Search Publications

Planck 2015 results. X. Diffuse component separation: Foreground maps
DOI: 10.1051/0004-6361/201525967 Bibcode: 2016A&A...594A..10P

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

Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz in polarization. In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive an internally co…

2016 Astronomy and Astrophysics
Planck 549
Planck 2015 results. XV. Gravitational lensing
DOI: 10.1051/0004-6361/201525941 Bibcode: 2016A&A...594A..15P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +227 more

We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40σ), using temperature and polarization data from the Planck 2015 full-mission release. Using a polarization-only estimator, we detect lensing at a significance of 5σ. We cross-check the accuracy of our measurement using t…

2016 Astronomy and Astrophysics
Planck 515
Planck intermediate results. XLVII. Planck constraints on reionization history
DOI: 10.1051/0004-6361/201628897 Bibcode: 2016A&A...596A.108P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +165 more

We investigate constraints on cosmic reionization extracted from the Planck cosmic microwave background (CMB) data. We combine the Planck CMB anisotropy data in temperature with the low-multipole polarization data to fit ΛCDM models with various parameterizations of the reionization history. We obtain a Thomson optical depth τ = 0.058 ± 0.012 for …

2016 Astronomy and Astrophysics
Planck 483
Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results
DOI: 10.1103/PhysRevLett.116.231101 Bibcode: 2016PhRvL.116w1101A

Mendes, L.; Madden, S.; Russano, G. +116 more

We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density of 5.2 ±0.1 fm s

2016 Physical Review Letters
LISAPathfinder 472
Planck 2015 results. XVI. Isotropy and statistics of the CMB
DOI: 10.1051/0004-6361/201526681 Bibcode: 2016A&A...594A..16P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +242 more

We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly on the full Planck mission for temperature, but also include some polarization measurements. In particular, we consider the CMB anisotropy maps derived from the multi-f…

2016 Astronomy and Astrophysics
Planck 463
Indirect dark matter signatures in the cosmic dark ages. I. Generalizing the bound on s -wave dark matter annihilation from Planck results
DOI: 10.1103/PhysRevD.93.023527 Bibcode: 2016PhRvD..93b3527S

Slatyer, Tracy R.

Recent measurements of the cosmic microwave background (CMB) anisotropies by Planck provide a sensitive probe of dark matter annihilation during the cosmic dark ages, and specifically constrain the annihilation parameter feff⟨σ v ⟩/mχ. Using new results (paper II) for the ionization produced by particles injected at arbitrary…

2016 Physical Review D
Planck 448
Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
DOI: 10.1051/0004-6361/201425034 Bibcode: 2016A&A...586A.133P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +231 more

The polarized thermal emission from diffuse Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100 GHz. In this paper we exploit the uniqueness of the Planck HFI polarization data from 100 to 353 GHz to measure the polarized dust angular power spectra C

2016 Astronomy and Astrophysics
Planck 437
A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
DOI: 10.3847/0004-637X/819/2/129 Bibcode: 2016ApJ...819..129O

Brammer, G.; Trenti, M.; Oesch, P. A. +15 more

We present Hubble WFC3/IR slitless grism spectra of a remarkably bright z ≳ 10 galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging data. A significant spectroscopic continuum break is detected at λ =1.47+/- 0.01 µ {{m}}. The new grism data, combined with the photometric data, rule out all plausible lower redshift solu…

2016 The Astrophysical Journal
eHST 426
Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
DOI: 10.1051/0004-6361/201628890 Bibcode: 2016A&A...596A.107P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +170 more

This paper describes the identification, modelling, and removal of previously unexplained systematic effects in the polarization data of the Planck High Frequency Instrument (HFI) on large angular scales, including new mapmaking and calibration procedures, new and more complete end-to-end simulations, and a set of robust internal consistency check…

2016 Astronomy and Astrophysics
Planck 423
Second ROSAT all-sky survey (2RXS) source catalogue
DOI: 10.1051/0004-6361/201525648 Bibcode: 2016A&A...588A.103B

Haberl, F.; Nandra, K.; Freyberg, M. J. +3 more


Aims: We present the second ROSAT all-sky survey source catalogue, hereafter referred to as the 2RXS catalogue. This is the second publicly released ROSAT catalogue of point-like sources obtained from the ROSAT all-sky survey (RASS) observations performed with the position-sensitive proportional counter (PSPC) between June 1990 and August 199…

2016 Astronomy and Astrophysics
XMM-Newton 407