EmulART: Emulating radiative transfer—a pilot study on autoencoder-based dimensionality reduction for radiative transfer models

Autor: João Rino-Silvestre, Santiago González-Gaitán, Marko Stalevski, Majda Smole, Pedro Guilherme-Garcia, Joao Paulo Carvalho, Ana Maria Mourão

Publikováno v: Neural Computing and Applications. 35:7719-7760

Dust is a major component of the interstellar medium. Through scattering, absorption and thermal re-emission, it can profoundly alter astrophysical observations. Models for dust composition and distribution are necessary to better understand and curb

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78428b3309d31453da9ffb356dca0805
https://doi.org/10.1007/s00521-022-08071-x

SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)

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

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caa34e69d28677da9a3db852d323e080