Items where Author is "Boutsia, K"

Article

DerKacy, JM ORCID: 0000-0002-7566-6080, Paugh, S ORCID: 0000-0002-6503-8865, Baron, E ORCID: 0000-0001-5393-1608, Brown, PJ ORCID: 0000-0001-6272-5507, Ashall, C ORCID: 0000-0002-5221-7557, Burns, CR ORCID: 0000-0003-4625-6629, Hsiao, EY ORCID: 0000-0003-1039-2928, Kumar, S ORCID: 0000-0001-8367-7591, Lu, J ORCID: 0000-0002-3900-1452, Morrell, N ORCID: 0000-0003-2535-3091, Phillips, MM ORCID: 0000-0003-2734-0796, Shahbandeh, M ORCID: 0000-0002-9301-5302, Shappee, BJ ORCID: 0000-0003-4631-1149, Stritzinger, MD ORCID: 0000-0002-5571-1833, Tucker, MA ORCID: 0000-0002-2471-8442, Yarbrough, Z ORCID: 0000-0002-9825-1136, Boutsia, K ORCID: 0000-0003-4432-5037, Hoeflich, P ORCID: 0000-0002-4338-6586, Wang, L ORCID: 0000-0001-7092-9374, Galbany, L ORCID: 0000-0002-1296-6887 et al (2023) SN 2021fxy: mid-ultraviolet flux suppression is a common feature of Type Ia supernovae. Monthly Notices of the Royal Astronomical Society, 522 (3). pp. 3481-3505. ISSN 0035-8711

Ashall, C ORCID: 0000-0002-5221-7557, Lu, J ORCID: 0000-0002-3900-1452, Shappee, BJ ORCID: 0000-0003-4631-1149, Burns, CR ORCID: 0000-0003-4625-6629, Hsiao, EY ORCID: 0000-0003-1039-2928, Kumar, S ORCID: 0000-0001-8367-7591, Morrell, N ORCID: 0000-0003-2535-3091, Phillips, MM ORCID: 0000-0003-2734-0796, Shahbandeh, M ORCID: 0000-0002-9301-5302, Baron, E ORCID: 0000-0001-5393-1608, Boutsia, K ORCID: 0000-0003-4432-5037, Brown, PJ ORCID: 0000-0001-6272-5507, DerKacy, JM ORCID: 0000-0002-7566-6080, Galbany, L ORCID: 0000-0002-1296-6887, Hoeflich, P ORCID: 0000-0002-4338-6586, Krisciunas, K ORCID: 0000-0002-6650-694X, Mazzali, P ORCID: 0000-0001-6876-8284, Piro, AL ORCID: 0000-0001-6806-0673, Stritzinger, MD ORCID: 0000-0002-5571-1833 and Suntzeff, NB ORCID: 0000-0002-8102-181X (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, 932 (1). ISSN 2041-8205