Search Publications

GOODS-Herschel: evidence of a UV extinction bump in galaxies at z > 1
DOI: 10.1051/0004-6361/201117264 Bibcode: 2011A&A...533A..93B

Magnelli, B.; Altieri, B.; Aussel, H. +16 more

Context. Dust attenuation curves in external galaxies are useful for studying their dust properties as well as interpreting their intrinsic spectral energy distributions. These functions are not very well known in the UV range whether at low or high redshift. In particular, the presence or absence of a UV bump at 2175 Å remains an open issue that …

2011 Astronomy and Astrophysics
Herschel eHST 81
Seasonal changes in Titan's meteorology
DOI: 10.1029/2010GL046266 Bibcode: 2011GeoRL..38.3203T

West, R. A.; Schaller, E. L.; McEwen, A. S. +5 more

The Cassini Imaging Science Subsystem has observed Titan for ∼1/4 Titan year, and we report here the first evidence of seasonal shifts in preferred locations of tropospheric methane clouds. South-polar convective cloud activity, common in late southern summer, has become rare. North-polar and northern mid-latitude clouds appeared during the approa…

2011 Geophysical Research Letters
Cassini 80
A Low Escape Fraction of Ionizing Photons of L > L* Lyman Break Galaxies at z = 3.3
DOI: 10.1088/0004-637X/736/1/41 Bibcode: 2011ApJ...736...41B

Fiore, F.; Castellano, M.; Pentericci, L. +12 more

We present an upper limit for the relative escape fraction (f rel esc) of ionizing radiation at z ~ 3.3 using a sample of 11 Lyman break galaxies (LBGs) with deep imaging in the U band obtained with the Large Binocular Camera, mounted on the prime focus of the Large Binocular Telescope. We selected 11 LBGs with secure redshif…

2011 The Astrophysical Journal
eHST 80
Iron line profiles in Suzaku spectra of bare Seyfert galaxies
DOI: 10.1111/j.1365-2966.2010.17852.x Bibcode: 2011MNRAS.411.2353P

Porquet, D.; Reeves, J. N.; Terashima, Y. +3 more

We methodically model the broad-band Suzaku spectra of a small sample of six 'bare' Seyfert galaxies: Ark 120, Fairall 9, MCG -02-14-009, Mrk 335, NGC 7469 and SWIFT J2127.4+5654. The analysis of bare Seyferts allows a consistent and physical modelling of active galactic nuclei due to a weak amount of any intrinsic warm absorption, removing the de…

2011 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 80
Electron Temperature Gradient Scale at Collisionless Shocks
DOI: 10.1103/PhysRevLett.107.215002 Bibcode: 2011PhRvL.107u5002S

Krasnoselskikh, Vladimir; Schwartz, Steven J.; Henley, Edmund +1 more

Shock waves are ubiquitous in space and astrophysics. They transform directed flow energy into thermal energy and accelerate energetic particles. The energy repartition is a multiscale process related to the spatial and temporal structure of the electromagnetic fields within the shock layer. While large scale features of ion heating are known, the…

2011 Physical Review Letters
Cluster 80
A tool for empirical forecasting of major flares, coronal mass ejections, and solar particle events from a proxy of active-region free magnetic energy
DOI: 10.1029/2009SW000537 Bibcode: 2011SpWea...9.4003F

Falconer, David; Barghouty, Abdulnasser F.; Khazanov, Igor +1 more

This paper describes a new forecasting tool developed for and currently being tested by NASA's Space Radiation Analysis Group (SRAG) at Johnson Space Center, which is responsible for the monitoring and forecasting of radiation exposure levels of astronauts. The new software tool is designed for the empirical forecasting of M- and X-class flares, c…

2011 Space Weather
SOHO 80
Hapke modeling of Rhea surface properties through Cassini-VIMS spectra
DOI: 10.1016/j.icarus.2011.05.010 Bibcode: 2011Icar..214..541C

Brown, R. H.; Buratti, B. J.; Clark, R. N. +8 more

The surface properties of the icy bodies in the saturnian system have been investigated by means of the Cassini-VIMS (Visual Infrared Mapping Spectrometer) hyperspectral imager which operates in the 0.35-5.1 µm wavelength range. In particular, we have analyzed 111 full disk hyperspectral images of Rhea ranging in solar phase between 0.08° an…

2011 Icarus
Cassini 80
Homologous Flares and Magnetic Field Topology in Active Region NOAA 10501 on 20 November 2003
DOI: 10.1007/s11207-010-9670-9 Bibcode: 2011SoPh..269...83C

Mandrini, C. H.; Schmieder, B.; Démoulin, P. +4 more

We present and interpret observations of two morphologically homologous flares that occurred in active region (AR) NOAA 10501 on 20 November 2003. Both flares displayed four homologous Hα ribbons and were both accompanied by coronal mass ejections (CMEs). The central flare ribbons were located at the site of an emerging bipole in the centre of the…

2011 Solar Physics
SOHO 80
Chromospheric Jet and Growing "Loop" Observed by Hinode: New Evidence of Fan-spine Magnetic Topology Resulting from Flux Emergence
DOI: 10.1088/0004-637X/728/2/103 Bibcode: 2011ApJ...728..103L

Liu, Wei; Berger, Thomas E.; Tarbell, Theodore D. +2 more

We present observations of a chromospheric jet and growing "loop" system that show new evidence of a fan-spine topology resulting from magnetic flux emergence. This event, occurring in an equatorial coronal hole on 2007 February 9, was observed by the Hinode Solar Optical Telescope in the Ca II H line in unprecedented detail. The predecessor of th…

2011 The Astrophysical Journal
Hinode SOHO 79
Hubble Space Telescope Observations of the Double-peaked Emission Lines in the Seyfert Galaxy Markarian 78: Mass Outflows from a Single Active Galactic Nucleus
DOI: 10.1088/0004-637X/727/2/71 Bibcode: 2011ApJ...727...71F

Kraemer, S. B.; Crenshaw, D. M.; Schmitt, H. R. +3 more

Previous ground-based observations of the Seyfert 2 galaxy Mrk 78 revealed a double set of emission lines, similar to those seen in several active galactic nuclei (AGNs) from recent surveys. Are the double lines due to two AGNs with different radial velocities in the same galaxy, or are they due to mass outflows from a single AGN? We present a stu…

2011 The Astrophysical Journal
eHST 79