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CERN Accelerating science

CERN Document Server 2,023 ჩანაწერია ნაპოვნი  1 - 10შემდეგიდასასრული  ჩანაწერთან გადასვლა: ძიებას დასჭირდა 2.31 წამი. 
1.
First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope / Lombardi, S. (Rome Observ. ; ASDC, Frascati) ; Catalano, O. (IASF, Palermo) ; Scuderi, S. (IASF, Milan) ; Antonelli, L.A. (Rome Observ. ; ASDC, Frascati) ; Pareschi, G. (Brera Observ.) ; Antolini, E. (Bologna Observ.) ; Arrabito, L. (U. Montpellier 2, LUPM) ; Bellassai, G. (Catania Astrophys. Observ.) ; Bernlöhr, K. (Heidelberg, Max Planck Inst.) ; Bigongiari, C. (Rome Observ.) et al.
We report on the first detection of very high-energy (VHE) gamma-ray emission from the Crab Nebula by a Cherenkov telescope in dual-mirror Schwarzschild-Couder (SC) configuration. The result has been achieved by means of the 4 m size ASTRI-Horn telescope, operated on Mt. [...]
arXiv:1909.12149.- 2020-02-01 - 6 p. - Published in : Astron. Astrophys. 634 (2020) A22 Fulltext: PDF;
2.
Euclid. IV. The NISP Calibration Unit / Euclid Collaboration
The near-infrared calibration unit (NI-CU) on board Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. [...]
arXiv:2405.13494.
- 21.
Fulltext
3.
Euclid preparation. Sensitivity to non-standard particle dark matter model / Euclid Collaboration
The Euclid mission of the European Space Agency will provide weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and its extensions, with an opportunity to test the properties of dark matter beyond the minimal cold dark matter paradigm. [...]
arXiv:2406.18274 ; TTK-24-26.
- 31.
Fulltext
4.
Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes / Euclid Collaboration
The future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein's general relativity at cosmic scales. We focus on modified gravity models characterised, at linear scales, by a scale-independent growth of perturbations while featuring different testable types of derivative screening mechanisms at smaller non-linear scales [...]
arXiv:2306.12368.- 2024-10-01 - 22 p. - Published in : Astron. Astrophys. 690 (2024) A133 Fulltext: 2306.12368 - PDF; Publication - PDF; document - PDF;
5.
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
6.
ORIGIN: Metal Creation and Evolution from the Cosmic Dawn / Herder, Jan-Willem den (SRON, Utrecht) ; Piro, Luigi (IASF, Bologna) ; Ohashi, Takaya (Tokyo Metropolitan U.) ; Kouveliotou, Chryssa (NASA, Marshall) ; Hartmann, Dieter H. (Stanford U., Phys. Dept.) ; Kaastra, Jelle S. (SRON, Utrecht) ; Amati, L. (IASF, Bologna) ; Andersen, M.I. (DARK Cosmology Ctr.) ; Arnaud, M. (Saclay) ; Attéia, J.-L. (Midi-Pyrenees Observ.) et al.
ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGIN will be able to identify the physical conditions of all abundant elements between C and Ni to red-shifts of z=10, and beyond. [...]
arXiv:1104.2048.- 2011 - 34 p. - Published in : Exper.Astron. 34 (2012) 519-549 Fulltext: PDF; External link: Preprint
7.
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;
8.
Gaia Data Release 3: The extragalactic content / Gaia Collaboration
The Gaia Galactic survey mission is designed and optimized to obtain astrometry, photometry, and spectroscopy of nearly two billion stars in our Galaxy. Yet as an all-sky multi-epoch survey, Gaia also observes several million extragalactic objects down to a magnitude of G~21 mag. [...]
arXiv:2206.05681.- 2023-06-01 - 33 p. - Published in : Astron. Astrophys. 674 (2023) A41 Fulltext: 2206.05681 - PDF; document - PDF;
9.
Gaia Data Release 3: Chemical cartography of the Milky Way / Gaia Collaboration
Gaia DR3 opens a new era of all-sky spectral analysis of stellar populations thanks to the nearly 5.6 million stars observed by the RVS and parametrised by the GSP-spec module. The all-sky Gaia chemical cartography allows a powerful and precise chemo-dynamical view of the Milky Way with unprecedented spatial coverage and statistical robustness. [...]
arXiv:2206.05534.- 2023-06 - 49 p. - Published in : Astron. Astrophys. 674 (2023) A38 Fulltext: 2206.05534 - PDF; Publication - PDF;
10.
Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane / Palmeirim, P. (Marseille, Lab. Astrophys. ; Porto U., Astron. Dept.) ; Zavagno, A. (Marseille, Lab. Astrophys.) ; Elia, D. (INAF, Rome) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Whitworth, A. (Cardiff U.) ; Tremblin, P. (MdlS, Saclay) ; Traficante, A. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Pezzuto, S. (INAF, Rome) et al.
We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environments. The compilation of ~70 000 star-forming sources, found in the proximity of the ionized (Hii) regions and detected in both Hi-GAL and GLIMPSE surveys, provided a broad overview of the different evolutionary stages of star-formation in bubbles, from prestellar objects to more evolved young stellar objects (YSOs). [...]
arXiv:1705.09877.- 2017-09-05 - 14 p. - Published in : Astron. Astrophys. 605 (2017) A35 Fulltext: PDF;

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