http://cade.ovgso.fr/ 2026-05-07T09:24:09+00:00 http://cade.ovgso.fr/ http://cade.ovgso.fr/lib/exe/fetch.php?media=wiki:dokuwiki.svg text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=abell_1763&rev=1773763151&do=diff Abell 1763 PI: D. Fadda Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=akari&rev=1773763151&do=diff 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 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=amigps&rev=1773763151&do=diff Arcminute Microkelvin Imager (AMI) Galactic Plane Survey (AMIGPS) This 15.7 GHz survey has been carried out using the Arcminute Microkelvin Imager Small Array , which is operated by the Cavendish Astrophysics Group at Lord's Bridge, Cambridgeshire. It is a radio synthesis telescope comprising ten 3.7-m diameter dishes. The AMI Galactic Plane Survey is a large survey of the Galactic Plane, covering the area 76°<l<170° between latitudes of ıbı<5°. The angular resolution is approximately 3'. The… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=blast&rev=1773763151&do=diff Balloon-borne Large-Aperture Submillimeter Telescope (BLAST) BLAST incorporates a 2-m primary mirror with large-format bolometer arrays operating at 250, 350 and 500 microns. BLAST provides surveys from 0.8 to 200 deg2 at a resolution of 30, 42 and text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=bolocam&rev=1773763151&do=diff Bolocam Galactic Plane Survey (BGPS) The survey has been done using Bolocam on the Caltech Submillimeter Observatory. The coverage is 170 deg2 along the Galactic plane, with an effective angular resolution of 33 arcseconds at 1.1 mm. The HEALPix maps have been generated for versions 2.0 and 2.1 fo the BGPS data. Units of the data are text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=c2d&rev=1773763151&do=diff C2D: From Molecular Cores to Planet-Froming Disks PI: N. Evans Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=cgps&rev=1773763151&do=diff Canadian Galactic Plane Survey (CGPS) Observations of the 21cm spectral line from atomic hydrogen (HI) and radio continuum emission at 1420 MHz were obtained using the Dominion Radio Astrophysical Observatory (DRAO) as part of the Canadian Galactic Plane Survey (CGPS). The surveys cover Galactic longitudes text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=chimps&rev=1773763151&do=diff CHIMPS The CO Heterodyne Inner Milky Way Plane Survey (CHIMPS) mapped the 13CO(3-2) and C18O(3-2) emission in the inner Galactic plane with the James Clerk Maxwell Telescope (JCMT). CHIMPS mapped the longitude range l = (28°,46°) and latitude range |b| ≤ 0.5°, across the radial velocity range VLSR = (-75, +150) km/s. The 12CO(3-2) emission across the same region was mapped by the text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=chipass&rev=1773763151&do=diff CHIPASS 1.4 GHz radio continuum This new 1.4 GHz radio continuum map corresponds to a reprocessing of archival data from the HI Parkes All-Sky Survey (HIPASS) and the HI Zone of Avoidance (HIZOA) survey of the sky south of declination +25°. The resolution is text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=clash&rev=1773763151&do=diff CLASH: Cluster Lensing and Supernova survey with Hubble PI : M. Postman Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 4 arcmin 3.6 microns 4.5 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=cobe&rev=1773763151&do=diff See DIRBE. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=cohrs&rev=1773763151&do=diff 12CO(3-2) High-resolution Survey of the Galactic Plane (COHRS) The CO(3-2) High-resolution Survey of the Galactic Plane mapped the 12CO(3-2) emission in the inner Galactic plane using the HARPS instrument on the James Clerk Maxwell Telescope (JCMT). text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=community&rev=1773763151&do=diff CADE FAQ & Community CADE Users' Survey (closed) Your opinion helps us to improve CADE! Please take our short (10-minute) CADE Users' Survey. CADE Mailing List If you use CADE data, please join our mailing list. The purpose of the list is to regularly update users with CADE news, and to receive user feedback and suggestions. Your input helps us to extend and improve the CADE database of maps and tools. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=comptel&rev=1773763151&do=diff MeV Compton gamma-ray telescope (COMPTEL) COMPTEL was the MeV Compton gamma-ray telescope on board of the NASA Compton Gamma-Ray observatory (CGRO). This was the second of NASA's Great Observatories, with 17 tons the heaviest scientific payload ever flown at the time of its launch on April 5, 1991 aboard the space shuttle Atlantis. Compton was re-entered into the Earth's atmosphere on June 4, 2000. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=credits&rev=1773763151&do=diff Credits If your research uses CADE data or analysis software, please include one of the following acknowledgements in your publications: We acknowledge the use of data provided by the Centre d'Analyse de Données Etendues (CADE), a service of IRAP-UPS/CNRS ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=cygnus-x&rev=1773763151&do=diff Cygnus-X: A Spitzer Legacy Survey of the Cygnus-X Complex PI: J. Hora Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=dirbe&rev=1773763151&do=diff Diffuse Infrared Background Experiment (DIRBE) It is an all-sky survey performed at the ~1° resolution in 10 bands: 1.25 microns (Band 1), 2.2 microns (Band 2), 3.5 microns (Band 3), 4.9 microns (Band 4), 12 microns (Band 5), 25 microns (Band 6), 60 microns (Band 7), 100 microns (Band 8), 140 microns (Band 9) and 240 microns (Band 10). text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=drao&rev=1773763151&do=diff DRAO 22 MHz radio continuum/ 1.4 GHz polarization This 22 MHz radio continuum survey covers ~73% of the sky between declination -28° and +80°, derived from observations with the radiotelescope at the Dominion Radio Astrophyical Observatory (DRAO), at a resolution of 1.1°x1.7°secant(zenith angle). Units of the map are text/html 2026-03-19T08:40:54+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=drizzlib&rev=1773909654&do=diff Drizzlib From this page you can download the drizzling software library, drizzlib, which reprojects data from HEALPix to local WCS FITS format. The current library is available in Python3. Older versions in Python2 are available, but no longer actively maintained. text/html 2026-03-19T08:40:54+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=drizzweb&rev=1773909654&do=diff DrizzWeb Drizzweb is a web interface to reproject data from HEALPix to local WCS FITS format. If you use drizzweb for your research, please include the following acknowledgement in your publications: “We acknowledge the use of the drizzweb interface provided by the Centre d'Analyse de Données Etendues (CADE), a service of IRAP-UPS/CNRS ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=drps1_ebv&rev=1773763151&do=diff Dust Reddening from Pan-STARRS1 Under construction. This dataset describes the dust reddening at 4.5 kpc derived from Pan-STARRS1 stellar photometry by Schlafly et al (2014). The map is based on the estimated distances and reddenings to more than 500 million stars. The map covers almost the entire sky north of declination -30 degrees at a resolution of 7 to 14 arcminutes. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=dustings&rev=1773763151&do=diff DUSTiNGS: Dust in Nearby Galaxies with Spitzer PI : M. Boyer Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin (“Files” then text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=dwingeloo&rev=1773763151&do=diff Dwingeloo 820 MHz This survey of continuum radiation at 820 MHz was made with the Dwingeloo telescope, with an effective resolution of 1.2°, and covers declinations in the range -7° < δ < 85°. The map is in Kelvins (brightness temperature units). text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=ebhis&rev=1773763151&do=diff The Effelsberg-Bonn HI Survey (EBHIS) This 21 cm survey has been performed with the 100-m telescope at Effelsberg. The surveys covers the northern sky (Dec >-5°) of the Milky-Way and the local volume out to a redshift of ~0.07. The angular resolution is 10.8'. Units of the Healpix map are text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=effelsberg&rev=1773763151&do=diff EFFELSBERG 1408/2695 MHz Radio continuum and Polarization Radio continuum These surveys of continuum radiation at 1408 MHz (21cm) and 2695 MHz (11cm) were made with the Effelsberg 100-m telescope, with an angular resolution of 9.4' (21cm) and 4.3' (11cm). Units of the Healpix maps are text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=elflock&rev=1773763151&do=diff ELFLock: The Eureka Lawrence Berkeley National Laboratory (LBNL) Far-infrared Lockman Hole Map PI : B. Grossan Map 40arcsec: 160 microns: 1arcmin: 160 microns: 4arcmin: 160 microns: HiPS Enter the following URLs in Aladin (“Files” then text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=extinction&rev=1773763151&do=diff PLEASE WAIT A BIT ... STILL SOME WORK TO DO ... Extinction Tokyo Gagukei University provide color excess and dust extinction maps based on the Digitized Sky Survey I (DSS-1, since December 2005), and on the 2MASS Point Source Catalog (2MASS PSC, since April 2010). text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=fermi&rev=1773763151&do=diff Fermi Gamma-ray Space Telescope The Fermi Gamma-ray Space Telescope was launched on 11 June 2008, becoming the most sensitive gamma-ray telescope on orbit, succeeding INTEGRAL. Fermi includes two scientific instruments, the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM): text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=fidel&rev=1773763151&do=diff FIDEL: Far-Infrared Deep Extragalactic Legacy Survey PI : M. Dickinson Maps 40 arcsec 24 microns 70 microns 160 microns 1 arcmin 24 microns 70 microns 160 microns 4 arcmin 24 microns 70 microns 160 microns HiPS Enter the following URLs in Aladin ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=fls&rev=1773763151&do=diff FLS: First Look Survey PI: T. Soifer Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=fqs&rev=1773763151&do=diff Forgotten Quadrant Survey The Forgotten Quadrant Survey (FQS) was an ESO large project that used the 12 m antenna of the Arizona Radio Observatory to map 12CO(1-0) and 13CO(1-0) emission in the Galactic plane. The 12CO(1-0) observations by the FQS cover a region within the longitude range l = (+220°,+240°) and latitude range b = (-2.°5,0°) where the visual extinction (Av) exceeds 3 mag. The coverage of the 13CO(1-0) observations is restricted to regions with Av > 4mag. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=fugin&rev=1773763151&do=diff FUGIN The FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) project was one of the legacy projects utilizing the new multi-beam receiver FOREST (FOur-beam REceiver System on the 45 m Telescope). FUGIN observed the the 12CO(1-0), 13CO(1-0) and C18O(1-0) molecular line transitions across the longitude ranges l = (+10°,+50°) and l = (+198°,+236°), within a latitude range of |b| < 1°. The total survey area is 80 square degrees for 12CO, and 76 square degre… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=galactic_reddening&rev=1773763151&do=diff Galactic Dust Reddening Schlegel, Finkbeiner & Davis (SFD98) derived an all-sky map of Galactic reddening, E(B-V), from a composite 100 micron emission map constructed from the IRAS/ISSA observations, and calibrated using DIRBE. The resulting E(B-V) map is in units of magnitudes and is frequently used to estimate Galactic foreground extinction. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=gass&rev=1773763151&do=diff Parkes Galactic All Sky Survey (GASS) This map corresponds to the 21-cm emission from Galactic neutral Hydrogen for the entire sky south of δ = +1° using the thirteen beam 20 cm multibeam receiver on the Parkes Radio Telescope. GASS covers all Milky Way velocities between LSR text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=gauribidanur&rev=1773763151&do=diff Gauribidanur 34.5 MHz radio continuum This 34.5 MHz radio continuum survey has been done using GEETEE, the low-frequency telescope at Guribidanur and covers the declination range of -50° to +70° and the complete 24 hours of ascension. The synthesized beam has a resolution of 26'x42'sec(delta-14.1°). Units of the map are text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=gbt&rev=1773763151&do=diff Green Bank Telescope (8.35 GHz and 14.35 GHz) These surveys correspond to the first images of the Galactic Plane (|b|<5°, -15°<l<255°) at 8.35 and 14.35 GHz, obtained with the National Radio Astronomy Observatory/NASA - Green Bank Earth Station. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=gleam&rev=1773763151&do=diff GaLactic and Extragalactic All-sky MWA survey The GLEAM survey, conducted with the Murchison Widefield Array (MWA), covers the entire radio sky south of declination +25° at frequencies between 72 and 231 MHz. All the data have not been released yet, notably along the Galactic Plane. The maps distributed by CADE are generated from the stacked WCS cut-outs. The position-dependent angular resolution of the maps is approximately 2'. The units are Jy/beam. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=glimpse&rev=1773763151&do=diff GLIMPSE (I/II/3D/360/Deep/Proper/APO) & Cygnus-X & Vela-Carina & SMOG: Galactic Legacy infrared Midplane Survey Extraordinaire (PI : E. Churchwell/ R. Benjamin) PIs: E. Churchwell/ R. Benjamin Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=goals&rev=1773763151&do=diff GOALS: Great Observatories All-sky LIRG Survey PI : L. Armus Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=grs&rev=1773763151&do=diff The BU-FCRAO Galactic Ring Survey (GRS) The Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey (GRS) was a survey of 13CO(1-0) emission in the Milky Way covering a longitude range of l = (+18°,+55.7°) and a latitude range of |b| < 1°. The total survey area is 75.4 square degrees. The angular resolution was 46 arcseconds and a velocity resolution of 0.21 km/s. The survey's velocity coverage was -5 to 135 km/s for Galactic longitudes l ≤ 40° and -5 to 85 km s-1 for G… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel&rev=1773763151&do=diff Herschel The European Space Agency's Herschel Space Observatory flew the largest single mirror (3.5-m in diameter) ever built for a space telescope. Herschel covered the spectral range from the far-infrared to submillimeter. This Space Observatory comprised three instruments : text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_debris&rev=1773763151&do=diff Disc Emission via a Bias-free Reconnaissance in the Infrared/Sub-millimetre (DEBRIS) PI : B. Matthews PACS Maps 70 microns 100 microns 160 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_dunes&rev=1773763151&do=diff Cold Disks around Nearby Stars. A Search for Edgeworth-Kuiper Belt analogues (DUNES: DUst disks around NEarby Stars) PI: C. Eiroa PACS Maps 70 microns 100 microns 160 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_epos&rev=1773763151&do=diff The earliest phases of star formation: From low- to high-mass objects PI: O. Krause PACS Maps 70 microns 100 microns 160 microns 37 arcsec 1 arcmin text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_galactic_cold_cores&rev=1773763151&do=diff Herschel Galactic Cold Cores PI: M. Juvela & I. Ristorcelli PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_goods&rev=1773763151&do=diff The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel PI: D. Elbaz PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_gould_belt&rev=1773763151&do=diff Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming clouds complexes PI: P. André PACS Maps 70 microns 160 microns 37 arcsec text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_h-atlas&rev=1773763151&do=diff The Herschel Thousand Degree Survey (aka H-ATLAS) PI: S. Eales PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_helga&rev=1773763151&do=diff HELGA: The Herschel Exploitation of the Local Galaxy Andromeda PI: J. Fritz PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_heritage&rev=1773763151&do=diff HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the Magellanic Clouds PI: M. Meixner PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_herm33es&rev=1773763151&do=diff Herschel M33 extended survey (HerM33es): star-formation interplay with the ISM PI: C. Kramer PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_hermes&rev=1773763151&do=diff The Herschel Multi-tiered Extragalactic Survey (HerMES): Measuring the Infrared Galaxy Formation History of the Universe PI: S Oliver PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_hevics&rev=1773763151&do=diff Herschel Virgo Cluster Survey (HeViCS) PI: J. Davies PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns 350 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_hi-gal&rev=1773763151&do=diff Hi-GAL: the Herschel infrared Galactic Plane Survey PI: S. Molinari PACS Maps 70 microns 160 microns 37 arcsec 1arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_hobys&rev=1773763151&do=diff HOBYS: the Herschel imaging survey of OB Young Stellar objects PI: F. Motte PACS Maps 70 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_hrs&rev=1773763151&do=diff The Herschel Reference Survey PI: S. Eales Maps 250 microns 350 microns 500 microns 37 arcsec 1 arcmin 4 arcmin Uncertainty Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_kingfish&rev=1773763151&do=diff Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) PI: R. Kennicutt PACS Maps 70 microns 100 microns 160 microns 37 arcsec text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_lensing_survey&rev=1773763151&do=diff Herschel Lensing Survey PI: E. Egami PACS Maps 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns 350 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_madden&rev=1773763151&do=diff The ISM in Low Metallicity Environments: Bridging the Gap Between Local Universe and Primordial Galaxies PI: S. Madden PACS Maps 70 microns 100 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_meisenheimer&rev=1773763151&do=diff The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>2 PI: K. Meisenheimer PACS Maps 70 microns 100 microns 160 microns 37 arcsec text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_sag-4&rev=1773763151&do=diff Evolution of interstellar dust PI: A. Abergel PACS Maps 70 microns 100 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=herschel_vngs&rev=1773763151&do=diff Physical Processes in the Interstellar Medium of Very Nearby Galaxies PI: C. Wilson PACS Maps 70 microns 160 microns 37 arcsec 1 arcmin 4 arcmin SPIRE Maps 250 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=hess-hgps&rev=1773763151&do=diff High Energy Spectroscopic System (H.E.S.S.) Galactic Plane Survey (HGPS) The HGPS survey was a decade-long observation program carried out by the H.E.S.S. I array of Cherenkov telescopes in Namibia from 2004 to 2013. The survey covers the Galactic plane at longitudes from text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=hi4pi&rev=1773763151&do=diff HI4PI The HI4PI survey is an all-sky HI survey, based on data from the and from the third revision of the . The procedure used to merge the EBHIS and GASS datasets is described in the HI4PI survey paper (HI4PI collaboration 2016, see below). The resulting composite HI4PI dataset has an angular resolution of 16.2', spectral resolution 1.49 km/s and RMS sensitivity of 43mK per channel. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=hipass-rrl&rev=1773763151&do=diff Radio Recombination Line (RRL) survey from the HI Parkes All-sky Survey (HIPASS) This 1.4 GHz Radio Recombination Line survey (H168α, H167α and H166α) of the Galactic Plane covering the region l=196°-0°-52° and |b|<5° has been obtained with the HI-Parkes All-sky survey (HIPASS) and associated Zone of Avoidance survey. This free-free emission map has been derived from the line-integrated RRL emission, assuming an electron temperature gradient with Galactocentric radius of 496 K/kpc. The angular… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=hops&rev=1773763151&do=diff The H2O southern Galactic Plane Survey (HOPS) The HOPS survey was a survey of selected molecular line transitions in the 12mm window with the Mopra radio-telescope. The HOPS survey covers a longitude range l = (-70°,+30°) and a latitude range of |b| < 0.5°. The total survey area is 100 square degrees. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=integral&rev=1773763151&do=diff INTEGRAL/IBIS The INTEGRAL observatory operating in a hard X-ray/gamma domain has gathered a large observational data since 2003. Most of the observing time was dedicated to the Galactic source population study, making possible the deepest Galactic survey in hard X-rays ever compiled. Sky images of the Galactic Plane (|b|<17.5 deg) obtained with the IBIS telescope have been produced in three energy bands : 17−60, 17−35, and 35−80 keV. All the surveys are based on the nine-year sky maps, and th… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=iris&rev=1773763151&do=diff Improved Reprocessing of the IRAS Survey (IRIS) The goal of the new reprocessing was to solve calibration, zero level and striping problems in the IRAS data. The almost all-sky survey has been performed in 4 bands : 12 microns (at 3.8'), 25 microns (at 3.8'), 60 microns (at 4.0') and 100 microns (at 4.3'). Observations were made in three different epochs (HCON1, HCON2 and HCON3). The IRIS NOHOLES files correspond to the original unobserved regions filled with DIRBE. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=irts&rev=1773763151&do=diff The Infrared Telescope in Space (IRTS) The IRTS is the first Japanese orbiting mission for infrared astronomy. The IRTS was equipped with a 15-cm cooled telescope and four scientific instruments : * the Near-InfraRed Spectrometer (NIRS; 1.4-4.0 µm text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=lab&rev=1773763151&do=diff Leiden/Argentine/Bonn (LAB) Galactic HI survey This survey correspond to 21-cm emission from Galactic neutral hydrogen over the entire sky. The following map is the result of observations made using the Dwingeloo 25m telescope (δ > -27°) and the Villa Elisa 30m telescope text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=lmc_polarization&rev=1773763151&do=diff LMC Polarization Large Magellanic Cloud’s maps of intensity and linear polarization parameters as derived in Alina et al. 2022. The maps were derived using Planck* PR3 release, at 353 GHz, nside = 1024, at the resolution of 16’ from which the foreground contribution has been subtracted using the method proposed in Alina et al. 2022. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=lvl&rev=1773763151&do=diff LVL: Spitzer Local Volume Legacy Survey PI: J. C. Lee Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=m31irac&rev=1773763151&do=diff M31IRAC: IRAC Observations of the Extended Disk and Halo of M31 PI : P. Barmby Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=maipu-mu&rev=1773763151&do=diff Maipu and MU 45 MHz continuum This 45 MHz continuum map is the result of the combination of data obtained with the 45-MHz array of the University of Chile at the Maipu Radio Astronomy Observatory and the circular filled array of the Japanese Middle and Upper (MU) atmosphere Radar. The Maipu data cover the southern hemisphere (declination below +19.1°), with a beam of 4.6°( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=mipsgal&rev=1773763151&do=diff MIPSGAL: A 24 and 70 Micron Survey of the inner Galactic Disk with MIPS PI : S. Carey Map 40 arcsec: 24 microns: 1 arcmin: 24 microns: 4 arcmin: 24 microns: HiPS Enter the following URL in Aladin (“Files” then “Use directly a URL text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=mips_local_galaxies&rev=1773763151&do=diff MIPS Local Galaxies PI : J. Bendo Maps 40 arcsec 24 microns 70 microns 160 microns 1 arcmin 24 microns 70 microns 160 microns 4 arcmin 24 microns 70 microns 160 microns HiPS Enter the following URLs in Aladin (“Files text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=miteor&rev=1773763151&do=diff MIT Epoch of Reionization (MITEoR) experiment This northern sky survey centred around 150 MHz has been made using the MITEoR data set collected in 2013 July, with an angular resolution of about 2°. The intensity and uncertainty maps are in units of text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=mopraco&rev=1773763151&do=diff The Mopra Southern Galactic Plane CO Survey The Mopra Southern Galactic Plane CO Survey was a survey of 12CO(1-0), 13CO(1-0), C18O(1-0) and C17O(1-0) emission in southern Galactic plane with the Mopra telescope in Australia. The survey covered a longitude range of l = (+300°,+350°) and a latitude range of |b| < 0.5°. The total survey area is 50 square degrees. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=msx&rev=1773763151&do=diff 18'' SOON Band A Band C Band D Band E text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=mwisp&rev=1773763151&do=diff MWISP The Milky Way Imaging Scroll Painting (MWISP) project is an ongoing unbiased Galactic plane survey of 12CO(1-0), 13CO(1-0) and C18O(1-0) emission using the Superconducting SpectroScopic Array Receiver system on the Purple Mountain Observatory 13.7m telescope. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=news&rev=1773763151&do=diff Latest CADE News April 2025 Please find here a short Jupyter notebook (Python) showing how to fetch and display some of our products. September 2024 First prediction maps of the dust emission (using Neural Networks) at 850 microns (353 GHz) and 1.38 mm (217 GHz) at the Herschel resolution (37 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=nnpredictions&rev=1773763151&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/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=nrao&rev=1773763151&do=diff Nobeyama text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=nro&rev=1773763151&do=diff 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 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=nro_continuum&rev=1773763151&do=diff Nobeyama 10GHz radio continuum The 10GHz radio continuum survey of the Galactic plane (355°<l<56°, -1.5°<b<+1.5°) was made at the Nobeyama Radio Observatory using the 45-m telescope, with an angular resolution of 3'. Units of the map are mJy/Beam text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=parkes&rev=1773763151&do=diff Parkes 85 MHz/150 MHz/5 GHz radio continuum The 5GHz radio continuum survey of the Galactic plane (0°<l<+40° and 190°<l<360°, -2°<b<+2°) was made with the Parkes 64-m radio telescope, with an angular resolution of 4.1'. Units of the map are text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=pilot&rev=1773763151&do=diff PILOT PILOT (Polarized Instrument for Long Wavelength Observation of the Tenuous ISM) is balloon-borne experiment to obtain wide-field maps of the polarised thermal dust emission at 240 microns in the Milky Way and Local Group galaxies. There have been two scientific PILOT flights, from Timmins, Canada in 2015 and from Alice Springs, Australia in 2017. A third scientific PILOT flight from Timmins is scheduled for September 2019. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=planck&rev=1773763151&do=diff Planck Planck was an ESA space telescope (2009 -- 2013) that observed the cosmic microwave background (CMB) radiation. The main goal of the Planck mission was to measure small deviations from isotropy with an unprecedented accuracy and level of detail in order to distinguish between competing cosmological models. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=planck_lmc_polarization&rev=1773763151&do=diff LMC Polarization Large Magellanic Cloud’s maps of intensity and linear polarization parameters as derived in Alina et al. 2022. The maps were derived using Planck* PR3 release, at 353 GHz, nside = 1024, at the resolution of 16’ from which the foreground contribution has been subtracted using the method proposed in Alina et al. 2022. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=publications&rev=1773763151&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 Galaxy text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=ramps&rev=1773763151&do=diff Radio Ammonia Mid-Plane Survey (RAMPS) The Radio Ammonia Mid-Plane Survey (RAMPS) has surveyed 24 square degrees of the Galactic plane using the Green Bank Telescope (GBT). RAMPS covers the longitude range l = (10º,40º) and latitude range |b| < 0.4º. The key spectral targets of RAMPS were the ammonia transitions NH3(1,1) to NH3(5,5). Other emission lines in the RAMPS band include transitions of HC5N, HC7N, CH3OH, HNCO, H2O and CCS. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=rass&rev=1773763151&do=diff ROSAT All Sky Survey (RASS) The ROSAT telescope performed an all-sky survey in the X-ray band. The angular resolution of the ROSAT telescope in combination with the PSPC camera is approximately 1.8'. Healpix maps made by D. Paradis. Maps in counts/sec or counts should be multiplied by text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=s-candels&rev=1773763151&do=diff S-CANDELS: Spitzer-Cosmic Assembly Deep Near-infrared Extragalactic Legacy Survey PIs: G. Fazio Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=s-cosmos&rev=1773763151&do=diff S-COSMOS: Spitzer Coverage of the Cosmic Evolution Survey field PI: D. Sanders Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=s4g&rev=1773763151&do=diff S4G: The Spitzer Survey of Stellar Structure in Galaxies PI : K. Sheth Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin (“ text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sage&rev=1773763151&do=diff SAGE (LMC and SMC): Surveying the Agents of a Galaxy's Evolution PI: M. Meixner/K. Gordon Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sdwfs&rev=1773763151&do=diff SDWFS: Spitzer Deep, Wide-Field Survey PI : D. Stern Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 4 arcmin 3.6 microns 4.5 microns 5.8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sedigism&rev=1773763151&do=diff SEDIGISM Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium (SEDIGISM) was a survey of molecular lines in the 217–221 GHz range with the SHeFI receiver on the APEX telescope. The key spectral targets were 13CO(2-1) and C18O(2-1). Other transitions include H2CO, CH3OH, SO, SO2, HNCO, HC3N, SiO, but their detection is typically restricted to the densest regions. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sed_extractor&rev=1773763151&do=diff 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 ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sep&rev=1773763151&do=diff SEP: Spitzer MIPS 24 and 70 micron Imaging of the South Ecliptic Pole PI : K. Scott Maps 40 arcsec 24 microns 70 microns 1 arcmin 24 microns 70 microns 4 arcmin 24 microns 70 microns Uncertainty maps 24 microns 70 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=servs&rev=1773763151&do=diff SERVS: Spitzer Extragalactic Representative Volume Survey PI : M. Lacy Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns Uncertainty maps 3.6 microns 4.5 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sgps&rev=1773763151&do=diff Southern Galactic Plane Survey (SGPS) The Southern Galactic Plane Survey (SGPS) provides 21-cm line emission from neutral atomic hydrogen and continuum data of the Southern Milky Way obtained with the Australia Telescope Compact Array and Parkes Radiotelescope text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=shassa&rev=1773763151&do=diff Southern H-Alpha Sky Survey Atlas (SHASSA) The Southern H-Alpha Sky Survey Atlas is the product of a wide-angle digital imaging survey of the H-alpha emission from the warm ionized interstellar gas of our Galaxy. The survey covers the southern hemisphere (declinations less than +15 degrees). The observations were taken with a robotic camera operating at Cerro Tololo Inter-American Observatory (CTIO) in Chile. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sidebar&rev=1773763151&do=diff * Welcome * CADE News * CADE FAQ & Community * Acknowledging CADE * Team * Publications * Software * Drizzlib * DrizzWeb * SED Extractor * Neural Network Predictions * Missions/Surveys * AKARI * AMIGPS * BLAST * Bolocam * CGPS * CHIMPS * CHIPASS * COHRS * COMPTEL * DIRBE * DHT-Nanten * DRAO * Dwingeloo * Effelsberg * EBHIS * EBV_SFD98 * Fermi * FUGIN * GASS * Gauribidanur * GLEAM * GRS * Herschel … text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sings&rev=1773763151&do=diff SINGS: The Spitzer infrared Nearby Galaxies Survey PI: R. Kennicutt Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=smog&rev=1773763151&do=diff SMOG: Spitzer Mapping of the Outer Galaxy PIs: S. Carey Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 4 arcmin 3.6 microns 4.5 microns 5.8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=smuvs&rev=1773763151&do=diff SMUVS: Spitzer Matching Survey of the Ultra-VISTA Deep Stripes PIs: K. Caputi Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=software&rev=1773763151&do=diff Software * Python package Drizzlib * Web application DrizzWeb * Web application SED Extractor text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=spies&rev=1773763151&do=diff SpIES: Spitzer IRAC Equatorial Survey PIs: G. Richards Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns Uncertainty maps 3.6 microns 4.5 microns HiPS Enter the following URLs in Aladin ( text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=spitzer&rev=1773763151&do=diff Spitzer NASA's Spitzer Space Telescope was launched on August 25, 2003 from Florida's Cape Canaveral Air Force Base. Spitzer incorporated an 85 cm diameter telescope primary mirror, cooled to as low as 5.5 K,and three scientific instruments providing imaging and spectroscopy at wavelengths from 3.6 to 160 microns. This Space Observatory comprised three instruments : text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=spuds&rev=1773763151&do=diff SpUDS: Spitzer Public Legacy Survey of the UKIDSS Ultra Deep Survey PI : J. Dunlop Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=srelics&rev=1773763151&do=diff SRELICS: Spitzer Reionization Lensing Cluster Survey PI : M. Bradac Maps 40 arcsec 3.6 microns 4.5 microns 1 arcmin 3.6 microns 4.5 microns 4 arcmin 3.6 microns 4.5 microns Uncertainty maps 3.6 microns 4.5 microns text/html 2026-03-19T08:40:54+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=start&rev=1773909654&do=diff 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 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=stockert&rev=1773763151&do=diff Stockert 1420/2720 MHz radio continuum The radio continuum survey of the northern Galactic plane was performed using the Stockert 25-m telescope at 2720 MHz (11 cm) between 1979 and 1985. This survey covers 80°<l<0° and -16°<b<+30°, with a resolution of 21'. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=sumss&rev=1773763151&do=diff The Survey University Molonglo Sky Survey (SUMSS) The survey of the radio sky at 843 MHz covers the whole sky south of declination -30 degrees with |b|>10 degrees. The Galactic Plane region |b|<10 degrees is covered by the second epoch Molonglo Galactic Plane Survey. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=swift&rev=1773763151&do=diff Swift-BAT The Swift gamma-ray burst (GRB) observatory was launched in 2004 November, and has been continually observing the hard X-ray (14–195 keV) sky ever since with the Burst Alert Telescope (BAT). The 70 month Swift-BAT survey is the most sensitive and uniform hard X-ray all-sky survey and reaches a flux level of 1.03×10−11 erg s−1cm−2 over 50% of the sky and 1.34×10−11 erg s−1cm−2 over 90% of the sky. Swift has three co-aligned instruments for studying gamma-ray … text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=swire&rev=1773763151&do=diff SWIRE: Spitzer Wide-area infraRed Extragalactic Survey PI: C. Lonsdale Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=taurus_2&rev=1773763151&do=diff Taurus 2: Finishing the Spitzer Map of the Taurus Molecular clouds PI : D. Padgett Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 24 microns 70 microns 160 microns 1 arcmin 3.6 microns 4.5 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=team&rev=1773763151&do=diff 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) * text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=thor&rev=1773763151&do=diff The HI/OH/Recombination line survey of the inner Milky Way (THOR) The THOR project mapped observations of the HI 21 cm line, four OH lines, nineteen Hnα radio recombination lines as well as the continuum emission from 1 to 2 GHz in full polarization over a large part of the first Galactic quadrant, using the Karl G. Jansky Very Large Array (VLA) in the C-array configuration. The first release of the THOR data covered observations for l = 14.0 - 37.9, and l = 47.1 - 51.2, |b| < 1.25. The second … text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=thrumms&rev=1773763151&do=diff Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) mapped the 12CO(1-0), 13CO(1-0), C18O(1-0), and CN(1-0) emission within the fourth Galactic quadrant using the Mopra Telescope. ThrUMMS covers a longitude range l = (-60°,0°) and a latitude range of |b| < 1°. The angular resolution of ThrUMMS is 1 arcminute and the velocity resolution is 0.3 km/s. The typical rms sensitivity per channel of the ThrUMMS data cubes is σ(T) ~ 2K for 12CO, an… text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=unwise&rev=1773763151&do=diff unWISE WISE is a 40 cm telescope aboard a satellite launched in 2009, surveying the entire sky in all four of its channels (W1–W4) during the first half of 2010. In the latter half of 2010, the reddest two channels (W3 and W4) became unusable due to cryogen depletion. Nevertheless, the WISE satellite continued surveying in W1 and W2 until early 2011 as part of the NEOWISE mission (Mainzer et al. 2011). In 2011 February, WISE was placed into hibernation for approximately 33 months, during which … text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=urumqi&rev=1773763151&do=diff Urumqi 6 cm Radio continuum and Polarization The Sino-German 6 cm surveys of the Galactic Plane (10°<l<230° and |b|<5°) were made using the Urumqi 25-m telescope, at an angular resolution of 9.5'. Units of the Healpix maps are micro KTB. Healpix maps made by D. Paradis. text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=vela-carina&rev=1773763151&do=diff Vela-Carina: Galactic Structure and Star Formation in Vela-Carina PI : S. Majewski Maps 40 arcsec 3.6 microns 4.5 microns 5.8 microns 8 microns 1 arcmin 3.6 microns 4.5 microns 5.8 microns 8 microns 4 arcmin 3.6 microns text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=vgps&rev=1773763151&do=diff VLA Galactic Plane Survey (VGPS) This survey of 21-cm line emission from neutral atomic hydrogen has been mapped at the 1' angular resolution, using the VLA telescope. These observations cover the following longitude and latitude ranges: 18° < l < 67° and -1° < b < 1° text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=vlssr&rev=1773763151&do=diff VLA Low-Frequency Sky Survey Redux (VLSSr) The VLSS data, at a frequency of 74 MHz cover 95% of the 3π sr of sky area above -30° declination. The original data have been reprocessed to create a revised version of the survey, called the VLSS redux (VLSSr). This reprocessing lead to substantial improvements allowing to release images of six unpublished fields and reducing the clean bias by 50%. The angular resolution is approximately 80 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=vtss&rev=1773763151&do=diff The Virginia Tech Spectral-Line Survey (VTSS) The VTSS is a wide-field image survey of the Galaxy's warm ionized interstellar medium (a 10,000 K plasma). The survey is carried out using the Virginia Tech Spectral Line Imaging Camera (SLIC), specially designed for obtaining sensitive, arcminute-resolution, 10-degree wide images of the text/html 2026-03-19T08:40:54+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=welcome&rev=1773909654&do=diff 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 text/html 2026-03-17T15:59:11+00:00 Anonymous (anonymous@undisclosed.example.com) http://cade.ovgso.fr/doku.php?id=wham&rev=1773763151&do=diff 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).