Subject: observational astronomy / Content Level: Research

ID:: ivo://archive.stsci.edu/catalogs/HLSP_30DOR
Title:: 30 Doradus Catalog ConeSearch
Short Name:: 30 DOR CS
Date:: 23 Jul 2020 20:40:48
Publisher:: Space Telescope Science Institute Archive
Description:: 30 Doradus (a.k.a. the Tarantula Nebula), with its ionizing cluster R136, is one of the few known starbursts in the Local Group. For size (~200 pc in diameter) and density of OB stars, 30 Doradus parallels the regions of intense star formation observed in the starburst knots found in the interacting galaxies in the Local Universe and the young galaxies at high redshift (z>5). HTTP is a panchromatic imaging survey of stellar populations in the Tarantula Nebula in the Large Magellanic Cloud that reaches into the sub-solar mass regime. HTTP utilizes the capability of the Hubble Space Telescope to operate the Advanced Camera for Surveys and the Wide Field Camera 3 in parallel to study this remarkable region in the near-ultraviolet, optical, and near-infrared spectral regions, including narrow-band Hα images. The high sensitivity, spatial resolution and broadband coverage of HTTP allow us to dissect the stellar populations and infer an accurate description of the anatomy of the Tarantula Nebula, and therefore to reconstruct for the first time the temporal and spatial evolution of a prototypical starburst on a sub-parsec scale. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.

ID:: ivo://CDS.VizieR/B/eso
Title:: ESO Science Archive Catalog
Short Name:: B/eso
Date:: 07 Mar 2022 06:43:11
Publisher:: CDS
Description:: The ESO Science Archive Catalog contains a log of observations performed with the ESO telescopes. Currently available in the observation log are the data from the VLT, NTT, MPG/ESO 2.2m, and the ESO 3.6m telescopes. The observations themselves are stored in an off-line archive and have a proprietary period of one year. After this period the archival data sets are available to the general astronomical community of the ESO member states and Chile.

ID:: ivo://CDS.VizieR/VI/43
Title:: EXOSAT Observation Log
Short Name:: VI/43
Date:: 21 Oct 2021
Publisher:: CDS
Description:: The EXOSAT Observation Log lists archival information on 2108 pointed observations made with the EXOSAT between May 1983 and April 1986. Data listed include start and stop times, instrumental pointings, object names, proposal identifications, principal investigator codes, and observing instruments and modes of observation. The log is intended as a reference to the data collected during the EXOSAT mission and provides the summary information necessary to determine what observations, if any, may be of interest in an investigation.

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://mast.stsci/ssap/euve
Title:: Extreme Ultraviolet Explorer Merged Spectra
Short Name:: EUVE
Date:: 22 Jul 2020 21:49:27
Publisher:: Space Telescope Science Institute Archive
Description:: The Extreme Ultraviolet Explorer (EUVE) was a NASA-funded satellite launched in June 1992 which obtained extreme ultraviolet spectra (70 - 760 Angstroms) of over 350 unique astronomical targets. The science payload, was designed and built at the Space Sciences Laboratory at the University of California, Berkeley, under the direction of Dr. Roger F. Malina. The program ended in January, 2001. These particular spectra were extracted by Damian Christian, formerly of the EUVE project, and reformatted by MAST staff.

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://mast.stsci/ssap/fuse
Title:: Far Ultraviolet Spectroscopic Explorer
Short Name:: FUSE
Date:: 22 Jul 2020 21:53:56
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 obtains 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. This service provides access to the FUSE spectra reprocessed using CalFUSE 3.2 and reformatted to be VO-compatible.

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.

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