomy and Astrophysics
Hipparcos 604
Astrophysical parameters of Galactic open clusters
DOI: 10.1051/0004-6361:20042523 Bibcode: 2005A&A...438.1163K

Scholz, R. -D.; Piskunov, A. E.; Kharchenko, N. V. +2 more

We present a catalogue of astrophysical data for 520 Galactic open clusters. These are the clusters for which at least three most probable members (18 on average) could be identified in the ASCC-2.5, a catalogue of stars based on the Tycho-2 observations from the Hipparcos mission. We applied homogeneous methods and algorithms to determine angular…

2005 Astronomy and Astrophysics
Hipparcos 604
In situ measurements of the physical characteristics of Titan's environment
DOI: 10.1038/nature04314 Bibcode: 2005Natur.438..785F

Neubauer, F. M.; Rodrigo, R.; Barucci, M. A. +40 more

On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and pressure profiles were poorly constrained because of uncertainties in the detailed composition. The extent of atmospheric electricity (`lightning') was also hitherto unknown. Here we report t…

2005 Nature
Huygens 542
Wave acceleration of electrons in the Van Allen radiation belts
DOI: 10.1038/nature03939 Bibcode: 2005Natur.437..227H

Meredith, Nigel P.; Horne, Richard B.; Glauert, Sarah A. +11 more

The Van Allen radiation belts are two regions encircling the Earth in which energetic charged particles are trapped inside the Earth's magnetic field. Their properties vary according to solar activity and they represent a hazard to satellites and humans in space. An important challenge has been to explain how the charged particles within these bel…

2005 Nature
Cluster 493
Spitzer View on the Evolution of Star-forming Galaxies from z = 0 to z ~ 3
DOI: 10.1086/431894 Bibcode: 2005ApJ...630...82P

Papovich, Casey; Pérez-González, Pablo G.; Rieke, George H. +11 more

We use a 24 µm-selected sample containing more than 8000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric redshifts for most of the sources in our survey using a method based on empirically built templates spanning from ultraviolet to mid-infrared wavelengths. The accuracy o…

2005 The Astrophysical Journal
eHST 485
The Effective Temperature Scale of FGK Stars. II. Teff:Color:[Fe/H] Calibrations
DOI: 10.1086/430102 Bibcode: 2005ApJ...626..465R

Meléndez, Jorge; Ramírez, Iván

We present up-to-date metallicity-dependent temperature versus color calibrations for main-sequence and giant stars based on temperatures derived with the infrared flux method (IRFM). Seventeen colors in the photometric systems UBV, uvby, Vilnius, Geneva, RI(Cousins), DDO, Hipparcos-Tycho, and Two Micron All Sky Survey (2MASS) have been calibrated…

2005 The Astrophysical Journal
Hipparcos 485
Optimization of Starburst99 for Intermediate-Age and Old Stellar Populations
DOI: 10.1086/427866 Bibcode: 2005ApJ...621..695V

Leitherer, Claus; Vázquez, Gerardo A.

We have incorporated the latest release of the Padova models into the evolutionary synthesis code Starburst99. The Padova tracks were extended to include the full asymptotic giant branch (AGB) evolution until the final thermal pulse over the mass range 0.9-5 Msolar. With this addition, Starburst99 accounts for all stellar phases that co…

2005 The Astrophysical Journal
eHST 478