Figure 1 from The Physics of the Accelerating Universe Camera

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The Physics of the Accelerating Universe Camera

Authors: Cristóbal Padilla, Francisco J. Castander, Alex Alarcón, Jelena Aleksic, Otger Ballester, Laura Cabayol, Laia Cardiel-Sas, Jorge Carretero, Ricard Casas, Javier Castilla, Martin Crocce, Manuel Delfino, Carlos Díaz, Martin Eriksen, Enrique Fernández, Pablo Fosalba, Juan García-Bellido, Enrique Gaztañaga, Javier Gaweda, Ferran Grañena, José Maía Ílla, Jorge Jiménez, Luis López, Pol Martí, Ramon Miquel, Christian Neissner, Cristóbal Pío, Eusebio Sánchez, Santiago Serrano, Ignacio Sevilla-Noarbe, Pau Tallada, Nadia Tonello, and Juan de Vicente

2019 The Astronomical Journal 157 246.

Provider: AAS Journals

Caption: Figure 1.

Comparison of the covered area (top) and the number of measured spectroscopic redshifts (bottom) vs. depth expressed as the equivalent i-band limiting magnitude between the VVDS (magenta) and different spectroscopic redshift surveys. The PAUS will be a few mag deeper (over 10 times denser) than current completed large-area flux-limited surveys (such as Gama) and 10 times larger than current completed deep flux-limited surveys (such as VVDS/VIPERS/Deep2; le Fevre et al. 2013).

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