Observations of the radial velocity of the Sun as measured with the novel SONG spectrograph: results from a 1-week campaign Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Denmark.
Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, CEA, F-91191, Gif-sur-Yvette, France.
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain; Department de Astrofísica, Universidad de la Laguna, E-38206 La Laguna, Tenerife, Spain.
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Denmark.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark.
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Denmark.
INAF, Osservatorio Astronomico di Brera, Italy.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark; Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, København K, 1350, Øster Voldgade 5-7, Denmark.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark; Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, København K, 1350, Øster Voldgade 5-7, Denmark.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark; Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, København K, 1350, Øster Voldgade 5-7, Denmark.
Niels Bohr Institute, University of Copenhagen, Kbenhavn Ø, 2100, Juliane Maries Vej 30, Denmark.
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2013 (Engelska) Ingår i: Journal of Physics, Conference Series, ISSN 1742-6588, E-ISSN 1742-6596, Vol. 440, s. 012051-012051Artikel i tidskrift (Refereegranskat) Published
Abstract [en]
Deployment of the prototype node of the SONG project took place in April 2012 at Observatorio del Teide (Canary Islands). Its key instrument (echelle spectrograph) was installed and operational a few weeks later while its 1 m feeding telescope suffered a considerable delay to meet the required specifications. Using a fibre-feed, solar light could be fed to the spectrograph and we carried out a 1-week observing campaign in June 2012 to evaluate its performance for measuring precision radial velocities. In this work we present the first results of this campaign by comparing the sensitivity of the SONG spectrograph with other helioseismology reference instruments (Mark-I and GOLF) when simultaneous data are considered.
Ort, förlag, år, upplaga, sidor Institute of Physics Publishing (IOPP), 2013. Vol. 440, s. 012051-012051
Nationell ämneskategori
Astronomi, astrofysik och kosmologi
Identifikatorer URN: urn:nbn:se:mau:diva-63323 DOI: 10.1088/1742-6596/440/1/012051 ISI: 000325951200051 Scopus ID: 2-s2.0-84880322600 OAI: oai:DiVA.org:mau-63323 DiVA, id: diva2:1808743
Konferens Eclipse on the Coral Sea: Cycle 24 Ascending (GONG 2012, LWS/SDO-5, and SOHO 27) 12–16 November 2012, Palm Cove, Queensland, Australia
2023-11-012023-11-012023-11-17 Bibliografiskt granskad