CADE
http://cade.ovgso.fr/
2026-11-05T13:17:00+00:00CADE
http://cade.ovgso.fr/
http://cade.ovgso.fr/lib/exe/fetch.php?media=wiki:dokuwiki.svgtext/html2026-11-04T10:09:02+00:00dparadis (dparadis@undisclosed.example.com)Publications
http://cade.ovgso.fr/doku.php?id=publications&rev=1793786942&do=diff
Publications
Method paper
Paradis et al. (2012) describes the method used in CADE's drizzling software.
List of publications using CADE
Paradis, D., Bernard, J.-P., Mény, C., 2009, A&A, 506, 745, Dust emissivity variations in the Milky-Way
Bernard, J.-P., Paradis, D., Marshall, D. J., et al., 2010, A&A, 518, 88, Dust Temperature tracing the ISRF intensity in the Galaxytext/html2026-10-15T12:21:56+00:00dparadis (dparadis@undisclosed.example.com)Neural Network Predictions
http://cade.ovgso.fr/doku.php?id=nnpredictions&rev=1792066916&do=diff
Neural Network Predictions
Based on supervised deep learning algorithms, the CADE service produced dust emission estimates at 850 microns (353 GHz) and 1.38 mm (217 GHz) at the Herschel resolution (37 arcsec). To perform this work, Herschel data of Galactic environments, smoothed to the 5 arcmin angular resolution, have been used to train the neural network to provide the best model able to reproduce Planck maps of dust emission (after removing CMB, CIB and 12CO contributions) in the two bands …text/html2026-09-21T10:31:29+00:00dparadis (dparadis@undisclosed.example.com)Atacama Cosmology Telescope (ACT) - Planck
http://cade.ovgso.fr/doku.php?id=act-planck&rev=1789986689&do=diff
Atacama Cosmology Telescope (ACT) - Planck
The Atacama Cosmology Telescope (ACT) is a six-meter diameter telescope on Cerro Toco in the Atacama Desert of northern Chile. The ACT DR4 data release collected data from 2013 to 2016. ACT was upgraded to the AdvancedACT camera and conducted a 2017–2022 survey, corresponding to ACT DR6 data release, covering about 45% of the sky.
At arcminute resolution, the surveys cover three frequency bands centered on 98, 150 and 220text/html2026-09-14T10:47:07+00:00dparadis (dparadis@undisclosed.example.com)
http://cade.ovgso.fr/doku.php?id=sidebar&rev=1789382827&do=diff
* Welcome
* CADE News
* CADE FAQ & Community
* Acknowledging CADE
* Team
* Publications
* Software
* Drizzlib
* DrizzWeb
* SED Extractor
* SED Extractor (web)
* Neural Network Predictions
* Missions/Surveys
* ACT-Planck
* AKARI
* AMIGPS
* APEX/LABOCA
* APEX/ArTéMiS
* BLAST
* Bolocam
* CGPS
* CHIMPS
* CHIPASS
* COHRS
* COMPTEL
* DIRBE
* DHT-Nanten
* DRAO
* Dwingeloo
* Effelsberg
* EBHIS
* EBV_SFD98
* Fermi
…text/html2026-09-14T09:26:57+00:00dparadis (dparadis@undisclosed.example.com)NRAO VLA D-array Sky Survey (NVSS)
http://cade.ovgso.fr/doku.php?id=nvss&rev=1789378017&do=diff
NRAO VLA D-array Sky Survey (NVSS)
The National Radio Astronomy Observatory (NRAO) observed the sky north of declination -40° using the Very Large Array (VLA) (D-array) at the 1.4 GHz frequency. We present the total intensity survey, covering 82% of the sky, at an angular resolution of 45