Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Covelo-Paz, A."'
Autor:
Heintz, Kasper E., Bennett, Jake S., Oesch, Pascal A., Sneppen, Albert, Rennehan, Douglas, Witstok, Joris, Smit, Renske, Vejlgaard, Simone, Terp, Chamilla, Koca, Umran S., Brammer, Gabriel B., Finlator, Kristian, Hayes, Matthew J., Sijacki, Debora, Naidu, Rohan P., Matthee, Jorryt, Valentino, Francesco, Tanvir, Nial R., Jakobsson, Páll, Laursen, Peter, Watson, Darach J., Davé, Romeel, Keating, Laura C., Covelo-Paz, Alba
Galaxy clusters are the most massive, gravitationally-bound structures in the Universe, emerging through hierarchical structure formation of large-scale dark matter and baryon overdensities. Early galaxy ``proto-clusters'' are believed to be importan
Externí odkaz:
http://arxiv.org/abs/2407.06287
Autor:
Meyer, R. A., Oesch, P. A., Giovinazzo, E., Weibel, A., Brammer, G., Matthee, J., Naidu, R. P., Bouwens, R. J., Chisholm, J., Covelo-Paz, A., Fudamoto, Y., Maseda, M., Nelson, E., Shivaei, I., Xiao, M., Herard-Demanche, T., Illingworth, G. D., Kerutt, J., Kramarenko, I., Labbe, I., Leonova, E., Magee, D., Matharu, J., Lyon, G. Prieto, Reddy, N., Schaerer, D., Shapley, A., Stefanon, M., Wozniak, M. A., Wuyts, S.
We present the census of H$\beta$+[O III] $4960,5008$ \AA emitters at $6.8
Externí odkaz:
http://arxiv.org/abs/2405.05111
Autor:
Matharu, Jasleen, Nelson, Erica J., Brammer, Gabriel, Oesch, Pascal A., Allen, Natalie, Shivaei, Irene, Naidu, Rohan P., Chisholm, John, Covelo-Paz, Alba, Fudamoto, Yoshinobu, Giovinazzo, Emma, Herard-Demanche, Thomas, Kerutt, Josephine, Kramarenko, Ivan, Marchesini, Danilo, Meyer, Romain A., Prieto-Lyon, Gonzalo, Reddy, Naveen, Shuntov, Marko, Weibel, Andrea, Wuyts, Stijn, Xiao, Mengyuan
We present the first results on the spatial distribution of star formation in 454 star-forming galaxies at $4.8
Externí odkaz:
http://arxiv.org/abs/2404.17629
Autor:
Neufeld, Chloe, van Dokkum, Pieter, Asali, Yasmeen, Covelo-Paz, Alba, Leja, Joel, Lin, Jamie, Matthee, Jorryt, Oesch, Pascal A., Reddy, Naveen A., Shivaei, Irene, Whitaker, Katherine E., Wuyts, Stijn, Brammer, Gabriel, Marchesini, Danilo, Maseda, Michael V., Naidu, Rohan P., Nelson, Erica J., Velichko, Anna, Weibel, Andrea, Xiao, Mengyuan
We present results from the JWST First Reionization Epoch Spectroscopically Complete Observations survey (FRESCO) on the star forming sequence of galaxies at $1.0
Externí odkaz:
http://arxiv.org/abs/2404.10816
Context. Stars that are members of stellar clusters are assumed to be formed at the same time and place from material with the same initial chemical composition. These additional constraints on the ensemble of cluster stars make these stars suitable
Externí odkaz:
http://arxiv.org/abs/2310.06757
Autor:
Oesch, P. A., Brammer, G., Naidu, R. P., Bouwens, R. J., Chisholm, J., Illingworth, G. D., Matthee, J., Nelson, E., Qin, Y., Reddy, N., Shapley, A., Shivaei, I., van Dokkum, P., Weibel, A., Whitaker, K., Wuyts, S., Covelo-Paz, A., Endsley, R., Fudamoto, Y., Giovinazzo, E., Herard-Demanche, T., Kerutt, J., Kramarenko, I., Labbe, I., Leonova, E., Lin, J., Magee, D., Marchesini, D., Maseda, M., Mason, C., Matharu, J., Meyer, R. A., Neufeld, C., Lyon, G. Prieto, Schaerer, D., Sharma, R., Shuntov, M., Smit, R., Stefanon, M., Wyithe, J. S. B., Xiao, M.
We present the JWST Cycle 1 53.8hr medium program FRESCO, short for "First Reionization Epoch Spectroscopically Complete Observations". FRESCO covers 62 arcmin$^2$ in each of the two GOODS/CANDELS fields for a total area of 124 arcmin$^2$ exploiting
Externí odkaz:
http://arxiv.org/abs/2304.02026
Akademický článek
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Autor:
Oesch, P A, Brammer, G, Naidu, R P, Bouwens, R J, Chisholm, J, Illingworth, G D, Matthee, J, Nelson, E, Qin, Y, Reddy, N, Shapley, A, Shivaei, I, van Dokkum, P, Weibel, A, Whitaker, K, Wuyts, S, Covelo-Paz, A, Endsley, R, Fudamoto, Y, Giovinazzo, E
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 10/20/2023, Vol. 525 Issue 2, p2864-2874, 11p
Autor:
Alba Covelo Paz
Publikováno v:
TheScienceBreaker. 9
Faraway galaxies are hard to detect, not only because they appear fainter, but also because the light that we detect from them is infrared. Many of these objects were invisible to us until the James Webb Space Telescope was launched. With this new te