​

• Lund, M. N.; Silva Aguirre, V., Davies, G. R., et al., Standing on the shoulders of dwarfs: the Kepler asteroseismic LEGACY sample. I. - oscillation mode parameters, (2016), Apj (in press) [Link]

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• Silva Aguirre, V., Lund, M. N.; Antia, H. M., et al., Standing on the shoulders of dwarfs: the Kepler asteroseismic LEGACY sample. II. - radii, masses, and ages, (2016), Apj (in press) [Link]

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• Lund, M. N., Handberg, R., Kjeldsen, H., Chaplin, W. J., & Christensen-Dalsgaard, J., Data preparation for asteroseismology with TESS, (2016), EPJ Web of Conferences (in press) [Link]

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• Handberg, R.; Lund, M. N., K2P²: Reduced data from campaigns 0-4 of the K2 mission, (2017), A&A, 597, 36 [Link]

 

• Lund, M. N.; Basu, S., Silva Aguirre, V., et al., Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster, (2016), MNRAS, 463, 2600 [Link]

 

• Lund, M. N.; Chaplin, W. J., Casagrande, L., et al., Asteroseismic properties of solar-type stars observed with the NASA K2 mission: results from Campaigns 1-3 and prospects for future observations, (2016), PASP, 128, 124204 [Link]

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• Campante, T. L.; Lund, M. N.; Kuszlewicz, J. S., et al., Spin-Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology, (2016), ApJ, 819, 85 [Link]​

 

• Chaplin, W. J.; Lund, M. N.; Handberg, R., et al., Asteroseismology of Solar-Type Stars with K2: Detection of Oscillations in C1 Data, (2015), PASP, 127, 1038 [Link]​

 

• Lund, M. N., Handberg, R., Davies, G. R., Chaplin, W. J., & Jones, C. D., K2P² - A photometry pipeline for the K2 mission, (2015), ApJ, 806, 30 [Link]​

 

• Handberg, R., & Lund, M. N., Automated preparation of Kepler time series of planet hosts for asteroseismic analysis, 2014, MNRAS, 445, 2698 [Link]​

 

• Lund, M. N., Lundkvist, M., Silva Aguirre, V., et al., Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7, (2014), A&A, 570, 54 [Link]​

 

• Lund, M. N., Miesch, M. S., & Christensen-Dalsgaard, J., Differential Rotation in Main-sequence Solar-like Stars: Qualitative Inference from Asteroseismic Data, (2014), ApJ, 790, 121 [Link]​

 

• Van Eylen, V., Lund, M. N., Silva Aguirre, V., et al., What Asteroseismology can do for Exoplanets: Kepler-410A b is a Small Neptune around a Bright Star, in an Eccentric Orbit Consistent with Low Obliquity, (2014), ApJ, 782, 14 [Link]

 

• Lund, M. N., Kjeldsen, H., Christensen-Dalsgaard, J., Handberg, R., & Silva Aguirre, V., Detection of l = 4 and l = 5 Modes in 12 Years of Solar VIRGO-SPM Data—Tests on Kepler Observations of 16 Cyg A and B, (2014), ApJ, 782, 2 [Link]​​​

 

• Lund, M. N., Chaplin, W. J., & Kjeldsen, H., A new method to detect solar-like oscillations at very low S/N using statistical significance testing, (2012), MNRAS, 427, 1784 [Link]

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