W. Chaplin

发表

The K2 Galactic Caps Project – going beyond the Kepler field and ageing the Galactic disc

C. Chiappini, K. Cunha, D. Feuillet, 2019, Monthly Notices of the Royal Astronomical Society.

PLATO as it is: a legacy mission for Galactic archaeology

N. A. Walton, D. Katz, R. Ibata, 2017, 1706.03778.

Signatures of Magnetic Activity in the Seismic Data of Solar-type Stars Observed by Kepler

W. Chaplin, T. Campante, G. Davies, 2018, The Astrophysical Journal Supplement Series.

Excitation and Damping of Low-Degree Solar p-Modes during Activity Cycle 23: Analysis of GOLF and VIRGO Sun Photometer Data

W. Chaplin, R. García, S. Jiménez-Reyes, 2003 .

Asteroseismic inferences on red giants in open clusters NGC 6791, NGC 6819, and NGC 6811 using Kepler

F. Grundahl, R. Gilliland, J. Ridder, 2011, 1104.4393.

THE APOGEE RED-CLUMP CATALOG: PRECISE DISTANCES, VELOCITIES, AND HIGH-RESOLUTION ELEMENTAL ABUNDANCES OVER A LARGE AREA OF THE MILKY WAY'S DISK

Lars Koesterke, Yvonne Elsworth, Annie C. Robin, 2014, 1405.1032.

Kepler observations of the asteroseismic binary HD 176465

H. M. Antia, P. Gaulme, T. Bedding, 2016, 1609.09581.

ASTEROSEISMIC DETERMINATION OF OBLIQUITIES OF THE EXOPLANET SYSTEMS KEPLER-50 AND KEPLER-65

W. D. Cochran, S. D. Kawaler, J. Christensen-Dalsgaard, 2013, 1302.3728.

Very regular high-frequency pulsation modes in young intermediate-mass stars

D. Huber, C. McCully, M. Ireland, 2020, Nature.

MEASUREMENT OF ACOUSTIC GLITCHES IN SOLAR-TYPE STARS FROM OSCILLATION FREQUENCIES OBSERVED BY KEPLER

J. Christensen-Dalsgaard, H. M. Antia, S. Mathur, 2013, 1312.4907.

Asteroseismic surface gravity for evolved stars

W. Chaplin, S. Basu, Y. Elsworth, 2013, 1305.6586.

Perspectives in Global Helioseismology and the Road Ahead

W. Chaplin, Sarbani Basu, 2008, 0801.4213.

Characterizing Host Stars Using Asteroseismology

D. Huber, W. Chaplin, M. Lundkvist, 2018 .

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

H. R. Coelho, H. M. Antia, P. Gaulme, 2015, 1507.01827.

Observational Upper Limits to Low-Degree Solar g-Modes

William J. Chaplin, W. Finsterle, Claus Fröhlich, 2000 .

Combining multiple structural inversions to constrain the solar modelling problem

V. Baturin, G. Meynet, W. Chaplin, 2018, Astronomy & Astrophysics.

TESS asteroseismology of the known planet host star λ2 Fornacis

K. Stassun, D. Buzasi, W. Chaplin, 2020, Astronomy & Astrophysics.

The solar-like CoRoT ? target HD 170987: spectroscopic and seismic observations

P. Gaulme, D. Huber, W. Chaplin, 2010, 1004.4891.

Establishing the accuracy of asteroseismic mass and radius estimates of giant stars - I. Three eclipsing systems at [Fe/H] ∼ -0.3 and the need for a large high-precision sample

F. Grundahl, C. Hansen, W. Chaplin, 2018, 1801.08167.

Quasi-biennial variations in helioseismic frequencies: can the source of the variation be localized?

R. Simoniello, W. Chaplin, Y. Elsworth, 2011, 1111.2492.

A comparison of frequentist and Bayesian inference: searching for low-frequency p modes and g modes in Sun-as-a-star data

W. Chaplin, Y. Elsworth, A. Broomhall, 2010, 1004.4505.

Observations

G. R. Davies, W. Chaplin, Y. Elsworth, 2009, Castlemaine Naturalist.

solarFLAG hare and hounds: estimation of p-mode frequencies from Sun-as-star helioseismology data

W. Chaplin, Y. Elsworth, R. Wachter, 2008, 0807.0989.

A framework for describing correlated excitation of solar p‐modes

Y. Elsworth, T. Toutain, W. Chaplin, 2008, 0804.3338.

A modified peak-bagging technique for fitting low-l solar p-modes

S. Fletcher, R. New, W. Chaplin, 2008, 0803.3033.

On the Variation of the Peak Asymmetry of Low-ℓ Solar p Modes

W. Chaplin, Y. Elsworth, H. Socas-Navarro, 2007 .

A Comparison of Low-Degree Solar p-Mode Parameters from BiSON and GONG: Underlying Values and Temporal Variations

W. Chaplin, Y. Elsworth, F. Hill, 2003 .

UvA-DARE ( Digital Academic Repository ) Asteroseismic Fundamental Properties of Solar-type Stars Observed by the NASA

P. Gaulme, H. Kjeldsen, S. Basu, 2013 .

DETECTION OF SOLAR-LIKE OSCILLATIONS, OBSERVATIONAL CONSTRAINTS, AND STELLAR MODELS FOR θ CYG, THE BRIGHTEST STAR OBSERVED BY THE KEPLER MISSION

P. Gaulme, F. Mullally, C. Aerts, 2016, 1607.01035.

UvA-DARE ( Digital Academic Repository ) Accurate fundamental parameters and detailed abundance patterns from spectroscopy of 93 solar-type Kepler targets

P. Quirion, T. Bedding, H. Kjeldsen, 2012 .

Challenges for asteroseismic analysis of Sun-like stars

W. Chaplin, Y. Elsworth, R. New, 2008, 0804.4371.

Mode lifetimes of stellar oscillations - Implications for asteroseismology

W. Chaplin, Y. Elsworth, C. Karoff, 2009, 0905.1722.

Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265

F. Baudin, T. Appourchaux, L. Gizon, 2011, 1105.3551.

PREDICTING THE DETECTABILITY OF OSCILLATIONS IN SOLAR-TYPE STARS OBSERVED BY KEPLER

P. Gaulme, M. Pinsonneault, P. Quirion, 2011, 1103.0702.

Prospects for asteroseismic inference on the envelope helium abundance in red giant stars

Y. Elsworth, A. Miglio, P. Eggenberger, 2014, 1403.7045.

On the relation between activity-related frequency shifts and the sunspot distribution over the solar cycle 23

W. Chaplin, T. Campante, P. Avelino, 2016, 1611.07475.

Corrections of Sun-as-a-star p-mode frequencies for effects of the solar cycle

W. Chaplin, Y. Elsworth, S. Fletcher, 2009, 0907.2855.

Solar-cycle variations of large frequency separations of acoustic modes: implications for asteroseismology

W. Chaplin, Y. Elsworth, A. Broomhall, 2011, 1102.0906.

Solar p-mode frequencies at (cid:1) = 2: What do analyses of unresolved observations actually measure?

R. New, T. Appourchaux, T. Toutain, 2008 .