Search Publications

HD 131861, a Double-Line Spectroscopic Triple System
DOI: 10.1086/507890 Bibcode: 2006AJ....132.1910F

Henry, Gregory W.; Pourbaix, D.; Fekel, Francis C. +1 more

Our red-wavelength spectroscopic observations of HD 131861, a previously known single-line multiple system, span 20 years. Now lines of two components, the short-period F5 V primary and G8 V secondary, have been detected. The inner orbit is circular with a period of 3.5507439 days, while the outer orbit of the system has a period of 1642 days or 4…

2006 The Astronomical Journal
Hipparcos 2
The Bright Ages Survey. I. Imaging Data
DOI: 10.1086/499095 Bibcode: 2006ApJ...638..603C

Salim, Samir; Rich, R. Michael; Frogel, Jay A. +3 more

This is the first paper in a series presenting and analyzing data for a K-selected sample of galaxies collected in order to identify and study galaxies at moderate to high redshift in rest-wavelength optical light. The sample contains 842 objects over six separate fields covering 75.6 arcmin2 down to K=20-20.5. We combine the K band wit…

2006 The Astrophysical Journal
eHST 2
Ground calibration of the XRS microcalorimeter onboard Suzaku
DOI: 10.1016/j.nima.2005.12.113 Bibcode: 2006NIMPA.559..617C

Ishisaki, Y.; Mitsuda, K.; Boyce, K. R. +13 more

The XRS microcalorimeter was launched in July 2005 as part of the Suzaku mission. It covers the energy band from 0.3 to 10 keV with a nearly constant energy resolution of 6 eV and a peak effective area of 200 cm 2 at 1.5 keV. The XRS will provide unprecedented throughput and resolving power, particularly at high energies and for extende…

2006 Nuclear Instruments and Methods in Physics Research A
Suzaku 2
Inferring the composition of the liquid surface on Titan at the Huygens probe landing site from Surface Science Package measurements
DOI: 10.1016/j.asr.2005.08.006 Bibcode: 2006AdSpR..38..794H

Lorenz, R. D.; Hagermann, A.; Leese, M. R. +5 more

With Huygens’ descent into Titan’s atmosphere drawing nearer, the composition and state of Titan’s surface remained largely unknown. The idea of a global ocean on Titan has become less popular over the last decade, though the possibility of lakes and seas has remained, and recently [Campbell, D.B., Black, G.J., Carter, L.M., Ostro, S.J. Radar evid…

2006 Advances in Space Research
Cassini 2
Diagnostics of the Heliospheric Interface: High Energy ENAs
Bibcode: 2006ISSIR...5..311C

Kallenbach, Reinald; Hilchenbach, Martin; Czechowski, Andrzej

Energetic neutral atoms (ENAs) detected near Earth's orbit in the energy range from a few to a few hundred keV/nucleon carry information about the ion acceleration and transport mechanisms in the distant heliosphere, processes that are sensitive to the magnetic field structure, turbulence, and the plasma flow pattern. We summarize here the ENA obs…

2006 ISSI Scientific Reports Series
SOHO 2
Performance verification of the Suzaku X-ray Spectrometer in the flight configuration
DOI: 10.1016/j.nima.2005.12.100 Bibcode: 2006NIMPA.559..614O

Ishisaki, Y.; Mitsuda, K.; Boyce, K. R. +12 more

The X-ray Spectrometer (XRS) is a high resolution, non-dispersive cryogenic detector on board the X-ray satellite, Suzaku (Astro-E2), which was successfully launched on July 10, 2005. The XRS achieves an energy resolution of 6 eV at 6 keV (FWHM) and covers a broad energy range of ∼0.07 10 keV. The XRS will enable powerful plasma diagnostics of a v…

2006 Nuclear Instruments and Methods in Physics Research A
Suzaku 2
An information-theoretical methodology for profile parameter estimation of solar coronal spectra
DOI: 10.1051/0004-6361:20054580 Bibcode: 2006A&A...455.1081N

Nakagawa, A.

Aims.An attempt is made to establish an information-theoretical methodology for profile parameter estimation of the spectral lines of the solar corona.
Methods: .In this formalism, "description lengths" of a target line profile are defined for every possible profile model and are used to identify the optimal one among possible models. To prope…

2006 Astronomy and Astrophysics
SOHO 2
Star formation in hosts of young radio galaxies
DOI: 10.1016/j.newar.2006.06.033 Bibcode: 2006NewAR..50..776L

O'Dea, C. P.; Labiano, A.; Baum, S. A. +2 more

We present near ultraviolet imaging with the Hubble Space Telescope Advanced Camera for Surveys, targeting young radio galaxies (gigahertz peaked spectrum and compact steep spectrum sources), in search of star formation regions in their hosts. We find near UV light which could be the product of recent star formation in eight of the nine observed s…

2006 New Astronomy Reviews
eHST 2
Fourier-resolved spectroscopy of AGN using XMM-Newton data
DOI: 10.1002/asna.200610642 Bibcode: 2006AN....327.1047P

Papadakis, I. E.; Kazanas, D.; Ioannou, Z.

% We present a brief account of the theory on which the novel method of `Fourier-resolved spectroscopy' is based. We summarize the results from the past application of this method to the study of Galactic Black Hole candidate sources and MCG-6-30-15, and we present new results from the Fourier-resolved spectroscopy of archival XMM-Newton data of f…

2006 Astronomische Nachrichten
XMM-Newton 2
Simulation of post-impact rotational changes through multi-dimensional parametrization
DOI: 10.1016/j.icarus.2006.07.014 Bibcode: 2006Icar..185...83G

Gauchez, Damien; Souchay, Jean

In this paper we propose firstly a full parametrization of an impact on a target body considered as ellipsoidal, including several geometrical parameters which are generally not included. Then we construct a more detailed and complete theoretical model of the rotational changes of the target body arising from a single impact, by taking into accoun…

2006 Icarus
Rosetta 2