Zobrazeno 1 - 10
of 390
pro vyhledávání: '"Cieśla Ł"'
Autor:
Ciesla, L., Adscheid, S., Magnelli, B., Boquien, M., Laporte, N., Bethermin, M., Carvajal, C., Schinnerer, E., Liu, D.
[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representative of the bulk of the sources at these redshifts. In this work, we a
Externí odkaz:
http://arxiv.org/abs/2412.02557
Autor:
Arango-Toro, R. C., Ilbert, O., Ciesla, L., Shuntov, M., Aufort, G., Mercier, W., Laigle, C., Franco, M., Bethermin, M., Borgne, D. Le, Dubois, Y., McCracken, H. J., Paquereau, L., Huertas-Company, M., Kartaltepe, J., Casey, C. M., Akins, H., Allen, N., Andika, I., Brinch, M., Drakos, N. E., Faisst, A., Gozaliasl, G., Harish, S., Kaminsky, A., Koekemoer, A., Kokorev, V., Liu, D., Magdis, G., Martin, C. L., Moutard, T., Rhodes, J., Rich, R. M., Robertson, B., Sanders, D. B., Sheth, K., Talia, M., Toft, S., Tresse, L., Valentino, F., Vijayan, A., Weaver, J.
The stellar mass-star formation rate (M$_\star$ - SFR) plane is essential for distinguishing galaxy populations, but how galaxies move within this plane over cosmic time remains unclear. This study aims to describe galaxy migrations in the M$_\star$
Externí odkaz:
http://arxiv.org/abs/2410.05375
Autor:
Aufort, G., Laigle, C., McCracken, H. J., Borgne, D. Le, Arango-Toro, R., Ciesla, L., Ilbert, O., Tresse, L., Dubois, Y.
We propose a novel method to reconstruct the full posterior distribution of the star formation histories (SFHs) of galaxies from broad-band photometry. Our method combines simulation-based inference (SBI) using a neural network trained with SFHs and
Externí odkaz:
http://arxiv.org/abs/2410.00795
Autor:
Bisigello, L., Gruppioni, C., Bolatto, A., Ciesla, L., Pope, A., Armus, L., Smith, J. D., Somerville, R., Yung, L. Y. A., Wright, R. J., Bradford, C. M., Glenn, J., Feltre, A.
Publikováno v:
A&A 689, A125 (2024)
The most active phases of star formation and black hole accretion are strongly affected by dust extinction, making far-infrared (far-IR) observations the best way to disentangle and study the co-evolution of galaxies and super massive black holes. Th
Externí odkaz:
http://arxiv.org/abs/2404.17634
Autor:
Epinat, B., Contini, T., Mercier, W., Ciesla, L., Lemaux, B. C., Johnson, S. D., Richard, J., Brinchmann, J., Boogaard, L. A., Carton, D., Michel-Dansac, L., Bacon, R., Krajnovic, D., Finley, H., Schroetter, I., Ventou, E., Abril-Melgarejo, V., Boselli, A., Bouché, N. F., Kollatschny, W., Kovac, K., Paalvast, M., Soucail, G., Urrutia, T., Weilbacher, P. M.
Publikováno v:
A&A, 683, A205 (2024)
We introduce the MUSE gAlaxy Groups in COSMOS (MAGIC) survey, which was built to study the impact of environment on galaxy evolution over the last 8 Gyr. It consists of 17 MUSE fields targeting 14 massive structures at intermediate redshift ($0.3
Externí odkaz:
http://arxiv.org/abs/2312.00924
Autor:
Mercier, W., Shuntov, M., Gavazzi, R., Nightingale, J. W., Arango, R., Ilbert, O., Amvrosiadis, A., Ciesla, L., Casey, C., Jin, S., Faisst, A. L., Andika, I. T., Drakos, N. E., Enia, A., Franco, M., Gillman, S., Gozaliasl, G., Hayward, C. C., Huertas-Company, M., Kartaltepe, J. S., Koekemoer, A. M., Laigle, C., Borgne, D. Le, Magdis, G., Mahler, G., Maraston, C., Martin, C. L., Massey, R., McCracken, H. J., Moutard, T., Paquereau, L., Rhodes, J. D., Robertson, B. E., Sanders, D. B., Trebitsch, M., Tresse, L., Vijayan, A. P.
Publikováno v:
A&A 687, A61 (2024)
Aims. We provide an in-depth analysis of the COSMOS-Web ring, an Einstein ring at z=2 that we serendipitously discovered in the COSMOS-Web survey and possibly the most distant lens discovered to date. Methods. We extract the visible and NIR photometr
Externí odkaz:
http://arxiv.org/abs/2309.15986
Autor:
Ciesla, L., Elbaz, D., Ilbert, O., Buat, V., Magnelli, B., Narayanan, D., Daddi, E., Gómez-Guijarro, C., Arango-Toro, R.
Publikováno v:
A&A 686, A128 (2024)
Star formation histories (SFH) of early (6$
Externí odkaz:
http://arxiv.org/abs/2309.15720
Autor:
Mercier, W., Epinat, B., Contini, T., Krajnović, D., Ciesla, L., Lemaux, B. C., Abril-Melgarejo, V., Boogaard, L., Pelliccia, D.
Publikováno v:
A&A 677, A143 (2023)
Aims: At intermediate redshift, galaxy groups/clusters are thought to impact galaxies (e.g. their angular momentum). We investigate whether the environment has an impact on the galaxies' angular momentum and identify underlying driving physical mecha
Externí odkaz:
http://arxiv.org/abs/2307.13355
Autor:
Mountrichas, G., Yang, G., Buat, V., Darvish, B., Boquien, M., Ni, Q., Burgarella, D., Ciesla, L.
Publikováno v:
A&A 675, A137 (2023)
In this work, we study the relation of cosmic environment and morphology with the star-formation (SF) and the stellar population of galaxies. Most importantly, we examine if this relation differs for systems with active and non-active supermassive bl
Externí odkaz:
http://arxiv.org/abs/2306.03129
Publikováno v:
A&A 675, A126 (2023)
Radio used as a star formation rate (SFR) tracer presents enormous advantages by being unaffected by dust and radio sources being pinpointed at the sub-arc-second level. The interpretation of the low frequency 1.4 GHz luminosity is hampered by the di
Externí odkaz:
http://arxiv.org/abs/2304.13758