The Dark Energy Survey (DES) is a photometric survey in 5 bands from optical to infrared (grizY) whose main goal is to determine the equation of state of dark energy. DES observed ~700 million objects detected in ~5000 square degrees in the Southern Hemisphere over 6 years. The articles with the main results of the data analysis from the first three years of observation are available on this page.
The second data release (DR2), already containing data from six years of observation, is available to the public and can be accessed at LIneA via User Query (here) or the Python library dblinea on LIneA JupyterHub.
LIneA User Query is based on daiquiri, a framework for the publication of scientific databases. For details, visit the daiquiri documentation page.
Texto para colocar na home do daiquiri (o mesmo do notebook de tutorial do dblinea no jupyterhub)
LIneA User Query
The Dark Energy Survey (DES) is a photometric survey in 5 bands from optical to infrared (grizY) whose main goal is to determine the equation of state of dark energy. DES observed ~700 million objects detected in ~5000 square degrees in the Southern Hemisphere over 6 years. The articles with the main results of the data analysis from the first three years of observation are available on this page.
Figure: Footprint Data Release 2 (source: www.darkenergysurvey.org).
The second data release (DR2), already containing data from six years of observation, is available to the public and can be accessed at LIneA via User Query (here) or the Python library
dblinea
on LIneA JupyterHub.LIneA User Query is based on daiquiri, a framework for the publication of scientific databases. For details, visit the daiquiri documentation page.