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61. Sloan Digital Sky Survey (DR8)
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
62. Sloan Digital Sky Survey (DR7)
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
63. Sloan Digital Sky Survey (DR3)
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
64. Sloan Digitized Sky Survey(DR4)
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
65. Sloan Digitized Sky Survey(DR1)
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
66. Sloan Digitized Sky Survey(DR2)
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
67. Space Telescope Imaging Spectrograph
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.
68. Stars with Debris Disks and Planets
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.
69. STELIB library
ID:
ivo://svo.cab/cat/stelib
Title:
STELIB library
Short Name:
STELIB library
Date:
03 Jun 2020 15:30:50
Publisher:
SVO/CAB
Description:
STELIB stellar library
70. Subaru Suprime-Cam data service
ID:
ivo://jvo/subaru/spcam
Title:
Subaru Suprime-Cam data service
Short Name:
SUBARU_SUP
Date:
04 Nov 2020 06:00:31
Publisher:
JVO
Description:
The Subaru Prime Focus Camera (Suprime-Cam) is a mosaic of ten 2048 x 4096 CCDs, located at the prime focus of Subaru Telescope, which covers a 34' x 27' field of view with a pixel scale of 0.20''. This service provides access to the JVO Subaru Suprime-Cam mosaic image archive. The purpose of this archive is to provide quick look images taken by Subaru/Suprime-Cam. Those images were processed by a pipeline developed by JVO.

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