Relevant bibliographies by topics / Euclid mission

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  1. Journal articles

Academic literature on the topic 'Euclid mission'

Author: Grafiati
Published: 1 April 2023

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Journal articles on the topic "Euclid mission"

1

de Teodoro, P., S. Nieto, and B. Altieri. "Data Management in the Euclid Science Archive System." Proceedings of the International Astronomical Union 12, S325 (2016): 385–88. http://dx.doi.org/10.1017/s1743921316012874.

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AbstractEuclid is the ESA M2 mission and a milestone in the understanding of the geometry of the Universe. In total Euclid will produce up to 26 PB per year of observations. The Science Archive Systems (SAS) belongs to the Euclid Archive System (EAS) that sits in the core of the Euclid Science Ground Segment (SGS). The SAS is being built at the ESAC Science Data Centre (ESDC), which is responsible for the development and operations of the scientific archives for the Astronomy, Planetary and Heliophysics missions of ESA. The SAS is focused on the needs of the scientific community and is intende
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Tereno, I., C. S. Carvalho, J. Dinis, et al. "Euclid Space Mission: building the sky survey." Proceedings of the International Astronomical Union 10, S306 (2014): 379–81. http://dx.doi.org/10.1017/s174392131401093x.

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AbstractThe Euclid space mission proposes to survey 15000 square degrees of the extragalactic sky during 6 years, with a step-and-stare technique. The scheduling of observation sequences is driven by the primary scientific objectives, spacecraft constraints, calibration requirements and physical properties of the sky. We present the current reference implementation of the Euclid survey and on-going work on survey optimization.
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Beaulieu, Jean-Philippe, David P. Bennett, Eamonn Kerins, and Matthew Penny. "Towards habitable Earths with EUCLID and WFIRST." Proceedings of the International Astronomical Union 6, S276 (2010): 349–53. http://dx.doi.org/10.1017/s1743921311020424.

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AbstractThe discovery of extrasolar planets is arguably the most exciting development in astrophysics during the past 15 years, rivalled only by the detection of dark energy. Two projects are now at the intersection of the two communities of exoplanet scientists and cosmologists: EUCLID, proposed as an ESA M-class mission; and WFIRST, the top-ranked large space mission for the next decade by the Astro 2010 Decadal Survey report. The missions are to have several important science programs: a dark energy survey using weak lensing, baryon acoustic oscillations, Type Ia supernova, a survey of exop
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Dubath, Pierre, Nikolaos Apostolakos, Andrea Bonchi, et al. "The Euclid Data Processing Challenges." Proceedings of the International Astronomical Union 12, S325 (2016): 73–82. http://dx.doi.org/10.1017/s1743921317001521.

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AbstractEuclid is a Europe-led cosmology space mission dedicated to a visible and near infrared survey of the entire extra-galactic sky. Its purpose is to deepen our knowledge of the dark content of our Universe. After an overview of the Euclid mission and science, this contribution describes how the community is getting organized to face the data analysis challenges, both in software development and in operational data processing matters. It ends with a more specific account of some of the main contributions of the Swiss Science Data Center (SDC-CH).
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Laureijs, René. "Observing the high redshift Universe with Euclid." Proceedings of the International Astronomical Union 12, S333 (2017): 238–41. http://dx.doi.org/10.1017/s1743921318000595.

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AbstractEuclid enables the exploration of large sky areas with diffraction limited resolution in the optical and near-infrared, and is sensitive enough to detect targets at cosmological distances. This combination of capabilities gives Euclid a clear advantage over telescope facilities with larger apertures, both on ground and in space. The decision to mount in the NISP instrument one extra grism for the wavelength range 0.92-1.3 μm with a spectral resolution of R ≈260 makes possible a rest-frame UV survey of the early Universe in the redshift range 6.5 < z < 9.7. Euclid’s standard imagi
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6

Martin, E. L. "Ultracool dwarf legacy science with ESA's Euclid mission." EPJ Web of Conferences 47 (2013): 15003. http://dx.doi.org/10.1051/epjconf/20134715003.

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7

Adam, R., M. Vannier, S. Maurogordato, et al. "Euclid preparation." Astronomy & Astrophysics 627 (June 26, 2019): A23. http://dx.doi.org/10.1051/0004-6361/201935088.

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Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clusters from surveys with a well-known selection function and robust mass estimates, which is particularly challenging at high redshift. The Euclid wide survey will cover 15 000 deg2 of the sky, avoiding contamination by light from our Galaxy and our solar system in the optical and near-infrared bands, down to magnitude 24 in the H-band. The resulting data will make it possible to detect a large number of galaxy clusters
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Inserra, C., R. C. Nichol, D. Scovacricchi, et al. "Euclid: Superluminous supernovae in the Deep Survey." Astronomy & Astrophysics 609 (January 2018): A83. http://dx.doi.org/10.1051/0004-6361/201731758.

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Context. In the last decade, astronomers have found a new type of supernova called superluminous supernovae (SLSNe) due to their high peak luminosity and long light-curves. These hydrogen-free explosions (SLSNe-I) can be seen to z ~ 4 and therefore, offer the possibility of probing the distant Universe. Aims. We aim to investigate the possibility of detecting SLSNe-I using ESA’s Euclid satellite, scheduled for launch in 2020. In particular, we study the Euclid Deep Survey (EDS) which will provide a unique combination of area, depth and cadence over the mission. Methods. We estimated the redshi
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9

Scaramella, R., Y. Mellier, J. Amiaux, et al. "Euclid space mission: a cosmological challenge for the next 15 years." Proceedings of the International Astronomical Union 10, S306 (2014): 375–78. http://dx.doi.org/10.1017/s1743921314011089.

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AbstractEuclid is the next ESA mission devoted to cosmology. It aims at observing most of the extragalactic sky, studying both gravitational lensing and clustering over ~15,000 square degrees. The mission is expected to be launched in year 2020 and to last six years. The sheer amount of data of different kinds, the variety of (un)known systematic effects and the complexity of measures require efforts both in sophisticated simulations and techniques of data analysis. We review the mission main characteristics, some aspects of the the survey and highlight some of the areas of interest to this me
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10

Bretonnière, H., M. Huertas-Company, A. Boucaud, et al. "Euclid preparation." Astronomy & Astrophysics 657 (January 2022): A90. http://dx.doi.org/10.1051/0004-6361/202141393.

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We present a machine learning framework to simulate realistic galaxies for the Euclid Survey, producing more complex and realistic galaxies than the analytical simulations currently used in Euclid. The proposed method combines a control on galaxy shape parameters offered by analytic models with realistic surface brightness distributions learned from real Hubble Space Telescope observations by deep generative models. We simulate a galaxy field of 0.4 deg2 as it will be seen by the Euclid visible imager VIS, and we show that galaxy structural parameters are recovered to an accuracy similar to th
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