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RN

R. New

astro-ph.SRastro-phastro-ph.EPastro-ph.IMhep-th

On Valency

published · living versions
W_q4evxp3r·v1 · currentpublished
The asteroseismic potential of Kepler: first results for solar-type stars
with W. J. Chaplin, T. Appourchaux, Y. Elsworth, R. A. Garcia +103
1 version

Preprints & journals

30 papers in the corpus · 1997–2011
Ensemble asteroseismology of solar-type stars with the NASA Kepler mission.21474754 · Chaplin, W J, Kjeldsen, H, Christensen-Dalsgaard, J et al.2011 · 314 citationsScience (New York, N.Y.). 2011;332(6026):213-6
Predicting the detectability of oscillations in solar-type stars observed by Kepler1103.0702v1 · W. J. Chaplin, H. Kjeldsen, T. R. Bedding et al.2011 · 154 citationsarXiv
Solar cycle variations of large frequency separations of acoustic modes: Implications for asteroseismology1102.0906v2 · A.-M. Broomhall, W.J. Chaplin, Y. Elsworth et al.2011 · 17 citationsarXiv
Are short-term variations in solar oscillation frequencies the signature of a second solar dynamo?1012.4933v1 · Anne-Marie Broomhall, Stephen T. Fletcher, David Salabert et al.2010 · 13 citationsarXiv
A precise asteroseismic age and radius for the evolved Sun-like star KIC 110267641010.4329v1 · T.S. Metcalfe, M.J.P.F.G. Monteiro, M.J. Thompson et al.2010 · 160 citationsAstrophys.J.723:1583-1598,2010
A seismic signature of a second dynamo?1006.4305v1 · Stephen T. Fletcher, Anne-Marie Broomhall, David Salabert et al.2010 · 135 citationsarXiv
The New Solar Minimum: How deep does the problem go?1003.4228v1 · Stephen Fletcher, Roger New, Anne-Marie Broomhall et al.2010 · 1 citationarXiv
Differences between the current solar minimum and earlier minima1003.4262v1 · Sarbani Basu, Anne-Marie Broomhall, William J. Chaplin et al.2010 · 4 citationsarXiv
The asteroseismic potential of Kepler: first results for solar-type stars1001.0506v2 · W. J. Chaplin, T. Appourchaux, Y. Elsworth et al.2010 · 154 citationsarXivon Valency
Is the current lack of solar activity only skin deep?0907.3417v1 · A. -M. Broomhall, W. J. Chaplin, Y. Elsworth et al.2009 · 63 citationsAstrophysical Journal Letters 700 (2009) L162-L165
Corrections of Sun-as-a-star p-mode frequencies for effects of the solar cycle0907.2855v1 · A. -M. Broomhall, W. J. Chaplin, Y. Elsworth et al.2009 · 6 citationsarXiv
Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission0906.0766v1 · D. Stello, W. J. Chaplin, H. Bruntt et al.2009 · 183 citationsAstrophys.J.700:1589-1602,2009on Valency
Mode lifetimes of stellar oscillations - Implications for asteroseismology0905.1722v3 · W. J. Chaplin, G. Houdek, C. Karoff et al.2009 · 78 citationsarXiv
New aspects of Doppler imaging in Sun-as-a-star observations0904.4122v1 · A. M. Broomhall, W. J. Chaplin, Y. Elsworth et al.2009 · 8 citationsarXiv
Pseudo-global Fitting of Gapped Helioseismic Data0904.4126v1 · S. T. Fletcher, W. J. Chaplin, Y. Elsworth et al.2009 · 0 citationsarXiv
Excitation and damping of p-mode oscillations of alpha Cen B0810.5022v1 · W. J. Chaplin, G. Houdek, Y. Elsworth et al.2008 · 14 citationsAstrophys.J.692:531-537,2009
The inhomogeneous response across the solar disc of unresolved Doppler velocity observations0810.3856v1 · A. M. Broomhall, W. J. Chaplin, Y. Elsworth et al.2008 · 0 citationsarXiv
Are low-degree p mode frequencies predictable from one cycle to the next?0810.3591v1 · A. M. Broomhall, W. J. Chaplin, Y. Elsworth et al.2008 · 0 citationsarXiv
solarFLAG hare and hounds: estimation of p-mode frequencies from Sun-as-star helioseismology data0807.0989v1 · S. J. Jimenez-Reyes, W. J. Chaplin, R. A. Garcia et al.2008 · 18 citationsarXiv
Challenges for asteroseismic analysis of Sun-like stars0804.4371v2 · W. J. Chaplin, G. Houdek, T. Appourchaux et al.2008 · 74 citationsarXiv
AsteroFLAG: first results from hare-and-hounds Exercise 10803.4143v1 · W.J. Chaplin, T. Appourchaux, T. Arentoft et al.2008 · 39 citationsarXiv
A modified peak-bagging technique for fitting low-ℓ\ell solar p-modes0803.3033v1 · S. T. Fletcher, W. J. Chaplin, Y. Elsworth et al.2008 · 3 citationsarXiv
A devil in the detail: parameter cross-talk from the solar cycle and estimation of solar p-mode frequencies0801.1431v2 · W. J. Chaplin, S. J. Jimenez-Reyes, A. Eff-Darwich et al.2008 · 2 citationsarXiv
Solar abundances and helioseismology: fine structure spacings and separation ratios of low-degree p modesastro-ph/0610052v1 · Sarbani Basu (Yale), William J. Chaplin (Birmingham, U.K.) et al.2006 · 89 citationsAstrophys.J.655:660-671,2007
solarFLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star dataastro-ph/0606748v1 · W. J. Chaplin, T. Appourchaux, F. Baudin et al.2006 · 46 citationsMon.Not.Roy.Astron.Soc.369:985-996,2006
The solar core: new low-l p-mode fine-spacing results from BiSONastro-ph/9702141v3 · W. J. Chaplin, Y. Elsworth, G. R. Isaak et al.1997 · 4 citationsarXiv
Solar internal sound speed as inferred from combined BiSON and LOWL oscillation frequenciesastro-ph/9702105v1 · Sarbani Basu, W. J. Chaplin, J. Christensen-Dalsgaard et al.1997 · 120 citationsMon.Not.Roy.Astron.Soc.292:243-251,1997
Career total: 143 works. 30 are in this corpus.

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