- ID:
- ivo://archive.stsci.edu/catalogs/ultravista
- Title:
- UltraVISTA ConeSearch
- Short Name:
- UltraVISTA CS
- Date:
- 23 Jul 2020 20:36:35
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the UltraVISTA survey: This is the deepest and narrowest VISTA survey. It is imaging one patch of sky over and over again to unprecedented depths. The science goals of UltraVISTA include studying the first galaxies, understanding the stellar mass build-up during the peak epoch of star formation activity and dust-obscured star formation. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
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- ID:
- ivo://archive.stsci.edu/catalogs/USNOB
- Title:
- USNO-B Catalog ConeSearch
- Short Name:
- USNOB CS
- Date:
- 13 Feb 2020 17:42:39
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- USNO-B is an all-sky catalog that presents positions, proper motions, magnitudes in various optical passbands, and star/galaxy estimators for 1,042,618,261 objects derived from 3,643,201,733 separate observations. The data were obtained from scans of 7435 Schmidt plates taken for the various sky surveys during the last 50 years. USNO-B1.0 is believed to provide all-sky coverage, completeness down to V = 21, 0>2 astrometric accuracy at J2000, 0.3 mag photometric accuracy in up to five colors, and 85% accuracy for distinguishing stars from nonstellar objects. A more detailed description of the construction and contents of the USNO-B1 catalog can be found in Monet et al. (2003, "The USNO-B Catalog", AJ, 125, 984), http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/usno-b1.0/resolveuid/41be0c1a4d1a8372289bad3baf27cde5. A mirror of USNOB exists in the MAST holdings and is thus available as a cone search. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/vistavhs
- Title:
- Vista Hemisphere Survey ConeSearch
- Short Name:
- VISTA VHS CS
- Date:
- 13 Feb 2020 17:43:47
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the VISTA Hemisphere Survey All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/FIRST
- Title:
- VLA FIRST ConeSearch
- Short Name:
- VLAFIRST CS
- Date:
- 23 Jul 2020 20:20:25
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. The Very Large Array (VLA) FIRST -- Faint Images of the Radio Sky at Twenty-cm -- is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North and South Galactic Caps. Using the NRAO Very Large Array (VLA) and an automated mapping pipeline, we produce images with 1.8" pixels, a typical rms of 0.15 mJy, and a resolution of 5". At the 1 mJy source detection threshold, there are ~90 sources per square degree, ~35% of which have resolved structure on scales from 2-30". 30% of the sources have counterparts in the Sloan Digital Sky Survey. The VLA FIRST catalog at MAST was published December 17, 2014. More information is available at http://sundog.stsci.edu All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/vstatlas
- Title:
- VST Atlas ConeSearch
- Short Name:
- VSTAtlas CS
- Date:
- 23 Jul 2020 20:37:54
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the VST Atlas: This survey is targeting 4500 square degrees of the Southern sky in five filters (U, V, R, I and Z) to depths comparable to those of the SDSS. This survey is also complemented by near-infrared data from the VISTA Hemisphere Survey. The primary aim is to examine ‘baryon wiggles’ (small-amplitude oscillations observed in the power spectrum of galaxies) by looking at luminous red galaxies in order to determine the dark energy equation of state. Along with this, the VST ATLAS will provide an imaging base for spectroscopic surveys by the VLT. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/viking
- Title:
- VST Kilo-Degree Infrared Galaxy (VIKING) Survey ConeSearch
- Short Name:
- VIKING CS
- Date:
- 23 Jul 2020 20:37:13
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the VST Kilo-degree Infrared Galaxy (VIKING) Survey All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/kids
- Title:
- VST Kilo-Degree Survey ConeSearch
- Short Name:
- KIDS CS
- Date:
- 23 Jul 2020 20:33:38
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the VST Kilo-degree survey All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/hst/wfpc2
- Title:
- Wide Field Planetary Camera 2
- Short Name:
- HST.WFPC2
- Date:
- 23 Jul 2020 19:52:01
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The WFPC2 is used to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Å).
- ID:
- ivo://archive.stsci.edu/hst/wfpc1
- Title:
- Wide Field Planetary Camera 1
- Short Name:
- HST.WFPC1
- Date:
- 23 Jul 2020 19:51:30
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The WF/PC-1 was used from April 1990 to November 1993, to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Angstroms).
- ID:
- ivo://CDS.VizieR/VI/90
- Title:
- Wide-Field Plate Database
- Short Name:
- VI/90
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The Wide-Field Plate Database (WFPDB) contains the descriptive information for the astronomical wide-field (~>1deg.) photographic observations stored in numerous archives all over the world. When finished it will provide an on-line access to the information for about 2 million observations from nearly 300 archives, obtained since the end of last century. Presently the WFPDB includes data for about 330 000 observations from 57 plate catalogues. About 120 000 observations more from 32 plate catalogs are in preparation to be included in the database. The WFPDB provides for each observation information for the corresponding archive, the parameters of the observational instrument, the observation parameters (position on sky, observation time, object name, method, exposure time, emulsion type, filter type, spectral band, plate size), as well as data on the plate quality, comments, and observers. Data on the plate availability and digitization will be supplemented in the WFPDB in the future.