Search Publications

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
The global shape, density and rotation of Comet 67P/Churyumov-Gerasimenko from preperihelion Rosetta/OSIRIS observations
DOI: 10.1016/j.icarus.2016.05.002 Bibcode: 2016Icar..277..257J

Jorda, L.; Lara, L. M.; Lamy, P. +45 more

The Rosetta spacecraft reached Comet 67P/Churyumov-Gerasimenko (hereafter 67P/C-G) in August 2014 at an heliocentric distance of 3.6 a.u. and was then put in orbit around its nucleus to perform detailed observations. Among the collected data are the images acquired by the OSIRIS instrument up to the perihelion passage of the comet in August 2015, …

2016 Icarus
Rosetta 269
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
The realm of the galaxy protoclusters. A review
DOI: 10.1007/s00159-016-0100-3 Bibcode: 2016A&ARv..24...14O

Overzier, Roderik A.

The study of galaxy protoclusters is beginning to fill in unknown details of the important phase of the assembly of clusters and cluster galaxies. This review describes the current status of this field and highlights promising recent findings related to galaxy formation in the densest regions of the early universe. We discuss the main search techn…

2016 Astronomy and Astrophysics Review
eHST 269
SDSS-IV/MaNGA: Spectrophotometric Calibration Technique
DOI: 10.3847/0004-6256/151/1/8 Bibcode: 2016AJ....151....8Y

Bizyaev, Dmitry; Schlegel, David J.; Bershady, Matthew A. +19 more

Mapping Nearby Galaxies at Apache Point Observatory (MaNGA), one of three core programs in the Sloan Digital Sky Survey-IV, is an integral-field spectroscopic survey of roughly 10,000 nearby galaxies. It employs dithered observations using 17 hexagonal bundles of 2″ fibers to obtain resolved spectroscopy over a wide wavelength range of 3600-10300 …

2016 The Astronomical Journal
eHST 268
Space Telescope and Optical Reverberation Mapping Project. III. Optical Continuum Emission and Broadband Time Delays in NGC 5548
DOI: 10.3847/0004-637X/821/1/56 Bibcode: 2016ApJ...821...56F

Im, M.; Geier, S.; Brandt, W. N. +94 more

We present ground-based optical photometric monitoring data for NGC 5548, part of an extended multiwavelength reverberation mapping campaign. The light curves have nearly daily cadence from 2014 January to July in nine filters (BVRI and ugriz). Combined with ultraviolet data from the Hubble Space Telescope and Swift, we confirm significant time de…

2016 The Astrophysical Journal
eHST 267
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
Eight per cent leakage of Lyman continuum photons from a compact, star-forming dwarf galaxy
DOI: 10.1038/nature16456 Bibcode: 2016Natur.529..178I

Schaerer, D.; Thuan, T. X.; Izotov, Y. I. +4 more

One of the key questions in observational cosmology is the identification of the sources responsible for ionization of the Universe after the cosmic ‘Dark Ages’, when the baryonic matter was neutral. The currently identified distant galaxies are insufficient to fully reionize the Universe by redshift z ≈ 6 (refs 1, 2, 3), but low-mass, star-formin…

2016 Nature
eHST 262
A homogeneous nucleus for comet 67P/Churyumov-Gerasimenko from its gravity field
DOI: 10.1038/nature16535 Bibcode: 2016Natur.530...63P

Jorda, L.; Pätzold, M.; Sierks, H. +13 more

Cometary nuclei consist mostly of dust and water ice. Previous observations have found nuclei to be low-density and highly porous bodies, but have only moderately constrained the range of allowed densities because of the measurement uncertainties. Here we report the precise mass, bulk density, porosity and internal structure of the nucleus of come…

2016 Nature
Rosetta 261