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

ID:: ivo://sdss.jhu/services/DR3CONE
Title:: Sloan Digital Sky Survey (DR3)
Short Name:: SDSS-DR3
Date:: 14 Sep 2011 18:12:21
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://sdss.jhu/services/DR1CONE
Title:: Sloan Digitized Sky Survey(DR1)
Short Name:: SDSS-DR1
Date:: 14 Sep 2011 18:11:54
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/DR2CONE
Title:: Sloan Digitized Sky Survey(DR2)
Short Name:: SDSS-DR2
Date:: 14 Sep 2011 17:51:43
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://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://svo.cab/debris
Title:: Stars with Debris Disks and Planets
Date:: 23 Jan 2017 10:09:28
Publisher:: SVO CAB
Description:: Planetary systems are built by planets and planetesimals formed in circumstellar disks surrounding young pre-main sequence stars. Once in the main-sequence collisions of planetesimals produce small dust particles giving rise to the so-called debris disks. The mutual interaction among planets, planetesimals and debris disks, and with their host stars determines the fate of planetary systems. Currently thousands of main-sequence stars are known to host planets and debris disks. The Solar System with its peculiarities is just one of such planetary systems. However, only few tens of stars are known to host simultaneously both planets and debris disks. Therefore, the study of those systems is particularly valuable to widen our knowledge of planetary systems and their evolution. This page just collects some of the properties of the known, to our knowledge, solar-type stars hosting both planets and debris disk.

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).

Search