C Meldorf, A Palmese, D Brout, R Chen, D Scolnic, L Kelsey, L Galbany, W G Hartley, T M Davis, A Drlica-Wagner, M Vincenzi, J Annis, M Dixon, O Graur, C Lidman, A Möller, P Nugent, B Rose, M Smith, S Allam, D L Tucker, J Asorey, J Calcino, D Carollo, K Glazebrook, G F Lewis, G Taylor, B E Tucker, A G Kim, H T Diehl, M Aguena, F Andrade-Oliveira, D Bacon, E Bertin, S Bocquet, D Brooks, D L Burke, J Carretero, M Carrasco Kind, F J Castander, M Costanzi, L N da Costa, S Desai, P Doel, S Everett, I Ferrero, D Friedel, J Frieman, J García-Bellido, M Gatti, D Gruen, J Gschwend, G Gutierrez, S R Hinton, D L Hollowood, K Honscheid, D J James, K Kuehn, M March, J L Marshall, F Menanteau, R Miquel, R Morgan, F Paz-Chinchón, M E S Pereira, A A Plazas Malagón, E Sanchez, V Scarpine, I Sevilla-Noarbe, E Suchyta, G Tarle, T N Varga, Collaboration DES, The Dark Energy Survey Supernova Program results: Type Ia Supernova brightness correlates with host galaxy dust, Monthly Notices of the Royal Astronomical Society, 2022;, stac3056, https://doi.org/10.1093/mnras/stac3056
https://news.google.com/__i/rss/rd/articles/CBMiUWh0dHBzOi8vYWNhZGVtaWMub3VwLmNvbS9tbnJhcy9hZHZhbmNlLWFydGljbGUvZG9pLzEwLjEwOTMvbW5yYXMvc3RhYzMwNTYvNjc3NTEyMtIBAA?oc=5
2022-10-26 17:15:39Z
CBMiUWh0dHBzOi8vYWNhZGVtaWMub3VwLmNvbS9tbnJhcy9hZHZhbmNlLWFydGljbGUvZG9pLzEwLjEwOTMvbW5yYXMvc3RhYzMwNTYvNjc3NTEyMtIBAA
Tidak ada komentar:
Posting Komentar