Search Publications

Planck 2018 results. VI. Cosmological parameters
DOI: 10.1051/0004-6361/201833910 Bibcode: 2020A&A...641A...6P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +179 more

We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization opti…

2020 Astronomy and Astrophysics
eHST 15139
Planck 2018 results. I. Overview and the cosmological legacy of Planck
DOI: 10.1051/0004-6361/201833880 Bibcode: 2020A&A...641A...1P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +192 more

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz.…

2020 Astronomy and Astrophysics
XMM-Newton 1575
The Solar Orbiter mission. Science overview
DOI: 10.1051/0004-6361/202038467 Bibcode: 2020A&A...642A...1M

Williams, D.; Livi, S.; Peter, H. +32 more


Aims: Solar Orbiter, the first mission of ESA's Cosmic Vision 2015-2025 programme and a mission of international collaboration between ESA and NASA, will explore the Sun and heliosphere from close up and out of the ecliptic plane. It was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and …

2020 Astronomy and Astrophysics
SolarOrbiter Ulysses 754
Painting a portrait of the Galactic disc with its stellar clusters
DOI: 10.1051/0004-6361/202038192 Bibcode: 2020A&A...640A...1C

Castro-Ginard, A.; Jordi, C.; Casamiquela, L. +10 more

Context. The large astrometric and photometric survey performed by the Gaia mission allows for a panoptic view of the Galactic disc and its stellar cluster population. Hundreds of stellar clusters were only discovered after the latest Gaia data release (DR2) and have yet to be characterised.
Aims: Here we make use of the deep and homogeneous …

2020 Astronomy and Astrophysics
Gaia 410
TDCOSMO. IV. Hierarchical time-delay cosmography - joint inference of the Hubble constant and galaxy density profiles
DOI: 10.1051/0004-6361/202038861 Bibcode: 2020A&A...643A.165B

Treu, T.; Christensen, L.; Koopmans, L. V. E. +24 more

The H0LiCOW collaboration inferred via strong gravitational lensing time delays a Hubble constant value of H0 = 73.3-1.8+1.7 km s-1 Mpc-1, describing deflector mass density profiles by either a power-law or stars (constant mass-to-light ratio) plus standard dark matter halos. The mass-sheet tr…

2020 Astronomy and Astrophysics
eHST 333
The third realization of the International Celestial Reference Frame by very long baseline interferometry
DOI: 10.1051/0004-6361/202038368 Bibcode: 2020A&A...644A.159C

Charlot, P.; Lambert, S.; Bourda, G. +17 more

A new realization of the International Celestial Reference Frame (ICRF) is presented based on the work achieved by a working group of the International Astronomical Union (IAU) mandated for this purpose. This new realization follows the initial realization of the ICRF completed in 1997 and its successor, ICRF2, adopted as a replacement in 2009. Th…

2020 Astronomy and Astrophysics
Gaia 307
The XMM-Newton serendipitous survey. IX. The fourth XMM-Newton serendipitous source catalogue
DOI: 10.1051/0004-6361/201937353 Bibcode: 2020A&A...641A.136W

Motch, C.; Page, M. J.; Ballet, J. +28 more

Context. Sky surveys produce enormous quantities of data on extensive regions of the sky. The easiest way to access this information is through catalogues of standardised data products. XMM-Newton has been surveying the sky in the X-ray, ultra-violet, and optical bands for 20 years.
Aims: The XMM-Newton Survey Science Centre has been producin…

2020 Astronomy and Astrophysics
AKARI Gaia XMM-Newton 297
The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager
DOI: 10.1051/0004-6361/201936663 Bibcode: 2020A&A...642A...8R

Vial, J. -C.; Zhang, X.; Peter, H. +146 more

Context. The Extreme Ultraviolet Imager (EUI) is part of the remote sensing instrument package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and observe the Sun from vantage points close to the Sun and out of the ecliptic. Solar Orbiter will advance the "connection science" between solar activity and the heliosphere…

2020 Astronomy and Astrophysics
SolarOrbiter 292
Universal bolometric corrections for active galactic nuclei over seven luminosity decades
DOI: 10.1051/0004-6361/201936817 Bibcode: 2020A&A...636A..73D

Maiolino, R.; Fiore, F.; Bianchi, S. +12 more

Context. The AGN bolometric correction is a key element for understanding black hole (BH) demographics and computing accurate BH accretion histories from AGN luminosities. However, current estimates still differ from each other by up to a factor of two to three, and rely on extrapolations at the lowest and highest luminosities.
Aims: Here we …

2020 Astronomy and Astrophysics
ISO 264
Clusters and mirages: cataloguing stellar aggregates in the Milky Way
DOI: 10.1051/0004-6361/201936691 Bibcode: 2020A&A...633A..99C

Anders, F.; Cantat-Gaudin, T.

Context. Many of the open clusters listed in modern catalogues were initially reported by visual astronomers as apparent overdensities of bright stars. As observational techniques and analysis methods continue to improve, some of them have been shown to be chance alignments of stars and not true clusters. Recent publications making use of Gaia DR2…

2020 Astronomy and Astrophysics
Gaia 243