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

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://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/DR4CONE
Title:: Sloan Digitized Sky Survey(DR4)
Short Name:: SDSS-DR4
Date:: 05 Dec 2018 20:08:39
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://archive.stsci.edu/hst/stis
Title:: Space Telescope Imaging Spectrograph
Short Name:: HST.STIS
Date:: 23 Jul 2020 19:50:49
Publisher:: Space Telescope Science Institute Archive
Description:: The Space Telescope Imaging Spectrograph (STIS) was installed in HST on Feb. 14, 1997, replacing the GHRS spectrograph. STIS provides spectra and images at ultraviolet and visible wavelengths, probing the Universe from our solar system out to cosmological distances.

ID:: ivo://org.gavo.dc/supercosmos/q/s
Title:: SuperCOSMOS Sources
Short Name:: supercosmos scs
Date:: 27 Dec 2024 08:31:02
Publisher:: The GAVO DC team
Description:: The SuperCOSMOS data primarily originate from scans of the UK Schmidt and Palomar POSS II blue, red and near-IR sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide an early (1st) epoch red measurement. Mirrored here is the source table containing four-plate multi-colour, multi-epoch data which are merged into a single source catalogue for general science exploitation. Within the GAVO DC, some column names have been adapted to local customs (primarily positions, proper motions).

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