|
1.
|
|
|
Euclid. I. Overview of the Euclid mission
/ Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. [...]
arXiv:2405.13491.
-
94.
Fulltext
|
|
|
2.
|
Updated design of the CMB polarization experiment satellite LiteBIRD
/ Sugai, H. (Tokyo U., IPMU) ; Ade, P.A.R. (Cardiff U.) ; Akiba, Y. (KEK, Tsukuba ; Sokendai, Tsukuba) ; Alonso, D. (Oxford U.) ; Arnold, K. (UC, San Diego) ; Aumont, J. (IRAP, Toulouse) ; Austermann, J. (NIST, Boulder) ; Baccigalupi, C. (CNR, Italy ; INFN, Trieste ; SISSA, Trieste) ; Banday, A.J. (IRAP, Toulouse) ; Banerji, R. (Oslo U.) et al.
Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite CMB polarization experiments. LiteBIRD is in the most advanced phase among such future satellites, targeting its launch in Japanese Fiscal Year 2027 (2027FY) with JAXA's H3 rocket. [...]
arXiv:2001.01724.-
2020-01-27 - 11 p.
- Published in : J. Low Temp. Phys. 199 (2020) 1107-1117
Fulltext: s10909-019-02329-w - PDF; 2001.01724 - PDF;
|
|
|
3.
|
Planck 2018 results. I. Overview and the cosmological legacy of Planck
/ Planck Collaboration
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 857GHz. [...]
arXiv:1807.06205.-
2020-09-01 - 56 p.
- Published in : Astron. Astrophys. 641 (2020) A1
Fulltext: 1807.06205 - PDF; arXiv:1807.06205 - PDF;
|
|
|
4.
|
The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0)
/ Elia, Davide (INAF, Rome) ; Molinari, S. (INAF, Rome) ; Schisano, E. (INAF, Rome) ; Pestalozzi, M. (INAF, Rome) ; Pezzuto, S. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Noriega-Crespo, A. (Baltimore, Space Telescope Sci.) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Mottram, J.C. (Heidelberg, Max Planck Inst. Astron.) et al.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. [...]
arXiv:1706.01046.-
2017 - 44 p.
- Published in : Mon. Not. R. Astron. Soc. 471 (2017) 100-143
Fulltext: PDF;
|
|
|
5.
|
Exploring cosmic origins with CORE: Survey requirements and mission design
/ CORE Collaboration
Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. [...]
arXiv:1706.04516.-
2018-04-05 - 79 p.
- Published in : JCAP
Fulltext: PDF; Preprint: PDF;
|
|
|
6.
|
Exploring Cosmic Origins with CORE: Inflation
/ Finelli, Fabio (Bologna Observ. ; INFN, Bologna) ; Bucher, Martin (APC, Paris) ; Achúcarro, Ana (Leiden U. ; Basque U., Bilbao) ; Ballardini, Mario (Bologna U. ; Bologna Observ. ; INFN, Bologna) ; Bartolo, Nicola (Padua U. ; INFN, Padua ; Padua Observ.) ; Baumann, Daniel (Cambridge U., DAMTP ; Amsterdam U.) ; Clesse, Sébastien (Aachen, Tech. Hochsch.) ; Errard, Josquin (ILP, Paris ; Paris U., VI-VII) ; Handley, Will (Cambridge U. ; Cambridge U., KICC) ; Hindmarsh, Mark (Sussex U. ; Helsinki Inst. of Phys. ; Helsinki U.) et al.
/CORE
We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a medium-size mission opportunity. The CORE satellite will map the CMB anisotropies in temperature and polarization in 19 frequency channels spanning the range 60-600 GHz. [...]
arXiv:1612.08270.-
2018-04-05 - 100 p.
- Published in : JCAP 04 (2018) 016
Fulltext: PDF;
|
|
|
7.
|
|
Simulation plans (15'+5')
/ Natoli, Paolo (speaker) (University of Ferrara)
2016 - 1528.
Seminars/Workshops; Towards a next space probe for CMB observations and cosmic origins exploration
External links: Talk details; Event details
In : Towards a next space probe for CMB observations and cosmic origins exploration
|
|
|
8.
|
Pre-Inflationary Relics in the CMB?
/ Gruppuso, A. (IASF, Bologna ; INFN, Bologna) ; Kitazawa, N. (Tokyo Metropolitan U.) ; Mandolesi, N. (Ferrara U. ; INFN, Ferrara ; IASF, Bologna) ; Natoli, P. (Ferrara U. ; INFN, Ferrara) ; Sagnotti, A. (CERN ; Pisa, Scuola Normale Superiore ; INFN, Pisa)
String Theory and Supergravity allow, in principle, to follow the transition of the inflaton from pre-inflationary fast roll to slow roll. This introduces an infrared depression in the primordial power spectrum that might have left an imprint in the CMB anisotropy, if it occurred at accessible wavelengths. [...]
CERN-PH-TH-2015-181; arXiv:1508.00411.-
Geneva : CERN, 2016-03 - 6 p.
- Published in : Phys. Dark Universe 11 (2016) 68-73
Preprint: PDF; External link: Preprint
|
|
|
9.
|
|
|
10.
|
|