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GMASS ultradeep spectroscopy of galaxies at z ~ 2 . I. The stellar metallicity
DOI: 10.1051/0004-6361:20078673 Bibcode: 2008A&A...479..417H

Berta, S.; Cimatti, A.; Daddi, E. +12 more

Context: Galaxy metallicities have been measured to redshift z∼2 by gas-phase oxygen abundances of the interstellar medium using the R{23} and N2 methods. Galaxy stellar metallicities provide crucial data for chemical evolution models but have not been assessed reliably much outside the local Universe.
Aims: We determine the iron-abundance, st…

2008 Astronomy and Astrophysics
eHST 62
A Test of Three Optical Flow Techniques—LCT, DAVE, and NAVE
DOI: 10.1086/592761 Bibcode: 2008ApJ...689..593C

Chae, Jongchul; Sakurai, Takashi

A time sequence of high-quality images currently produced by high-resolution observations either from the ground or in space may be utilized to determine the transverse flow field on the plane of the sky with the help of optical flow techniques. We have examined the performance of three different methods—a well-known technique called local correla…

2008 The Astrophysical Journal
Hinode 62
Observational Test of Coronal Magnetic Field Models. I. Comparison with Potential Field Model
DOI: 10.1086/588645 Bibcode: 2008ApJ...680.1496L

Liu, Yu; Lin, Haosheng

Recent advances have made it possible to obtain two-dimensional line-of-sight magnetic field maps of the solar corona from spectropolarimetric observations of the Fe XIII 1075 nm forbidden coronal emission line. Together with the linear polarization measurements that map the azimuthal direction of the coronal magnetic field projected in the plane …

2008 The Astrophysical Journal
SOHO 62
Is the Gini Coefficient a Stable Measure of Galaxy Structure?
DOI: 10.1086/591795 Bibcode: 2008ApJS..179..319L

Lisker, Thorsten

The Gini coefficient, a nonparametric measure of galaxy morphology, has recently taken up an important role in the automated identification of galaxy mergers. I present a critical assessment of its stability, based on a comparison of HST ACS imaging data from the GOODS and UDF surveys. Below a certain signal-to-noise level, the Gini coefficient de…

2008 The Astrophysical Journal Supplement Series
eHST 62
Impact effects from small size meteoroids and space debris
DOI: 10.1016/j.asr.2007.09.007 Bibcode: 2008AdSpR..41.1123D

Drolshagen, Gerhard

When the impact risk from meteoroids and orbital debris is assessed the main concern is usually structural damage. With their high impact velocities of typically 10 20 km/s millimeter or centimeter sized objects can puncture pressure vessels and other walls or lead to destruction of complete subsystems or even whole spacecraft. Fortunately chances…

2008 Advances in Space Research
XMM-Newton 62
Conservation of open solar magnetic flux and the floor in the heliospheric magnetic field
DOI: 10.1029/2008GL035813 Bibcode: 2008GeoRL..3520108O

St. Cyr, O. C.; Owens, M. J.; Crooker, N. U. +5 more

The near-Earth heliospheric magnetic field intensity, |B|, exhibits a strong solar cycle variation, but returns to the same ``floor'' value each solar minimum. The current minimum, however, has seen |B| drop below previous minima, bringing in to question the existence of a floor, or at the very least requiring a re-assessment of its value. In this…

2008 Geophysical Research Letters
SOHO 62
Kinematic properties of solar coronal mass ejections: Correction for projection effects in spacecraft coronagraph measurements
DOI: 10.1029/2007JA012500 Bibcode: 2008JGRA..113.1104H

Howard, T. A.; Nandy, D.; Koepke, A. C.

One of the main sources of uncertainty in quantifying the kinematic properties of coronal mass ejections (CMEs) using coronagraphs is the fact that coronagraph images are projected into the sky plane, resulting in measurements which can differ significantly from their actual values. By identifying solar surface source regions of CMEs using X-ray a…

2008 Journal of Geophysical Research (Space Physics)
SOHO 62
Two-dimensional kinematics of SLACS lenses - I. Phase-space analysis of the early-type galaxy SDSSJ2321-097 at z ~ 0.1
DOI: 10.1111/j.1365-2966.2007.12784.x Bibcode: 2008MNRAS.384..987C

Treu, Tommaso; Czoske, Oliver; Koopmans, Léon V. E. +2 more

We present the first results of a combined VLT VIMOS integral-field unit and Hubble Space Telescope (HST)/ACS study of the early-type lens galaxy SDSSJ2321-097 at z = 0.0819, extending kinematic studies to a look-back time of 1Gyr. This system, discovered in the Sloan Lens ACS Survey, has been observed as part of a VLT Large Programme with the goa…

2008 Monthly Notices of the Royal Astronomical Society
eHST 62
XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007
DOI: 10.1051/0004-6361:200810100 Bibcode: 2008A&A...489..327H

Pietsch, W.; Haberl, F.; Eger, P.

Aims: We analysed eight XMM-Newton observations toward the Small Magellanic Cloud (SMC), performed between October 2006 and June 2007, to investigate high mass X-ray binary systems.
Methods: We produced images from the European Photon Imaging Cameras (EPIC) and extracted X-ray spectra and light curves in different energy bands from sources tha…

2008 Astronomy and Astrophysics
XMM-Newton 61
X-Ray and Near-IR Variability of the Anomalous X-Ray Pulsar 1E 1048.1-5937: From Quiescence Back to Activity
DOI: 10.1086/528368 Bibcode: 2008ApJ...677..503T

Kaspi, Victoria M.; Bassa, Cees; Woods, Peter M. +3 more

We report on new and archival X-ray and near-IR observations of the anomalous X-ray pulsar 1E 1048.1-5937 performed between 2001 and 2007 with the Rossi X-Ray Telescope Explorer (RXTE), the Chandra X-Ray Observatory, the Swift Gamma-Ray Burst Explorer, the Hubble Space Telescope (HST), and the Very Large Telescope. Monitoring with RXTE revealed th…

2008 The Astrophysical Journal
XMM-Newton eHST 61