Search Publications

In and out star formation in z 1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared
DOI: 10.1051/0004-6361/201629852 Bibcode: 2017A&A...599A..95G

Cimatti, A.; Daddi, E.; Béthermin, M. +18 more

We present a sample of 34 spectroscopically confirmed BzK-selected 1011M quiescent galaxies (pBzK) in the COSMOS field. The targets were initially observed with VIMOS on the VLT to facilitate the calibration of the photometric redshifts of massive galaxies at z ≳ 1.5. Here we describe the reduction and analysis of the data, …

2017 Astronomy and Astrophysics
eHST 24
Understanding Problem Forecasts of ISEST Campaign Flare-CME Events
DOI: 10.1007/s11207-017-1166-4 Bibcode: 2017SoPh..292..142W

Nitta, Nariaki; Webb, David

The goal of the International Study of Earth-affecting Solar Transients (ISEST) project as part of the Variability of the Sun and Its Terrestrial Impact (VarSITI) program is to understand the origin, evolution, and propagation of solar transients through the space between the Sun and Earth, and to improve our prediction capability for space weathe…

2017 Solar Physics
SOHO 24
The Optical-Mid-infrared Extinction Law of the l = 165° Sightline in the Galactic Plane: Diversity of the Extinction Law in the Diffuse Interstellar Medium
DOI: 10.3847/1538-4357/aa8db7 Bibcode: 2017ApJ...848..106W

Wang, Shu; de Grijs, Richard; Zhao, He +2 more

Understanding the effects of dust extinction is important to properly interpret observations. The optical total-to-selective extinction ratio, {R}V={A}V/E(B-V), is widely used to describe extinction variations in ultraviolet and optical bands. Since the {R}V=3.1 extinction curve adequately represents the average ex…

2017 The Astrophysical Journal
Planck 24
Plasma Environment around Comet 67P/Churyumov-Gerasimenko at Perihelion: Model Comparison with Rosetta Data
DOI: 10.3847/1538-3881/153/1/30 Bibcode: 2017AJ....153...30M

Altwegg, K.; Goetz, C.; Goldstein, R. +6 more

The plasma environment near comet 67P/Churyumov-Gerasimenko (67P/CG) is dynamically affected by various factors, including the incident solar wind and outgassing from the nucleus. The Rosetta spacecraft MAGnetometer (MAG) instrument observations near perihelion showed crossing events into a magnetic field-free region at about 170 km from the nucle…

2017 The Astronomical Journal
Rosetta 24
Revision of Stellar Intrinsic Colors in the Infrared by Spectroscopic Surveys
DOI: 10.3847/1538-3881/153/1/5 Bibcode: 2017AJ....153....5J

Jiang, Biwei; Zhao, He; Gao, Shuang +1 more

Intrinsic colors of normal stars are derived in the popularly used infrared bands involving the Two Micron All-Sky Survey/JHKS, Wide-field Infrared Survey Explorer, Spitzer/IRAC, and AKARI/S9W filters. Based on three spectroscopic surveys—LAMOST, RAVE, and APOGEE, stars are classified into groups of giants and dwarfs, as well as metal-n…

2017 The Astronomical Journal
AKARI 24
Geomorphology of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx1096 Bibcode: 2017MNRAS.469S..50B

Soderblom, J. M.; Sierks, H.; Vincent, J. -B. +10 more

We present a global geomorphological map of comet 67P/Churyumov-Gerasimenko (67P/C-G) using data acquired by the Rosetta Orbiter's OSIRIS Narrow Angle Camera. The images used in our study were acquired between 2014 August and 2015 May, before 67P/C-G passed through perihelion. Imagery of the Southern hemisphere was included in our study, allowing …

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 24
Quasilinear analysis of saturation properties of broadband whistler mode waves
DOI: 10.1002/2017GL074881 Bibcode: 2017GeoRL..44.8122T

Chen, L.; Liu, X.; Wang, S. +2 more

Saturation properties of parallel propagating broadband whistler mode waves are investigated using quasilinear theory. By assuming that the electron distribution stays bi-Maxwellian, we combine the previously obtained energy equation of quasilinear theory with wave equation to self-consistently model the excitation of broadband whistler waves. The…

2017 Geophysical Research Letters
Cluster 24
The Hard X-Ray Emission of the Blazar PKS 2155-304
DOI: 10.3847/1538-4357/aa95bc Bibcode: 2017ApJ...850..209G

Misra, R.; Dewangan, G. C.; Gaur, Haritma +4 more

The synchrotron peak of the X-ray bright High Energy Peaked Blazar PKS 2155-304 occurs in the UV-EUV region and hence its X-ray emission (0.6-10 keV) lies mostly in the falling part of the synchrotron hump. We aim to study the X-ray emission of PKS 2155-304 during different intensity states in 2009-2014 using the XMM-Newton satellite. We studied t…

2017 The Astrophysical Journal
XMM-Newton 24
Herschel survey and modelling of externally-illuminated photoevaporating protoplanetary disks
DOI: 10.1051/0004-6361/201629404 Bibcode: 2017A&A...604A..69C

Kamp, I.; Le Petit, F.; Goicoechea, J. R. +5 more

Context. Protoplanetary disks undergo substantial mass-loss by photoevaporation, a mechanism that is crucial to their dynamical evolution. However, the processes regulating the gas energetics have not so far been well constrained by observations.
Aims: We aim to study the processes involved in disk photoevaporation when it is driven by far-UV…

2017 Astronomy and Astrophysics
Herschel eHST 24
Deep HST Imaging in 47 Tucanae: A Global Dynamical Model
DOI: 10.3847/1538-4357/aa974f Bibcode: 2017ApJ...850..186H

Anderson, J.; Heyl, J.; Kalirai, J. +3 more

Multi-epoch observations with the Advanced Camera Survey and WFC3 on the Hubble Space Telescope provide a unique and comprehensive probe of stellar dynamics within 47 Tucanae. We confront analytic models of the globular cluster with the observed stellar proper motions that probe along the main sequence from just above 0.8-0.1M as well…

2017 The Astrophysical Journal
eHST 24