Search Publications

Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars
DOI: 10.1051/0004-6361/201423969 Bibcode: 2015A&A...574A..59D

Pâris, Isabelle; Petitjean, Patrick; Aubourg, Éric +35 more

We report a detection of the baryon acousticoscillation (BAO) feature in the flux-correlation function of the Lyα forest of high-redshift quasars with a statistical significance of five standard deviations. The study uses 137 562 quasars in the redshift range 2.1 ≤ z ≤ 3.5 from the data release 11 (DR11) of the Baryon Oscillation Spectroscopic Sur…

2015 Astronomy and Astrophysics
Planck 827
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
DOI: 10.1051/0004-6361/201424082 Bibcode: 2015A&A...576A.104P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +200 more

This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse maps of dust polarization fraction and polarization angle at 1° resolution, taking into account noise bias and possible systematic effects. The sensitivity of the Planck H…

2015 Astronomy and Astrophysics
Planck 376
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
DOI: 10.1051/0004-6361/201424088 Bibcode: 2015A&A...576A.107P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +177 more

Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We make use of the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the Planck and WMAP data at 12 frequencies from …

2015 Astronomy and Astrophysics
Planck 176
XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact
DOI: 10.1051/0004-6361/201424085 Bibcode: 2015A&A...575A..30S

Lovisari, L.; David, L.; Reiprich, T. H. +2 more

Context. Robust X-ray temperature measurements of the intracluster medium (ICM) of galaxy clusters require an accurate energy-dependent effective area calibration. Since the hot gas X-ray emission of galaxy clusters does not vary on relevant timescales, they are excellent cross-calibration targets. Moreover, cosmological constraints from clusters …

2015 Astronomy and Astrophysics
Planck XMM-Newton 166
Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
DOI: 10.1051/0004-6361/201424086 Bibcode: 2015A&A...576A.105P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +186 more

Polarized emission observed by Planck HFI at 353 GHz towards a sample of nearby fields is presented, focusing on the statistics of polarization fractions p and angles ψ. The polarization fractions and column densities in these nearby fields are representative of the range of values obtained over the whole sky. We find that: (i) the largest polariz…

2015 Astronomy and Astrophysics
Planck 134
Planck intermediate results. XXIV. Constraints on variations in fundamental constants
DOI: 10.1051/0004-6361/201424496 Bibcode: 2015A&A...580A..22P

Kneissl, R.; Miville-Deschênes, M. -A.; Bernard, J. -P. +167 more

Any variation in the fundamental physical constants, more particularly in the fine structure constant, α, or in the mass of the electron, me, affects the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show that the Planck data allow one to improve the constraint on…

2015 Astronomy and Astrophysics
Planck 113
Planck's dusty GEMS: The brightest gravitationally lensed galaxies discovered with the Planck all-sky survey
DOI: 10.1051/0004-6361/201425128 Bibcode: 2015A&A...581A.105C

Kneissl, R.; Altieri, B.; Le Floc'h, E. +30 more

We present an analysis of CO spectroscopy and infrared-to-millimetre dust photometry of 11 exceptionally bright far-infrared (FIR) and sub-mm sources discovered through a combination of the Planck all-sky survey and follow-up Herschel-SPIRE imaging - "Planck's Dusty Gravitationally Enhanced subMillimetre Sources". Each source has a secure spectros…

2015 Astronomy and Astrophysics
Herschel Planck 112
Molecular clouds have power-law probability distribution functions
DOI: 10.1051/0004-6361/201525650 Bibcode: 2015A&A...576L...1L

Alves, João; Lada, Charles J.; Lombardi, Marco

In this Letter we investigate the shape of the probability distribution of column densities (PDF) in molecular clouds. Through the use of low-noise, extinction-calibrated Herschel/Planck emission data for eight molecular clouds, we demonstrate that, contrary to common belief, the PDFs of molecular clouds are not described well by log-normal functi…

2015 Astronomy and Astrophysics
Planck 110
Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data
DOI: 10.1051/0004-6361/201424434 Bibcode: 2015A&A...580A..13P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +189 more

Planck data when combined with ancillary data provide a unique opportunity to separate the diffuse emission components of the inner Galaxy. The purpose of the paper is to elucidate the morphology of the various emission components in the strong star-formation region lying inside the solar radius and to clarify the relationship between the various …

2015 Astronomy and Astrophysics
Planck 104
Planck 2013 results. XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources
DOI: 10.1051/0004-6361/201525787 Bibcode: 2015A&A...581A..14P

Böhringer, H.; Kneissl, R.; Dahle, H. +275 more

We update the all-sky Planck catalogue of 1227 clusters and cluster candidates (PSZ1) published in March 2013, derived from detections of the Sunyaev-Zeldovich (SZ) effect using the first 15.5 months of Planck satellite observations. As an addendum, we deliver an updated version of the PSZ1 catalogue, reporting the further confirmation of 86 Planc…

2015 Astronomy and Astrophysics
Planck 97