no code implementations • 8 Mar 2021 • T. Trifonov, J. A. Caballero, J. C. Morales, A. Seifahrt, I. Ribas, A. Reiners, J. L. Bean, R. Luque, H. Parviainen, E. Pallé, S. Stock, M. Zechmeister, P. J. Amado, G. Anglada-Escudé3, M. Azzaro, T. Barclay, V. J. S. Béjar, P. Bluhm, N. Casasayas-Barris, C. Cifuentes, K. A. Collins, K. I. Collins, M. Cortés-Contreras, J. de Leon, S. Dreizler, C. D. Dressing, E. Esparza-Borges, N. Espinoza, M. Fausnaugh, A. Fukui, A. P. Hatzes, C. Hellier, Th. Henning, C. E. Henze, E. Herrero, S. V. Jeffers, J. M. Jenkins, E. L. N. Jensen, A. Kaminski, D. Kasper, D. Kossakowski, M. Kürster, M. Lafarga, D. W. Latham, A. W. Mann, K. Molaverdikhani, D. Montes, B. T. Montet, F. Murgas, N. Narita, M. Oshagh, V. M. Passegger, D. Pollacco, S. N. Quinn, A. Quirrenbach, G. R. Ricker, C. Rodríguez López, J. Sanz-Forcada, R. P. Schwarz, A. Schweitzer, S. Seager, A. Shporer, M. Stangret, J. Stürmer, T. G. Tan, P. Tenenbaum, J. D. Twicken, R. Vanderspek, J. N. Winn
The host star is at a distance of ~8. 1 parsecs, has a J-band magnitude of ~7. 2, and is observable from both hemispheres of Earth.
Earth and Planetary Astrophysics
no code implementations • 14 Jan 2021 • Ch. Helling, M. Worters, D. Samra, K. Molaverdikhani, N. Iro
We analyse plasma and magnetic processes in the atmosphere of the ultra-hot Jupiter HAT-P-7b to investigate the formation of a thermal ionosphere and the possibility of magnetically coupling the atmospheric gas as the base for an extended exosphere.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
1 code implementation • 29 Apr 2019 • R. Luque, E. Pallé, D. Kossakowski, S. Dreizler, J. Kemmer, N. Espinoza, G. Anglada-Escudé, V. J. S. Béjar, J. A. Caballero, M. Cortés-Contreras, E. Díez-Alonso, A. Hatzes, C. Hellier, T. Henning, S. V. Jeffers, L. Kaltenegger, M. Kürster, K. Molaverdikhani, D. Montes, N. Narita, G. Nowak, A. Ofir, M. Oshagh, H. Parviainen, A. Quirrenbach, S. Reffert, A. Reiners, C. Rodríguez-López, M. Schlecker, S. Stock, T. Trifonov, M. R. Zapatero Osorio, M. Zechmeister, P. J. Amado, D. R. Anderson, N. E. Batalha, F. F. Bauer, P. Bluhm, C. J. Burke, J. Burt, R. P. Butler, D. A. Caldwell, G. Chen, K. A. Collins, K. I. Collins, J. D. Crane, C. D. Dressing, S. Dynes, F. Feng, J. M. Jenkins, A. Kaminski, H. Klahr, T. Kotani, M. Lafarga, D. W. Latham, S. McDermott, P. Montañés-Rodríguez, J. C. Morales, F. Murgas, E. Nagel, S. Pedraz, I. Ribas, G. R. Ricker, P. Rowden, S. A. Shectman, M. Tamura, J. Teske, J. D. Twicken, S. X. Wang, J. W. Winn, B. Wohler
We report the detection of a transiting Earth-size planet around Gl 357, a nearby M2. 5 V star, using data from the Transiting Exoplanet Survey Satellite (TESS).
Earth and Planetary Astrophysics
3 code implementations • 25 Apr 2019 • P. Mollière, J. P. Wardenier, R. van Boekel, Th. Henning, K. Molaverdikhani, I. A. G. Snellen
The code is fast, accurate, and versatile; it can calculate both transmission and emission spectra within a few seconds at low resolution ($\lambda/\Delta\lambda$ = 1000; correlated-k method) and high resolution ($\lambda/\Delta\lambda = 10^6$; line-by-line method), using only a few lines of input instruction.
Earth and Planetary Astrophysics
