Zobrazeno 1 - 10
of 501
pro vyhledávání: '"Oshagh M"'
Autor:
Cegla, H. M., Roguet-Kern, N., Lendl, M., Akinsanmi, B., McCormac, J., Oshagh, M., Wheatley, P. J., Chen, G., Allart, R., Mortier, A., Bourrier, V., Buchschacher, N., Lovis, C., Sosnowska, D., Sulis, S., Turner, O., Casasayas-Barris, N., Palle, E., Yan, F., Burleigh, M. R., Casewell, S. L., Goad, M. R., Hawthorn, F., Wyttenbach, A.
Publikováno v:
A&A 674, A174 (2023)
We analyse spectroscopic and photometric transits of the hot Jupiters WASP-52b and HAT-P30b obtained with ESPRESSO, Eulercam and NGTS for both targets, and additional TESS data for HAT-P-30. Our goal is to update the system parameters and refine our
Externí odkaz:
http://arxiv.org/abs/2304.11022
Publikováno v:
Indian Journal of Dental Research, Vol 20, Iss 4, Pp 437-441 (2009)
Objective : Expansion screws like Hyrax, Haas and other types, produce heavy interrupted forces which are unfavorable for dental movement and could be harmful to the tooth and periodontium. The other disadvantage of these screws is the need for patie
Externí odkaz:
https://doaj.org/article/0be1c58c66c746cb9f07a7650fc1e5e0
Autor:
Maas, A. J., Ilin, E., Oshagh, M., Pallé, E., Parviainen, H., Molaverdikhani, K., Quirrenbach, A., Esparza-Borges, E., Murgas, F., Béjar, V. J. S., Narita, N., Fukui, A., Lin, C. -L., Mori, M., Klagyivik, P.
Publikováno v:
A&A 668, A111 (2022)
Although high energetic radiation from flares is a potential threat to exoplanet atmospheres and may lead to surface sterilization, it might also provide the extra energy for low-mass stars needed to trigger and sustain prebiotic chemistry. We invest
Externí odkaz:
http://arxiv.org/abs/2210.11103
Publikováno v:
Journal of Dental Biomaterial, Vol 2, Iss 2 (2015)
Statement of Problem: T-loop is one of the most popular closing loops in orthodontic profession. However its activation is in the contrary to Bouschinger effect theory, since the formed bends would be opened during activation. The purpose of this
Externí odkaz:
https://doaj.org/article/2d9b87e8531841089377aa78634ee5d9
Autor:
Esparza-Borges, E., Parviainen, H., Murgas, F., Pallé, E., Maas, A., Morello, G., Zapatero-Osorio, M. R., Barkaoui, K., Narita, N., Fukui, A., Casasayas-Barris, N., Oshagh, M., Crouzet, N., Galán, D., Fernández, G. E., Kagetani, T., Kawauchi, K., Kodama, T., Korth, J., Kusakabe, N., Laza-Ramos, A., Luque, R., Livingston, J., Madrigal-Aguado, A., Mori, M., Orell-Miquel, J., Puig-Subirá, M., Stangret, M., Terada, Y., Watanabe, N., Zou, Y., Savel, A. Baliga, Belinski, A. A., Collins, K., Dressing, C. D., Giacalone, S., Gill, H., Goliguzova, M. V., Ikoma, M., Jenkins, J. M., Tamura, M., Twicken, J. D., Ricker, G. R., Schwarz, R. P., Seager, S., Shporer, A., Vanderspek, R., Winn, J.
Publikováno v:
A&A 666, A10 (2022)
We report the discovery and validation of two TESS exoplanets orbiting faint M dwarfs: TOI-4479b and TOI-2081b. We have jointly analyzed space (TESS mission) and ground based (MuSCAT2, MuSCAT3 and SINISTRO instruments) lightcurves using our multi-col
Externí odkaz:
http://arxiv.org/abs/2206.10643
Autor:
Morello, G., Parviainen, H., Murgas, F., Pallé, E., Oshagh, M., Fukui, A., Hirano, T., Ishikawa, H. T., Mori, M., Narita, N., Collins, K. A., Barkaoui, K., Lewin, P., Cadieux, C., de Leon, J. P., Soubkiou, A., Garcia, N. Abreu, Crouzet, N., Esparza-Borges, E., Rodríguez, G. E. Fernández, Galán, D., Hori, Y., Ikoma, M., Isogai, K., Kagetani, T., Kawauchi, K., Kimura, T., Kodama, T., Korth, J., Kotani, T., Krishnamurthy, V., Kurita, S., Laza-Ramos, A., Livingston, J. H., Luque, R., Madrigal-Aguado, A., Nishiumi, T., Orell-Miquel, J., Puig-Subirà, M., Sánchez-Benavente, M., Stangret, M., Tamura, M., Terada, Y., Watanabe, N., Zou, Y., Benkhaldoun, Z., Collins, K. I., Doyon, R., Garcia, L., Ghachoui, M., Gillon, M., Jehin, E., Pozuelos, F. J., Schwarz, R. P., Timmermans, M.
Publikováno v:
A&A, 673, A32 (2023)
Context. Exoplanets with orbital periods of less than one day are known as ultra-short period (USP) planets. They are relatively rare products of planetary formation and evolution processes, but especially favourable for characterisation with current
Externí odkaz:
http://arxiv.org/abs/2201.13274
Autor:
Cristo, E., Santos, N. C., Demangeon, O., Martins, J. H. C., Figueira, P., Casasayas-Barris, N., Osorio, M. R. Zapatero, Borsa, F., Sousa, S. G., Oshagh, M., Micela, G., Tabernero, H. M., Seidel, J. V., Cristiani, S., Pepe, F., Rebolo, R., Adibekyan, V., Allart, R., Alibert, Y., Silva, T. Azevedo, Bourrier, V., Cabral, A., Borges, E. Esparza, Hernández, J. I. González, Lillo-Box, J., Curto, G. Lo, Lovis, C., Manescau, A., Di Marcantonio, P., Martins, C. J. A. P., Mascareño, A. S., Mégevand, D., Mehner, A., Nunes, N. J., Palle, E., Sozzetti, A., Udry, S.
Publikováno v:
A&A 660, A52 (2022)
In this paper we introduce CaRM, a semi-automatic code for the retrieval of broadband transmission spectra of transiting planets through the chromatic Rossiter-McLaughlin method. We applied it to HARPS and ESPRESSO observations of two exoplanets to r
Externí odkaz:
http://arxiv.org/abs/2201.06531
Autor:
Mascareño, A. Suárez, Damasso, M., Lodieu, N., Sozzetti, A., Béjar, V. J. S., Benatti, S., Osorio, M. R. Zapatero, Micela, G., Rebolo, R., Desidera, S., Murgas, F., Claudi, R., Hernández, J. I. González, Malavolta, L., del Burgo, C., D'Orazi, V., Amado, P. J., Locci, D., Tabernero, H. M., Marzari, F., Aguado, D. S., Turrini, D., Guillén, C. Cardona, Toledo-Padrón, B., Maggio, A., Aceituno, J., Bauer, F. F., Caballero, J. A., Chinchilla, P., Esparza-Borges, E., González-Álvarez, E., Granzer, T., Luque, R., Martín, E. L., Nowak, G., Oshagh, M., Pallé, E., Parviainen, H., Quirrenbach, A., Reiners, A., Ribas, I., Strassmeier, K. G., Weber, M., Mallonn, M.
Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years. These theoretical expectations remain u
Externí odkaz:
http://arxiv.org/abs/2111.09193
Autor:
Bourrier, V., Lovis, C., Cretignier, M., Allart, R., Dumusque, X., Delisle, J. -B., Deline, A., Sousa, S. G., Adibekyan, V., Alibert, Y., Barros, S. C. C., Borsa, F., Cristiani, S., Demangeon, O., Ehrenreich, D., Figueira, P., Hernández, J. I. González, Lendl, M., Lillo-Box, J., Curto, G. Lo, Di Marcantonio, P., Martins, C. J. A. P., Mégevand, D., Mehner, A., Micela, G., Molaro, P., Oshagh, M., Palle, E., Pepe, F., Poretti, E., Rebolo, R., Santos, N. C., Scandariato, G., Seidel, J. V., Sozzetti, A., Mascareño, A. Suárez, Osorio, M. R Zapatero
Comparisons of the alignment of exoplanets with a common host star can be used to distinguish among concurrent evolution scenarios. However, multi-planet systems usually host mini-Neptunes and super-Earths, whose size make orbital architecture measur
Externí odkaz:
http://arxiv.org/abs/2110.14214
Autor:
Garai, Z., Pribulla, T., Parviainen, H., Pallé, E., Claret, A., Szigeti, L., Béjar, V. J. S., Casasayas-Barris, N., Crouzet, N., Fukui, A., Chen, G., Kawauchi, K., Klagyivik, P., Kurita, S., Kusakabe, N., de Leon, J. P., Livingston, J. H., Luque, R., Mori, M., Murgas, F., Narita, N., Nishiumi, T., Oshagh, M., Szabó, Gy. M., Tamura, M., Terada, Y., Watanabe, N.
Up to now, WASP-12b is the only hot Jupiter confirmed to have a decaying orbit. The case of WASP-43b is still under debate. Recent studies preferred or ruled out the orbital decay scenario, but further precise transit timing observations are needed t
Externí odkaz:
http://arxiv.org/abs/2110.04761