output
19922026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2010Show all

57 papers · 1 filter

astro-ph.IM2010★ 112 cited

The Cosmic Origins Spectrograph: On-Orbit Instrument Performance

S. Osterman, J. Green, C. Froning +31

The Cosmic Origins Spectrograph (COS) was installed in the Hubble Space Telescope in May, 2009 as part of Servicing Mission 4 to provide high sensitivity, medium and low resolution…

astro-ph.HE2010★ 11 cited

Confirmation of IGR J01363+6610 as a Be X-ray binary with very low quiescent X-ray luminosity

John A. Tomsick, Craig Heinke, Jules Halpern +4

The field containing the candidate High Mass X-ray Binary IGR J01363+6610 was observed by XMM-Newton on 2009 July 31 for 28 ks. A Be star was previously suggested as the possible c…

astro-ph.HE2010★ 17 cited

Suzaku observes weak flares from IGR J17391-3021 representing a common low-activity state in this SFXT

A. Bodaghee, J. A. Tomsick, J. Rodriguez +4

We present an analysis of a 37-ks observation of the supergiant fast X-ray transient (SFXT) IGR J17391-3021 (=XTE J1739-302) gathered with Suzaku. The source evolved from quiescenc…

astro-ph.SR2010★ 398 cited

The Exoplanet Orbit Database

Jason T Wright, Onsi Fakhouri, Geoffrey W. Marcy +8

We present a database of well determined orbital parameters of exoplanets. This database comprises spectroscopic orbital elements measured for 427 planets orbiting 363 stars from r…

astro-ph.SR2010★ 36 cited

Imaging Spectroscopy of a White-Light Solar Flare

J. C. Martinez Oliveros, S. Couvidat, J. Schou +4

We report observations of a white-light solar flare (SOL2010-06-12T00:57, M2.0) observed by the Helioseismic Magnetic Imager (HMI) on the Solar Dynamics Observatory (SDO) and the R…

astro-ph.SR2010★ 18 cited

RXTE and XMM observations of intermediate polar candidates

O. W. Butters, A. J. Norton, K. Mukai +1

Aims. To determine the credentials of nine candidate intermediate polars in order to confirm whether or not they are magnetic cataclysmic variables. Methods. Frequency analysis of…

astro-ph.CO2010★ 23 cited

The geometry of the filamentary environment of galaxy clusters

Yookyung Noh, J. D. Cohn

We construct a filament catalogue using an extension of the halo based filament finder of Zhang et al.(2009), in a 250 Mpc/h side N-body simulation, and study the properties of fil…

astro-ph.EP2010

System Geometries and Transit / Eclipse Probabilities

Kaspar von Braun, Stephen R. Kane, Suvrath Mahadevan +3

Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar planets. Long-period transiting planets allow insight into plane…

astro-ph.HE2010★ 114 cited

Search for Gravitational Wave Bursts from Six Magnetars

J. Abadie, B. P. Abbott, R. Abbott +765

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized b…

astro-ph.EP2010★ 102 cited

The NASA-UC Eta-Earth Program: III. A Super-Earth orbiting HD 97658 and a Neptune-mass planet orbiting Gl 785

Andrew W. Howard, John Asher Johnson, Geoffrey W. Marcy +7

We report the discovery of planets orbiting two bright, nearby early K dwarf stars, HD 97658 and Gl 785. These planets were detected by Keplerian modelling of radial velocities mea…

physics.space-ph2010★ 113 cited

STEREO and Wind observations of a fast ICME flank triggering a prolonged geomagnetic storm on 5-7 April 2010

Christian Möstl, Manuela Temmer, Tanja Rollett +6

On 5 April 2010 an interplanetary (IP) shock was detected by the Wind spacecraft ahead of Earth, followed by a fast (average speed 650 km/s) IP coronal mass ejection (ICME). During…

astro-ph.SR2010★ 15 cited

Flaring Solar Hale Sector Boundaries

Leif Svalgaard, Iain G. Hannah

Magnetic fields and the occurrence of flares and microflares are strongly concentrated near that portion (the Hale boundary) in each solar hemisphere where the change in magnetic s…

astro-ph.SR2010★ 5 cited

GEANT4 Simulations of Gamma-Ray Emission from Accelerated Particles in Solar Flares

Shichao Tang, David M. Smith

Gamma-ray spectroscopy provides diagnostics of particle acceleration in solar flares, but care must be taken when interpreting the spectra due to effects of the angular distributio…

astro-ph.EP2010★ 173 cited

The Oblique Orbit of the Super-Neptune HAT-P-11b

Joshua N. Winn, John Asher Johnson, Andrew W. Howard +6

We find the orbit of the Neptune-sized exoplanet HAT-P-11b to be highly inclined relative to the equatorial plane of its host star. This conclusion is based on spectroscopic observ…

astro-ph.GA2010★ 40 cited

O vi in the local interstellar medium

M. A. Barstow, D. D. Boyce, B. Y. Welsh +2

We report the results of a search for O VI absorption in the spectra of 80 hot DA white dwarfs observed by the FUSE satellite. We have carried out a detailed analysis of the radial…

astro-ph.SR2010★ 51 cited

Constraining the hard X-ray properties of the quiet Sun with new RHESSI observations

I. G. Hannah, H. S. Hudson, G. J. Hurford +1

We present new RHESSI upper limits in the 3-200 keV energy range for solar hard X-ray emission in the absence of flares and active regions, i.e. the quiet Sun, using data obtained…

astro-ph.HE2010★ 83 cited

Broad-band study with Suzaku of the magnetar class

Teruaki Enoto, Kazuhiro Nakazawa, Kazuo Makishima +3

Broad-band (0.8-70 keV) spectra of the persistent X-ray emission from 9 magnetars were obtained with Suzaku, including 3 objects in apparent outburst. The soft X-ray component was…

astro-ph.HE2010★ 13 cited

A Tale of Two Current Sheets

Jonathan Arons

I outline a new model of particle acceleration in the current sheet separating the closed from the open field lines in the force-free model of pulsar magnetospheres, based on recon…

astro-ph.SR2010★ 159 cited

Reconstructing CMEs with Coordinated Imaging and In Situ Observations: Global Structure, Kinematics, and Implications for Space Weather Forecasting

Ying Liu, Arnaud Thernisien, Janet G. Luhmann +4

See the pdf for details

astro-ph.SR2010★ 24 cited

Scaling the energy conversion rate from magnetic field reconnection to different bodies

Forrest S. Mozer, Arthur Hull

Magnetic field reconnection is often invoked to explain electromagnetic energy conversion in planetary magnetospheres, stellar coronae, and other astrophysical objects. Because of…

physics.space-ph2010★ 138 cited

Anisotropy of Alfvénic Turbulence in the Solar Wind and Numerical Simulations

C. H. K. Chen, A. Mallet, T. A. Yousef +2

We investigate the anisotropy of Alfvénic turbulence in the inertial range of slow solar wind and in both driven and decaying reduced magnetohydrodynamic simulations. A direct comp…

astro-ph.SR2010★ 28 cited

Observations of radio pulses from CU Virginis

V. Ravi, G. Hobbs, D. Wickramasinghe +7

The magnetic chemically peculiar star CU Virginis is a unique astrophysical laboratory for stellar magnetospheres and coherent emission processes. It is the only known main sequenc…

astro-ph.GA2010★ 4 cited

Far-ultraviolet Emission-line Morphologies of the Supernova Remnant G65.3+5.7

I. -J. Kim, K. -I. Seon, K. -W. Min +3

We present the first far-ultraviolet (FUV) emission-line morphologies of the whole region of the supernova remnant (SNR) G65.3+5.7 using the FIMS/SPEAR data. The morphologies of th…

physics.atom-ph2010★ 22 cited

Measurement of anomalously strong emission from the 1s-9p transition in the spectrum of H-like phosphorus following charge exchange with molecular hydrogen

M. A. Leutenegger, P. Beiersdorfer, G. V. Brown +3

We have measured K-shell x-ray spectra of highly ionized argon and phosphorus following charge exchange with molecular hydrogen at low collision energy in an electron beam ion trap…