Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data

W. J. Chaplin; M. N. Lund; R. Handberg; S. Basu; L. A. Buchhave; T. L. Campante; G. R. Davies; D. Huber; D. W. Latham; C. A. Latham; A. Serenelli; H. M. Antia; T. Appourchaux; W. H. Ball; O. Benomar; L. Casagrande; J. Christensen-Dalsgaard; H. R. Coelho; O. L. Creevey; Y. Elsworth; R. A. García; P. Gaulme; S. Hekker; T. Kallinger; C. Karoff; S. D. Kawaler; H. Kjeldsen; M. S. Lundkvist; F. Marcadon; S. Mathur; A. Miglio; B. Mosser; C. Régulo; I. W. Roxburgh; V. Silva Aguirre; D. Stello; K. Verma; T. R. White; T. R. Bedding; T. Barclay; D. L. Buzasi; S. Dehuevels; L. Gizon; G. Houdek; S. B. Howell; D. Salabert; D. R. Soderblom

doi:10.1086/683103

Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data

W. J. Chaplin
, M. N. Lund
, R. Handberg
, S. Basu
, L. A. Buchhave
, T. L. Campante
, G. R. Davies
, D. Huber
, D. W. Latham
, C. A. Latham
, A. Serenelli
, H. M. Antia
, T. Appourchaux
, W. H. Ball
, O. Benomar
, L. Casagrande
, J. Christensen-Dalsgaard
, H. R. Coelho
, O. L. Creevey
, Y. Elsworth

R. A. García, P. Gaulme, S. Hekker, T. Kallinger, C. Karoff, S. D. Kawaler, H. Kjeldsen, M. S. Lundkvist, F. Marcadon, S. Mathur, A. Miglio, B. Mosser, C. Régulo, I. W. Roxburgh, V. Silva Aguirre, D. Stello, K. Verma, T. R. White, T. R. Bedding, T. Barclay, D. L. Buzasi, S. Dehuevels, L. Gizon, G. Houdek, S. B. Howell, D. Salabert, D. R. Soderblom

Research output: Contribution to journal › Article › peer-review

30 Citations (Scopus)

Abstract

We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We understand the asteroseismic detection thresholds for C1-like levels of photometric performance, and we can detect oscillations in subgiants having dominant oscillation frequencies around 1000 μHz. Changes to the operation of the fine-guidance sensors are expected to give significant improvements in the high-frequency performance from C3 onwards. A reduction in the excess high-frequency noise by a factor of 2.5 in amplitude would bring main-sequence stars with dominant oscillation frequencies as high as ≃2500 μHz into play as potential asteroseismic targets for K2.

Original language	English
Pages (from-to)	1038-1044
Number of pages	7
Journal	Publications of the Astronomical Society of the Pacific
Volume	127
Issue number	956
DOIs	https://doi.org/10.1086/683103
Publication status	Published - Oct 2015

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Chaplin, W. J., Lund, M. N., Handberg, R., Basu, S., Buchhave, L. A., Campante, T. L., Davies, G. R., Huber, D., Latham, D. W., Latham, C. A., Serenelli, A., Antia, H. M., Appourchaux, T., Ball, W. H., Benomar, O., Casagrande, L., Christensen-Dalsgaard, J., Coelho, H. R., Creevey, O. L., ... Soderblom, D. R. (2015). Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data. Publications of the Astronomical Society of the Pacific, 127(956), 1038-1044. https://doi.org/10.1086/683103

@article{5171e1977cc04e4ca0c4da548d15dbdd,

title = "Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data",

abstract = "We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We understand the asteroseismic detection thresholds for C1-like levels of photometric performance, and we can detect oscillations in subgiants having dominant oscillation frequencies around 1000 μHz. Changes to the operation of the fine-guidance sensors are expected to give significant improvements in the high-frequency performance from C3 onwards. A reduction in the excess high-frequency noise by a factor of 2.5 in amplitude would bring main-sequence stars with dominant oscillation frequencies as high as ≃2500 μHz into play as potential asteroseismic targets for K2.",

author = "Chaplin, \{W. J.\} and Lund, \{M. N.\} and R. Handberg and S. Basu and Buchhave, \{L. A.\} and Campante, \{T. L.\} and Davies, \{G. R.\} and D. Huber and Latham, \{D. W.\} and Latham, \{C. A.\} and A. Serenelli and Antia, \{H. M.\} and T. Appourchaux and Ball, \{W. H.\} and O. Benomar and L. Casagrande and J. Christensen-Dalsgaard and Coelho, \{H. R.\} and Creevey, \{O. L.\} and Y. Elsworth and Garc{\'i}a, \{R. A.\} and P. Gaulme and S. Hekker and T. Kallinger and C. Karoff and Kawaler, \{S. D.\} and H. Kjeldsen and Lundkvist, \{M. S.\} and F. Marcadon and S. Mathur and A. Miglio and B. Mosser and C. R{\'e}gulo and Roxburgh, \{I. W.\} and Aguirre, \{V. Silva\} and D. Stello and K. Verma and White, \{T. R.\} and Bedding, \{T. R.\} and T. Barclay and Buzasi, \{D. L.\} and S. Dehuevels and L. Gizon and G. Houdek and Howell, \{S. B.\} and D. Salabert and Soderblom, \{D. R.\}",

year = "2015",

month = oct,

doi = "10.1086/683103",

language = "English",

volume = "127",

pages = "1038--1044",

journal = "Publications of the Astronomical Society of the Pacific",

issn = "0004-6280",

publisher = "Institute of Physics",

number = "956",

}

Chaplin, WJ, Lund, MN, Handberg, R, Basu, S, Buchhave, LA, Campante, TL, Davies, GR, Huber, D, Latham, DW, Latham, CA, Serenelli, A, Antia, HM, Appourchaux, T, Ball, WH, Benomar, O, Casagrande, L, Christensen-Dalsgaard, J, Coelho, HR, Creevey, OL, Elsworth, Y, García, RA, Gaulme, P, Hekker, S, Kallinger, T, Karoff, C, Kawaler, SD, Kjeldsen, H, Lundkvist, MS, Marcadon, F, Mathur, S, Miglio, A, Mosser, B, Régulo, C, Roxburgh, IW, Aguirre, VS, Stello, D, Verma, K, White, TR, Bedding, TR, Barclay, T, Buzasi, DL, Dehuevels, S, Gizon, L, Houdek, G, Howell, SB, Salabert, D & Soderblom, DR 2015, 'Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data', Publications of the Astronomical Society of the Pacific, vol. 127, no. 956, pp. 1038-1044. https://doi.org/10.1086/683103

TY - JOUR

T1 - Asteroseismology of Solar-Type Stars with K2

T2 - Detection of oscillations in C1 Data

AU - Chaplin, W. J.

AU - Lund, M. N.

AU - Handberg, R.

AU - Basu, S.

AU - Buchhave, L. A.

AU - Campante, T. L.

AU - Davies, G. R.

AU - Huber, D.

AU - Latham, D. W.

AU - Latham, C. A.

AU - Serenelli, A.

AU - Antia, H. M.

AU - Appourchaux, T.

AU - Ball, W. H.

AU - Benomar, O.

AU - Casagrande, L.

AU - Christensen-Dalsgaard, J.

AU - Coelho, H. R.

AU - Creevey, O. L.

AU - Elsworth, Y.

AU - García, R. A.

AU - Gaulme, P.

AU - Hekker, S.

AU - Kallinger, T.

AU - Karoff, C.

AU - Kawaler, S. D.

AU - Kjeldsen, H.

AU - Lundkvist, M. S.

AU - Marcadon, F.

AU - Mathur, S.

AU - Miglio, A.

AU - Mosser, B.

AU - Régulo, C.

AU - Roxburgh, I. W.

AU - Aguirre, V. Silva

AU - Stello, D.

AU - Verma, K.

AU - White, T. R.

AU - Bedding, T. R.

AU - Barclay, T.

AU - Buzasi, D. L.

AU - Dehuevels, S.

AU - Gizon, L.

AU - Houdek, G.

AU - Howell, S. B.

AU - Salabert, D.

AU - Soderblom, D. R.

PY - 2015/10

Y1 - 2015/10

N2 - We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We understand the asteroseismic detection thresholds for C1-like levels of photometric performance, and we can detect oscillations in subgiants having dominant oscillation frequencies around 1000 μHz. Changes to the operation of the fine-guidance sensors are expected to give significant improvements in the high-frequency performance from C3 onwards. A reduction in the excess high-frequency noise by a factor of 2.5 in amplitude would bring main-sequence stars with dominant oscillation frequencies as high as ≃2500 μHz into play as potential asteroseismic targets for K2.

AB - We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We understand the asteroseismic detection thresholds for C1-like levels of photometric performance, and we can detect oscillations in subgiants having dominant oscillation frequencies around 1000 μHz. Changes to the operation of the fine-guidance sensors are expected to give significant improvements in the high-frequency performance from C3 onwards. A reduction in the excess high-frequency noise by a factor of 2.5 in amplitude would bring main-sequence stars with dominant oscillation frequencies as high as ≃2500 μHz into play as potential asteroseismic targets for K2.

UR - https://www.scopus.com/pages/publications/84944596937

U2 - 10.1086/683103

DO - 10.1086/683103

M3 - Article

SN - 0004-6280

VL - 127

SP - 1038

EP - 1044

JO - Publications of the Astronomical Society of the Pacific

JF - Publications of the Astronomical Society of the Pacific

IS - 956

ER -

Asteroseismology of Solar-Type Stars with K2: Detection of oscillations in C1 Data

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