Zobrazeno 1 - 10
of 705
pro vyhledávání: '"Guijarro, C"'
Autor:
Blánquez-Sesé, David, Magdis, G. E., Gómez-Guijarro, C., Shuntov, M., Kokorev, V., Brammer, G., Valentino, F., Díaz-Santos, T., Paspaliaris, E. -D., Rigopoulou, D., Hjorth, J., Langeroodi, D., Gobat, R., Jin, S., Sillassen, N. B., Gillman, S., Greve, T. R., Lee, M.
Publikováno v:
A&A 679, L2 (2023)
We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep $JWST$ imaging in the SMACS-0723 cluster field we identify a mass limited ($M_{*} >10^{9}$M$_{\odot}$) sample of intermediate redshift Q
Externí odkaz:
http://arxiv.org/abs/2310.01601
Autor:
Ciesla, L., Elbaz, D., Ilbert, O., Buat, V., Magnelli, B., Narayanan, D., Daddi, E., Gómez-Guijarro, C., Arango-Toro, R.
Publikováno v:
A&A 686, A128 (2024)
Star formation histories (SFH) of early (6$
Externí odkaz:
http://arxiv.org/abs/2309.15720
Autor:
Blánquez-Sesé, David, Gómez-Guijarro, C., Magdis, G. E., Magnelli, B., Gobat, R., Daddi, E., Franco, M., Whitaker, K., Valentino, F., Adscheid, S., Schinnerer, E., Zanella, A., Xiao, M., Wang, T., Liu, D., Kokorev, V., Elbaz, D.
Publikováno v:
A&A 674, A166 (2023)
We present a 1.1mm stacking analysis of moderately massive (log($M_{*}$/$M_{\odot}$) = 10.7 $\pm$ 0.2) quiescent galaxies (QGs) at $\langle z\rangle \sim1.5$, searching for cold dust continuum emission, an excellent tracer of dust and gas mass. Using
Externí odkaz:
http://arxiv.org/abs/2303.12110
Autor:
Ciesla, L., Gómez-Guijarro, C., Buat, V., Elbaz, D., Jin, S., Béthermin, M., Daddi, E., Franco, M., Inami, H., Magdis, G., Magnelli, B.
Publikováno v:
A&A 672, A191 (2023)
Recently, a population of compact main sequence (MS) galaxies exhibiting starburst-like properties have been identified in the GOODS-ALMA blind survey at 1.1mm. Several evolution scenarios were proposed to explain their particular physical properties
Externí odkaz:
http://arxiv.org/abs/2211.02510
Autor:
Jiménez-Andrade, E. F., Cantalupo, S., Magnelli, B., Romano-Díaz, E., Gómez-Guijarro, C., Mackenzie, R., Smolčić, V., Murphy, E., Matthee, J., Toft, S.
Ly$\alpha$ $\lambda$1216 (Ly$\alpha$) emission extending over $\gtrsim\,\rm 10\,kiloparsec\,(kpc)$ around dusty, massive starbursts at $z\gtrsim3$ might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obt
Externí odkaz:
http://arxiv.org/abs/2210.07982
Autor:
Daddi, E., Delvecchio, I., Dimauro, P., Magnelli, B., Gomez-Guijarro, C., Coogan, R., Elbaz, D., Kalita, B. S., Bail, A. Le, Rich, R. M., Tan, Q.
We analyse measurements of the evolving stellar mass (M0) at which the bending of the star-forming main sequence (MS) occurs over 0
Externí odkaz:
http://arxiv.org/abs/2203.10880
Autor:
Gómez-Guijarro, C., Elbaz, D., Xiao, M., Kokorev, V. I., Magdis, G. E., Magnelli, B., Daddi, E., Valentino, F., Sargent, M. T., Dickinson, M., Béthermin, M., Franco, M., Pope, A., Kalita, B. S., Ciesla, L., Demarco, R., Inami, H., Rujopakarn, W., Shu, X., Wang, T., Zhou, L., Alexander, D. M., Bournaud, F., Chary, R., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Iono, D., Juneau, S., Kartaltepe, J. S., Lagache, G., Floc'h, E. Le, Leiton, R., Leroy, L., Lin, L., Motohara, K., Mullaney, J., Okumura, K., Pannella, M., Papovich, C., Treister, E.
Publikováno v:
A&A 659, A196 (2022)
Compact star formation appears to be generally common in dusty star-forming galaxies (SFGs). However, its role in the framework set by the scaling relations in galaxy evolution remains to be understood. In this work we follow up on the galaxy sample
Externí odkaz:
http://arxiv.org/abs/2201.02633
Autor:
Gómez-Guijarro, C., Elbaz, D., Xiao, M., Béthermin, M., Franco, M., Magnelli, B., Daddi, E., Dickinson, M., Demarco, R., Inami, H., Rujopakarn, W., Magdis, G. E., Shu, X., Chary, R., Zhou, L., Alexander, D. M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Iono, D., Juneau, S., Kartaltepe, J. S., Lagache, G., Floc'h, E. Le, Leiton, R., Lin, L., Motohara, K., Mullaney, J., Nagar, N. M., Okumura, K., Pannella, M., Papovich, C., Pope, A., Sargent, M. T., Silverman, J. D., Treister, E., Wang, T.
Publikováno v:
A&A 658, A43 (2022)
Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally occurs in compact regions smaller than the stellar distribution. Howev
Externí odkaz:
http://arxiv.org/abs/2106.13246
Autor:
Fraternali, F., Karim, A., Magnelli, B., Gómez-Guijarro, C., Jiménez-Andrade, E. F., Posses, A. C.
Publikováno v:
A&A 647, A194 (2021)
Massive starburst galaxies in the early Universe are estimated to have depletion times of $\sim 100$ Myr and thus be able to convert their gas very quickly into stars, possibly leading to a rapid quenching of their star formation. For these reasons,
Externí odkaz:
http://arxiv.org/abs/2011.05340
Autor:
Donevski, D., Lapi, A., Małek, K., Liu, D., Gómez-Guijarro, C., Davé, R., Kraljic, K., Pantoni, L., Man, A., Fujimoto, S., Feltre, A., Pearson, W., Li, Q., Narayanan, D.
Publikováno v:
A&A 644, A144 (2020)
The dust-to-stellar mass ratio ($M_{\rm dust}$/$M_{\rm \star}$) is a crucial yet poorly constrained quantity to understand the production mechanisms of dust, metals and stars in galaxy evolution. In this work we explore and interpret the nature of $M
Externí odkaz:
http://arxiv.org/abs/2008.09995