Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Sophie E. van Mierlo"'
Autor:
Sophie E. van Mierlo, Karina I. Caputi, Matthew L. N. Ashby, Vasily Kokorev, Rafael Navarro-Carrera, Pierluigi Rinaldi
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 12 (2024)
We have characterized 26 Spitzer/IRAC-selected sources from the SMUVS program that are undetected in the UltraVISTA DR5 H - and/or K _s -band images, covering 94 arcmin ^2 of the COSMOS field, which have deep multiwavelength JWST photo
Externí odkaz:
https://doaj.org/article/e7d28d7059eb4926b4098d86abb3d5cd
Autor:
Rafael Navarro-Carrera, Pierluigi Rinaldi, Karina I. Caputi, Edoardo Iani, Vasily Kokorev, Sophie E. van Mierlo
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 2, p 207 (2024)
We analyze a sample of 3300 galaxies between redshifts z ≃ 3.5 and z ≃ 8.5 selected from James Webb Space Telescope (JWST) images in the Hubble Ultra Deep Field and UKIDSS Ultra Deep Survey field, including objects with stellar masses as low as
Externí odkaz:
https://doaj.org/article/31446c9b788f4b169a96cf33629e3c9d
Publikováno v:
The Astrophysical Journal Letters, Vol 945, Iss 2, p L21 (2023)
Recent controversy regarding the existence of massive ( $\mathrm{log}({M}_{* }/{M}_{\odot })\gtrsim 11$ ) galaxies at z > 6 poses a challenge for galaxy formation theories. Hence, it is of critical importance to understand the effects of SED fitting
Externí odkaz:
https://doaj.org/article/4839b2c1495746ca9f753ac7189d5dff
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 82 (2023)
Submillimeter observations reveal the star formation activity obscured by dust in the young Universe. It still remains unclear how galaxies detected at submillimeter wavelengths are related to ultraviolet/optical-selected galaxies in terms of their o
Externí odkaz:
https://doaj.org/article/1c74944dbfc64678b842d624bb61679d
Autor:
Pierluigi Rinaldi, Karina I. Caputi, Sophie E. van Mierlo, Matthew L. N. Ashby, Gabriel B. Caminha, Edoardo Iani
Publikováno v:
The Astrophysical Journal, 930:128. IOP PUBLISHING LTD
We study the relation between stellar mass (M*) and star formation rate (SFR) for star-forming galaxies over approximately five decades in stellar mass (5.5 ~ 10^9 Msun at these redshifts and reach a peak of 40% at z=4-5. More importantly, 60% to 90%
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b453b1763c1cd1cd9650fda52ef09d61
https://research.rug.nl/en/publications/c3b654e8-3024-45d6-8fe5-499269fc7b8a
https://research.rug.nl/en/publications/c3b654e8-3024-45d6-8fe5-499269fc7b8a