ESPRESSO (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "ESPRESSO" in English language version.

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arxiv.org

  • Pepe, F.; Molaro, P.; Cristiani, S.; Rebolo, R.; Santos, N. C.; Dekker, H.; Mégevand, D.; Zerbi, F. M.; Cabral, A.; et al. (January 2014). "ESPRESSO: The next European exoplanet hunter". Astronomische Nachrichten. 335 (1): 8–20. arXiv:1401.5918. doi:10.1002/asna.201312004. S2CID 55957013.
  • Pepe, F.; Molaro, P.; Cristiani, S.; Rebolo, R.; Santos, N. C.; Dekker, H.; Mégevand, D.; Zerbi, F. M.; Cabral, A.; Di Marcantonio, P.; Abreu, M.; Affolter, M.; Aliverti, M.; Allende Prieto, C.; Amate, M.; Avila, G.; Baldini, V.; Bristow, P.; Broeg, C.; Cirami, R.; Coelho, J.; Conconi, P.; Coretti, I.; Cupani, G.; D'Odorico, V.; De Caprio, V.; Delabre, B.; Dorn, R.; Figueira, P.; et al. (2014). "ESPRESSO: The next European exoplanet hunter". arXiv:1401.5918 [astro-ph.IM].
  • Pepe, F.; et al. (2021). "ESPRESSO at VLT". Astronomy & Astrophysics. 645: A96. arXiv:2010.00316v1. doi:10.1051/0004-6361/202038306. S2CID 228854234. A Laser Frequency Comb (LFC) is also available and should have replaced both the ThAr lamp and the Fabry-Pérot (Pasquini& Hubin 2018; Frank et al. 2018; Huke et al. 2018), but, due to lack of reliability and limited spectral coverage, it is currently not integrated in the operational scheme ... This situation might compromize the ability of ESPRESSO of guaranteeing RV repeatability at the 10 cm s−1 level over years.
  • Suárez Mascareño, A.; Faria, J. P.; Figueira, P.; Lovis, C.; Damasso, M.; González Hernández, J. I.; Rebolo, R.; Cristiano, S.; Pepe, F.; Santos, N. C.; Zapatero Osorio, M. R.; Adibekyan, V.; Hojjatpanah, S.; Sozzetti, A.; Murgas, F.; Abreo, M.; Affolter, M.; Alibert, Y.; Aliverti, M.; Allart, R.; Allende Prieto, C.; Alves, D.; Amate, M.; Avila, G.; Baldini, V.; Bandi, T.; Barros, S. C. C.; Bianco, A.; Benz, W.; et al. (2020). "Revisiting Proxima with ESPRESSO". Astronomy & Astrophysics. 639: A77. arXiv:2005.12114. Bibcode:2020A&A...639A..77S. doi:10.1051/0004-6361/202037745. S2CID 218869742.
  • Pepe, F; Molaro, P; Cristiani, S; Rebolo, R; et al. (2014). "ESPRESSO: The next European exoplanet hunter". arXiv:1401.5918v1 [astro-ph.IM].
  • Demory, Brice-Olivier; Ehrenreich, David; Queloz, Didier; Seager, Sara; et al. (25 March 2015). "Hubble Space Telescope search for the transit of the Earth-mass exoplanet Alpha Centauri Bb". Monthly Notices of the Royal Astronomical Society. 450 (2): 2043–2051. arXiv:1503.07528. Bibcode:2015MNRAS.450.2043D. doi:10.1093/mnras/stv673. S2CID 119162954.
  • Osterman, S; Diddams, S; Quinlan, F; Bally, J; Ge, J; Ycas, G (2010). "A near infrared laser frequency comb for high precision Doppler planet surveys". EPJ Web of Conferences. 16: 02002. arXiv:1003.0136. Bibcode:2011EPJWC..1602002O. doi:10.1051/epjconf/20111602002. S2CID 52026520.

cnn.com

doi.org

eso.org

exoplanet.eu

exoplanets.org

harvard.edu

ui.adsabs.harvard.edu

inaf.it

media.inaf.it

nccr-planets.ch

  • Vonarburg, Barbara (2017-12-07). "First light of ESPRESSO". NCCR PlanetS. National Centre of Competence in Research PlanetS. Retrieved 2018-11-07. The first observation was for the star Tau Ceti. It was done using the UT1 of the VLT, the observations made on the four united telescopes will be done later.
  • Bratschi, Pierre (2018-02-14). "ESPRESSO: first time with the 4 UTs of the VLT". NCCR PlanetS. National Centre of Competence in Research PlanetS. Retrieved 2018-11-07. ... first light of ESPRESSO with the four VLT 8.2-meter Unit Telescopes (4UT mode) took place on Saturday February 3rd, 2018... star observed by ESPRESSO with the 4UT mode was the so-called Pepe star
  • Barbara, Vonarburg (2018-11-28). "Fine-tuning Espresso". NCCR PlanetS. National Centre of Competence in Research PlanetS. Retrieved 2018-12-28. ESPRESSO has been opened to the astronomical community and finally started operations on the 24th of October 2018.

obsunige.ch

phys.org

semanticscholar.org

api.semanticscholar.org

  • Pepe, F.; Molaro, P.; Cristiani, S.; Rebolo, R.; Santos, N. C.; Dekker, H.; Mégevand, D.; Zerbi, F. M.; Cabral, A.; et al. (January 2014). "ESPRESSO: The next European exoplanet hunter". Astronomische Nachrichten. 335 (1): 8–20. arXiv:1401.5918. doi:10.1002/asna.201312004. S2CID 55957013.
  • Pepe, F.; et al. (2021). "ESPRESSO at VLT". Astronomy & Astrophysics. 645: A96. arXiv:2010.00316v1. doi:10.1051/0004-6361/202038306. S2CID 228854234. A Laser Frequency Comb (LFC) is also available and should have replaced both the ThAr lamp and the Fabry-Pérot (Pasquini& Hubin 2018; Frank et al. 2018; Huke et al. 2018), but, due to lack of reliability and limited spectral coverage, it is currently not integrated in the operational scheme ... This situation might compromize the ability of ESPRESSO of guaranteeing RV repeatability at the 10 cm s−1 level over years.
  • Suárez Mascareño, A.; Faria, J. P.; Figueira, P.; Lovis, C.; Damasso, M.; González Hernández, J. I.; Rebolo, R.; Cristiano, S.; Pepe, F.; Santos, N. C.; Zapatero Osorio, M. R.; Adibekyan, V.; Hojjatpanah, S.; Sozzetti, A.; Murgas, F.; Abreo, M.; Affolter, M.; Alibert, Y.; Aliverti, M.; Allart, R.; Allende Prieto, C.; Alves, D.; Amate, M.; Avila, G.; Baldini, V.; Bandi, T.; Barros, S. C. C.; Bianco, A.; Benz, W.; et al. (2020). "Revisiting Proxima with ESPRESSO". Astronomy & Astrophysics. 639: A77. arXiv:2005.12114. Bibcode:2020A&A...639A..77S. doi:10.1051/0004-6361/202037745. S2CID 218869742.
  • Demory, Brice-Olivier; Ehrenreich, David; Queloz, Didier; Seager, Sara; et al. (25 March 2015). "Hubble Space Telescope search for the transit of the Earth-mass exoplanet Alpha Centauri Bb". Monthly Notices of the Royal Astronomical Society. 450 (2): 2043–2051. arXiv:1503.07528. Bibcode:2015MNRAS.450.2043D. doi:10.1093/mnras/stv673. S2CID 119162954.
  • Osterman, S; Diddams, S; Quinlan, F; Bally, J; Ge, J; Ycas, G (2010). "A near infrared laser frequency comb for high precision Doppler planet surveys". EPJ Web of Conferences. 16: 02002. arXiv:1003.0136. Bibcode:2011EPJWC..1602002O. doi:10.1051/epjconf/20111602002. S2CID 52026520.

uni-muenchen.de

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