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2008 (v1)Journal articleUploaded on: December 4, 2022
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March 4, 2019 (v1)Journal article
We will study the formation history of the Milky Way, and the earliest phases of its chemical enrichment, with a sample of more than 1.5 million stars at high galactic latitude. Elemental abundances of up to 20 elements with a precision of better than 0.2 dex will be derived for these stars. The sample will include members of kinematically...
Uploaded on: December 4, 2022 -
2007 (v1)Journal article
Astronomy and Astrophysics Review, 14, pp. 217-360, http://dx.doi.org./10.1007/s00159-007-0007-0
Uploaded on: February 22, 2023 -
2007 (v1)Journal article
Astronomy and Astrophysics Review, 14, pp. 217-360, http://dx.doi.org./10.1007/s00159-007-0007-0
Uploaded on: December 3, 2022 -
April 19, 2022 (v1)Conference paper
The current instrumentation plan for the E-ELT foresees a High Resolution Spectrograph conventionally indicated as HIRES. Shaped on the study of extra-solar planet atmospheres, Pop-III stars and fundamental physical constants, HIRES is intended to embed observing modes at high-resolution (up to R=150000) and large spectral range (from the blue...
Uploaded on: December 3, 2022 -
September 2014 (v1)Journal article
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Uploaded on: December 4, 2022 -
2009 (v1)Journal article
The discovery of extrasolar planets is one of the greatest achievements of modern astronomy. The detection of planets that vary widely in mass demonstrates that extrasolar planets of low mass exist. In this paper, we describe a mission, called Darwin, whose primary goal is the search for, and characterization of, terrestrial extrasolar planets...
Uploaded on: December 3, 2022 -
January 2013 (v1)Journal article
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Uploaded on: December 4, 2022 -
January 2013 (v1)Journal article
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Uploaded on: February 22, 2023 -
April 2015 (v1)Journal article
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Uploaded on: December 4, 2022 -
2017 (v1)Publication
We report on the discovery of a new fast radio burst (FRB), FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure (DM) of 1105.6 ± 0.8 pc cm-3, a pulse duration of 2.8+1.2-0.5ms, and a measured peak flux density assuming that the burst was at beam centre of 0.7+0.2-0.1Jy....
Uploaded on: March 27, 2023 -
November 2014 (v1)Journal article
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Uploaded on: March 25, 2023