Zobrazeno 1 - 10
of 158
pro vyhledávání: '"K Boutsia"'
Autor:
G., Calderone, K., Boutsia, S., Cristiani, A., Grazian, R., Amorin, V., D'Odorico, G., Cupani, F., Fontanot, M, Salvato
The study of absorptions along the lines of sight to bright high-$z$ QSOs is an invaluable cosmological tool that provides a wealth of information on the inter-/circum-galactic medium, Dark Matter, primordial elements, reionization, fundamental const
Externí odkaz:
http://arxiv.org/abs/1909.06391
Autor:
P. Ruiz-Lapuente, J. I. González Hernández, R. Cartier, K. Boutsia, F. Figueras, R. Canal, L. Galbany
Publikováno v:
The Astrophysical Journal, Vol 947, Iss 2, p 90 (2023)
We use the Gaia EDR3 to explore the Galactic supernova remnant (SNR) G272.2-3.2, produced by the explosion of a Type Ia supernova (SN Ia) about 7500 yr ago, to search for a surviving companion. From the abundances in the SNR ejecta, G272.2-3.2 is a n
Externí odkaz:
https://doaj.org/article/b0b3c1b304904d738e744e03cc596871
Autor:
J M DerKacy, S Paugh, E Baron, P J Brown, C Ashall, C R Burns, E Y Hsiao, S Kumar, J Lu, N Morrell, M M Phillips, M Shahbandeh, B J Shappee, M D Stritzinger, M A Tucker, Z Yarbrough, K Boutsia, P Hoeflich, L Wang, L Galbany, E Karamehmetoglu, K Krisciunas, P Mazzali, A L Piro, N B Suntzeff, A Fiore, C P Gutiérrez, P Lundqvist, A Reguitti
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:3481-3505
We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT, UV spectroscopy from HST/STIS, and high-cadence optical photometry with t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c65d1f77a10981714e6ea7070e0fd739
https://doi.org/10.1093/mnras/stad1171
https://doi.org/10.1093/mnras/stad1171
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
P. Ruiz-Lapuente, J. I. González Hernández, R. Cartier, K. Boutsia, F. Figueras, R. Canal, L. Galbany
We use the {\it Gaia} EDR3 to explore the Galactic supernova remnant SNR G272.2-3.2, produced by the explosion of a Type Ia supernova (SNIa), about 7,500 years ago, to search for a surviving companion. From the abundances in the SNR ejecta, G272.2-3.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10539fba58a4c5463580c57c6ffc3b97
http://arxiv.org/abs/2206.01855
http://arxiv.org/abs/2206.01855
Autor:
C. Ashall, J. Lu, B. J. Shappee, C. R. Burns, E. Y. Hsiao, S. Kumar, N. Morrell, M. M. Phillips, M. Shahbandeh, E. Baron, K. Boutsia, P. J. Brown, J. M. DerKacy, L. Galbany, P. Hoeflich, K. Krisciunas, P. Mazzali, A. L. Piro, M. D. Stritzinger, N. B. Suntzeff
Publikováno v:
Ashall, C, Lu, J, Shappee, B J, Burns, C R, Hsiao, E Y, Kumar, S, Morrell, N, Phillips, M M, Shahbandeh, M, Baron, E, Boutsia, K, Brown, P J, DerKacy, J M, Galbany, L, Hoeflich, P, Krisciunas, K, Mazzali, P, Piro, A L, Stritzinger, M D & Suntzeff, N B 2022, ' A Speed Bump : SN 2021aefx Shows that Doppler Shift Alone Can Explain Early Excess Blue Flux in Some Type Ia Supernovae ', Astrophysical Journal Letters, vol. 932, no. 1, L2 . https://doi.org/10.3847/2041-8213/ac7235
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
We present early-time photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2021aefx. The early-time u-band light curve shows an excess flux when compared to normal SNe Ia. We suggest that the early excess blue flux may be due t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6606a6f578be6a8d46274d71396a99f3
https://pure.au.dk/portal/da/publications/a-speed-bump(b0b1fad6-cbdf-42b4-9a1a-c1e915ae9436).html
https://pure.au.dk/portal/da/publications/a-speed-bump(b0b1fad6-cbdf-42b4-9a1a-c1e915ae9436).html
Autor:
T. Treu, G. Roberts-Borsani, M. Bradac, G. Brammer, A. Fontana, A. Henry, C. Mason, T. Morishita, L. Pentericci, X. Wang, A. Acebron, M. Bagley, P. Bergamini, D. Belfiori, A. Bonchi, K. Boyett, K. Boutsia, A. Calabró, G. B. Caminha, M. Castellano, A. Dressler, K. Glazebrook, C. Grillo, C. Jacobs, T. Jones, P. L. Kelly, N. Leethochawalit, M. A. Malkan, D. Marchesini, S. Mascia, A. Mercurio, E. Merlin, T. Nanayakkara, M. Nonino, D. Paris, B. Poggianti, P. Rosati, P. Santini, C. Scarlata, H. V. Shipley, V. Strait, M. Trenti, C. Tubthong, E. Vanzella, B. Vulcani, L. Yang
Publikováno v:
Treu, T, Roberts-Borsani, G, Bradac, M, Brammer, G, Fontana, A, Henry, A, Mason, C, Morishita, T, Pentericci, L, Wang, X, Acebron, A, Bagley, M, Bergamini, P, Belfiori, D, Bonchi, A, Boyett, K, Boutsia, K, Calabro, A, Caminha, G B, Castellano, M, Dressler, A, Glazebrook, K, Grillo, C, Jacobs, C, Jones, T, Kelly, P L, Leethochawalit, N, Malkan, M A, Marchesini, D, Mascia, S, Mercurio, A, Merlin, E, Nanayakkara, T, Nonino, M, Paris, D, Poggianti, B, Rosati, P, Santini, P, Scarlata, C, Shipley, H, Strait, V, Trenti, M, Tubthong, C, Vanzella, E, Vulcani, B & Yang, L 2022, ' The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans ', Astrophysical Journal, vol. 935, no. 2, 110 . https://doi.org/10.3847/1538-4357/ac8158
The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, “what sources
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e5f6180ffc2ad4ba6e3ba87fb5b9472
http://hdl.handle.net/20.500.12386/32681
http://hdl.handle.net/20.500.12386/32681
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
E. Giallongo, K. Boutsia, A. Grazian, Francesca Civano, Fabrizio Fiore, N. Menci, S. Cristiani, F. Fontanot, G. Cupani, Mark Dickinson, M. Romano
It is a widespread opinion that hydrogen reionization is mainly driven by primeval star-forming galaxies, with a minor role of high-z active galactic nuclei. Recent observations, however, challenge this notion, indicating a number of issues related t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2960788465cecf99c8f13d3016522d7d
http://hdl.handle.net/11577/3355852
http://hdl.handle.net/11577/3355852