Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Géza Csörnyei"'
Autor:
Attila Moór, Péter Ábrahám, Ágnes Kóspál, Kate Y L Su, George H Rieke, Krisztián Vida, Gianni Cataldi, Attila Bódi, Zsófia Bognár, Borbála Cseh, Géza Csörnyei, Nóra Egei, Anikó Farkas, Ottó Hanyecz, Bernadett Ignácz, Csilla Kalup, Réka Könyves-Tóth, Levente Kriskovics, László Mészáros, András Pál, András Ordasi, Krisztián Sárneczky, Bálint Seli, Ádám Sódor, Róbert Szakáts, József Vinkó, Gabriella Zsidi
Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and is likely related to a recent giant collision occurring close to the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08044f3a3fc9882eab47c1aa8e967351
We investigate the effect of strong emission line galaxies on the performance of empirical photometric redshift estimation methods. In order to artificially control the contribution of photometric error and emission lines to total flux, we develop a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::447714720f8bd984776ad3451dabf989
http://arxiv.org/abs/2101.11368
http://arxiv.org/abs/2101.11368
Autor:
Tamás Szalai, József Vinkó, Réka Könyves-Tóth, Andrea P. Nagy, K. Azalee Bostroem, Krisztián Sárneczky, Peter J. Brown, Ondrej Pejcha, Attila Bódi, Borbála Cseh, Géza Csörnyei, Zoltán Dencs, Ottó Hanyecz, Bernadett Ignácz, Csilla Kalup, Levente Kriskovics, András Ordasi, András Pál, Bálint Seli, Ádám Sódor
Publikováno v:
Astrophysical Journal; 5/1/2019, Vol. 876 Issue 1, p1-1, 1p
Autor:
Qinan Wang, Armin Rest, Yossef Zenati, Ryan Ridden-Harper, Georgios Dimitriadis, Gautham Narayan, V. Ashley Villar, Mark R. Magee, Ryan J. Foley, Edward J. Shaya, Peter Garnavich, Lifan Wang, Lei Hu, Attila Bódi, Patrick Armstrong, Katie Auchettl, Thomas Barclay, Geert Barentsen, Zsófia Bognár, Joseph Brimacombe, Joanna Bulger, Jamison Burke, Peter Challis, Kenneth Chambers, David A. Coulter, Géza Csörnyei, Borbála Cseh, Maxime Deckers, Jessie L. Dotson, Lluís Galbany, Santiago González-Gaitán, Mariusz Gromadzki, Michael Gully-Santiago, Ottó Hanyecz, Christina Hedges, Daichi Hiramatsu, Griffin Hosseinzadeh, D. Andrew Howell, Steve B. Howell, Mark E. Huber, Saurabh W. Jha, David O. Jones, Réka Könyves-Tóth, Csilla Kalup, Charles D. Kilpatrick, Levente Kriskovics, Wenxiong Li, Thomas B Lowe, Steven Margheim, Curtis McCully, Ayan Mitra, Jose A. Muñoz, Matt Nicholl, Jakob Nordin, András Pál, Yen-Chen Pan, Anthony L. Piro, Sofia Rest, João Rino-Silvestre, César Rojas-Bravo, Krisztián Sárneczky, Matthew R. Siebert, Stephen J. Smartt, Ken Smith, Ádám Sódor, Maximilian D. Stritzinger, Róbert Szabó, Róbert Szakáts, Brad E. Tucker, József Vinkó, Xiaofeng Wang, J. Craig Wheeler, David R. Young, Alfredo Zenteno, KaiCheng Zhang, Gabriella Zsidi
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Wang, Q, Rest, A, Zenati, Y, Ridden-Harper, R, Dimitriadis, G, Narayan, G, Villar, V A, Magee, M R, Foley, R J, Shaya, E J, Garnavich, P, Wang, L, Hu, L, Bodi, A, Armstrong, P, Auchettl, K, Barclay, T, Barentsen, G, Bognar, Z, Brimacombe, J, Bulger, J, Burke, J, Challis, P, Chambers, K, Coulter, D A, Csornyei, G, Cseh, B, Deckers, M, Dotson, J L, Galbany, L, Gonzalez-Gaitan, S, Gromadzki, M, Gully-Santiago, M, Hanyecz, O, Hedges, C, Hiramatsu, D, Hosseinzadeh, G, Howell, D A, Howell, S B, Huber, M E, Jha, S W, Jones, D O, Konyves-Toth, R, Kalup, C, Kilpatrick, C D, Kriskovics, L, Li, W, Lowe, T B, Margheim, S, McCully, C, Mitra, A, Munoz, J A, Nicholl, M, Nordin, J, Pal, A, Pan, Y-C, Piro, A L, Rest, S, Rino-Silvestre, J, Rojas-Bravo, C, Sarneczky, K, Siebert, M R, Smartt, S J, Smith, K, Sodor, A, Stritzinger, M D, Szabo, R, Szakats, R, Tucker, B E, Vinko, J, Wang, X, Wheeler, J C, Young, D R, Zenteno, A, Zhang, K & Zsidi, G 2021, ' SN 2018agk : A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2) ', Astrophysical Journal, vol. 923, no. 2, 167 . https://doi.org/10.3847/1538-4357/ac2c84
instname
Wang, Q, Rest, A, Zenati, Y, Ridden-Harper, R, Dimitriadis, G, Narayan, G, Villar, V A, Magee, M R, Foley, R J, Shaya, E J, Garnavich, P, Wang, L, Hu, L, Bodi, A, Armstrong, P, Auchettl, K, Barclay, T, Barentsen, G, Bognar, Z, Brimacombe, J, Bulger, J, Burke, J, Challis, P, Chambers, K, Coulter, D A, Csornyei, G, Cseh, B, Deckers, M, Dotson, J L, Galbany, L, Gonzalez-Gaitan, S, Gromadzki, M, Gully-Santiago, M, Hanyecz, O, Hedges, C, Hiramatsu, D, Hosseinzadeh, G, Howell, D A, Howell, S B, Huber, M E, Jha, S W, Jones, D O, Konyves-Toth, R, Kalup, C, Kilpatrick, C D, Kriskovics, L, Li, W, Lowe, T B, Margheim, S, McCully, C, Mitra, A, Munoz, J A, Nicholl, M, Nordin, J, Pal, A, Pan, Y-C, Piro, A L, Rest, S, Rino-Silvestre, J, Rojas-Bravo, C, Sarneczky, K, Siebert, M R, Smartt, S J, Smith, K, Sodor, A, Stritzinger, M D, Szabo, R, Szakats, R, Tucker, B E, Vinko, J, Wang, X, Wheeler, J C, Young, D R, Zenteno, A, Zhang, K & Zsidi, G 2021, ' SN 2018agk : A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2) ', Astrophysical Journal, vol. 923, no. 2, 167 . https://doi.org/10.3847/1538-4357/ac2c84
Wang, Qinan, et al.
We present the 30 minutes cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase, and the decline until 40 days after peak. We addition
We present the 30 minutes cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase, and the decline until 40 days after peak. We addition
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caa34e69d28677da9a3db852d323e080