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Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
DOI: 10.1051/0004-6361/201526538 Bibcode: 2016A&A...586A.103W

Waters, L. B. F. M.; Pinte, C.; Ménard, F. +19 more

We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of gas and ice, and line radiative transfer from optical to cm wavelengths. The first paper of this series focuses on the assumptions about the shape of the disk, the d…

2016 Astronomy and Astrophysics
XMM-Newton eHST 308
Extended Lyman α haloes around individual high-redshift galaxies revealed by MUSE
DOI: 10.1051/0004-6361/201527384 Bibcode: 2016A&A...587A..98W

Steinmetz, M.; Carollo, C. M.; Verhamme, A. +22 more

We report the detection of extended Lyα emission around individual star-forming galaxies at redshifts z = 3-6 in an ultradeep exposure of the Hubble Deep Field South obtained with MUSE on the ESO-VLT. The data reach a limiting surface brightness (1σ) of ~1 × 10-19 erg s-1 cm-2 arcsec-2 in azimuthally ave…

2016 Astronomy and Astrophysics
eHST 270
Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
DOI: 10.1051/0004-6361/201629022 Bibcode: 2016A&A...596A.109P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +157 more

Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we implement a specifically tailored component-separation method, the so-called generalized needlet internal linear combination (GNILC) method, which uses spatial information (t…

2016 Astronomy and Astrophysics
Planck 270
Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps
DOI: 10.1051/0004-6361/201525820 Bibcode: 2016A&A...594A...8P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +223 more

This paper describes the processing applied to the cleaned, time-ordered information obtained from the Planck High Frequency Instrument (HFI) with the aim of producing photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the entire 2.5-year HFI mission include almost five full-sky surveys. HFI obse…

2016 Astronomy and Astrophysics
Planck 269
Planck 2015 results. IX. Diffuse component separation: CMB maps
DOI: 10.1051/0004-6361/201525936 Bibcode: 2016A&A...594A...9P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +237 more

We present foreground-reduced cosmic microwave background (CMB) maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, the total data volume is larger by a factor of 3.2 for frequencies between 30 and 70 GHz, and by 1.9 for frequencies between 100 and 857 GHz…

2016 Astronomy and Astrophysics
Planck 263
Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for the inner Milky Way: +68° ≥ l ≥ -70°
DOI: 10.1051/0004-6361/201526380 Bibcode: 2016A&A...591A.149M

Bernard, J. -P.; Martin, P. G.; Natoli, P. +61 more


Aims: We present the first public release of high-quality data products (DR1) from Hi-GAL, the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum Galactic plane surveys from the near-IR to the radio and covers five wavebands at 70, 160, 250, 350 and 500 µm, encompassing the peak of the spectral energ…

2016 Astronomy and Astrophysics
Herschel Planck 259
The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
DOI: 10.1051/0004-6361/201526766 Bibcode: 2016A&A...592A...1P

Smith, G. P.; Chiappetti, L.; Altieri, B. +89 more

Context. The quest for the cosmological parameters that describe our universe continues to motivate the scientific community to undertake very large survey initiatives across the electromagnetic spectrum. Over the past two decades, the Chandra and XMM-Newton observatories have supported numerous studies of X-ray-selected clusters of galaxies, acti…

2016 Astronomy and Astrophysics
XMM-Newton 253
Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources
DOI: 10.1051/0004-6361/201526914 Bibcode: 2016A&A...594A..26P

Böhringer, H.; Kneissl, R.; Miville-Deschênes, M. -A. +240 more

The Second Planck Catalogue of Compact Sources is a list of discrete objects detected in single-frequency maps from the full duration of the Planck mission and supersedes previous versions. It consists of compact sources, both Galactic and extragalactic, detected over the entire sky. Compact sources detected in the lower frequency channels are ass…

2016 Astronomy and Astrophysics
Herschel Planck 238
Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
DOI: 10.1051/0004-6361/201526803 Bibcode: 2016A&A...594A..25P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +237 more

We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-separation tool has been used to separate t…

2016 Astronomy and Astrophysics
Planck 205
The habitability of Proxima Centauri b. I. Irradiation, rotation and volatile inventory from formation to the present
DOI: 10.1051/0004-6361/201629576 Bibcode: 2016A&A...596A.111R

Guinan, Edward F.; Engle, Scott G.; Reiners, Ansgar +9 more

Proxima b is a planet with a minimum mass of 1.3M orbiting within the habitable zone (HZ) of Proxima Centauri, a very low-mass, active star and the Sun's closest neighbor. Here we investigate a number of factors related to the potential habitability of Proxima b and its ability to maintain liquid water on its surface. We set the stage …

2016 Astronomy and Astrophysics
XMM-Newton eHST 181