Subject: galactic and extragalactic astronomy / Resource Type: Archive

ID:: ivo://mast.stsci/siap/coma
Title:: HST ACS Coma cluster (Abell 1656) Treasury Survey (COMA)
Short Name:: HST.COMA
Date:: 23 Jul 2020 19:33:05
Publisher:: Space Telescope Science Institute Archive
Description:: The HST ACS Coma cluster Treasury survey is a deep two-passband imaging survey of one of the nearest rich clusters of galaxies, the Coma cluster (Abell 1656).

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://mast.stsci/siap/merggal
Title:: Hubble Space Telescope gallery of Interacting and Merging Galaxies
Short Name:: HST.merggal
Date:: 22 Jul 2020 22:00:54
Publisher:: Space Telescope Science Institute Archive
Description:: A gallery of images of interacting and merging galaxies from Hubble Space Telescope press releases. These data were originally acquired under HST programs 6276, 10592, 11091, 11092, and 11095, and include WFPC2 images of Arp 87, NGC 6050, and Arp 148 (and two ACS images of Arp 148).

ID:: ivo://mast.stsci/hudf09
Title:: Hubble Ultra Deep Field 2009 (HUDF09)
Short Name:: HUDF09
Date:: 22 Jul 2020 22:33:31
Publisher:: Space Telescope Science Institute Archive
Description:: The Hubble Ultra Deep Field 2009 (HUDF09) program observations were obtained as HST program 11563 (PI: Garth Illingworth) from August 2009 to February 2011 (Cycle 17). The program uses WFC3/IR as the prime instrument for 192 orbits to image the deep ACS fields that were obtained in the original HUDF (PI: Steven Beckwith) program and in the HUDF05 (PI: Massimo Stiavelli) program. The data are organized into sets of images by HUDF09 pointing and by passband (WFC3/IR F105W, F125W & F160W). Each image is approximately 3k x 3k pixels in size and a scale of 0.06 arcsec/pixel. All three pointings reside in the GOODS/Chandra South field and each pointing includes a drizzled science image and a weight image.

ID:: ivo://archive.stsci.edu/kic10
Title:: Kepler Input Catalog
Short Name:: KIC
Date:: 12 Feb 2020 19:43:29
Publisher:: Space Telescope Science Institute Archive
Description:: The KIC, or Kepler Input Catalog, is the primary source of information about objects observed as part of the ground-based Kepler Spectral Classification Program (SCP) in preparation for the selection of Kepler PI and GO targets. The KIC lists objects down to 21st magnitude, but it is not complete to this limit. Light from only about 1/3 of these 14 million objects falls on the Kepler CCD detector. A small number of the KIC objects are calibration objects distributed across the sky.

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.

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