The Fundamental Stellar Parameters of FGK Stars in the SEEDS Survey Norman, OK 73071, USA
Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our understanding of the formation and evolution of planetary systems also requires a detailed understanding of the basic properties of their host stars. We...
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| Vydáno v: | Monthly notices of the Royal Astronomical Society Ročník 472; číslo 2; s. 1736 - 1752 |
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| Médium: | Journal Article |
| Jazyk: | angličtina |
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Goddard Space Flight Center
Oxford University Press
01.12.2017
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| ISSN: | 0035-8711, 1365-2966, 1365-2966 |
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| Abstract | Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our understanding of the formation and evolution of planetary systems also requires a detailed understanding of the basic properties of their host stars. We have determined the basic stellar properties of F, K and G stars in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) survey from Echelle spectra taken at the Apache Point Observatory's 3.5m telescope. Using ROBOSPECT to extract line equivalent widths and Temperature Gravity microtrubulent Velocity ITerations to calculate the fundamental parameters, we have computed T(sub eff), log(g), v(sub t), [Fe/H], chromospheric activity and the age for our sample. Our methodology was calibrated against previously published results for a portion of our sample. The distribution of [Fe/H] in our sample is consistent with that typical of the Solar neighbourhood. Additionally, we find the ages of most of our sample are less than 500 Myr, but note that we cannot determine robust ages from significantly older stars via chromospheric activity age indicators. The future meta-analysis of the frequency of wide stellar and sub-stellar companions imaged via the SEEDS survey will utilize our results to constrain the occurrence of detected comoving companions with the properties of their host stars. |
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| AbstractList | Abstract
Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our understanding of the formation and evolution of planetary systems also requires a detailed understanding of the basic properties of their host stars. We have determined the basic stellar properties of F, K and G stars in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) survey from Echelle spectra taken at the Apache Point Observatory's 3.5m telescope. Using robospect to extract line equivalent widths and Temperature Gravity microtrubulent Velocity ITerations to calculate the fundamental parameters, we have computed Teff, log(g), vt, [Fe/H], chromospheric activity and the age for our sample. Our methodology was calibrated against previously published results for a portion of our sample. The distribution of [Fe/H] in our sample is consistent with that typical of the Solar neighbourhood. Additionally, we find the ages of most of our sample are <500 Myr, but note that we cannot determine robust ages from significantly older stars via chromospheric activity age indicators. The future meta-analysis of the frequency of wide stellar and sub-stellar companions imaged via the SEEDS survey will utilize our results to constrain the occurrence of detected comoving companions with the properties of their host stars. Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our understanding of the formation and evolution of planetary systems also requires a detailed understanding of the basic properties of their host stars. We have determined the basic stellar properties of F, K and G stars in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) survey from Echelle spectra taken at the Apache Point Observatory's 3.5m telescope. Using ROBOSPECT to extract line equivalent widths and Temperature Gravity microtrubulent Velocity ITerations to calculate the fundamental parameters, we have computed T(sub eff), log(g), v(sub t), [Fe/H], chromospheric activity and the age for our sample. Our methodology was calibrated against previously published results for a portion of our sample. The distribution of [Fe/H] in our sample is consistent with that typical of the Solar neighbourhood. Additionally, we find the ages of most of our sample are less than 500 Myr, but note that we cannot determine robust ages from significantly older stars via chromospheric activity age indicators. The future meta-analysis of the frequency of wide stellar and sub-stellar companions imaged via the SEEDS survey will utilize our results to constrain the occurrence of detected comoving companions with the properties of their host stars. Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our understanding of the formation and evolution of planetary systems also requires a detailed understanding of the basic properties of their host stars. We have determined the basic stellar properties of F, K and G stars in the Strategic Exploration of Exoplanets and Disks with Subaru (SEEDS) survey from Echelle spectra taken at the Apache Point Observatory's 3.5m telescope. Using ROBOSPECT to extract line equivalent widths and TemperatureGravity microtrubulentVelocity ITerations to calculate the fundamental parameters, we have computed T-eff, log(g), v(t), [Fe/H], chromospheric activity and the age for our sample. Our methodology was calibrated against previously published results for a portion of our sample. The distribution of [Fe/H] in our sample is consistent with that typical of the Solar neighbourhood. Additionally, we find the ages of most of our sample are < 500 Myr, but note that we cannot determine robust ages from significantly older stars via chromospheric activity age indicators. The futuremeta-analysis of the frequency ofwide stellar and sub-stellar companions imaged via the SEEDS survey will utilize our results to constrain the occurrence of detected comoving companions with the properties of their host stars. |
| Audience | PUBLIC |
| Author | Morino, Jun-Ichi Takahashi, Yasuhiro H. Janson, Markus Brandner, Wolfgang Takato, Naruhisa Hayashi, Masahiko Hashimoto, Jun Knapp, Gillian R. Wisniewski, John P. Matsuo, Taro Abe, Lyu Grady, Carol A. Miyama, Shoken Pyo, Tae-Soo Moro-Martin, Amaya Schlieder, Joshua Watanade, Makoto Oh, Daehyeon Terada, Hiroshi Kusakabe, Nobuhiko Hebb, Leslie Fukagawa, Misato Sitko, Michael L. Kandori, Ryo Thalmann, Christian McElwain, Michael W. Akiyama, Eiji Cargile, Phillip Usuda, Tomonori Henning, Thomas Kuzuhara, Masayuki Tomono, Daigo Mayama, Satoshi Ishii, Miki Yamada, Toru Rich, Evan A. Okamoto, Yoshiko K. Takami, Hideki Brandt, Timothy D. Nishimura, Tetsuo Momose, Munetake Currie, Thayne M. Turner, Edwin L. Tamura, Motohide Takami, Michihiro Goto, Miwa Serabyn, Eugene Kwon, Jungmi Nakagawa, Takao Kudo, Tomoyuki Suenaga, Takuya Suzuki, Ryuji Suto, Hiroshi Hayano, Yutaka Carson, Joseph C. Feldt, Markus Helminiak, Krzysztof G. Iye, Masanori Hodapp, Klaus W. Guyon, Olivier Hayashi, Saeko S. Egner, Sebastian |
| Author_xml | – sequence: 1 givenname: Evan A. surname: Rich fullname: Rich, Evan A. organization: Oklahoma Univ – sequence: 2 givenname: John P. surname: Wisniewski fullname: Wisniewski, John P. organization: Oklahoma Univ – sequence: 3 givenname: Michael W. surname: McElwain fullname: McElwain, Michael W. organization: NASA Goddard Space Flight Center – sequence: 4 givenname: Jun surname: Hashimoto fullname: Hashimoto, Jun organization: National Inst. of Natural Sciences – sequence: 5 givenname: Tomoyuki surname: Kudo fullname: Kudo, Tomoyuki organization: Subaru Telescope – sequence: 6 givenname: Nobuhiko surname: Kusakabe fullname: Kusakabe, Nobuhiko organization: National Astronomical Observatory – sequence: 7 givenname: Yoshiko K. surname: Okamoto fullname: Okamoto, Yoshiko K. organization: Ibaraki Univ – sequence: 8 givenname: Lyu surname: Abe fullname: Abe, Lyu organization: Universite de Nice-Sophia Antipolis – sequence: 9 givenname: Eiji surname: Akiyama fullname: Akiyama, Eiji organization: Universite de Nice-Sophia Antipolis – sequence: 10 givenname: Wolfgang surname: Brandner fullname: Brandner, Wolfgang organization: Max-Planck-Inst. fuer Astronomie – sequence: 11 givenname: Timothy D. surname: Brandt fullname: Brandt, Timothy D. organization: Institute for Advanced Study – sequence: 12 givenname: Phillip surname: Cargile fullname: Cargile, Phillip organization: Harvard-Smithsonian Center for Astrophysics – sequence: 13 givenname: Joseph C. surname: Carson fullname: Carson, Joseph C. organization: College of Charleston – sequence: 14 givenname: Thayne M. surname: Currie fullname: Currie, Thayne M. organization: Subaru Telescope – sequence: 15 givenname: Sebastian surname: Egner fullname: Egner, Sebastian organization: Subaru Telescope – sequence: 16 givenname: Markus surname: Feldt fullname: Feldt, Markus organization: Subaru Telescope – sequence: 17 givenname: Misato surname: Fukagawa fullname: Fukagawa, Misato organization: Osaka Univ – sequence: 18 givenname: Miwa surname: Goto fullname: Goto, Miwa organization: NASA Goddard Space Flight Center – sequence: 19 givenname: Carol A. surname: Grady fullname: Grady, Carol A. organization: Eureka Scientific, Inc – sequence: 20 givenname: Olivier surname: Guyon fullname: Guyon, Olivier organization: Subaru Telescope – sequence: 21 givenname: Yutaka surname: Hayano fullname: Hayano, Yutaka organization: Subaru Telescope – sequence: 22 givenname: Masahiko surname: Hayashi fullname: Hayashi, Masahiko organization: National Astronomical Observatory – sequence: 23 givenname: Saeko S. surname: Hayashi fullname: Hayashi, Saeko S. organization: Subaru Telescope – sequence: 24 givenname: Leslie surname: Hebb fullname: Hebb, Leslie organization: Hobart and William Smith Coll – sequence: 25 givenname: Krzysztof G. surname: Helminiak fullname: Helminiak, Krzysztof G. organization: Nicolaus Copernicus Univ – sequence: 26 givenname: Thomas surname: Henning fullname: Henning, Thomas organization: Max-Planck-Inst. fuer Astronomie – sequence: 27 givenname: Klaus W. surname: Hodapp fullname: Hodapp, Klaus W. organization: Hawaii Univ – sequence: 28 givenname: Miki surname: Ishii fullname: Ishii, Miki organization: National Astronomical Observatory – sequence: 29 givenname: Masanori surname: Iye fullname: Iye, Masanori organization: National Astronomical Observatory – sequence: 30 givenname: Markus surname: Janson fullname: Janson, Markus organization: Stockholm Univ – sequence: 31 givenname: Ryo surname: Kandori fullname: Kandori, Ryo organization: National Astronomical Observatory – sequence: 32 givenname: Gillian R. surname: Knapp fullname: Knapp, Gillian R. organization: Princeton Univ – sequence: 33 givenname: Masayuki surname: Kuzuhara fullname: Kuzuhara, Masayuki organization: Tokyo Inst. of Tech – sequence: 34 givenname: Jungmi surname: Kwon fullname: Kwon, Jungmi organization: Tokyo Univ – sequence: 35 givenname: Taro surname: Matsuo fullname: Matsuo, Taro organization: Kyoto Univ – sequence: 36 givenname: Satoshi surname: Mayama fullname: Mayama, Satoshi organization: Graduate Univ. for Advanced Studies – sequence: 37 givenname: Shoken surname: Miyama fullname: Miyama, Shoken organization: Hiroshima Univ – sequence: 38 givenname: Munetake surname: Momose fullname: Momose, Munetake organization: Ibaraki Univ – sequence: 39 givenname: Jun-Ichi surname: Morino fullname: Morino, Jun-Ichi organization: National Astronomical Observatory – sequence: 40 givenname: Amaya surname: Moro-Martin fullname: Moro-Martin, Amaya organization: Space Telescope Science Inst – sequence: 41 givenname: Takao surname: Nakagawa fullname: Nakagawa, Takao organization: Institute of Space and Astronautical Science – sequence: 42 givenname: Tetsuo surname: Nishimura fullname: Nishimura, Tetsuo organization: National Astronomical Observatory – sequence: 43 givenname: Daehyeon surname: Oh fullname: Oh, Daehyeon organization: National Meteorological Satellite Center – sequence: 44 givenname: Tae-Soo surname: Pyo fullname: Pyo, Tae-Soo organization: Subaru Telescope – sequence: 45 givenname: Joshua surname: Schlieder fullname: Schlieder, Joshua organization: Max-Planck-Inst. fuer Astronomie – sequence: 46 givenname: Eugene surname: Serabyn fullname: Serabyn, Eugene organization: Jet Propulsion Lab., California Inst. of Tech – sequence: 47 givenname: Michael L. surname: Sitko fullname: Sitko, Michael L. organization: Cincinnati Univ – sequence: 48 givenname: Takuya surname: Suenaga fullname: Suenaga, Takuya organization: National Astronomical Observatory – sequence: 49 givenname: Hiroshi surname: Suto fullname: Suto, Hiroshi organization: National Astronomical Observatory – sequence: 50 givenname: Ryuji surname: Suzuki fullname: Suzuki, Ryuji organization: National Astronomical Observatory – sequence: 51 givenname: Yasuhiro H. surname: Takahashi fullname: Takahashi, Yasuhiro H. organization: National Astronomical Observatory – sequence: 52 givenname: Michihiro surname: Takami fullname: Takami, Michihiro organization: Academia Sinica – sequence: 53 givenname: Naruhisa surname: Takato fullname: Takato, Naruhisa organization: Subaru Telescope – sequence: 54 givenname: Hiroshi surname: Terada fullname: Terada, Hiroshi organization: Subaru Telescope – sequence: 55 givenname: Christian surname: Thalmann fullname: Thalmann, Christian organization: Eidgenoessische Technische Hochschule – sequence: 56 givenname: Daigo surname: Tomono fullname: Tomono, Daigo organization: Subaru Telescope – sequence: 57 givenname: Edwin L. surname: Turner fullname: Turner, Edwin L. organization: Institute for Advanced Study – sequence: 58 givenname: Makoto surname: Watanade fullname: Watanade, Makoto organization: Hokkaido Univ – sequence: 59 givenname: Toru surname: Yamada fullname: Yamada, Toru organization: Tohoku Univ – sequence: 60 givenname: Hideki surname: Takami fullname: Takami, Hideki organization: National Astronomical Observatory – sequence: 61 givenname: Tomonori surname: Usuda fullname: Usuda, Tomonori organization: National Astronomical Observatory – sequence: 62 givenname: Motohide surname: Tamura fullname: Tamura, Motohide organization: National Astronomical Observatory |
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| Keywords | Temperature Gravity Microtrubulent Velocity Iterations Strategic Exploration Of Exoplanets And Disks With Subaru (seeds stars: fundamental parameters – planetary systems stars: abundances |
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| Snippet | Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our... Abstract Large exoplanet surveys have successfully detected thousands of exoplanets to-date. Utilizing these detections and non-detections to constrain our... |
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| SubjectTerms | Astrophysics Earth Resources And Remote Sensing planetary systems stars: abundances stars: fundamental parameters |
| Title | The Fundamental Stellar Parameters of FGK Stars in the SEEDS Survey Norman, OK 73071, USA |
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