Please use numbered references in your WP document. Here include under your WP title the list of references corresponding to your numbering.
- Suárez et al. 2014, “Measuring mean densities of δ Scuti stars with asteroseismology. Theoretical properties of large separations using TOUCAN”, A&A 563, 7 (2014)
MOST: Walker, G., et al., 2003, PASP, 115, 1023
CoRoT: Bagline at al., 2006, ESA SP-1306, Nordwik, 33
Kepler: Borucki et al. 2010, Science, 327, 977
GAIA: Perryman et al. 2001, A&A 369, 339
CHEOPS: Fortier et al. 2013, Proc. SPIE 9143, id. 91432J
TESS: Ricker et al. 2014, J. Astron. Telesc. Instrum. Syst. 1, 014003
HARPS@ESO: Mayor et al. 2003, The Messenger, 114, 20
HARPS-N@TNG: Cosentino et al. 2014, Proc. SPIE 9147, id. 91478C
CARMENES: Quirrenbach et al. 2014, Proc. SPIE 9147, id 91471F.
About OSN, I guess you (or Rafa) are better placed than me to give a reference …
SOPHIE instrument:Perruchot et al., 2008, Proc. SPIE 7014, id. 70140J
[0] Balona, L. (2013), “Activity in A-type stars”, in MNRAS, 431, 2240B
[1] Balona, L. (2014), “Mode density and frequency extraction in the δ Scuti star HD 50844”, in MNRAS, 439, 3453B
[2] Espinosa Lara F. and Rieutord M. (2007), “The dynamics of a fully radiative rapidly rotating star enclosed within a spherical box”, in Astron. Astrophys., vol. 470, p. 1013-1022
[3] Espinosa Lara F. and Rieutord M. (2013), “Self-consistent 2D models of fast rotating early-type stars”, in Astron. Astrophys., vol. 552, A35
[4] García Hernández, A.; Moya, A.; Michel, E.; Garrido, R.; Suárez, J. C.; Rodríguez, E.; Amado, P. J.; Martín-Ruiz, S.; Rolland, A.; Poretti, E.; Samadi, R.; Baglin, A.; Auvergne, M.; Catala, C.; Lefevre, L.; Baudin, F. (2009), “Asteroseismic analysis of the CoRoT δ Scuti star HD 174936”, in Astron. Astrophys., 506, 79G
[5] García Hernández, A.; Moya, A.; Michel, E.; Suárez, J. C.; Poretti, E.; Martín-Ruíz, S.; Amado, P. J.; Garrido, R.; Rodríguez, E.; Rainer, M.; Uytterhoeven, K.; Rodrigo, C.; Solano, E.; Rodón, J. R.; Mathias, P.; Rolland, A.; Auvergne, M.; Baglin, A.; Baudin, F.; Catala, C.; Samadi, R. (2013), “An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars”, in Astron. Astrophys., 559A, 63G
[6] Lignières, F.; Rieutord, M.; Reese, D. (2006), “Acoustic oscillations of rapidly rotating polytropic stars. I. Effects of the centrifugal distortion”, in Astron. Astrophys., 455, 607L
[7] Lignières, F.; Georgeot, B.; Ballot, J. (2010), “P-modes in rapidly rotating stars: Looking for regular patterns in synthetic asymptotic spectra”, in Astron. Nachr., 331, 1053L
[8] Miglio, A.; Montalbán, J.; Noels, A.; Eggenberger, P. (2008), “Probing the properties of convective cores through g modes: high-order g modes in SPB and γ Doradus stars”, MNRAS, 386, 1487M
[9] Pascual-Granado, J.; Garrido, R.; Suárez, J. C. (2015), “MIARMA: A minimal-loss information method for filling gaps in time series. Application to CoRoT light curves”, in Astron. Astrophys., 575A, 78P
[10] Poretti, E.; Michel, E.; Garrido, R.; Lefèvre, L.; Mantegazza, L.; Rainer, M.; Rodríguez, E.; Uytterhoeven, K.; Amado, P. J.; Martín-Ruiz, S.; Moya, A.; Niemczura, E.; Suárez, J. C.; Zima, W.; Baglin, A.; Auvergne, M.; Baudin, F.; Catala, C.; Samadi, R.; Alvarez, M.; Mathias, P.; Paparò, M.; Pápics, P.; Plachy, E. (2009), “HD 50844: a new look at δ Scuti stars from CoRoT space photometry”, 506, 85P
[11] Reese, D.; Lignières, F.; Rieutord, M. (2006), “Acoustic oscillations of rapidly rotating polytropic stars. II. Effects of the Coriolis and centrifugal accelerations”, in Astron. Astrophys., 455, 621R
[12] Reese, D.; Lignières, F.; Rieutord, M. (2008), “Regular patterns in the acoustic spectrum of rapidly rotating stars”, in Astron. Astrophys., 481, 499R
[13] Reese, D. R.; MacGregor, K. B.; Jackson, S.; Skumanich, A.; Metcalfe, T. S. (2009), “Pulsation modes in rapidly rotating stellar models based on the self-consistent field method”, in Astron. Astrophys., 506, 189R
[14] Reese, D. R. (2013), “Stable higher order finite-difference schemes for stellar pulsation calculations”, in Astron. Astrophys., 555A, 148R
[15] Rieutord M. and Espinosa Lara F. (2009), “On the dynamics of a radiative rapidly rotating star”, in Comm. Asterosismology, vol. 158., pp. 99-103
[16] Rieutord M. and Espinosa Lara F. (2013), “Ab initio modelling of steady rotating stars”, in Seismology for studies of stellar rotation and convection , Edts Goupil et al., Lecture Notes in Physics, vol. 865, p. 49, Springer
[17] Suárez, J. C.; García Hernández, A.; Moya, A.; Rodrigo, C.; Solano, E.; Garrido, R.; Rodón, J. R. (2014), “Measuring mean densities of δ Scuti stars with asteroseismology. Theoretical properties of large separations using TOUCAN”, in Astron. Astrophys., 563A, 7S
[18] Van Reeth, T.; Tkachenko, A.; Aerts, C.; Pápics, P. I.; Degroote, P.; Debosscher, J.; Zwintz, K.; Bloemen, S.; De Smedt, K.; Hrudkova, M.; Raskin, G.; Van Winckel, H. (2015), “Detecting non-uniform period spacings in the Kepler photometry of γ Doradus stars: methodology and case studies”, in Astron. Astrophys., 574A, 71V
Christiansen et al., 2013, Kepler Data Characteristics Handbook (KSCI-19040-004).
Scargle, J. D., Astrophys. J. 1982 263, 835-853
Pascual-Granado, J., Garrido, R., & Suárez, J. C. 2014, in IAU Symp. 301, eds. J. A. Guzik, W. J. Chaplin, G. Handler, & A. Pigulski, 85