Subject: stars / Capability Type: Simple Cone Search - STScI NAVO Directory Search Results

ID:: ivo://archive.stsci.edu/hst/nicmos
Title:: Near Infrared Camera and Multi Object Spectrograph
Short Name:: HST.NICMOS
Date:: 23 Jul 2020 19:50:23
Publisher:: Space Telescope Science Institute Archive
Description:: The HST Near Infrared Camera and Multi-Object Spectrometer (NICMOS) provides imaging capabilities in broad, medium, and narrow band filters, broad-band imaging polarimetry, coronographic imaging, and slitless grism spectroscopy, in the wavelength range 0.8-2.5 microns. NICMOS has three adjacent but not contiguous cameras, designed to operate independently, each with a dedicated array at a different magnification scale.

ID:: ivo://org.gavo.dc/ppmx/res/ppmx/scs
Title:: PPMX query
Short Name:: ppmx_scs
Date:: 27 Dec 2024 08:31:00
Publisher:: The GAVO DC team
Description:: PPM-Extended (PPMX) is a catalogue of 18 088 919 stars on the ICRS system containing astrometric and photometric information. Its limiting magnitude is about 15.2 in the GSC photometric system.

ID:: ivo://org.gavo.dc/rave/q/cone
Title:: RAVE DR5 Cone Search
Short Name:: rave_scs
Date:: 27 Dec 2024 08:31:12
Publisher:: The GAVO DC team
Description:: The RAdial Velocity Experiment (RAVE) contains stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, chemical abundances and distances. Observations between 2003 and 2013 were used to build the five RAVE data releases.

ID:: ivo://archive.stsci.edu/skiff_spclass
Title:: Skiff Spectral Catalog
Short Name:: skiff_spclass
Date:: 08 Jun 2017 15:34:41
Publisher:: Space Telescope Science Institute Archive
Description:: This service provides access to a modified version of the Skiff Spectral catalog. The full catalog is available from VizieR. The table includes the standard spectral classifications (with spaces removed) and their encoded values as described in the IVOA note titled "An Encoding system to Represent Stellar Spectral Classes in Archival Databases and Catalogs". The table contains roughly 450,000 targets. Note Skiff does not list novae or supernovae.

ID:: ivo://sdss.jhu/services/CONE
Title:: Sloan Digital Sky Survey Cone Search (Latest Release)
Short Name:: SDSS-CONE
Date:: 05 Feb 2015 21:18:36
Publisher:: The Johns Hopkins University
Description:: The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey

ID:: ivo://sdss.jhu/services/DR5CONE
Title:: Sloan Digital Sky Survey (DR5)
Short Name:: SDSS-DR5
Date:: 05 Dec 2018 20:08:59
Publisher:: The Johns Hopkins Univer
Description:: The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey

ID:: ivo://sdss.jhu/services/DR9CONE
Title:: Sloan Digital Sky Survey (DR9)
Short Name:: SDSS-DR9
Date:: 05 Feb 2015 20:33:12
Publisher:: The Johns Hopkins University
Description:: The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey

ID:: ivo://sdss.jhu/services/DR8CONE
Title:: Sloan Digital Sky Survey (DR8)
Short Name:: SDSS-DR8
Date:: 05 Feb 2015 20:32:31
Publisher:: The Johns Hopkins University
Description:: The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey

ID:: ivo://sdss.jhu/services/DR7CONE
Title:: Sloan Digital Sky Survey (DR7)
Short Name:: SDSS-DR7
Date:: 05 Feb 2015 20:31:02
Publisher:: The Johns Hopkins University
Description:: The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey

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