Search Publications

Acceleration of individual, decimetre-sized aggregates in the lower coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stw2179 Bibcode: 2016MNRAS.462S..78A

Jorda, L.; Lamy, P. L.; Lara, L. M. +41 more

We present observations of decimetre-sized, likely ice-containing aggregates ejected from a confined region on the surface of comet 67P/Churyumov-Gerasimenko. The images were obtained with the narrow angle camera of the Optical, Spectroscopic, and Infrared Remote Imaging System on board the Rosetta spacecraft in 2016 January when the comet was at …

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 57
Hořava Gravity in the Effective Field Theory formalism: From cosmology to observational constraints
DOI: 10.1016/j.dark.2016.03.002 Bibcode: 2016PDU....13....7F

Frusciante, Noemi; Hu, Bin; Raveri, Marco +2 more

We consider Hořava gravity within the framework of the effective field theory (EFT) of dark energy and modified gravity. We work out a complete mapping of the theory into the EFT language for an action including all the operators which are relevant for linear perturbations with up to sixth order spatial derivatives. We then employ an updated versi…

2016 Physics of the Dark Universe
Planck 57
Planck 2015 results. III. LFI systematic uncertainties
DOI: 10.1051/0004-6361/201526998 Bibcode: 2016A&A...594A...3P

Bernard, J. -P.; Planck Collaboration; Ade, P. A. R. +168 more

We present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis. We use two complementary approaches: (I) simulations based on measured da…

2016 Astronomy and Astrophysics
Planck 57
Three-dimensional Distribution of Ejecta in Supernova 1987A at 10,000 Days
DOI: 10.3847/1538-4357/833/2/147 Bibcode: 2016ApJ...833..147L

Larsson, J.; Sollerman, J.; Lundqvist, P. +19 more

Due to its proximity, SN 1987A offers a unique opportunity to directly observe the geometry of a stellar explosion as it unfolds. Here we present spectral and imaging observations of SN 1987A obtained ∼10,000 days after the explosion with HST/STIS and VLT/SINFONI at optical and near-infrared wavelengths. These observations allow us to produce the …

2016 The Astrophysical Journal
eHST 57
Why is a Flare-rich Active Region CME-poor?
DOI: 10.3847/0004-637X/826/2/119 Bibcode: 2016ApJ...826..119L

Wang, Yuming; Shen, Chenglong; Wang, Jingxiu +6 more

Solar active regions (ARs) are the major sources of two of the most violent solar eruptions, namely flares and coronal mass ejections (CMEs). The largest AR in the past 24 years, NOAA AR 12192, which crossed the visible disk from 2014 October 17 to 30, unusually produced more than one hundred flares, including 32 M-class and 6 X-class ones, but on…

2016 The Astrophysical Journal
SOHO 57
The Relation between Galaxy Structure and Spectral Type: Implications for the Buildup of the Quiescent Galaxy Population at 0.5 < z < 2.0
DOI: 10.3847/2041-8205/817/2/L21 Bibcode: 2016ApJ...817L..21Y

van der Wel, Arjen; Kriek, Mariska; Whitaker, Katherine E. +1 more

We present the relation between galaxy structure and spectral type, using a K-selected galaxy sample at 0.5 < z < 2.0. Based on similarities between the UV-to-NIR spectral energy distributions (SEDs), we classify galaxies into 32 spectral types. The different types span a wide range in evolutionary phases, and thus—in combination with availa…

2016 The Astrophysical Journal
eHST 57
The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey
DOI: 10.1051/0004-6361/201527586 Bibcode: 2016A&A...586A..13V

Ciesla, L.; Boquien, M.; Fritz, J. +11 more

The dust in nearby galaxies absorbs a fraction of the UV-optical-near-infrared radiation produced by stars. This energy is consequently re-emitted in the infrared. We investigate the portion of the stellar radiation absorbed by spiral galaxies from the Herschel Reference Survey (HRS) by modelling their UV-to-submillimetre spectral energy distribut…

2016 Astronomy and Astrophysics
Herschel 57
An ALMA Search for Substructure, Fragmentation, and Hidden Protostars in Starless Cores in Chamaeleon I
DOI: 10.3847/0004-637X/823/2/160 Bibcode: 2016ApJ...823..160D

Bourke, Tyler L.; Di Francesco, James; Johnstone, Doug +11 more

We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey of the complete population of dense cores in the Chamaeleon I molecular cloud. We detect a total of 24 continuum sources in 19 different target fields. All previously known Class 0 and Class I protostars in Chamaeleon I are detected, whereas all of …

2016 The Astrophysical Journal
Herschel 57
Modelling observations of the inner gas and dust coma of comet 67P/Churyumov-Gerasimenko using ROSINA/COPS and OSIRIS data: First results
DOI: 10.1051/0004-6361/201628085 Bibcode: 2016A&A...589A..90M

Jorda, L.; Altwegg, K.; Shi, X. +19 more

Context. This paper describes the initial modelling of gas and dust data acquired in August and September 2014 from the European Space Agency's Rosetta spacecraft when it was in close proximity to the nucleus of comet 67P/Churyumov-Gerasimenko.
Aims: This work is an attempt to provide a self-consistent model of the innermost gas and dust coma…

2016 Astronomy and Astrophysics
Rosetta 57
Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
DOI: 10.1088/1475-7516/2016/09/027 Bibcode: 2016JCAP...09..027S

Salvatelli, Valentina; Marinoni, Christian; Piazza, Federico

We use the effective field theory of dark energy (EFT of DE) formalism to constrain dark energy models belonging to the Horndeski class with the recent Planck 2015 CMB data. The space of theories is spanned by a certain number of parameters determining the linear cosmological perturbations, while the expansion history is set to that of a standard …

2016 Journal of Cosmology and Astroparticle Physics
Planck 57