CADE

Team

Déborah Paradis — 2026-03-12T10:31:04+02:00

Team Project Scientists : Déborah Paradis (IRAP) & Frédéric Paletou (IRAP) Project Manager : Jean-Michel Glorian (IRAP) Developper : Loïc Bertin (IRAP) ---------- The SED extractor has been developped by: * Michaël Devos (IRAP) *

Home

Déborah Paradis — 2026-03-09T12:53:51+02:00

Home Welcome to the “Centre d'Analyse de Données Etendues” (CADE) or “Analysis Center for Extended Data”. CADE provides maps of ancillary astronomical data to users in the astronomical community. The emphasis of CADE is on extended sky emission. The database is provided in the

Nobeyama

Déborah Paradis — 2026-02-16T14:18:21+02:00

Nobeyama Several surveys were performed using the 45-m telescope at the Nobeyama Radio Observatory. CADE produced HEALPix maps of some of them : - High-resolution CO Images of the Galactic Central Molecular Zone : 12CO (J=1-0), 13CO (J=1-0) and C180 (J=1-0) at the 15 arcsec resolution

Publications

Déborah Paradis — 2026-01-19T17:10:01+02:00

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 Galaxy

AKARI

Déborah Paradis — 2025-09-19T17:20:45+02:00

AKARI The Japanese AKARI mission was launched in February 2006. The telescope mirror had a diameter of 68.5 cm and was capable of observing infrared wavelengths between 2 and 180 microns. AKARI was equipped with two science instruments: the FIS (Far-Infrared Surveyor) for far-infrared observations and the

SED Extractor

Déborah Paradis — 2025-07-07T09:34:46+02:00

SED Extractor From this page you can download the SED extractor software library, a tool to extract a Spectral Energy Distribution from Healpix, WCS or mixture of Healpix and WCS files, in a specific region of the sky This tool guarantees the photometric accuracy, by using the drizzlib library (

Neural Network Predictions

Déborah Paradis — 2025-06-11T11:30:01+02:00

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 …

WHAM

Déborah Paradis — 2025-03-27T14:42:36+02:00

WHAM The Wisconsin H-alpha Mapper has surveyed the distribution and kinematics of ionized gas in the Northern sky in 1997-1998 and then in the Southern sky in 2009, at an angular resolution of 1°. The combination of the two survey represents the first all-sky survey of the diffuse H-alpha emission (6563 Angstroms) from the Milky-Way and consists of more than 49000 spectra (-100 Km/s < vLSR<+100 Km/s).

sed_extractor_1.0beta.zip - created

cade — 2023-03-13T23:34:43+02:00