Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
PAR Ade, N Aghanim, D Alina, MIR Alves… - Astronomy & …, 2015 - aanda.org
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 …
which is the most sensitive Planck channel for dust polarization. We construct and analyse …
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
JF Cardoso, J Delabrouille, K Ganga… - Astronomy and …, 2015 - orbit.dtu.dk
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 …
which is the most sensitive Planck channel for dust polarization. We construct and analyse …
Planck 2018 results-X. Constraints on inflation
We report on the implications for cosmic inflation of the 2018 release of the Planck cosmic
microwave background (CMB) anisotropy measurements. The results are fully consistent …
microwave background (CMB) anisotropy measurements. The results are fully consistent …
[HTML][HTML] Planck 2015 results-I. Overview of products and scientific results
R Adam, PAR Ade, N Aghanim, Y Akrami… - Astronomy & …, 2016 - aanda.org
The European Space Agency's Planck satellite, which is dedicated to studying the early
Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the …
Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the …
Planck 2018 results. VI. Cosmological parameters
P Collaboration, N Aghanim, Y Akrami, M Ashdown… - 2020 - repository.cam.ac.uk
We present cosmological parameter results from the final full-mission Planck measurements
of the CMB anisotropies. We find good consistency with the standard spatially-flat 6 …
of the CMB anisotropies. We find good consistency with the standard spatially-flat 6 …
Planck 2013 results. I. Overview of products and scientific results
PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2014 - aanda.org
The European Space Agency's Planck satellite, dedicated to studying the early Universe
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
PAR Ade, N Aghanim, C Armitage-Caplan… - Astronomy & …, 2014 - aanda.org
We present constraints on cosmological parameters using number counts as a function of
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …
Planck 2015 results-III. LFI systematic uncertainties
PAR Ade, J Aumont, C Baccigalupi, AJ Banday… - Astronomy & …, 2016 - aanda.org
We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
Planck 2013 results. I. Overview of products and scientific results
The European Space Agency's Planck satellite, dedicated to studying the early Universe
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the “dark gas” in our Galaxy
PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & …, 2011 - aanda.org
An all sky map of the apparent temperature and optical depth of thermal dust emission is
constructed using the Planck-HFI (350μm to 2 mm) andIRAS (100μm) data. The optical …
constructed using the Planck-HFI (350μm to 2 mm) andIRAS (100μm) data. The optical …