Zobrazeno 1 - 10
of 1 008
pro vyhledávání: '"INFRARED FLUX METHOD"'
The GALAH survey: effective temperature calibration from the InfraRed Flux Method in the Gaia system
Autor:
Casagrande, L., Lin, J., Rains, A. D., Liu, F., Buder, S., Horner, J., Asplund, M., Lewis, G. F., Martell, S. L., Nordlander, T., Stello, D., Ting, Y. -S., Wittenmyer, R. A., Bland-Hawthorn, J., Casey, A. R., De Silva, G. M., D'Orazi, V., Freeman, K. C., Hayden, M. R., Kos, J., Lind, K., Schlesinger, K. J., Sharma, S., Simpson, J. D., Zucker, D. B., Zwitter, T.
In order to accurately determine stellar properties, knowledge of the effective temperature of stars is vital. We implement Gaia and 2MASS photometry in the InfraRed Flux Method and apply it to over 360,000 stars across different evolutionary stages
Externí odkaz:
http://arxiv.org/abs/2011.02517
Autor:
Mucciarelli, A., Bellazzini, M.
The ESA/Gaia mission is providing accurate and precise all-sky photometry. We combined effective temperatures derived, for a sample of dwarf and giant stars, by Gonzalez Hernandez \& Bonifacio (2009) using the Infrared Flux Method, with the photometr
Externí odkaz:
http://arxiv.org/abs/2004.06140
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astron.Astrophys. 512 (2010) 54-75
Various effective temperature scales have been proposed over the years. Despite much work and the high internal precision usually achieved, systematic differences of order 100 K (or more) among various scales are still present. We present an investig
Externí odkaz:
http://arxiv.org/abs/1001.3142
We present a new implementation of the infrared flux method (IRFM) using the 2MASS catalogue. We compute the theoretical quantities in the 2MASS JHKs filters by integrating theoretical fluxes computed from ATLAS models, and compare them directly with
Externí odkaz:
http://arxiv.org/abs/0901.3034
Autor:
Ramirez, Ivan, Melendez, Jorge
Publikováno v:
Astrophys.J. 626 (2005) 446-464
The infrared flux method (IRFM) has been applied to a sample of 135 dwarf and 36 giant stars covering the following regions of the atmospheric parameters space: 1) the metal-rich ([Fe/H]>0) end (consisting mostly of planet-hosting stars), 2) the cool
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503108
Autor:
Ramirez, Ivan, Melendez, Jorge
Publikováno v:
Astrophys.J. 609 (2004) 417-422
Effective temperatures and radii for 92 planet-hosting stars as determined from the InfraRed Flux Method (IRFM) are presented and compared with those given by other authors using different approaches. The IRFM temperatures we have derived are systema
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403395
The GALAH survey: Effective temperature calibration from the InfraRed Flux Method in the Gaia system
Autor:
Sven Buder, Yuan-Sen Ting, Robert A. Wittenmyer, Joss Bland-Hawthorn, Thomas Nordlander, Kenneth C. Freeman, Martin Asplund, Sarah L. Martell, Janez Kos, Sanjib Sharma, Katharine J. Schlesinger, Jeffrey D. Simpson, Andrew R. Casey, Jonathan Horner, Dennis Stello, Gayandhi M. De Silva, Valentina D'Orazi, Jane Lin, Adam D. Rains, Geraint F. Lewis, Luca Casagrande, Daniel B. Zucker, F. Liu, Tomaž Zwitter, Karin Lind, Michael R. Hayden
Publikováno v:
Monthly Notices of the Royal Astronomical Society
In order to accurately determine stellar properties, knowledge of the effective temperature of stars is vital. We implement Gaia and 2MASS photometry in the InfraRed Flux Method and apply it to over 360,000 stars across different evolutionary stages
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::392202c87dec8f3005fbf6d9bc412d3f
http://hdl.handle.net/20.500.12386/32137
http://hdl.handle.net/20.500.12386/32137
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.