Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Rodríguez, Pilar Montañes"'
Autor:
Hayashi, Yuya, Narita, Norio, Fukui, Akihiko, Changeat, Quentin, Kawauchi, Kiyoe, Ikuta, Kai, Palle, Enric, Murgas, Felipe, Parviainen, Hannu, Esparza-Borges, Emma, Peláez-Torres, Alberto, Gallardo, Pedro Pablo Meni, Morello, Giuseppe, Fernández-Rodríguez, Gareb, García, Néstor Abreu, Torres, Sara Muñoz, Borrás, Yéssica Calatayud, Rodríguez, Pilar Montañés, Livingston, John H., Watanabe, Noriharu, de Leon, Jerome P., Kawai, Yugo, Isogai, Keisuke, Mori, Mayuko
We present ground-based photometric observations of secondary eclipses of the hottest known planet KELT-9b using MuSCAT2 and Sinistro. We detect secondary eclipse signals in $i$ and $z_{\rm s}$ with eclipse depths of $373^{+74}_{-75}$ ppm and $638^{+
Externí odkaz:
http://arxiv.org/abs/2408.15698
Autor:
Nowak, Grzegorz, Palle, Enric, Gandolfi, Davide, Deeg, Hans J., Hirano, Teruyuki, Barragán, Oscar, Kuzuhara, Masayuki, Dai, Fei, Luque, Rafael, Persson, Carina M., Fridlund, Malcolm, Johnson, Marshall C., Korth, Judith, Livingston, John H., Grziwa, Sascha, Mathur, Savita, Hatzes, Artie P., Prieto-Arranz, Jorge, Nespral, David, Hidalgo, Diego, Hjorth, Maria, Albrecht, Simon, Van Eylen, Vincent, Lam, Kristine W. F., Cochran, William D., Esposito, Massimiliano, Csizmadia, Szilárd, Guenther, Eike W., Kabath, Petr, Blay, Pere, Brahm, Rafael, Jordán, Andrés, Espinoza, Néstor, Rojas, Felipe, Barris, Núria Casasayas, Rodler, Florian, Sobrino, Roi Alonso, Cabrera, Juan, Carleo, Ilaria, Chaushev, Alexander, de Leon, Jerome, Eigmüller, Philipp, Endl, Michael, Erikson, Anders, Fukui, Akihiko, Georgieva, Iskra, González-Cuesta, Lucía, Knudstrup, Emil, Lund, Mikkel N., Rodríguez, Pilar Montañes, Murgas, Felipe, Narita, Norio, Niraula, Prajwal, Pätzold, Martin, Rauer, Heike, Redfield, Seth, Ribas, Ignasi, Skarka, Marek, Smith, Alexis M. S., Subjak, Jano
We present an independent discovery and detailed characterisation of K2-280b, a transiting low density warm sub-Saturn in a 19.9-day moderately eccentric orbit (e = 0.35_{-0.04}^{+0.05}) from K2 campaign 7. A joint analysis of high precision HARPS, H
Externí odkaz:
http://arxiv.org/abs/2007.07939
Autor:
Šubjak, Ján, Sharma, Rishikesh, Carmichael, Theron W., Johnson, Marshall C., Gonzales, Erica J., Matthews, Elisabeth, Boffin, Henri M. J., Brahm, Rafael, Chaturvedi, Priyanka, Chakraborty, Abhijit, Ciardi, David R., Collins, Karen A., Esposito, Massimiliano, Fridlund, Malcolm, Gan, Tianjun, Gandolfi, Davide, García, Rafael A., Guenther, Eike, Hatzes, Artie, Latham, David W., Persson, Carina M., Relles, Howard M., Schlieder, Joshua E., Barclay, Thomas, Dressing, Courtney, Crossfield, Ian, Howard, Andrew W., Rodler, Florian, Zhou, George, Quinn, Samuel N., Esquerdo, Gilbert A., Calkins, Michael L., Berlind, Perry, Stassun, Keivan G., Albrecht, Simon, Sobrino, Roi Alonso, Beck, Paul, Blažek, Martin, Cabrera, Juan, Carleo, Ilaria, Cochran, William D., Csizmadia, Szilard, Dai, Fei, Deeg, Hans J., de Leon, Jerome P., Eigmüller, Philipp, Endl, Michael, Erikson, Anders, Fukui, Akai, Georgieva, Iskra, González-Cuesta, Lucía, Grziwa, Sascha, Hidalgo, Diego, Hirano, Teruyuki, Hjorth, Maria, Knudstrup, Emil, Korth, Judith, Lam, Kristine W. F., Livingston, John H., Lund, Mikkel N., Luque, Rafael, Mathur, Savita, Rodríguez, Pilar Montanes, Murgas, Felipe, Narita, Norio, Nespral, David, Niraula, Prajwal, Nowak, Grzegorz, Pallé, Enric, Pätzold, Martin, Prieto-Arranz, Jorge, Rauer, Heike, Redfield, Seth, Ribas, Ignasi, Skarka, Marek, Smith, Alexis M. S., Špoková, Magdalena, Van Eylen, Vincent, Kabáth, Petr
We report the discovery of an intermediate-mass transiting brown dwarf, TOI-503b, from the TESS mission. TOI-503b is the first brown dwarf discovered by TESS and orbits a metallic-line A-type star with a period of $P=3.6772 \pm 0.0001$ days. The ligh
Externí odkaz:
http://arxiv.org/abs/1909.07984
Autor:
Lam, Kristine W. F., Korth, Judith, Masuda, Kento, Csizmadia, Szilárd, Eigmüller, Philipp, Stefánsson, Guðmundur Kári, Endl, Michael, Albrecht, Simon, Luque, Rafael, Livingston, John H., Hirano, Teruyuki, Sobrino, Roi Alonso, Barragán, Oscar, Cabrera, Juan, Carleo, Ilaria, Chaushev, Alexander, Cochran, William D., Dai, Fei, de Leon, Jerome, Deeg, Hans J., Erikson, Anders, Esposito, Massimiliano, Fridlund, Malcolm, Fukui, Akihiko, Gandolfi, Davide, Georgieva, Iskra, Cuesta, Lucá Gonzalez, Grziwa, Sascha, Guenther, Eike W., Hatzes, Artie P., Hidalgo, Diego, Hjorth, Maria, Kabath, Petr, Knudstrup, Emil, Lund, Mikkel N., Mahadevan, Suvrath, Mathur, Savita, Rodríguez, Pilar Montañes, Murgas, Felipe, Narita, Norio, Nespral, David, Niraula, Prajwal, Palle, Enric, Pätzold, Martin, Persson, Carina M., Prieto-Arranz, Jorge, Rauer, Heike, Redfield, Seth, Ribas, Ignasi, Robertson, Paul, Skarka, Marek, Smith, Alexis M. S., Subjak, Jan, Van Eylen, Vincent
K2-146 is a cool, 0.358 M_sun dwarf that was found to host a mini-Neptune with a 2.67-days period. The planet exhibited strong transit timing variations (TTVs) of greater than 30 minutes, indicative of the presence of a further object in the system.
Externí odkaz:
http://arxiv.org/abs/1907.11141
Autor:
Parviainen, Hannu, Tingley, Brandon, Deeg, Hans. J., Palle, Enric, Alonso, Roi, Rodriguez, Pilar Montanes, Murgas, Felipe, Narita, Norio, Fukui, Akihiko, Kusakabe, Nobuhiko, Tamura, Motohide, Nishiumi, Taku, Prieto-Arranz, Jorge, Klagyivik, Peter, Béjar, Victor J. S., Crouzet, Nicolas, Mori, Mayuko, Soto, Diego Hidalgo, Barris, Núria Casasayas, Luque, Rafael
Publikováno v:
A&A 630, A89 (2019)
Context. The TESS and PLATO missions are expected to find vast numbers of new transiting planet candidates. However, only a fraction of these candidates will be legitimate planets, and the candidate validation will require a significant amount of fol
Externí odkaz:
http://arxiv.org/abs/1907.09776
Autor:
Persson, Carina M., Csizmadia, Szilárd, Mustill, Alexander J., Fridlund, Malcolm, Hatzes, Artie P., Nowak, Grzegorz, Georgieva, Iskra, Gandolfi, Davide, Davies, Melvyn B., Livingston, John H., Palle, Enric, Rodríguez, Pilar Montañes, Endl, Michael, Hirano, Teruyuki, Prieto-Arranz, Jorge, Korth, Judith, Grziwa, Sascha, Esposito, Massimiliano, Albrecht, Simon, Johnson, Marshall C., Barragán, Oscar, Parviainen, Hannu, Van Eylen, Vincent, Sobrino, Roi Alonso, Beck, Paul G., Cabrera, Juan, Carleo, Ilaria, Cochran, William D., Dai, Fei, Deeg, Hans J., de Leon, Jerome P., Eigmüller, Philipp, Erikson, Anders, Fukui, Akai, González-Cuesta, Lucía, Guenther, Eike W., Hidalgo, Diego, Hjorth, Maria, Kabath, Petr, Knudstrup, Emil, Kusakabe, Nobuhiko, Lam, Kristine W. F., Lund, Mikkel N., Luque, Rafael, Mathur, Savita, Murgas, Felipe, Narita, Norio, Nespral, David, Niraula, Prajwal, Olofsson, A. O. Henrik, Pätzold, Martin, Rauer, Heike, Redfield, Seth, Ribas, Ignasi, Skarka, Marek, Smith, Alexis M. S., Subjak, Jan, Tamura, Motohide
Publikováno v:
A&A 628, A64 (2019)
Our aim is to investigate the nature and formation of brown dwarfs by adding a new well-characterised object to the small sample of less than 20 transiting brown dwarfs. One brown dwarf candidate was found by the KESPRINT consortium when searching fo
Externí odkaz:
http://arxiv.org/abs/1906.05048
Autor:
Gandolfi, Davide, Fossati, Luca, Livingston, John H., Stassun, Keivan G., Grziwa, Sascha, Barragán, Oscar, Fridlund, Malcolm, Kubyshkina, Daria, Persson, Carina M., Dai, Fei, Lam, Kristine W. F., Albrecht, Simon, Batalha, Natalie, Beck, Paul G., Justesen, Anders Bo, Cabrera, Juan, Cartwright, Scott, Cochran, William D., Csizmadia, Szilard, Davies, Misty D., Deeg, Hans J., Eigmüller, Philipp, Endl, Michael, Erikson, Anders, Esposito, Massimiliano, García, Rafael A., Goeke, Robert, González-Cuesta, Lucía, Guenther, Eike W., Hatzes, Artie P., Hidalgo, Diego, Hirano, Teruyuki, Hjorth, Maria, Kabath, Petr, Knudstrup, Emil, Korth, Judith, Li, Jie, Luque, Rafael, Mathur, Savita, Rodríguez, Pilar Montañes, Narita, Norio, Nespral, David, Niraula, Prajwal, Nowak, Grzegorz, Palle, Enric, Pätzold, Martin, Prieto-Arranz, Jorge, Rauer, Heike, Redfield, Seth, Ribas, Ignasi, Skarka, Marek, Smith, Alexis M. S., Rowden, Pamela, Torres, Guillermo, Van Eylen, Vincent, Vezie, Michael L.
Publikováno v:
ApJL, 876, L24 (2019)
We report the discovery of a super-Earth and a sub-Neptune transiting the star HD 15337 (TOI-402, TIC 120896927), a bright (V=9) K1 dwarf observed by the Transiting Exoplanet Survey Satellite (TESS) in Sectors 3 and 4. We combine the TESS photometry
Externí odkaz:
http://arxiv.org/abs/1903.05623
Autor:
Dai, Fei, Winn, Joshua N., Gandolfi, Davide, Wang, Sharon X., Teske, Johanna K., Burt, Jennifer, Albrecht, Simon, BarragÁn, Oscar, Cochran, William D., Endl, Michael, Fridlund, Malcolm, Hatzes, Artie P., Hirano, Teruyuki, Hirsch, Lea A., Johnson, Marshall C., Justesen, Anders Bo, Livingston, John, Persson, Carina M., Prieto-arranz, Jorge, Vanderburg, Andrew, Alonso, Roi, Antoniciello, Giuliano, Arriagada, Pamela, Butler, R. p., Cabrera, Juan, Crane, Jeffrey D., Cusano, Felice, Csizmadia, SzilÁrd, Deeg, Hans, Dieterich, Sergio B., EigmÜller, Philipp, Erikson, Anders, Everett, Mark E., Fukui, Akihiko, Grziwa, Sascha, Guenther, Eike W., Henry, Gregory W., Howell, Steve B., Johnson, John Asher, Korth, Judith, Kuzuhara, Masayuki, Narita, Norio, Nespral, David, Nowak, Grzegorz, Palle, Enric, PÄtzold, Martin, Rauer, Heike, RodrÍguez, Pilar MontaÑÉs, Shectman, Stephen A., Smith, Alexis M. s., Thompson, Ian B., Van Eylen, Vincent, Williamson, Michael W., Wittenmyer, Robert A.
We report the discovery of a new ultra-short-period planet and summarize the properties of all such planets for which the mass and radius have been measured. The new planet, EPIC~228732031b, was discovered in {\it K2} Campaign 10. It has a radius of
Externí odkaz:
http://arxiv.org/abs/1710.00076
Autor:
Tingley, Brandon, Palle, Enric, Parviainen, Hannu, Deeg, Hans-Jörg, Osorio, Maria Rosa Zapatero, Cabrera-Lavers, Antonio, Belmonte, Juan Antonio, Rodriguez, Pilar Montañés, Murgas, Felipe, Ribas, Ignasi
We report the detection of transit timing variations (TTVs) well in excess of one hour in the Kepler multi-planet candidate system KOI 806. This system exhibits transits consistent with three separate planets -- a Super-Earth, a Jupiter, and a Saturn
Externí odkaz:
http://arxiv.org/abs/1111.5107