Zobrazeno 1 - 10
of 318
pro vyhledávání: '"Galán D"'
Autor:
Peláez-Torres, A., Esparza-Borges, E., Pallé, E., Parviainen, H., Murgas, F., Morello, G., Zapatero-Osorio, M. R., Korth, J., Narita, N., Fukui, A., Carleo, I., Luque, R., García, N. Abreu, Barkaoui, K., Boyle, A., Béjar, V. J. S., Calatayud-Borras, Y., Cheryasov, D. V., Christiansen, J. L., Ciardi, D. R., Enoc, G., Essack, Z., Fukuda, I., Furesz, G., Galán, D., Geraldía-González, S., Giacalone, S., Gill, H., Gonzales, E. J., Hayashi, Y., Ikuta, K., Isogai, K., Kagetani, T., Kawai, Y., Kawauchi, K., Klagyvik, P., Kodama, T., Kusakabe, N., Laza-Ramos, A., de Leon, J. P., Livingston, J. H., Lund, M. B., Madrigal-Aguado, A., Meni, P., Mori, M., Torres, S. Muñoz, Orell-Miquel, J., Puig, M., Ricker, G., Sánchez-Benavente, M., Savel, A. B., Schlieder, J. E., Schwarz, R. P., Sefako, R., Sosa-Guillén, P., Stangret, M., Stockdale, C., Tamura, M., Terada, Y., Twicken, J. D., Watanabe, N., Winn, J., Zheltoukhov, S. G., Ziegler, C., Zou, Y.
The TESS mission searches for transiting exoplanets by monitoring the brightness of hundreds of thousands of stars across the entire sky. M-type planet hosts are ideal targets for this mission due to their smaller size and cooler temperatures, which
Externí odkaz:
http://arxiv.org/abs/2409.07400
Gliese 12 b: A temperate Earth-sized planet at 12 pc ideal for atmospheric transmission spectroscopy
Autor:
Kuzuhara, M., Fukui, A., Livingston, J. H., Caballero, J. A., de Leon, J. P., Hirano, T., Kasagi, Y., Murgas, F., Narita, N., Omiya, M., Orell-Miquel, Jaume, Palle, E., Changeat, Q., Esparza-Borges, E., Harakawa, H., Hellier, C., Hori, Yasunori, Ikuta, Kai, Ishikawa, H. T., Kodama, T., Kotani, T., Kudo, T., Morales, J. C., Mori, M., Nagel, E., Parviainen, H., Perdelwitz, V., Reiners, A., Ribas, I., Sanz-Forcada, J., Sato, B., Schweitzer, A., Tabernero, H. M., Takarada, T., Uyama, T., Watanabe, N., Zechmeister, M., García, N. Abreu, Aoki, W., Beichman, C., Béjar, V. J. S., Brandt, T. D., Calatayud-Borras, Y., Carleo, I., Charbonneau, D., Collins, K. A., Currie, T., Doty, J. P., Dreizler, S., Fernández-Rodríguez, G., Fukuda, I., Galán, D., Geraldía-González, S., González-Garcia, J., Hayashi, Y., Hedges, C., Henning, T., Hodapp, K., Ikoma, M., Isogai, K., Jacobson, S., Janson, M., Jenkins, J. M., Kagetani, T., Kambe, E., Kawai, Y., Kawauchi, K., Kokubo, E., Konishi, M., Korth, J., Krishnamurthy, V., Kurokawa, T., Kusakabe, N., Kwon, J., Laza-Ramos, A., Libotte, F., Luque, R., Madrigal-Aguado, A., Matsumoto, Y., Mawet, D., McElwain, M. W., Gallardo, P. P. Meni, Morello, G., Torres, S. Mu~noz, Nishikawa, J., Nugroho, S. K., Ogihara, M., Pel'aez-Torres, A., Rapetti, D., S'anchez-Benavente, M., Schlecker, M., Seager, S., Serabyn, E., Serizawa, T., Stangret, M., Takahashi, A., Teng, H., Tamura, M., Terada, Y., Ueda, A., Usuda, T., Vanderspek, R., Vievard, S., Watanabe, D., Winn, J. N., Osorio, M. R. Zapatero
Publikováno v:
Published on 2024 May 23 by Astrophysical Journal Letters (ApJL) 967 L21
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation i
Externí odkaz:
http://arxiv.org/abs/2405.14708
Autor:
Hori, Y., Fukui, A., Hirano, T., Narita, N., de Leon, J. P., Ishikawa, H. T., Hartman, J. D., Morello, G., García, N. Abreu, Hernández, L. Álvarez, Béjar, V. J. S., Calatayud-Borras, Y., Carleo, I., Enoc, G., Esparza-Borges, E., Fukuda, I., Galán, D., Geraldía-González, S., Hayashi, Y., Ikoma, M., Ikuta, K., Isogai, K., Kagetani, T., Kawai, Y., Kawauchi, K., Kimura, T., Kodama, T., Korth, J., Kusakabe, N., Laza-Ramos, A., Livingston, J. H., Luque, R., Miyakawa, K., Mori, M., Torres, S. Muñoz, Murgas, F., Orell-Miquel, J., Palle, E., Parviainen, H., Peláez-Torres, A., Puig-Subirá, M., Sánchez-Benavente, M., Sosa-Guillén, P., Stangret, M., Terada, Y., Watanabe, N., Bakos, G. Á., Barkaoui, K., Beichman, C., Benkhaldoun, Z., Boyle, A. W., Ciardi, D. R., Clark, C. A., Collins, K. A., Collins, K. I., Conti, D. M., Crossfield, I. J. M., Everett, M. E., Furlan, E., Ghachoui, M., Gillon, M., Gonzales, E. J., Higuera, J., Horne, K., Howell, S. B., Jehin, E., Lester, K. V., Lund, M. B., Matson, R., Matthews, E. C., Pozuelos, F. J., Safonov, B. S., Schlieder, J. E., Schwarz, R. P., Sefako, R., Srdoc, G., Strakhov, I. A., Waalkes, W. C., Ziegler, C., Charbonneau, D., Essack, Z., Timmermans, M., Guerrero, N. M., Harakawa, H., Hedges, C., Ishizuka, M., Jenkins, J. M., Konishi, M., Kotani, T., Kudo, T., Kurokawa, T., Kuzuhara, M., Nishikawa, J., Omiya, M., Ricker, G. R., Seager, S., Serizawa, T., Striegel, S., Tamura, M., Ueda, A., Vanderspek, R., Vievard, S., Winn, J. N.
Sub-Neptunes with $2-3R_\oplus$ are intermediate in size between rocky planets and Neptune-sized planets. The orbital properties and bulk compositions of transiting sub-Neptunes provide clues to the formation and evolution of close-in small planets.
Externí odkaz:
http://arxiv.org/abs/2405.12637
Autor:
Murgas, F., Nowak, G., Masseron, T., Parviainen, H., Luque, R., Pallé, E., Korth, Judith, Carleo, I., Csizmadia, Sz., Esparza-Borges, E., Alqasim, Ahlam, Cochran, William D., Dai, Fei, Deeg, Hans J., Gandolfi, D., Goffo, Elisa, Kabáth, Petr, Lam, K. W. F., Livingston, John, Muresan, Alexandra, Osborne, H. L. M., Persson, Carina M., Serrano, L. M., Smith, Alexis M. S., Van Eylen, Vincent, Orell-Miquel, J., Hinkel, Natalie R., Galán, D., Puig-Subirà, M., Stangret, M., Fukui, A., Kagetani, T., Narita, N., Ciardi, David R., Boyle, Andrew W., Ziegler, Carl, Briceño, César, Law, Nicholas, Mann, Andrew W., Jenkins, Jon M., Latham, David W., Quinn, Samuel N., Ricker, G., Seager, S., Shporer, Avi, Ting, Eric B., Vanderspek, R., Winn, Joshua N.
Publikováno v:
A&A 668, A158 (2022)
We used TESS light curves and HARPS-N spectrograph radial velocity measurements to establish the physical properties of the transiting exoplanet candidate found around the star HD 20329 (TOI-4524). We performed a joint fit of the light curves and rad
Externí odkaz:
http://arxiv.org/abs/2211.02547
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
Publikováno v:
In Journal of Logical and Algebraic Methods in Programming April 2023 132
Autor:
Rezaeian, M., Kuijper, C.B., van der Boon, A., Pastor-Galán, D., Cotton, L.J., Langereis, C.G., Krijgsman, W.
Publikováno v:
In Tectonophysics 5 July 2020 786
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Publikováno v:
In IFAC PapersOnLine 2018 51(4):316-321