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Documentation

Find information, examples, FAQs and extensive descriptions of the data, curated by the survey teams.

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DEVILS

The Deep Extragalactic VIsible Legacy Survey is a spectroscopic campaign at the AAT aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3<z<1.0).

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Authors

13

Overview
Info coming soon.
About

The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a spectroscopic campaign at the Anglo-Australian Telescope aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3<z<1.0). Our sample will consist of ~58k galaxies to Ymag<21.2, over ~6deg2 to >95% completeness in three well studies deep extragalactic fields (COSMOS, ECDFS and XMM-LSS).

https://devilsurvey.org/
Luke Davies
[javascript protected email address]
devilsurvey
Dec. 1, 2017
In Progress
Latest updates view all
Available bands Feb. 16, 2018, 4:12 p.m. luke.davies
2017B Observations Summary Feb. 16, 2018, 4:23 p.m. luke.davies
DEVILS DR0 Input Catalogue Feb. 16, 2018, 4:25 p.m. luke.davies

DEVILS Documentation

 Input Catalogue
Articles on the preparation of the DEVILS input catalogues and their generation. DEVILS target sources are selected from VISTA Y-band imaging (VIDEO in D02 & D03, UltraVISTA in D10). Source properties are derived using ProFound (Robotham et al., 2018)
Articles
DEVILS DR0 Input Catalogue luke.davies Feb. 16, 2018 Feb. 16, 2018, 4:25 p.m.
 Imaging
Descriptions of the available photometric datasets for DEVILS regions. DEVILS target sources are selected from VISTA Y-band imaging (VIDEO in D02 & D03, UltraVISTA in D10). Source properties are derived using ProFound (Robotham et al., 2018)
Articles
Available bands luke.davies Feb. 16, 2018 Feb. 16, 2018, 4:12 p.m.
 Spectra
DEVILS spectral observations will be taken with the AAT+AAOmega between 2017-2020.
Articles
2017B Observations Summary luke.davies Feb. 16, 2018 Feb. 16, 2018, 4:23 p.m.