M. Oshagh

发表

The PLATO 2.0 mission

P. Giommi, D. Pollacco, I. Skillen, 2013, 1310.0696.

A Pragmatic Bayesian Perspective on Correlation Analysis

P. Figueira, M. Oshagh, V. Zh. Adibekyan, 2016, Origins of Life and Evolution of Biospheres.

Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization

D. Dragomir, S. V. Jeffers, S. Dreizler, 2019, Astronomy & Astrophysics.

Revisiting the correlation between stellar activity and planetary surface gravity

P. Figueira, M. Oshagh, N. C. Santos, 2014, 1411.1767.

Effect of stellar spots on high-precision transit light-curve

I. Boisse, M. Oshagh, N. Haghighipour, 2013, 1306.0739.

Radial velocity information content of M dwarf spectra in the near-infrared

F. Pepe, P. Figueira, M. Oshagh, 2015, 1511.07468.

Near-InfraRed Planet Searcher to Join HARPS on the ESO 3.6-metre Telescope

Andrew Cumming, Jaymie M. Matthews, René Doyon, 2017 .

Uncovering the planets and stellar activity of CoRoT-7 using only radial velocities

A. Santerne, P. Figueira, M. Oshagh, 2016, 1601.07495.

Effect of stellar activity on the high precision transit light curve

A. Santerne, David Ehrenreich, Pedro Figueira, 2014 .

XXXV. The interesting case of HD41248: stellar activity, no planets?

D. Queloz, I. Boisse, A. Santerne, 2014 .

Impact of occultations of stellar active regions on transmission spectra: Can occultation of a plage mimic the signature of a blue sky?

A. Santerne, D. Ehrenreich, P. Figueira, 2014, 1407.2066.