Life beyond 30: Probing the-20 < M (UV) <-17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey

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Fältnamn	Indikatorer	Metadata
000		04941naa a2200805 4500
001		oai:DiVA.org:su-220835
003		SwePub
008		230914s2023 \| \|\|\|\|\|\|\|\|\|\|\|000 \|\|eng\|
024	7	a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2208352 URI
024	7	a https://doi.org/10.3847/2041-8213/acd9d02 DOI
040		a (SwePub)su
041		a engb eng
042		9 SwePub
072	7	a ref2 swepub-contenttype
072	7	a art2 swepub-publicationtype
100	1	a Perez-Gonzalez, Pablo G.4 aut
245	1 0	a Life beyond 30 :b Probing the-20 < M (UV) <-17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey
264	1	c 2023
338		a print2 rdacarrier
520		a We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at 8 < z < 13 derived from deep NIRCam observations taken in parallel with the MIRI Deep Survey of the Hubble Ultra Deep Field (HUDF), NIRCam covering the parallel field 2. Our deep (40 hr) NIRCam observations reach an F277W magnitude of 30.8 (5 & sigma;), more than 2 mag deeper than JWST public data sets already analyzed to find high-redshift galaxies. We select a sample of 44 z > 8 galaxy candidates based on their dropout nature in the F115W and/or F150W filters, a high probability for their photometric redshifts, estimated with three different codes, being at z > 8, good fits based on & chi; (2) calculations, and predominant solutions compared to z < 8 alternatives. We find mild evolution in the luminosity function from z & SIM; 13 to z & SIM; 8, i.e., only a small increase in the average number density of & SIM;0.2 dex, while the faint-end slope and absolute magnitude of the knee remain approximately constant, with values & alpha; = - 2.2 & PLUSMN; 0.1, and M * = - 20.8 & PLUSMN; 0.2 mag. Comparing our results with the predictions of state-of-the-art galaxy evolution models, we find two main results: (1) a slower increase with time in the cosmic star formation rate density compared to a steeper rise predicted by models; (2) nearly a factor of 10 higher star formation activity concentrated in scales around 2 kpc in galaxies with stellar masses & SIM;10(8) M (& ODOT;) during the first 350 Myr of the universe, z & SIM; 12, with models matching better the luminosity density observational estimations & SIM;150 Myr later, by z & SIM; 9.
650	7	a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650	7	a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
700	1	a Costantin, Luca4 aut
700	1	a Langeroodi, Danial4 aut
700	1	a Rinaldi, Pierluigi4 aut
700	1	a Annunziatella, Marianna4 aut
700	1	a Ilbert, Olivier4 aut
700	1	a Colina, Luis4 aut
700	1	a Norgaard-Nielsen, Hans Ulrik4 aut
700	1	a Greve, Thomas R.4 aut
700	1	a Östlin, Göran,d 1968-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ostlin
700	1	a Wright, Gillian4 aut
700	1	a Alonso-Herrero, Almudena4 aut
700	1	a Aalvarez-Marquez, Javier4 aut
700	1	a Caputi, Karina I.4 aut
700	1	a Eckart, Andreas4 aut
700	1	a Le Fevre, Olivier4 aut
700	1	a Labiano, Alvaro4 aut
700	1	a Garcia-Marin, Macarena4 aut
700	1	a Hjorth, Jens4 aut
700	1	a Kendrew, Sarah4 aut
700	1	a Pye, John P.4 aut
700	1	a Tikkanen, Tuomo4 aut
700	1	a van der Werf, Paul4 aut
700	1	a Walter, Fabian4 aut
700	1	a Ward, Martin4 aut
700	1	a Bik, Arjanu Stockholm Univ, AlbaNova Univ Ctr, Oscar Klein Ctr, Dept Astron, Stockholm, Sweden4 aut
700	1	a Boogaard, Leindert4 aut
700	1	a Bosman, Sarah E. I.4 aut
700	1	a Gomez, Alejandro Crespo4 aut
700	1	a Gillman, Steven4 aut
700	1	a Iani, Edoardo4 aut
700	1	a Jermann, Iris4 aut
700	1	a Melinder, Jens,d 1977-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jeand
700	1	a Meyer, Romain A.4 aut
700	1	a Moutard, Thibaud4 aut
700	1	a van Dishoek, Ewine4 aut
700	1	a Henning, Thomas4 aut
700	1	a Lagage, Pierre-Olivier4 aut
700	1	a Guedel, Manuel4 aut
700	1	a Peissker, Florian4 aut
700	1	a Ray, Tom4 aut
700	1	a Vandenbussche, Bart4 aut
700	1	a Garcia-Argumanez, Angela4 aut
700	1	a Merida, Rosa Maria4 aut
710	2	a Stockholms universitetb Institutionen för astronomi4 org
773	0	t Astrophysical Journal Lettersg 951:1q 951:1x 2041-8205x 2041-8213
856	4	u https://doi.org/10.3847/2041-8213/acd9d0y Fulltext
856	4 8	u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-220835
856	4 8	u https://doi.org/10.3847/2041-8213/acd9d0

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Av författaren/redakt...: Perez-Gonzalez, ...; Costantin, Luca; Langeroodi, Dani ...; Rinaldi, Pierlui ...; Annunziatella, M ...; Ilbert, Olivier; visa fler...; Colina, Luis; Norgaard-Nielsen ...; Greve, Thomas R.; Östlin, Göran, 1 ...; Wright, Gillian; Alonso-Herrero, ...; Aalvarez-Marquez ...; Caputi, Karina I ...; Eckart, Andreas; Le Fevre, Olivie ...; Labiano, Alvaro; Garcia-Marin, Ma ...; Hjorth, Jens; Kendrew, Sarah; Pye, John P.; Tikkanen, Tuomo; van der Werf, Pa ...; Walter, Fabian; Ward, Martin; Bik, Arjan; Boogaard, Leinde ...; Bosman, Sarah E. ...; Gomez, Alejandro ...; Gillman, Steven; Iani, Edoardo; Jermann, Iris; Melinder, Jens, ...; Meyer, Romain A.; Moutard, Thibaud; van Dishoek, Ewi ...; Henning, Thomas; Lagage, Pierre-O ...; Guedel, Manuel; Peissker, Floria ...; Ray, Tom; Vandenbussche, B ...; Garcia-Argumanez ...; Merida, Rosa Mar ...; visa färre...

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