Galaxy evolution with J-PAS

Bibcode
2025hsa..conf...74B
Bonoli, S.; Acharya, N.; Cortesi, A.; Díaz-García, L. A.; González Delgado, R. M.; Iglesias-Páramo, J.; López, I. E.; Rahna, P. T.; Rodríguez-Martín, J. E.; Torralba, A.; Abramo, R.; Alcaniz, J.; Benitez, N.; Carneiro, S.; Cenarro, J.; Cristóbal-Hornillos, D.; Dupke, R.; Ederoclite, A.; Hernán-Caballero, A.; Hernández-Monteagudo, C.; López-Sanjuan, C.; Marín-Franch, A.; Mendes de Oliveira, C.; Moles, M.; Sodré, L., Jr.; Taylor, K.; Varela, J.; Vázquez Ramió, H.
Referencia bibliográfica

Highlights of Spanish Astrophysics XII

Fecha de publicación:
5
2025
Número de autores
28
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
The Javalambre Physics of the Accelerating Universe Survey (J-PAS) has started observing wide areas of the northern sky with its unique set of 56 filters: 54 narrow band and 2 broader filters that cover the full optical range and effectively deliver a low-resolution spectrum for every object detected. Observations are carried out from the dedicated Javalambre Survey Telescope (JST/T250), based in the Observatorio Astrofísico de Javalambre (OAJ) and equipped with the wide field camera JPCam. The combination of the wide area coverage, the multi-band information and the high spatial resolution, make J-PAS an ideal survey not only for cosmological probes, but also for galaxy evolution studies. In this work we show the potential of J-PAS in the field of galaxy evolution by using ``mini-JPAS'', a small dataset of J-PAS-like data acquired during the testing phases of the JST/T250.
Tipo
Sin árbitro

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