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- ID:
- ivo://anusf.anu.au/wigglez/image/DownLoad
- Title:
- WiggleZ Image Download Service
- Short Name:
- WiggleZ getImage
- Date:
- 18 Jun 2019 20:18:26
- Publisher:
- ivo://anusf.anu.au
- Description:
- The WiggleZ Project Image Download Service
- ID:
- ivo://mast.stsci/ssap/hpol
- Title:
- Wisconsin Halfwave Spectropolarimeter
- Short Name:
- HPOL
- Date:
- 22 Jul 2020 21:56:07
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the Univsity of Wisconsin Pine Bluff Observatory in the 3,200 - 7,750 Å range, resolution ~ 80, V_max ~ 15, ~ 2800 observations of ~ 400 targets, 1989-1998. Note spectropolarimetry data is also included. Observations complement those obtained from the ASTRO WUPPE project.
- ID:
- ivo://mast.stsci/ssap/wuppe
- Title:
- Wisconsin Ultraviolet Photo-Polarimeter Experiment
- Short Name:
- WUPPE
- Date:
- 22 Jul 2020 21:57:38
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- UV spectra in the 1,400 - 3,200 Å range, resolution ~ 140, V_max ~ 14, ~ 400 observations of ~ 200 targets, 2 NASA-funded shuttle missions (12/90 & 3/95). Note spectropolarimetry data is also available.
- ID:
- ivo://archive.stsci.edu/wuppe
- Title:
- Wisconsin Ultraviolet Photo-Polarimeter Experiment
- Short Name:
- WUPPE
- Date:
- 22 Jul 2020 21:33:04
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE) was the spectropolarimetry component of the three ASTRO instruments that flew on Space Shuttle missions in December 1990 and March 1995. A halfwave spectropolarimeter provided medium resolution spectropolarimetry for research into the interstellar medium, hot stars, stars with circumstellar material, interacting binary stars, novae, solar system objects, and active galaxies. A Lyot analyzer obtained low resolution observations of faint targets, but due to calibration problems did not produce scientifically useful data. The WUPPE instrument provides a unique data set, one of the few providing polarimetric data in the ultraviolet portion of the spectrum.
- ID:
- ivo://nasa.heasarc/skyview/wise
- Title:
- WISE 3\.4 Micron All-Sky Survey>: All-WISE data release
- Short Name:
- WISE
- Date:
- 07 Mar 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- From the <a href="https://wise2.ipac.caltech.edu/docs/release/allsky">WISE mission site:</a>. <hr> NASA's Wide-field Infrared Survey Explorer (WISE) mapped the sky at 3.4, 4.6, 12 and 22 micrometers in 2010 with an angular resolution of 6.1", 6.4", 6.5" and 12.0" in the four bands. WISE achieved a 5 sigma point source sensitivities better and 0.08, 0.11 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodaical background. <p> The WISE All-WISE includes all data taking during the WISE full cryogenic phase, from January 7, 2010 to August 6, 2010, that were processed with improved calibrations and reduction algorithms and combines this with the NEOWISE postcryogenic survey to form the most comprehensive view of the full mid-infrared sky. bibcode=1995ApJ...451..564V,2010ApJ...713..912W <hr> <p> SkyView includes the four WISE bands as separate surveys. Many non-image data products are available at the WISE site. Note that WISE data is distributed in relatively large (>50 MB) image files. When SkyView generates an image for a part of the sky where it has not yet cached the data from the IPAC server there may be a delay as full tiles are downloaded even when only a small fraction of a tile is needed. Images in cached regions, are generated much faster. Access to the WISE data uses the VO SIA interface maintained at IPAC. Even when data is cached, the SIA service must still be available for successful queries. Provenance: WISE Archive (IRSA/IPAC). This is a service of NASA HEASARC.
- ID:
- ivo://nasa.heasarc/skyview/wmap
- Title:
- WMAP Nine Year Galaxy Removed
- Short Name:
- WMAP
- Date:
- 07 Mar 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- These survey represents a combination of the 9-year data combined in a way that is intended to minimize the contribution from the galaxy. The data measure the temperature deviation from a uniform black body. <p> The original data are available at the <https://lambda.gsfc.nasa.gov>LAMBDA archive</a>. <p> The original data are stored in HEALPix pixels. SkyView treats HEALPix as a standard projection but assumes that the HEALPix data is in a projection plane with a rotation of -45 degrees. The rotation transforms the HEALPix pixels from diamonds to squares so that the boundaries of the pixels are treated properly. The special HealPixImage class is used so that SkyView can use the HEALPix FITS files directly. The HealPixImage simulates a rectangular image but translates the pixels from that image to the nested HEALPix structure that is used by the WMAP data. </p> Provenance: WMAP Mission/LAMBDA archive. This is a service of NASA HEASARC.
- ID:
- ivo://msc.koa/hires
- Title:
- W. M. Keck Observatory Archive
- Short Name:
- KOA
- Date:
- 11 Jul 2006 18:51:46
- Publisher:
- Michelson Science Center
- Description:
- The W. M. Keck Observatory Archive (KOA) serves level 0 (uncalibrated) observations made with the CCD mosaic upgrade to the High Resolution Echelle Spectrograph (HIRES), commissioned on the Keck Telescope in August 2004. The data are subject to the proprietary policy agreed upon by NASA and the California Association for Research in Astronomy (CARA).
- ID:
- ivo://badc.naoc.cn/WDC-Astro
- Title:
- World Data Center for Astronomy
- Short Name:
- WDC-Astronomy
- Date:
- 04 Apr 2008 16:54:29
- Publisher:
- National Astronomical Observatory of China
- Description:
- World Data Center for Astronomy, hosted at National Astronomical Observatory of China, Beijing, China
- ID:
- ivo://arches/3xmme/cs
- Title:
- 3XMM Enhanced Catalogue
- Short Name:
- 3XMMe-CONESEARCH
- Date:
- 03 Feb 2025 08:21:34
- Publisher:
- ARCHES - Astronomical Resource Cross-matching for High Energy Studies
- Description:
- The enhanced 3XMM catalogue (designated 3XMMe) is one of the core elements of the Arches project, representing the X-ray source basis for the cross-correlations with other multi-wavelength catalogues. The 3XMMe catalogue is a derivative of the latest increment of the 3XMM catalogue, i.e. 3XMM-DR5, that was publicly released in April 2015 (Rosen et al., 2015 (submitted to A&A)), tailored for the purposes of the Arches project. The 3XMM-DR5 catalogue, available from the XMM-Newton Science Archive, the XMM-Newton Survey Science Centre (SSC) and other sites listed on the SSC site, contains 565962 detections arising from 396910 unique sources drawn from 7781 XMM observations. These numbers include detections from 356 sub-pointings made in mosaic
![the Fornax VST Survey is licensed under the `Creative Commons Attribution 4.0 License <http://creativecommons.org/licenses/by/4.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY]](/registry-search/?f%5BcontentLevel_facet%5D%5B%5D=Research&f%5Brights_facet%5D%5B%5D=the+Fornax+VST+Survey+is+licensed+under+the+%60Creative+Commons+Attribution+4.0+License+%3Chttp%3A%2F%2Fcreativecommons.org%2Flicenses%2Fby%2F4.0%2F%3E%60_%0A%0A..+image%3A%3A+%2Fstatic%2Fimg%2Fccby.png%0A+++%3Aalt%3A+%5BCC-BY%5D%0A%0A&f%5Btype_facet%5D%5B%5D=Archive){kind=link}