DJp.2.10 — J-PAS: The Javalambre-Physics of the Accelerating Universe Astrophysical Survey

Date & Time

Aug 10th at 6:00 PM until 6:00 PM

Track

Presentations 

Location

Rating ( votes)

Author(s): Renato a Dupke4, Narciso Benitez2, Mariano Moles1, Laerte Sodre3, J-PAS Collaboration1

Institution(s): 1. Centro de Estudios de Fisica del Cosmos de Aragon, 2. Instituto de Astrofisica de Andalucia, 3. Instituto de Astronomia, Geofísica e Ciências Atmosféricas, 4. National Observatory

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) is a narrow band, very wide field Cosmological Survey to be carried out from the Javalambre Astrophysical Observatory in Spain with a dedicated 2.5m telescope and a 4.7deg^2 camera with 1.2Gpix. Starting in 2016, J-PAS will observe 8600 deg^2 of the Northern Sky and measure 0.003(1+z) precision photometric redshifts for nearly 1E08 LRG and ELG galaxies plus several million QSOs, sampling an effective volume of ~14 Gpc^3 up to z = 1.3. J-PAS will also detect and measure the mass of more than a hundred thousand galaxy clusters, setting constrains on Dark Energy which rival those obtained from BAO measurements.
The key to the J-PAS potential is its innovative approach the combination of 54 145°A filters, placed 100°A apart, and a multi-degree field of view (FOV) which makes it a powerful “redshift machine”, with the survey speed of a 4000 multiplexing low resolution spectrograph, but many times cheaper and much faster to build. Moreover, since the J-PAS camera is equivalent to a very large, 4.7deg^2 “IFU”, it will produce a time-resolved, 3D image of the Northern Sky with a very wide range of Astrophysical applications in Galaxy Evolution, the nearby Universe and the study of resolved stellar populations. J-PAS will have a lasting legacy value in many areas of Astrophysics, serving as a fundamental dataset for future Cosmological projects.
Here, we present the overall description, status and scientific potential of the survey.