Search Publications

Hα star formation rates in massive galaxies at z∼ 1
DOI: 10.1111/j.1365-2966.2011.20057.x Bibcode: 2012MNRAS.420.1061T

Weiner, Benjamin J.; Conselice, Christopher J.; Bauer, Amanda E. +4 more

We present a near-infrared spectroscopic study of a stellar mass selected sample of galaxies at z∼ 1 utilizing the Long-slit Intermediate Resolution Infrared Spectrograph multi-object spectrograph on the William Herschel Telescope. We detect continuum, and the Hα line for our sample, which is one of the better direct tracers of star formation in e…

2012 Monthly Notices of the Royal Astronomical Society
eHST 17
Dependence of kinematics on the age of stars in the solar neighborhood
DOI: 10.1134/S1063773712120031 Bibcode: 2012AstL...38..771G

Gontcharov, G. A.

The variations of kinematic parameters with age are considered for a sample of 15 402 thin-disk O-F stars with accurate α, δ, µ, and π > 3 mas from the Hipparcos catalogue and radial velocities from the PCRV catalogue. The ages have been calculated from the positions of the stars on the Hertzsprung-Russell diagram relative to the isochrones fro…

2012 Astronomy Letters
Hipparcos 17
Geometry of the 20 November 2003 magnetic cloud
DOI: 10.1029/2011JA016802 Bibcode: 2012JGRA..117.1101M

Park, Sung-Hong; Cho, Kyung-Suk; Kim, Yeon-Han +2 more

This study is an attempt to find a coherent interpretation of the link between the 20 November 2003 magnetic cloud (MC) and its solar source. Most previous studies agree on the orientation of the MC, but the orientation is nearly perpendicular to the axis of the post-eruption arcade (PEA) or the orientation of the neutral line in the solar source …

2012 Journal of Geophysical Research (Space Physics)
SOHO 17
Spectral comparison of weak short bursts to the persistent X-rays from the magnetar 1E 1547.0-5408 in its 2009 outburst
DOI: 10.1111/j.1365-2966.2012.22086.x Bibcode: 2012MNRAS.427.2824E

Sakamoto, T.; Enoto, T.; Makishima, K. +1 more

In 2009 January, the 2.1-s anomalous X-ray pulsar 1E 1547.0-5408 evoked intense burst activity. A follow-up Suzaku observation on January 28 recorded enhanced persistent emission in both soft and hard X-rays. Through a reanalysis of the same Suzaku data, 18 short bursts were identified in the X-ray events recorded by the Hard X-ray Detector (HXD) …

2012 Monthly Notices of the Royal Astronomical Society
Suzaku 17
Black-hole-Bulge Relationship of Post-starburst Quasars at z ~ 0.3
DOI: 10.1088/0004-637X/756/2/162 Bibcode: 2012ApJ...756..162H

Canalizo, Gabriela; Brotherton, Michael S.; Cales, Sabrina L. +2 more

The M BH* relation has been studied extensively for local galaxies, but to date there have been scarce few direct measurements of stellar velocity dispersions for systems beyond the local universe. We investigate black hole and host galaxy properties of six "post-starburst quasars" (PSQs) at z ~ 0.3. Spectra of these object…

2012 The Astrophysical Journal
eHST 17
Direct wind measurements from November 2007 in Venus' upper atmosphere using ground-based heterodyne spectroscopy of CO 2 at 10 µm wavelength
DOI: 10.1016/j.icarus.2011.03.019 Bibcode: 2012Icar..217..863S

Sornig, M.; Sonnabend, G.; Kroetz, P. +2 more

Between November 23 and 28, 2007, the Cologne Tuneable Heterodyne Infrared Spectrometer THIS was installed at the McMath-Pierce Solar Telescope (Kitt Peak, Arizona, USA) to determine zonal wind velocities and to estimate the subsolar-to-antisolar flow. We investigate dynamics in the upper atmosphere of Venus by measuring the Doppler shift of fully…

2012 Icarus
VenusExpress 17
Transiting exoplanets from the CoRoT space mission . XIX. CoRoT-23b: a dense hot Jupiter on an eccentric orbit
DOI: 10.1051/0004-6361/201117916 Bibcode: 2012A&A...537A..54R

Mazeh, T.; Aigrain, S.; Alonso, R. +40 more

We report the detection of CoRoT-23b, a hot Jupiter transiting in front of its host star with a period of 3.6314 ± 0.0001 days. This planet was discovered thanks to photometric data secured with the CoRoT satellite, combined with spectroscopic radial velocity (RV) measurements. A photometric search for possible background eclipsing binaries conduc…

2012 Astronomy and Astrophysics
CoRoT 17
A Strongly Lensed Massive Ultracompact Quiescent Galaxy at z ~ 2.4 in the COSMOS/UltraVISTA Field
DOI: 10.1088/0004-637X/761/2/142 Bibcode: 2012ApJ...761..142M

Franx, Marijn; Muzzin, Adam; Labbé, Ivo +14 more

We report the discovery of a massive ultracompact quiescent galaxy that has been strongly lensed into multiple images by a foreground galaxy at z = 0.960. This system was serendipitously discovered as a set of extremely Ks -bright high-redshift galaxies with red J - Ks colors using new data from the UltraVISTA YJHKs

2012 The Astrophysical Journal
eHST 17
Statistical model of electron pitch angle diffusion in the outer radiation belt
DOI: 10.1029/2012JA017826 Bibcode: 2012JGRA..117.8219A

Krasnoselskikh, V.; Breuillard, H.; Agapitov, O. +2 more

We calculated the bounce averaged electron pitch angle diffusion coefficients ? using the statistical characteristics of lower band chorus activity collected by the Cluster mission from 2001-2009. Nine years of Cluster observations provide the distributions of the θ angle between wave vectors and the background magnetic field; and the distribution…

2012 Journal of Geophysical Research (Space Physics)
Cluster 16
The X-ray warm absorber and nuclear obscuration in the Seyfert 1.8 galaxy ESO 113-G010
DOI: 10.1051/0004-6361/201218896 Bibcode: 2012A&A...542A..30M

Mehdipour, M.; Page, M. J.; Branduardi-Raymont, G.

We present the first analysis of the X-ray warm absorber and nuclear obscuration in the Seyfert 1.8 galaxy ESO 113-G010. We used archival data from a 100 ks XMM-Newtonobservation made in 2005. From high resolution spectroscopy analysis of the RGS data, we detect absorption lines originating from a warm absorber consisting of two…

2012 Astronomy and Astrophysics
AKARI INTEGRAL XMM-Newton 16