Subject: galaxies / Resource Type: Archive / Capability Type: Simple Cone Search

ID:: ivo://archive.stsci.edu/hst/acs
Title:: Advanced Camera for Surveys
Short Name:: HST.ACS
Date:: 23 Jul 2020 19:47:47
Publisher:: Space Telescope Science Institute Archive
Description:: HST Advanced Camera for Surveys (ACS) - Images: CCD images between 3,700 - 11

ID:: ivo://archive.stsci.edu/befs
Title:: Berkeley Extreme and Far-UV Spectrometer
Short Name:: BEFS
Date:: 22 Jul 2020 21:27:59
Publisher:: Space Telescope Science Institute Archive
Description:: The Berkeley Extreme and Far-UV Spectrometer (BEFS), flew on the Orbiting and Retrievable Far and Extreme Ultraviolet Spectrograph (ORFEUS)-SPAS I and II space shuttle missions in 1993 and 1996, returning high-resolution (/3000) FUV spectra (900-1200 Å) of 75 astrophysical objects from the first flight and more than 100 from the second. EUV spectra (400-900 Å) were obtained for a subset of these targets.

ID:: ivo://cxc.harvard.edu/cda
Title:: Chandra X-ray Observatory Data Archive
Short Name:: CDA
Date:: 18 Jul 2019
Publisher:: Chandra X-ray Observatory
Description:: The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range.

ID:: ivo://archive.stsci.edu/euve
Title:: Extreme Ultraviolet Explorer
Short Name:: EUVE
Date:: 22 Jul 2020 21:28:51
Publisher:: Space Telescope Science Institute Archive
Description:: Launched in June, 1992, The Extreme Ultraviolet Explorer (EUVE) conducted the first extreme ultraviolet (70-760 Angstroms) survey of the sky and subsequently began a Guest Observer Program of pointed

ID:: ivo://archive.stsci.edu/hst/foc
Title:: Faint Object Camera
Short Name:: HST.FOC
Date:: 23 Jul 2020 19:48:27
Publisher:: Space Telescope Science Institute Archive
Description:: The Faint Object Camera (FOC) was one of the 4 original axial instruments on the Hubble Space Telescope (HST). FOC is used to make high-resolution observations of faint sources at UV and visible wavel

ID:: ivo://archive.stsci.edu/hst/fos
Title:: Faint Object Spectrograph
Short Name:: HST.FOS
Date:: 23 Jul 2020 19:48:53
Publisher:: Space Telescope Science Institute Archive
Description:: The Faint Object Spectrograph (FOS) was one of the 4 original axial instruments aboard the Hubble Space Telescope (HST). The FOS was designed to make spectroscopic observations of astrophysical sources from the near ultraviolet to the near infrared (1150 - 8000 Angstroms). The instrument was removed from HST during the Second Servicing Mission in February 1997.

ID:: ivo://archive.stsci.edu/fuse
Title:: Far Ultraviolet Spectroscopic Explorer
Short Name:: FUSE
Date:: 22 Jul 2020 21:29:31
Publisher:: Space Telescope Science Institute Archive
Description:: The Far Ultraviolet Spectroscopic Explorer (FUSE), launched on June 24, 1999, covers the 905-1187 Å spectral region and will obtain high resolution spectra of hot and cool stars, AGNs, supernova remnants, planetary nebulae, solar system objects as well as perform detailed studies of the interstellar medium. FUSE will be able to observe sources 10 000 times fainter than Copernicus, an early FUV mission, and has superior resolving power than the Hopkins Ultraviolet Telescope (HUT) and the Berkeley Spectrograph (BEFS) and the Tübingen Echelle Spectrograph (TUES) of the Orbiting Retrievable Far and Extreme Ultraviolet Spectrometers (ORFEUS). FUSE was planned for a 3 year lifetime with funding for an additional 2 years expected.

ID:: ivo://vopdc.iap/fss
Title:: Five Supernova Survey Galaxies
Short Name:: FSS
Date:: 10 Jan 2017
Publisher:: Institut d'Astrophysique de Paris
Description:: VO-compliant publication of the properties of the 3838 galaxies that were monitored for SNe events, including newly determined morphologies and their DENIS and POSS-II/UKST I, 2MASS and DENIS J and Ks and 2MASS H magnitudes.

ID:: ivo://archive.stsci.edu/hst/ghrs
Title:: Goddard High Resolution Spectrograph
Short Name:: HST.GHRS
Date:: 23 Jul 2020 19:49:16
Publisher:: Space Telescope Science Institute Archive
Description:: GHRS was used to make finely detailed spectroscopic observations of ultraviolet sources, but was removed from HST in February 1997.

ID:: ivo://archive.stsci.edu/hut
Title:: Hopkins Ultraviolet Telescope
Short Name:: HUT
Date:: 22 Jul 2020 21:30:05
Publisher:: Space Telescope Science Institute Archive
Description:: The Hopkins Ultraviolet Telescope (HUT) was a shuttle-borne instrument used to obtain ultraviolet spectra in the far ultraviolet region of the spectrum. It was part of the ASTRO payload complement of three co-mounted instruments that flew in December 1990 and March 1995 as Space Shuttle missions. More than 650 spectra were obtained of 340 targets. In April, 2013, the HUT data was reprocessed to improve calibration, expand metadata, add new data products, and update file formats. The current cone service uses the metadata from these reprocessed files.

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