Search Publications

Aperture synthesis imaging of the carbon AGB star R Sculptoris. Detection of a complex structure and a dominating spot on the stellar disk
DOI: 10.1051/0004-6361/201630214 Bibcode: 2017A&A...601A...3W

de Gregorio-Monsalvo, I.; Eriksson, K.; Lindqvist, M. +16 more


Aims: We present near-infrared interferometry of the carbon-rich asymptotic giant branch (AGB) star R Sculptoris (R Scl).
Methods: We employ medium spectral resolution K-band interferometry obtained with the instrument AMBER at the Very Large Telescope Interferometer (VLTI) and H-band low spectral resolution interferometric imaging obser…

2017 Astronomy and Astrophysics
ISO 43
Identification of Young Stellar Variables with KELT for K2. I. Taurus Dippers and Rotators
DOI: 10.3847/1538-4357/aa8c78 Bibcode: 2017ApJ...848...97R

Cargile, Phillip A.; Pepper, Joshua; Stassun, Keivan G. +13 more

One of the most well-studied young stellar associations, Taurus-Auriga, was observed by the extended Kepler mission, K2, in the spring of 2017. K2 Campaign 13 (C13) is a unique opportunity to study many stars in this young association at high photometric precision and cadence. Using observations from the Kilodegree Extremely Little Telescope (KELT…

2017 The Astrophysical Journal
Gaia 43
A gravitationally boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224
DOI: 10.1093/mnras/stx245 Bibcode: 2017MNRAS.467.3306S

Kneib, J. -P.; Richard, Johan; Smail, Ian +3 more

We present a Very Large Telescope/Multi Unit Spectroscopic Explorer (MUSE) survey of lensed high-redshift galaxies behind the z = 0.77 cluster RCS 0224-0002. We study the detailed internal properties of a highly magnified (µ ∼ 29) z = 4.88 galaxy seen through the cluster. We detect widespread nebular C IV λλ1548,1551 Å emission from this gal…

2017 Monthly Notices of the Royal Astronomical Society
eHST 43
Broad-band X-ray spectral analysis of the Seyfert 1 galaxy GRS 1734-292
DOI: 10.1093/mnras/stw3301 Bibcode: 2017MNRAS.466.4193T

Harrison, F. A.; Stern, D.; Bianchi, S. +14 more

We discuss the broad-band X-ray spectrum of GRS 1734-292 obtained from non-simultaneous XMM-Newton and NuSTAR (Nuclear Spectroscopic Telescope Array) observations, performed in 2009 and 2014, respectively. GRS1734-292 is a Seyfert 1 galaxy, located near the Galactic plane at z = 0.0214. The NuSTAR spectrum (3-80 keV) is dominated by a primary powe…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 43
The Philae lander mission and science overview
DOI: 10.1098/rsta.2016.0248 Bibcode: 2017RSPTA.37560248B

Krüger, Harald; Bibring, Jean-Pierre; Mottola, Stefano +12 more

The Philae lander accomplished the first soft landing and the first scientific experiments of a human-made spacecraft on the surface of a comet. Planned, expected and unexpected activities and events happened during the descent, the touch-downs, the hopping across and the stay and operations on the surface. The key results were obtained during 12-…

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 43
EMPIRE: A robust empirical reconstruction of solar irradiance variability
DOI: 10.1002/2016JA023733 Bibcode: 2017JGRA..122.3888Y

Solanki, S. K.; Yeo, K. L.; Krivova, N. A.

We present a new empirical model of total and spectral solar irradiance (TSI and SSI) variability entitled EMPirical Irradiance REconstruction (EMPIRE). As with existing empirical models, TSI and SSI variability is given by the linear combination of solar activity indices. In empirical models, UV SSI variability is usually determined by fitting th…

2017 Journal of Geophysical Research (Space Physics)
SOHO 43
Retrieving cloud, dust and ozone abundances in the Martian atmosphere using SPICAM/UV nadir spectra
DOI: 10.1016/j.pss.2017.04.011 Bibcode: 2017P&SS..142....9W

Vandaele, A. C.; Montmessin, F.; Willame, Y. +4 more

We present the retrieval algorithm developed to analyse nadir spectra from SPICAM/UV aboard Mars-Express. The purpose is to retrieve simultaneously several parameters of the Martian atmosphere and surface: the dust optical depth, the ozone total column, the cloud opacity and the surface albedo. The retrieval code couples the use of an existing com…

2017 Planetary and Space Science
ExoMars-16 MEx 43
Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46
DOI: 10.3847/2041-8213/aa71ad Bibcode: 2017ApJ...841L..21H

Tamura, Yoichi; Kohno, Kotaro; Suzuki, Tomoko L. +7 more

We report a survey of molecular gas in galaxies in the XMMXCS J2215.9-1738 cluster at z = 1.46. We have detected emission lines from 17 galaxies within a radius of R 200 from the cluster center, in Band 3 data of the Atacama Large Millimeter/submillimeter Array, with a coverage of 93-95 GHz in frequency and 2.33 arcmin2 in sp…

2017 The Astrophysical Journal
eHST 43
The pebbles/boulders size distributions on Sais: Rosetta's final landing site on comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx1620 Bibcode: 2017MNRAS.469S.636P

Jorda, L.; Lamy, P. L.; Lara, L. M. +53 more

By using the imagery acquired by the Optical, Spectroscopic, and Infrared Remote Imaging System Wide-Angle Camera (OSIRIS WAC), we prepare a high-resolution morphological map of the Rosetta Sais final landing site, characterized by an outcropping consolidated terrain unit, a coarse boulder deposit and a fine particle deposit. Thanks to the 0.014 m…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 43
Statistical Detection of the He II Transverse Proximity Effect: Evidence for Sustained Quasar Activity for >25 Million Years
DOI: 10.3847/1538-4357/aa83ac Bibcode: 2017ApJ...847...81S

Hennawi, Joseph F.; Prochaska, J. Xavier; Crighton, Neil H. M. +2 more

The He II transverse proximity effect—enhanced He II {Ly}α transmission in a background sightline caused by the ionizing radiation of a foreground quasar—offers a unique opportunity to probe the morphology of quasar-driven He II reionization. We conduct a comprehensive spectroscopic survey to find z∼ 3 quasars in the foreground of 22 background qu…

2017 The Astrophysical Journal
eHST 43