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Benchmarking the power of amateur observatories for TTV exoplanets detection. / Baluev, R.V.; Sokov, E.N.; Shaidulin, V.S.; Sokova, I.A.; Jones, H.R.A.; Tuomi, M.; Anglada-Escudé, G.; Benni, P.; Colazo, C.A.; Schneiter, M.E.; Villarreal D'Angelo, C.S.; Burdanov, A.Y.; Fernández-Laj s, E.; Ba türk, O.; Hentunen, V.-P.; Shadick, A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 450, No. 3, 2015, p. 3101-3113.

Research output: Contribution to journal › Article

Harvard

Baluev, RV, Sokov, EN, Shaidulin, VS, Sokova, IA, Jones, HRA, Tuomi, M, Anglada-Escudé, G, Benni, P, Colazo, CA, Schneiter, ME, Villarreal D'Angelo, CS, Burdanov, AY, Fernández-Laj s, E, Ba türk, O, Hentunen, V-P & Shadick, A 2015, 'Benchmarking the power of amateur observatories for TTV exoplanets detection', Monthly Notices of the Royal Astronomical Society, vol. 450, no. 3, pp. 3101-3113. https://doi.org/10.1093/mnras/stv788

APA

Baluev, R. V., Sokov, E. N., Shaidulin, V. S., Sokova, I. A., Jones, H. R. A., Tuomi, M., Anglada-Escudé, G., Benni, P., Colazo, C. A., Schneiter, M. E., Villarreal D'Angelo, C. S., Burdanov, A. Y., Fernández-Laj s, E., Ba türk, O., Hentunen, V-P., & Shadick, A. (2015). Benchmarking the power of amateur observatories for TTV exoplanets detection. Monthly Notices of the Royal Astronomical Society, 450(3), 3101-3113. https://doi.org/10.1093/mnras/stv788

Vancouver

Baluev RV, Sokov EN, Shaidulin VS, Sokova IA, Jones HRA, Tuomi M et al. Benchmarking the power of amateur observatories for TTV exoplanets detection. Monthly Notices of the Royal Astronomical Society. 2015;450(3):3101-3113. https://doi.org/10.1093/mnras/stv788

Author

Baluev, R.V. ; Sokov, E.N. ; Shaidulin, V.S. ; Sokova, I.A. ; Jones, H.R.A. ; Tuomi, M. ; Anglada-Escudé, G. ; Benni, P. ; Colazo, C.A. ; Schneiter, M.E. ; Villarreal D'Angelo, C.S. ; Burdanov, A.Y. ; Fernández-Laj s, E. ; Ba türk, O. ; Hentunen, V.-P. ; Shadick, A. / Benchmarking the power of amateur observatories for TTV exoplanets detection. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 450, No. 3. pp. 3101-3113.

BibTeX

@article{6f35ca769f094ea1bad5f5dd4a7485f1,
title = "Benchmarking the power of amateur observatories for TTV exoplanets detection",
abstract = "We perform an analysis of ~80 000 photometric measurements for the following 10 stars hosting transiting planets: WASP-2, -4, -5, -52, Kelt-1, CoRoT-2, XO-2, TrES-1, HD 189733, GJ 436. Our analysis includes mainly transit light curves from the Exoplanet Transit Database, public photometry from the literature, and some proprietary photometry privately supplied by other authors. Half of these light curves were obtained by amateurs. From this photometry we derive 306 transit timing measurements, as well as improved planetary transit parameters. Additionally, for 6 of these 10 stars we present a set of radial velocity measurements obtained from the spectra stored in the HARPS, HARPS-N and SOPHIE archives using the HARPS-TERRA pipeline. Our analysis of these transit timing and radial velocity data did not reveal significant hints of additional orbiting bodies in almost all of the cases. In the WASP-4 case, we found hints of marginally significant TTV signals having amplitude 10-20 s, although their parameters are",
author = "R.V. Baluev and E.N. Sokov and V.S. Shaidulin and I.A. Sokova and H.R.A. Jones and M. Tuomi and G. Anglada-Escud{\'e} and P. Benni and C.A. Colazo and M.E. Schneiter and {Villarreal D'Angelo}, C.S. and A.Y. Burdanov and {Fern{\'a}ndez-Laj s}, E. and {Ba t{\"u}rk}, O. and V.-P. Hentunen and A. Shadick",
year = "2015",
doi = "10.1093/mnras/stv788",
language = "English",
volume = "450",
pages = "3101--3113",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "3",

}

RIS

TY - JOUR

T1 - Benchmarking the power of amateur observatories for TTV exoplanets detection

AU - Baluev, R.V.

AU - Sokov, E.N.

AU - Shaidulin, V.S.

AU - Sokova, I.A.

AU - Jones, H.R.A.

AU - Tuomi, M.

AU - Anglada-Escudé, G.

AU - Benni, P.

AU - Colazo, C.A.

AU - Schneiter, M.E.

AU - Villarreal D'Angelo, C.S.

AU - Burdanov, A.Y.

AU - Fernández-Laj s, E.

AU - Ba türk, O.

AU - Hentunen, V.-P.

AU - Shadick, A.

PY - 2015

Y1 - 2015

N2 - We perform an analysis of ~80 000 photometric measurements for the following 10 stars hosting transiting planets: WASP-2, -4, -5, -52, Kelt-1, CoRoT-2, XO-2, TrES-1, HD 189733, GJ 436. Our analysis includes mainly transit light curves from the Exoplanet Transit Database, public photometry from the literature, and some proprietary photometry privately supplied by other authors. Half of these light curves were obtained by amateurs. From this photometry we derive 306 transit timing measurements, as well as improved planetary transit parameters. Additionally, for 6 of these 10 stars we present a set of radial velocity measurements obtained from the spectra stored in the HARPS, HARPS-N and SOPHIE archives using the HARPS-TERRA pipeline. Our analysis of these transit timing and radial velocity data did not reveal significant hints of additional orbiting bodies in almost all of the cases. In the WASP-4 case, we found hints of marginally significant TTV signals having amplitude 10-20 s, although their parameters are

AB - We perform an analysis of ~80 000 photometric measurements for the following 10 stars hosting transiting planets: WASP-2, -4, -5, -52, Kelt-1, CoRoT-2, XO-2, TrES-1, HD 189733, GJ 436. Our analysis includes mainly transit light curves from the Exoplanet Transit Database, public photometry from the literature, and some proprietary photometry privately supplied by other authors. Half of these light curves were obtained by amateurs. From this photometry we derive 306 transit timing measurements, as well as improved planetary transit parameters. Additionally, for 6 of these 10 stars we present a set of radial velocity measurements obtained from the spectra stored in the HARPS, HARPS-N and SOPHIE archives using the HARPS-TERRA pipeline. Our analysis of these transit timing and radial velocity data did not reveal significant hints of additional orbiting bodies in almost all of the cases. In the WASP-4 case, we found hints of marginally significant TTV signals having amplitude 10-20 s, although their parameters are

U2 - 10.1093/mnras/stv788

DO - 10.1093/mnras/stv788

M3 - Article

VL - 450

SP - 3101

EP - 3113

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

ID: 3935277