WFRF:(Puget S.)
Sökning: WFRF:(Puget S.) > The SPHERE infrared...
- 40 av 61
- Föregående post
- Nästa post
- Till träfflistan
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06863naa a2201609 4500 | |
| 001 | oai:DiVA.org:su-202678 | |
| 003 | SwePub | |
| 008 | 220314s2021 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2026782 URI |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2020388062 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Desidera, S.4 aut |
| 245 | 1 0 | a The SPHERE infrared survey for exoplanets (SHINE) I. Sample definition and target characterization |
| 264 | c 2021-07-14 | |
| 264 | 1 | b EDP Sciences,c 2021 |
| 338 | a print2 rdacarrier | |
| 520 | a Context. Large surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from ~5 to 300 au. A careful assessment of the stellar properties is crucial for a proper understanding of when, where, and how frequently planets form, and how they evolve. The sensitivity of detection limits to stellar age makes this a key parameter for direct imaging surveys.Aims. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the context of the SPHERE Guaranteed Time Observations of the SPHERE consortium. In this first paper we present the selection and the properties of the complete sample of stars surveyed with SHINE, focusing on the targets observed during the first phase of the survey (from February 2015 to February 2017). This early sample composed of 150 stars is used to perform a preliminary statistical analysis of the SHINE data, deferred to two companion papers presenting the survey performance, main discoveries, and the preliminary statistical constraints set by SHINE.Methods. Based on a large database collecting the stellar properties of all young nearby stars in the solar vicinity (including kinematics, membership to moving groups, isochrones, lithium abundance, rotation, and activity), we selected the original sample of 800 stars that were ranked in order of priority according to their sensitivity for planet detection in direct imaging with SPHERE. The properties of the stars that are part of the early statistical sample wererevisited, including for instance measurements from the Gaia Data Release 2. Rotation periods were derived for the vast majority of the late-type objects exploiting TESS light curves and dedicated photometric observations.Results. The properties of individual targets and of the sample as a whole are presented. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a stars: fundamental parameters | |
| 653 | a stars: rotation | |
| 653 | a stars: activity | |
| 653 | a stars: pre-main sequence | |
| 653 | a stars: kinematics and dynamics | |
| 653 | a planets and satellites: general | |
| 700 | 1 | a Chauvin, G.4 aut |
| 700 | 1 | a Bonavita, M.4 aut |
| 700 | 1 | a Messina, S.4 aut |
| 700 | 1 | a LeCoroller, H.4 aut |
| 700 | 1 | a Schmidt, T.4 aut |
| 700 | 1 | a Gratton, R.4 aut |
| 700 | 1 | a Lazzoni, C.4 aut |
| 700 | 1 | a Meyer, M.4 aut |
| 700 | 1 | a Schlieder, J.4 aut |
| 700 | 1 | a Cheetham, A.4 aut |
| 700 | 1 | a Hagelberg, J.4 aut |
| 700 | 1 | a Bonnefoy, M.4 aut |
| 700 | 1 | a Feldt, M.4 aut |
| 700 | 1 | a Lagrange, A-M4 aut |
| 700 | 1 | a Langlois, M.4 aut |
| 700 | 1 | a Vigan, A.4 aut |
| 700 | 1 | a Tan, T. G.4 aut |
| 700 | 1 | a Hambsch, F-J4 aut |
| 700 | 1 | a Millward, M.4 aut |
| 700 | 1 | a Benatti, S.4 aut |
| 700 | 1 | a Brandner, W.4 aut |
| 700 | 1 | a Carson, J.4 aut |
| 700 | 1 | a Covino, E.4 aut |
| 700 | 1 | a Delorme, P.4 aut |
| 700 | 1 | a D'Orazi, V4 aut |
| 700 | 1 | a Janson, Markusu Stockholms universitet,Institutionen för astronomi,Max Planck Institute for Astronomy, Germany4 aut0 (Swepub:su)mjanso |
| 700 | 1 | a Rigliaco, E.4 aut |
| 700 | 1 | a Beuzit, J-L4 aut |
| 700 | 1 | a Biller, B.4 aut |
| 700 | 1 | a Boccaletti, A.4 aut |
| 700 | 1 | a Dominik, C.4 aut |
| 700 | 1 | a Cantalloube, F.4 aut |
| 700 | 1 | a Fontanive, C.4 aut |
| 700 | 1 | a Galicher, R.4 aut |
| 700 | 1 | a Henning, Th4 aut |
| 700 | 1 | a Lagadec, E.4 aut |
| 700 | 1 | a Ligi, R.4 aut |
| 700 | 1 | a Maire, A-L4 aut |
| 700 | 1 | a Menard, F.4 aut |
| 700 | 1 | a Mesa, D.4 aut |
| 700 | 1 | a Samland, M.4 aut |
| 700 | 1 | a Schmid, H. M.4 aut |
| 700 | 1 | a Sissa, E.4 aut |
| 700 | 1 | a Turatto, M.4 aut |
| 700 | 1 | a Udry, S.4 aut |
| 700 | 1 | a Zurlo, A.4 aut |
| 700 | 1 | a Asensio-Torres, R.4 aut |
| 700 | 1 | a Kopytova, T.4 aut |
| 700 | 1 | a Rickman, E.4 aut |
| 700 | 1 | a Abe, L.4 aut |
| 700 | 1 | a Antichi, J.4 aut |
| 700 | 1 | a Baruffolo, A.4 aut |
| 700 | 1 | a Baudoz, P.4 aut |
| 700 | 1 | a Baudrand, J.4 aut |
| 700 | 1 | a Blanchard, P.4 aut |
| 700 | 1 | a Bazzon, A.4 aut |
| 700 | 1 | a Buey, T.4 aut |
| 700 | 1 | a Carbillet, M.4 aut |
| 700 | 1 | a Carle, M.4 aut |
| 700 | 1 | a Charton, J.4 aut |
| 700 | 1 | a Cascone, E.4 aut |
| 700 | 1 | a Claudi, R.4 aut |
| 700 | 1 | a Costille, A.4 aut |
| 700 | 1 | a De Caprio, V4 aut |
| 700 | 1 | a Dohlen, K.4 aut |
| 700 | 1 | a Fantinel, D.4 aut |
| 700 | 1 | a Feautrier, P.4 aut |
| 700 | 1 | a Fusco, T.4 aut |
| 700 | 1 | a Gigan, P.4 aut |
| 700 | 1 | a Giro, E.4 aut |
| 700 | 1 | a Gisler, D.4 aut |
| 700 | 1 | a Gluck, L.4 aut |
| 700 | 1 | a Hubin, N.4 aut |
| 700 | 1 | a Hugot, E.4 aut |
| 700 | 1 | a Jaquet, M.4 aut |
| 700 | 1 | a Kasper, M.4 aut |
| 700 | 1 | a Madec, F.4 aut |
| 700 | 1 | a Magnard, Y.4 aut |
| 700 | 1 | a Martinez, P.4 aut |
| 700 | 1 | a Maurel, D.4 aut |
| 700 | 1 | a Le Mignant, D.4 aut |
| 700 | 1 | a Llored, M.4 aut |
| 700 | 1 | a Moulin, T.4 aut |
| 700 | 1 | a Pavlov, A.4 aut |
| 700 | 1 | a Perret, D.4 aut |
| 700 | 1 | a Petit, C.4 aut |
| 700 | 1 | a Pragt, J.4 aut |
| 700 | 1 | a Puget, P.4 aut |
| 700 | 1 | a Rabou, P.4 aut |
| 700 | 1 | a Ramos, J.4 aut |
| 700 | 1 | a Rigal, F.4 aut |
| 700 | 1 | a Rochat, S.4 aut |
| 700 | 1 | a Roelfsema, R.4 aut |
| 700 | 1 | a Rousset, G.4 aut |
| 700 | 1 | a Roux, A.4 aut |
| 700 | 1 | a Salasnich, B.4 aut |
| 700 | 1 | a Sauvage, J-F4 aut |
| 700 | 1 | a Sevin, A.4 aut |
| 700 | 1 | a Soenke, C.4 aut |
| 700 | 1 | a Stadler, E.4 aut |
| 700 | 1 | a Suarez, M.4 aut |
| 700 | 1 | a Weber, L.4 aut |
| 700 | 1 | a Wildi, F.4 aut |
| 710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 651q 651x 0004-6361x 1432-0746 |
| 856 | 4 | u http://arxiv.org/pdf/2103.04366 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-202678 |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/202038806 |
Hitta via bibliotek
- Astronomy and Astrophysics (Sök värdpublikationen i LIBRIS)
Till lärosätets databas
- 40 av 61
- Föregående post
- Nästa post
- Till träfflistan
Hitta mer i SwePub
- Av författaren/redakt...
- Desidera, S.
- Chauvin, G.
- Bonavita, M.
- Messina, S.
- LeCoroller, H.
- Schmidt, T.
- visa fler...
- Gratton, R.
- Lazzoni, C.
- Meyer, M.
- Schlieder, J.
- Cheetham, A.
- Hagelberg, J.
- Bonnefoy, M.
- Feldt, M.
- Lagrange, A-M
- Langlois, M.
- Vigan, A.
- Tan, T. G.
- Hambsch, F-J
- Millward, M.
- Benatti, S.
- Brandner, W.
- Carson, J.
- Covino, E.
- Delorme, P.
- D'Orazi, V
- Janson, Markus
- Rigliaco, E.
- Beuzit, J-L
- Biller, B.
- Boccaletti, A.
- Dominik, C.
- Cantalloube, F.
- Fontanive, C.
- Galicher, R.
- Henning, Th
- Lagadec, E.
- Ligi, R.
- Maire, A-L
- Menard, F.
- Mesa, D.
- Samland, M.
- Schmid, H. M.
- Sissa, E.
- Turatto, M.
- Udry, S.
- Zurlo, A.
- Asensio-Torres, ...
- Kopytova, T.
- Rickman, E.
- Abe, L.
- Antichi, J.
- Baruffolo, A.
- Baudoz, P.
- Baudrand, J.
- Blanchard, P.
- Bazzon, A.
- Buey, T.
- Carbillet, M.
- Carle, M.
- Charton, J.
- Cascone, E.
- Claudi, R.
- Costille, A.
- De Caprio, V
- Dohlen, K.
- Fantinel, D.
- Feautrier, P.
- Fusco, T.
- Gigan, P.
- Giro, E.
- Gisler, D.
- Gluck, L.
- Hubin, N.
- Hugot, E.
- Jaquet, M.
- Kasper, M.
- Madec, F.
- Magnard, Y.
- Martinez, P.
- Maurel, D.
- Le Mignant, D.
- Llored, M.
- Moulin, T.
- Pavlov, A.
- Perret, D.
- Petit, C.
- Pragt, J.
- Puget, P.
- Rabou, P.
- Ramos, J.
- Rigal, F.
- Rochat, S.
- Roelfsema, R.
- Rousset, G.
- Roux, A.
- Salasnich, B.
- Sauvage, J-F
- Sevin, A.
- Soenke, C.
- Stadler, E.
- Suarez, M.
- Weber, L.
- Wildi, F.
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- Artiklar i publikationen
- Astronomy and As ...
- Av lärosätet
- Stockholms universitet
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
