Search Publications

Automated Processing of LASCO Coronal Images: Spurious Point-Source-Filtering and Missing-Blocks Correction
DOI: 10.1007/s11207-013-0402-9 Bibcode: 2014SoPh..289.1433P

Llebaria, A.; Lamy, P.; Boclet, B. +1 more

We report on automated procedures for correcting the images of the LASCO coronagraph for i) spurious quasi-point-sources such as the impacts of cosmic rays, stars, and planets, and ii) the absence of signal due to transmission errors or dropouts, which results in blocks of missing information in the images. Correcting for these undesirable artifac…

2014 Solar Physics
SOHO 6
A mass threshold in the number density of passive galaxies at z ~ 2
DOI: 10.1051/0004-6361/201322301 Bibcode: 2014A&A...571A..99S

Giavalisco, M.; McLure, R. J.; Dunlop, J. S. +17 more

The process that quenched star formation in galaxies at intermediate and high redshifts is still the subject of considerable debate. One way to investigate this puzzling issue is to study the number density of quiescent galaxies at z ≃ 2 and its dependence on mass. Here we present the results of a new study based on very deep Ks-band im…

2014 Astronomy and Astrophysics
eHST 6
The radio-loud AGN population at z ≳ 1 in the COSMOS field. I. selection and spectral energy distributions
DOI: 10.1051/0004-6361/201423906 Bibcode: 2014A&A...567A..76B

Chiaberge, Marco; Capetti, Alessandro; Baldi, Ranieri D. +1 more

We select a sample of radio galaxies at high redshifts (z ≳ 1) in the COSMOS field by cross-matching optical and infrared (IR) images with the FIRST radio data. The aim of this study is to explore the high-z radio-loud (RL) active galactic nuclei (AGN) population at much lower luminosities than the classical samples of distant radio sources, which…

2014 Astronomy and Astrophysics
eHST 6
X-ray Flares Observed from Six Young Stars Located in the Region of Star Clusters NGC 869 and IC 2602
DOI: 10.1007/s12036-014-9297-6 Bibcode: 2014JApA...35...39B

Pandey, J. C.; Singh, K. P.; Kumar, Brijesh +2 more

We present, for the first time, an analysis of seven intense X-ray flares observed from six stars (LAV 796, LAV 1174, SHM2002 3734, 2MASS 02191082+5707324, V553 Car, V557 Car). These stars are located in the region of young open star clusters NGC 869 and IC 2602. These flares detected in the XMM-Newton data show a rapid rise (10–40 min) and a slow…

2014 Journal of Astrophysics and Astronomy
XMM-Newton 6
Searching for small-scale diffuse emission around SGR 1806-20
DOI: 10.1016/j.jheap.2014.10.001 Bibcode: 2014JHEAp...3...41V

Tiengo, A.; Mereghetti, S.; Stella, L. +6 more

Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20 after its 2004 powerful giant flare. We study the possible extended X-ray emission at small scales around SGR 1806-20, in two observations by the High Resolution Camera Spectrometer (HRC-S) on board of the Chandra X-ray Observatory: in 2005, 115 days after the giant…

2014 Journal of High Energy Astrophysics
XMM-Newton 6
Analysis of Rosetta/VIRTIS spectra of earth using observations from ENVISAT/AATSR, TERRA/MODIS and ENVISAT/SCIAMACHY, and radiative-transfer simulations
DOI: 10.1016/j.pss.2013.06.012 Bibcode: 2014P&SS...90...37H

Oliva, F.; Irwin, P. G. J.; Capaccioni, F. +7 more

Rosetta, the Solar System cornerstone mission of ESA's Horizon 2000 programme, consists of an orbiter and a lander, and is due to arrive at the comet 67P/Churyumov-Gerasimenko in May 2014. Following its 2004 launch, Rosetta carried out a series of planetary fly-bys and gravitational assists. On these close fly-bys of the Earth, measurements were t…

2014 Planetary and Space Science
Rosetta 6
High-resolution absorption spectroscopy of the circumgalactic medium of the Milky Way
DOI: 10.1002/asna.201312013 Bibcode: 2014AN....335...92R

Richter, P.; Fox, A. J.; Bomans, D. +3 more

In this article we discuss the importance of high-resolution absorption spectroscopy for our understanding of the distribution and physical nature of the gaseous circumgalactic medium (CGM) that surrounds the Milky Way. Observational and theoretical studies indicate a high complexity of the gas kinematics and an extreme multi-phase nature of the C…

2014 Astronomische Nachrichten
eHST 6
Comparison of low-harmonics spectra and maps according to the WMAP and Planck space missions
DOI: 10.1134/S1990341314030092 Bibcode: 2014AstBu..69..330V

Verkhodanov, O. V.

We present a comparison of the angular power spectra and maps represented by the WMAP and Planck mission teams. The spectra are compared in the the multi pole range (2 ≤ ℓ ≤ 50). The ℓ =5, 7, 13, 29, 37, 41–46 harmonics have a discrepancy in the angular power spectra. The maps of the microwave background and their phase characteristics are studied…

2014 Astrophysical Bulletin
Planck 6
Herschel Observations of Circinus X-1 during Outburst and Quiescence
DOI: 10.1088/0004-6256/148/1/22 Bibcode: 2014AJ....148...22H

Harrison, Thomas E.; Gelino, Dawn M.; Buxton, Michelle +1 more

We have used the Photodetector Array Camera and Spectrometer and Spectral and Photometric Imaging REceiver instruments on the Herschel Space Observatory to observe Cir X-1 both in and out of outburst. We detected Cir X-1 during outburst at 70 µm. Unfortunately, a cold background source dominates Cir X-1 at longer wavelengths. We have assembl…

2014 The Astronomical Journal
Herschel 6
The location of Airy-0, the Mars prime meridian reference, from stereo photogrammetric processing of THEMIS IR imaging and digital elevation data
DOI: 10.1002/2014JE004678 Bibcode: 2014JGRE..119.2471D

Neukum, G.; Kirk, R. L.; Neumann, G. A. +7 more

The small crater Airy-0 was selected from Mariner 9 images to be the reference for the Mars prime meridian. Initial analyses in the year 2000 tied Viking Orbiter and Mars Orbiter Camera images of Airy-0 to the evolving Mars Orbiter Laser Altimeter global digital terrain model to update the location of Airy-0. Based upon this tie and radiometric tr…

2014 Journal of Geophysical Research (Planets)
MEx 6