Subject: stars / 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/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/hsc
Title:: Hubble Source Catalog Detailed Search
Short Name:: HSC
Date:: 30 Oct 2024 18:53:53
Publisher:: Space Telescope Science Institute Archive
Description:: The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive (HLA) into a single master catalog. The Hubble Source Catalog (HSC) detailed search displays an entry for each separate detection (or nondetection if nothing is found at that position) using all the relevant Hubble observations for a given object (i.e., different filters, detectors, separate visits). The catalog currently contains over 100 million entries.

ID:: ivo://archive.stsci.edu/hst/hsc_sum
Title:: Hubble Source Catalog Summary Search
Short Name:: HSC_SUM
Date:: 30 Oct 2024 18:54:13
Publisher:: Space Telescope Science Institute Archive
Description:: The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands visit-based source lists in the Hubble Legacy Archive (HLA) into a single master catalog. The HSC Summary search displays a single row entry for each object, as defined by a set of detections that have been cross-matched and hence are believed to be a single object. Averaged values for magnitudes and other relevant parameters are provided. The catalog currently contains over 16 million entries.

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/iue
Title:: International Ultraviolet Explorer
Short Name:: IUE
Date:: 22 Jul 2020 21:30:36
Publisher:: Space Telescope Science Institute Archive
Description:: The International Ultraviolet Explorer (IUE) performed spectrophotometry at high (0.1-0.3 Å) and low (6-7 Å) resolution between 1150 Å and 3200 Å. The data cover a dynamic range of approximately 17 astronomical magnitudes: -2 to 10 for high dispersion; -2 and 14.9 for low dispersion. Over 104,000 ultraviolet spectra were obtained with IUE between January 26, 1978, and September 30, 1996.

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