Subject: cosmology / Publisher: Space Telescope Science Institute Archive / Facility: HST / Validation Level: 2

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/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/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/hst
Title:: Hubble Space Telescope
Short Name:: HST
Date:: 23 Jul 2020 19:47:19
Publisher:: Space Telescope Science Institute Archive
Description:: Hubble Space Telescope (HST) is an orbiting astronomical observatory operating from the near-infrared into the ultraviolet. Launched in 1990 and scheduled to operate through 2010, HST carries and has carried a wide variety of instruments producing imaging, spectrographic, astrometric, and photometric data through both pointed and parallel observing programs. MAST is the primary archive and distribution center for HST data, distributing science, calibration, and engineering data to HST users and the astronomical community at large. Over 100 000 observations of more than 20 000 targets are available for retrieval from the Archive.

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://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://archive.stsci.edu/hst/wfpc2
Title:: Wide Field Planetary Camera 2
Short Name:: HST.WFPC2
Date:: 23 Jul 2020 19:52:01
Publisher:: Space Telescope Science Institute Archive
Description:: The WFPC2 is used to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Å).

ID:: ivo://archive.stsci.edu/hst/wfpc1
Title:: Wide Field Planetary Camera 1
Short Name:: HST.WFPC1
Date:: 23 Jul 2020 19:51:30
Publisher:: Space Telescope Science Institute Archive
Description:: The WF/PC-1 was used from April 1990 to November 1993, to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Angstroms).

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