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- ID:
- ivo://mast.stsci/acsggct
- Title:
- ACS Galactic Globular Cluster Survey (ACSGGCT)
- Short Name:
- HST.ACSGGCT
- Date:
- 22 Jul 2020 22:26:50
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The ACSGGCT program used the HST ACS/WFC instrument to obtain uniform imaging of 65 of the nearest globular clusters to provide an extensive homogeneous dataset for a broad range of scientific investigations. An overview of the project was published by Sarajedini, A. et al. 2007, "The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters Without Previous Hubble Space Telescope Photometry" AJ, 133, 1658.
- 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://mast.stsci/angrrr
- Title:
- Archive of Nearby Galaxies: Reduce, Reuse, Recycle (ANGRRR)
- Short Name:
- HST.ANGRRR
- Date:
- 22 Jul 2020 22:28:43
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- An archive of stellar photometry for galaxies within 3.5 Mpc, excluding Local Group galaxies, based on primary and parallel wide-filter UV and optical observations taken with HST ACS/WFC or WFPC2.The sample includes all observations taken through Dec. 2008, as well as observations taken as part of Cycle 16 Supplemental GO programs 11986 and 11987. This release includes the ANGST targets within 3.5 Mpc; these observations have been rereduced using updated CTE corrections and zeropoints. Galaxies with 3.5 < D <= 5 Mpc will be included in a later release.
- 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://mast.stsci/ssap/befs
- Title:
- Berkeley Extreme and Far-UV Spectrometer
- Short Name:
- BEFS
- Date:
- 03 Feb 2021 15:45:57
- 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://archive.stsci.edu/borg
- Title:
- Brightest of Reionizing Galaxies (BoRG)
- Short Name:
- BoRG
- Date:
- 22 Jul 2020 22:24:07
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Brightest of Reionizing Galaxies (BoRG) observations were first obtained in HST Cycle 17 in program GO 11700 (PI: Michele Trenti). BoRG is an ongoing pure-parallel program that obtains WFC3 imaging in four filters (F606W, F098M, F125W, F160W) on random sightlines at high Galactic latitudes (|b| > 30 degrees). BoRG also assimilates data from the similar Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) pure-parallel program (GO 11702; PI: Yan). Data from the HIPPIES program uses the F600LP filter instead of F606W.
- ID:
- ivo://mast.stsci/clash
- Title:
- Cluster Lensing And Supernova survey with Hubble (CLASH)
- Short Name:
- HST.CLASH
- Date:
- 22 Jul 2020 22:29:29
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- By observing 25 massive galaxy clusters with HST's new panchromatic imaging capabilities (Wide-field Camera 3, WFC3, and the Advanced Camera for Surveys, ACS), CLASH will accomplish its four primary science goals: - Map, with unprecedented accuracy, the distribution of dark matter in galaxy clusters using strong and weak gravitational lensing; - Detect Type Ia supernovae out to redshift z ~ 2, allowing us to test the constancy of dark energy's repulsive force over time and look for any evolutionary effects in the supernovae themselves; - Detect and characterize some of the most distant galaxies yet discovered at z > 7 (when the Universe was younger than 800 million years old - or less than 6% of its current age); - Study the internal structure and evolution of the galaxies in and behind these clusters.
- ID:
- ivo://mast.stsci/candels
- Title:
- Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS)
- Short Name:
- CANDELS
- Date:
- 12 Feb 2020 21:03:03
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- CANDELS is designed to document the first third of galactic evolution from z = 8 to 1.5 via deep imaging of more than 250,000 galaxies with WFC3/IR and ACS. It will also find the first Type Ia SNe beyond z greater than 1.5 and establish their accuracy as standard candles for cosmology. Five premier multi-wavelength sky regions are selected; each has multi-wavelength data from Spitzer and other facilities, and has extensive spectroscopy of the brighter galaxies. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to 109 solar masses out to z ~ 8.
- ID:
- ivo://archive.stsci.edu/catalogs/HLSP_47TUC
- Title:
- Deep Imaging of 47 Tuc Catalog ConeSearch
- Short Name:
- 47 TUC CS
- Date:
- 23 Jul 2020 20:41:29
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Kalirai et al. have observed the globular cluster 47 Tucanae for 121 orbits using the Advanced Camera for Surveys. These extremely deep images were taken in two filters: F606W (broad V-band) and F814W (I-band). Using these observations, Kalirai et al. were able to construct one of the deepest and most complete color-magnitude diagrams of a stellar population, probing down to 30th magnitude and extending from the faintest end of the main sequence to the coolest white dwarf members. As an added bonus, members of the Small Magellanic Cloud represent background sources, and these observations are able to resolve SMC targets down to 0.2 solar masses. The team have released their stacked ACS mosaics (FITS files), source catalog (ASCII text table), and artificial source lists (ASCII text table) used for testing photometry, astrometry, and completeness, as High Level Science Products. We summarize the creation of the stacked images and generation of the catalogs below, but refer you to the original publication for complete details. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://mast.stsci/andromeda
- Title:
- Deep Optical Photometry of Six Fields in the Andromeda Galaxy
- Short Name:
- HST.Andromeda
- Date:
- 22 Jul 2020 22:25:44
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Using the Advanced Camera for Surveys on the Hubble Space Telescope, Thomas Brown (STScI) et al. obtained deep optical images reaching well below the oldest main sequence turnoff in six fields of the Andromeda Galaxy. The fields fall at four positions on the southeast minor axis, one position in the giant stellar stream, and one position on the northeast major axis. These data were obtained as part of three large observing programs (9453, 10265, 10816) designed to probe the star formation history of the stellar population in various structures of the galaxy.
- 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://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.
- ID:
- ivo://archive.stsci.edu/catalogs/UCAC5
- Title:
- Fifth U.S. Naval Observatory CCD Astrograph Catalog (UCAC5) ConeSearch
- Short Name:
- UCAC5 CS
- Date:
- 13 Feb 2020 17:41:52
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- New astrometric reductions of the US Naval Observatory CCD Astrograph Catalog (UCAC) all-sky observations were performed from first principles using the TGAS stars in the 8 to 11 magnitude range as reference star catalog. Significant improvements in the astrometric solutions were obtained and the UCAC5 catalog of mean positions at a mean epoch near 2001 was generated. By combining UCAC5 with Gaia DR1 data new proper motions on the Gaia coordinate system for over 107 million stars were obtained with typical accuracies of 1 to 2 mas/yr (R = 11 to 15 mag), and about 5 mas/yr at 16th mag. Proper motions of most TGAS stars are improved over their Gaia data and the precision level of TGAS proper motions is extended to many millions more, fainter stars. External comparisons were made using stellar cluster fields and extragalactic sources. The TGAS data allow us to derive the limiting precision of the UCAC x,y data, which is significantly better than 1/100 pixel. A mirror of UCAC5 exists in the MAST holdings and is thus available as a cone search. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/GAIADR2
- Title:
- GAIA DR2 ConeSearch
- Short Name:
- GAIADR2 CS
- Date:
- 23 Jul 2020 20:18:57
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST mirror of the GAIA catalog data release 2. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/GAIADR1
- Title:
- GAIA DR1 ConeSearch
- Short Name:
- GAIADR1 CS
- Date:
- 23 Jul 2020 20:18:44
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST mirror of the GAIA catalog data release 1. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/ghosts
- Title:
- Galaxy Halos, Outer disks, Substructure, Thick disks and Star clusters (GHOSTS)
- Short Name:
- GHOSTS
- Date:
- 22 Jul 2020 21:59:56
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The GHOSTS survey is the largest study to date of the resolved stellar populations in the outskirts of disk galaxies. The sample consists of 14 disk galaxies within 17 Mpc, whose outer disks and halos are imaged with the Hubble Space Telescope Advanced Camera for Surveys (ACS).
- ID:
- ivo://mast.stsci/siap/galex_atlas
- Title:
- GALEX Atlas of Nearby Galaxies
- Short Name:
- GALEX_Atlas
- Date:
- 25 Jun 2018 19:13:16
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The GALEX Atlas of Nearby Galaxies contains images of 1034 nearby galaxies recently observed by the GALEX satellite in its far-ultraviolet (FUV; 1516A) and near-ultraviolet (NUV; 2267A) bands. The Atlas was prepared by A. Gil de Paz,S. Boissier, B.F. Madore, M. Seibert and associated members of the GALEX Team. The full paper is posted on astroph/0606440 and will be published in ApJS in 2007.
24. GALEX ConeSearch
- ID:
- ivo://archive.stsci.edu/catalogs/GALEX
- Title:
- GALEX ConeSearch
- Short Name:
- GALEX CS
- Date:
- 23 Jul 2020 20:30:39
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. GALEX data are available via the standard MAST CS service,and an auxiliary service for GALEX data only. This catalog includes Galex GR 6/7 data, thus including the closeout release, as described at https://galex.stsci.edu/GR6/. The Galaxy Evolution Explorer (GALEX), a NASA Small Explorer mission, performed the first all-sky, deep imaging and spectroscopic ultraviolet surveys in space. The prime goal of GALEX was to study star formation in galaxies and its evolution with time. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- 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://mast.stsci/siap/goods.hst
- Title:
- Great Observatories Origins Deep Survey (GOODS)
- Short Name:
- HST.GOODS
- Date:
- 23 Jul 2020 19:32:07
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- GOODS aims to unite extremely deep observations from NASA's Great Observatories, the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS will survey a total of roughly 320 square arcminutes in two fields centered on the Hubble Deep Field North and the Chandra Deep Field South.
- ID:
- ivo://mast.stsci/siap-cutout/goods.hst
- Title:
- Great Observatories Origins Deep Survey (GOODS) Cutout Service
- Short Name:
- HST.GOODS.Cutout
- Date:
- 05 Dec 2018 16:38:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- GOODS aims to unite extremely deep observations from NASA's Great Observatories, the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS will survey a total of roughly 320 square arcminutes in two fields centered on the Hubble Deep Field North and the Chandra Deep Field South.
- ID:
- ivo://archive.stsci.edu/gsc/gsc2.3
- Title:
- Guide Star Catalog 2.3 Cone Search
- Short Name:
- GSC23
- Date:
- 13 Feb 2020 17:10:38
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Guide Star Catalog II (GSC-II) is an all-sky optical catalog based on 1" resolution scans of the photographic Sky Survey plates, at two epochs and three bandpasses, from the Palomar and UK Schmidt telescopes. This all-sky catalog will ultimately contains positions, proper motions, classifications, and magnitudes in multiple bandpasses for almost a billion objects down to approximately Jpg=21, Fpg=20. The GSC-II is currently used for HST Bright Object Protection and HST pointing. Looking ahead, the GSC-II will form the basis of the Guide Star Catalog for JWST. This was constructed in collaboration with ground-based observatories for use with the GEMINI, VLT and GALILEO telescopes
- ID:
- ivo://archive.stsci.edu/gsc/gsc1.1
- Title:
- Guide Star Catalog 1.1 Cone Search
- Short Name:
- GSC11
- Date:
- 13 Feb 2020 17:10:22
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The GSC-I catalog is an all-sky catalog of positions and magnitudes for approximately 19 million stars and other objects in the sixth to fifteenth magnitude range. The GSC is primarily based on an all-sky, single-epoch collection of Schmidt plates. For centers at +6 degrees and north, a 1982 epoch "Quick V" survey was obtained from the Palomar Observatory, while for southern fields, materials from the UK SERC J survey (epoch = 1975) and its equatorial extension (epoch = 1982) were used.
- ID:
- ivo://archive.stsci.edu/catalogs/GSPC2
- Title:
- Guide Star Photometric ConeSearch
- Short Name:
- GSP2 CS
- Date:
- 13 Feb 2020 17:37:54
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Guide Star Catalog (GSC) is a star catalog compiled to support the Hubble Space Telescope with targeting off-axis stars. GSC-II contains 945,592,683 stars out to magnitude 21. Photometric calibrations for GSC2 are available through this interface. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/hst/hsp
- Title:
- High Speed Photometer
- Short Name:
- HST.HSP
- Date:
- 23 Jul 2020 19:49:53
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The High Speed Photometer (HSP) was one of the four original axial instruments on the Hubble Space Telescope (HST). The HSP was designed to make very rapid photometric observations of astrophysical sources in a variety of filters and passbands from the near ultraviolet to the visible. The HSP was removed from HST during the First Servicing Mission in December, 1993.
- ID:
- ivo://archive.stsci.edu/catalogs/HLASTARCLUSTERS
- Title:
- HLA Star Clusters ConeSearch
- Short Name:
- STARCLUSTERS CS
- Date:
- 13 Feb 2020 17:47:36
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. A high-level science product was produced cataloging star clusters within the HLA: compact star cluster catalogs are presented for 20 nearby, star-forming galaxies using observations from the Advanced Catalog for Surveys (ACS) and source lists generated by the Hubble Legacy Archive. Results based on these cluster catalogs are published in the paper "The Luminosity Function of Star Clusters in 20 Star-Forming Galaxies Based on Hubble Legacy Archive Photometry" Whitmore, AJ 147:78. A typical cluster luminosity function can be approximated by a power-law, with an average value for the index of -2.37 and rms scatter = 0.18. The uniform database provided by these HLA catalogs results in a small scatter (0.5 magnitude) in the correlation between the magnitude of the brightest cluster (M_brightest) and Log of the number of clusters brighter than M_I = -9 (Log N). More information on the catalog is available at https://archive.stsci.edu/prepds/hlastarclusters/. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://mast.stsci/ssap/hut
- Title:
- Hopkins Ultraviolet Telescope
- Short Name:
- HUT
- Date:
- 22 Jul 2020 21:48:21
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hopkins Ultraviolet Telescope (HUT) was one of three ultraviolet instruments of the ASTRO-1 mission flown on the space shuttle Columbia during 2-10 December 1990. 106 spectrophotometric observations of 77 targets were obtained in the far-UV (i.e., 912-1850 Ã…) at a resolution of ~3 Ã…. A few sources were observed in the 415-912 Ã… region with a 1.5 Ã… resolution. The same three instruments were later flown on the space shuttle Endeavour from 3-17 March 1995 as part of the ASTRO-2 mission. During the longer ASTRO-2 mission, 385 observations of 265 targets were obtained.
- 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.
- 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://mast.stsci/siap/hst.m51
- Title:
- HST ACS mosaic images of M51
- Short Name:
- HST.M51
- Date:
- 23 Jul 2020 14:15:40
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- In January 2005, the Hubble Heritage Team obtained a large 4-color mosaic image of the Whirlpool Galaxy NGC 5194 (M51), and its companion NGC 5195, with the Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope (HST observing program 10452, PI: Steven V. W. Beckwith). A six-pointing ACS WFC mosaic of the galaxy pair M51 was obtained in four filters: B, V, I, and H-alpha.
- ID:
- ivo://mast.stsci/siap/hst.appp
- Title:
- HST Archival Pure Parallels Project
- Short Name:
- HST.APPP
- Date:
- 23 Jul 2020 19:33:56
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Archival Pure Parallel Project processed and combined about 2,000 WFPC2 images, primarily in the wide UBVI filters, obtained in parallel with other HST instruments. Combined, drizzled, cosmic-ray cleaned images were produced for each pointing. These data can be used to address a wide range of science topics: measuring the cosmic shear on scales from 20" to 2'; discovering ~ 50 starforming galaxies at z ~ 4; finding optical counterparts to AGNs in wide-area radio and X-ray catalogs; improving the determination of the scale length of the Galactic disk; and studying stellar populations down to 1 solar mass for about 25 separate lines of sight in the Magellanic Clouds.
- ID:
- ivo://mast.stsci/siap/hst.cosmos
- Title:
- HST Cosmic Evolution Survey
- Short Name:
- HST.COSMOS
- Date:
- 23 Jul 2020 19:35:16
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- COSMOS (P.I. Nicholas Scoville, California Institute of Technology, USA/CA) is an HST Treasury Program to survey a 2 square degree equatorial field, centered on RA=10:00:28.6 and DEC=+02:12:21.0 with the ACS in the I band of the VIMOS equatorial field. Parallel observations with WFPC2 and NICMOS were also obtained.
- ID:
- ivo://mast.stsci/siap/hst.gems
- Title:
- HST Galaxy Evolution from Morphology and SEDs
- Short Name:
- HST.GEMS
- Date:
- 22 Jul 2020 22:30:27
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- GEMs is a large-area (800 arcmin 2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope. Centered on the Chandra Deep Field-South, it covers an area of ~ 28'x28', or about 120 HDF areas, to a depth of MAB(F606W)=28.5(5s) for compact sources. Focusing on the redshift range ~ 0.2<z<1.1, GEMS provides morphologies and structural parameters for nearly 10,000 galaxies where redshift estimates, luminosities, and SEDs exist from COMBO-17.
- ID:
- ivo://mast.stsci/siap/hst.hdf
- Title:
- HST Hubble Deep Field
- Short Name:
- HST.HDF
- Date:
- 23 Jul 2020 19:35:54
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hubble Deep Field (HDF) is a Director's Discretionary program on HST in Cycle 5 to image a typical field at high galactic latitude in four wavelength passbands as deeply as reasonably possible. In order to optimize observing in the time available, a field in the northern continuous viewing zone (CVZ) was selected and images were taken for 10 consecutive days, or approximately 150 orbits. Shorter 1-orbit images were also obtained of the fields immediately adjacent to the primary HDF in order to facilitate spectroscopic follow-up by ground-based telescopes. The observations were carried out from 18-30 December 1995, and the data are available to the community for study.
- ID:
- ivo://mast.stsci/siap/hst.hdf_south
- Title:
- HST Hubble Deep Field South
- Short Name:
- HST.HDF_SOUTH
- Date:
- 23 Jul 2020 19:36:18
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- A second Hubble Deep Field campaign was carried out between late September and October of 1998. The raw, pipeline calibrated and reprocessed data were released to the community on November 23, 1998. The rationale for undertaking a second deep field campaign followed from the wealth of information that has come out of HDF-N, and from the desire to provide a point of focus for similar studies of the distant universe from southern-hemisphere facilities. Simultaneous, parallel observations were made with the three HST instruments STIS, WFPC2 and NICMOS of separate, neighboring fields. As was the case for HDF-N, approximately 150 consecutive orbits were devoted to a single telescope pointing.
- ID:
- ivo://mast.stsci/siap/hst.helix
- Title:
- HST Hubble HELIX Observations
- Short Name:
- HST.HELIX
- Date:
- 22 Jul 2020 22:22:06
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- For the 14 hours of peak Leonid meteoroid flux in November 2002, the Hubble Space Telescope was pointed away from the radiant, and the solar arrays were oriented to minimize their cross-section. By coincidence, one of the nearest and largest planetary nebulae, the Helix Nebula (NGC 7293), was nearly opposite the incoming Leonids and could be observed. A "Hubble Helix Team" (below) of volunteers led by Margaret Meixner (STScI) organized a nine-orbit campaign to observe the Helix with the ACS, WFPC2, NICMOS, and STIS.
- ID:
- ivo://mast.stsci/ssap/hst/stis
- Title:
- HST Space Telescope Imaging Spectrograph
- Short Name:
- HST STIS Spectra
- Date:
- 22 Jul 2020 21:58:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- MAST-produced spectral container files for STIS spectra. STIS spectra range from 1150 to 10,300 at low to medium spectral resolution, high spatial resolution echelle spectroscopy in the ultraviolet. STIS began operation in 1997. (Note the included echelle spectra are technically not yet supported by the SSAP.)
- ID:
- ivo://mast.stsci/siap/hst.tno
- Title:
- HST trans-Neptunian Objects Search field images
- Short Name:
- HST.TNO
- Date:
- 22 Jul 2020 22:31:56
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The "TNO Search Field" images are the sidereally summed images of a search for trans-Neptunian objects (TNOs) using the Wide Field Camera of the HST/ACS instrument. The observations were taken under Cycle 11 program GO-9433, "The Size Distribution of Kuiper Belt Bodies," with G. Bernstein as PI. The TNO search consisted of approximately 96x400 s exposures in the F606W filter for each of six contiguous ACS fields of view. The TNO search field is approximately 6'x10', centered near 14h 07M 53.3s -11d 21' 38" (J2000).
- ID:
- ivo://mast.stsci/siap/hst.udf
- Title:
- HST Ultra Deep Field (UDF) Images
- Short Name:
- HST.UDF
- Date:
- 22 Jul 2020 22:32:35
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The ACS Ultra Deep Field (UDF) is a cycle 12 survey carried out using the Advanced Camera for Surveys (ACS) on HST and taking advantage of the Director's Discretionary time. The UDF consists of a single ultra-deep field (412 orbits in total taken in 4 bands) within the CDF-S GOODS area. It is the deepest image ever obtained with Hubble. This service also includes data from the UDF follow-Up program by PI Massimo Stiavelli and colleagues obtained under HST cycle 14 program 10632 titled Searching for galaxies at z>6.5 in the Hubble Ultra Deep Field (also known as UDF05).
- ID:
- ivo://mast.stsci/siap/hst.maoz_atlas
- Title:
- HST Ultraviolet Atlas of Nearby Galaxies
- Short Name:
- HST.maoz_atlas
- Date:
- 23 Jul 2020 19:27:41
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- A pictorial atlas of UV (2300 Å) images, obtained with the Hubble Space Telescope (HST) Faint Object Camera, of the central 22''× 22'' of 110 galaxies (Maoz, Filippenko, Ho, Macchetto, Rix, & Schneider 1996). The observed galaxies are an unbiased selection constituting about one half of a complete sample of all large (D>6 arcmin) and nearby (V< 2000 km/s ) galaxies. This is the first extensive UV imaging survey of normal galaxies. The data are useful for studying star formation, low-level nuclear activity, and UV emission by evolved stellar populations in galaxies. At the HST resolution (~ 0.05''), the images display an assortment of morphologies and UV brightnesses. These include bright nuclear point sources, compact young star clusters scattered in the field or arranged in circumnuclear rings, centrally-peaked diffuse light distributions, and galaxies with weak or undetected UV emission. We measure the integrated ~2300 Å flux in each image, and classify the UV morphology.
- ID:
- ivo://mast.stsci/siap/hst.sgal
- Title:
- HST WFPC2 Spiral Galaxies
- Short Name:
- HST.SGAL
- Date:
- 23 Jul 2020 19:36:54
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Holwerda et al. examined 32 HST/WFPC2 archival fields of 29 spiral galaxies (Sab and later) for their paper The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks (2005, AJ,129:1396-1411). The majority of the data are from the Cepheid distance scale Key Project. The explicit goal was to provide deep mosaics in both V- and I-band with a better sampling in order to identify background galaxies through the foreground disk.
- ID:
- ivo://mast.stsci/hippies
- Title:
- Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES)
- Short Name:
- HST.HIPPIES
- Date:
- 22 Jul 2020 22:31:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) utilizes long-duration pure parallel visits (~> 3 orbits) of HST at high Galactic latitude (|b|>20o) to take deep, multi-band images in WFC3 (since Cycle 17) and in ACS (starting Cycle 18). It is unique in its large number of descrete fields along random sightlines, and thus is complementary to other surveys over contiguous fields but along limited sightlines.
- ID:
- ivo://archive.stsci.edu/siap/hla
- Title:
- Hubble Legacy Archive
- Short Name:
- HLA
- Date:
- 21 Jul 2020 20:46:18
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hubble Space Telecope Legacy Archive (HLA) was developed at the Space Telescope Science Institute to optimize the science return from HST instruments. This resource is an image service which accesses all HLA observation data. The calibrated data is fully online with several forms of access including footprint visualization, composite images, extracted spectra and source lists.
- ID:
- ivo://archive.stsci.edu/hst/hsc
- Title:
- Hubble Source Catalog Detailed Search
- Short Name:
- HSC
- Date:
- 16 Sep 2020 20:28:11
- 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:
- 03 Nov 2022 16:20:11
- 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://mast.stsci/siap/angst
- Title:
- Hubble Space Telescope ACS Nearby Galaxy Survey (ANGST)
- Short Name:
- HST.angst
- Date:
- 23 Jul 2020 19:38:15
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The ACS Nearby Galaxy Survey observed roughly 14 million stars in 69 galaxies. The survey explored a region called the "Local Volume," and the galaxy distances ranged from 6.5 million light-years to 13 million light-years from Earth. The Local Volume resides beyond the Local Group of galaxies, an even nearer collection of a few dozen galaxies within about 3 million light-years of our Milky Way Galaxy. The observations were made in November 2006 with Hubble's Advanced Camera for Surveysi (ACS).
- ID:
- ivo://mast.stsci/ssap/hst/fos
- Title:
- Hubble Space Telescope Faint Object Spectrograph
- Short Name:
- HST.FOS Spectra
- Date:
- 22 Jul 2020 21:50:21
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the HST FOS instrument (processed by ESO and CADC) in the 1,150 - 8,500 Å range, resolution ~ 250 and 1,300, V_max ~ 20, 1990 - 1997. Links point to VO-compatible FITS files created by MAST staff.
- 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/ssap/hst/ghrs
- Title:
- Hubble Space Telescope Goddard High Resolution Spectrograph
- Short Name:
- HST.GHRS Spectra
- Date:
- 22 Jul 2020 21:54:42
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the HST GHRS instrument (processed by ESO and CADC) in the 1,100 - 3,300 Å range, resolution ~ 2,000, 25,000, and 80,000 (echelle), V_max ~ 18, 16, and 12 respectively, 1990 - 1997. Links point to VO-compatible FITS files created by MAST staff.
- ID:
- ivo://mast.stsci/siap/heritage
- Title:
- Hubble Space Telescope Heritage Press Release Images
- Short Name:
- HST.heritage
- Date:
- 23 Jul 2020 19:38:59
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- WFPC2 and ACS images used to create the Heritage project color composite press releases. The data has been expertly prepared, significantly beyond the standard pipeline processing. This usually involves careful image registration, combination, and cleaning via drizzling, making it ready for further scientific analysis and educational use. These data will typically be made available at the time of the associated press release.
- ID:
- ivo://mast.stsci/siap/m82
- Title:
- Hubble Space Telescope multi-color ACS mosaic of M82
- Short Name:
- HST.M82
- Date:
- 23 Jul 2020 19:39:46
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- In March 2006, the Hubble Heritage Team obtained a large 4-color (B, V, I, and H-alpha) mosaic image of the M82 with the Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope.
- ID:
- ivo://mast.stsci/siap/hst.previews
- Title:
- Hubble Space Telescope Preview Images
- Short Name:
- HST Previews
- Date:
- 22 Jul 2020 22:27:41
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Quick-look preview images produced and processed by CADC. Data from the following HST instruments are included: WFPC, WFPC2, STIS, NICMOS, FOC, and ACS.
- ID:
- ivo://mast.stsci/siap/3cr
- Title:
- Hubble Space Telescope Snapshots of 3CR Radio Galaxies
- Short Name:
- HST.3cr
- Date:
- 23 Jul 2020 19:40:22
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The revised 3C catalogue (3CR, Bennett 1962) forms a flux-limited sample of the most radio-powerful sources in the northern hemisphere. Over the decade and a half of HST operation we have performed "snapshot" imaging from the near-IR to the near-UV of a large number of these sources. Most recently we have completed a NICMOS 1.6 micron survey of low-redshift (z less than 0.3) 3CR sources (Madrid et al. 2006, Floyd et al 2008). The fully-reduced data for all 101 sources included in those papers are presented here in numerical order.
- ID:
- ivo://mast.stsci/ssap/hst
- Title:
- Hubble Space Telescope Spectra
- Short Name:
- HST Spectra
- Date:
- 22 Jul 2020 21:49:04
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the following HST instruments are available: GHRS (processed by CADC), FOS (processed by ECF), and STIS (1st order). Separate SSAP services are registered for each instrument. VO-compatible FITS files were created by MAST staff.
- ID:
- ivo://mast.stsci/siap/udfuv
- Title:
- Hubble Space Telescope Ultraviolet Images of the UDF and HDF
- Short Name:
- HST.udfuv
- Date:
- 22 Jul 2020 22:22:46
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Wavelength coverage of the Hubble Ultra Deep Field (UDF) has been extended to ultraviolet wavelength observations. Observations include ACS-SBC images in the Far-UV {1500 Angstrom} and WFPC2 images in the Near-UV {F300W} during excution of the HST Treasury program 10403 ( PI Harry Teplitz -- California Institute of Technology). Included with this set of data are ACS/SBC observations of the Hubble Deep Field (HDF) North.
- 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://mast.stsci/ssap/iue
- Title:
- International Ultraviolet Explorer
- Short Name:
- IUE
- Date:
- 22 Jul 2020 21:56:49
- 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. This service currently provides access to the low dispersion "NEWSIPS" data, reformatted to be VO-compatible.
- 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.
- ID:
- ivo://archive.stsci.edu/kepler_planets
- Title:
- Kepler Confirmed Planets
- Short Name:
- Kepler Planets
- Date:
- 22 Jul 2020 20:51:12
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The list of currently confirmed exoplanets discovered by Kepler (from data compiled by http://nexsci.caltech.edu).
- ID:
- ivo://archive.stsci.edu/kepler
- Title:
- Kepler Data Search
- Short Name:
- Kepler CS
- Date:
- 22 Jul 2020 21:17:20
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of those exoplanets. Although Kepler completed its primary mission to determine the fraction of stars that have planets in 2013, it is continuing the search, using a more limited survey mode, under the new name K2. This service is the main Kepler data search.
- ID:
- ivo://archive.stsci.edu/kepler_ktc
- Title:
- Kepler Data Search
- Short Name:
- KTC
- Date:
- 22 Jul 2020 21:12:32
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- This interface joins the Kepler Target Catalog (KTC) with other tables to allow users to access the Kepler data archive. Observed Kepler targets are included with their associated data set names. Since most of the Kepler light curve data is still proprietary, public data can be found by searching for release dates earlier than todays date.
- 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/k2
- Title:
- Kepler K2 Data Search Catalog
- Short Name:
- K2
- Date:
- 22 Jul 2020 21:33:57
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of those exoplanets. Although Kepler completed its primary mission to determine the fraction of stars that have planets in 2013, it is continuing the search, using a more limited survey mode, under the new name K2. The K2 Data Search Service provides the main catalog for all K2 data.
- ID:
- ivo://archive.stsci.edu/kepler/k2_epic
- Title:
- Kepler K2 Ecliptic Plane Input Catalog
- Short Name:
- K2 EPIC
- Date:
- 12 Feb 2020 19:53:23
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of those exoplanets. Although Kepler completed its primary mission to determine the fraction of stars that have planets in 2013, it is continuing the search, using a more limited survey mode, under the new name K2. The K2 Ecliptic Plane Input Catalog is the primary source of information about objects observed as potential targets for the K2 mission, as the Kepler Input Catalog was used for the original Kepler mission.
- ID:
- ivo://archive.stsci.edu/kepler_koi
- Title:
- Kepler Objects of Interest (KOI)
- Short Name:
- KOI CS
- Date:
- 12 Feb 2020 19:51:12
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of those exoplanets. Although Kepler completed its primary mission to determine the fraction of stars that have planets in 2013, it is continuing the search, using a more limited survey mode, under the new name K2. KOI is the Kepler Objects of Interest catalog listing observed Kepler targets which are flagged as potentially having exoplanets but may be false positives caused by other types of transient detection. This catalog is produced by the Kepler project and brought to MAST via NExScI.
- ID:
- ivo://archive.stsci.edu/kepler_published_planets
- Title:
- Kepler Published Planets
- Short Name:
- K Pub Planets
- Date:
- 12 Feb 2020 19:41:28
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- "Kepler Published Planets" is a catalog created from NExScI catalogs listing of published exoplanets found using Kepler. All included metadata is from the published paper.
- ID:
- ivo://archive.stsci.edu/kepler_fov
- Title:
- Kepler Target Search
- Short Name:
- KIC_CT
- Date:
- 12 Feb 2020 19:50:32
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Kepler Target Search interface provides access to a 12.5 million row table created by MAST by joining entries from the Kepler Input catalog (KIC) with the Kepler Characteristics table (CT) and merging these with "associated" entries from the United Kingdom Infrared Telescope (IRT) project, the USNOb catalog, GALEX, the Kepler Isaac Newton Telescope Survey (KIS), and the Everett KPNO (UBV) survey. The search interface allows users to find targets within the Kepler field of view (FOV) and allows searches on magnitudes, colors, and other parameters for both KIC and associated non-KIC targets. This is the recommended interface for potential guest observers to locate possible targets for observation. GO proposers however should check on the target's position by either (or both) looking to one of our posted FFI images and seeing if it is on a chip, and (2) confirming this with the GO office.
75. 2MASS ConeSearch
- ID:
- ivo://archive.stsci.edu/catalogs/2MASS
- Title:
- 2MASS ConeSearch
- Short Name:
- 2MASS CS
- Date:
- 13 Feb 2020 17:34:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. The Two Micron All Sky Survey (2MASS) catalog holdings at MAST are available with this access url. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://mast.stsci.edu
- Title:
- MAST Authority Name
- Short Name:
- MAST
- Date:
- 04 Apr 2008 16:13:37
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- This authority name is used to identify resources from the STScI multi-mission archive.
- ID:
- ivo://archive.stsci.edu/catalogs/obspointing
- Title:
- MAST CAOM ObsPointing ConeSearch
- Short Name:
- MAST ObsPointing
- Date:
- 16 Sep 2020 20:18:53
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. This service provides access to MAST holdings with pointing positional information in the Common Archive Observation Model (CAOM) database, by providing access to the ObsPointing table as a cone search. Available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
78. MAST ConeSearch
- ID:
- ivo://archive.stsci.edu/catalogs/mastcs
- Title:
- MAST ConeSearch
- Short Name:
- MAST CS
- Date:
- 23 Jul 2020 19:55:10
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. This service provides access to all, with an optional non-standard parameter for an individual catalog to query. The available missions are listed at http://archive.stsci.edu/vo/mast_services.html, and include Hubble (HST) data, Kepler, K2, IUE, HUT, EUVE, FUSE, UIT, WUPPE, BEFS, TUES, IMAPS, High Level Science Products (HLSP), Copernicus, HPOL, VLA First, XMM-OM, and SWIFT.
- ID:
- ivo://archive.stsci.edu/catalogs/obscore
- Title:
- MAST ObsCore ConeSearch
- Short Name:
- MAST ObsCore
- Date:
- 16 Sep 2020 20:23:33
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. This service provides access to all MAST holdings with positional information that have been ingested into the Common Archive Observation Model (CAOM) and its summarized ObsCore format. Available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/skymapperdr4
- Title:
- MAST SkyMapper Southern Survey Data Release 4 (SMSS DR4)
- Short Name:
- MAST SkyMapper
- Date:
- 16 Apr 2024 20:18:39
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- MAST hosts a copy of the SkyMapper DR4 catalog. SMSS DR4 contains optical photometry in the 6 SkyMapper filters (u,v,g,r,i,z) for ~700 million astrophysical sources over 26,000 sq.deg, ranging from the South Celestial Pole to Dec=+16 degrees for objects with data in all bands, and some sources as far North as +29 degrees. The photometry is drawn from over 15 billion measurements made from more than 400,000 images acquired by the 1.3m SkyMapper telescope between March 2014 and September 2021. The typical 10-sigma depths for each field range between 18.5 and 20.5 ABmag, depending on the filter, but certain sky regions include longer exposures that reach as deep as 22 ABmag. Compared to previous SkyMapper data releases, DR4 includes significant enhancements in data processing, most notably a new photometric calibration anchored to synthetic photometry from Gaia low-resolution spectroscopy, which resolves reddening- and spatial-trends identified in previous releases, especially in the bluest filters, u and v. A large number of other photometric and spectroscopic surveys have been cross-matched to the dr4.master table of objects, to facilitate various scientific investigations.
- ID:
- ivo://archive.stsci.edu/tors_spclass
- Title:
- MAST Spectral Classes of Like Stars
- Short Name:
- tors_spclass
- Date:
- 08 Jun 2017 15:34:18
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- This table was created by cross correlating entries from the MAST "Table of Representative Spectra" with targets listed in the Skiff Spectral catalog, the Sky2000 catalog, and/or provided by Simbad. Spectra from IUE, STIS, FUSE, EUVE, HUT, GHRS, FOS, WUPPE, BEFS, and TUES are included. Most correlations were based on cross-matching target names and coordinates, usually with a 5" tolerance, but a few matches may be wrong. The table lists roughly 28,000 observations including novae and supernovae of which more than 22,000 have assigned spectral types.
- ID:
- ivo://archive.stsci.edu/caomtap
- Title:
- MAST STScI CAOM and ObsCore TAP service
- Short Name:
- STScI CAOMTAP
- Date:
- 08 Mar 2024 16:24:41
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The MAST Archive at STScI TAP end point for observational data, saved in the Common Archive Data Model format and made available through the ObsCore limited view. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported. Missions and projects with data available through the CAOMTAP service include: BEFS, EUVE, FUSE, GALEX, HLA, HST, HUT, IUE, JWST, K2, KEPLER, PS1 (PanSTARRS 1) Data Release 2, SPITZER_SHA, SWIFT, TESS, TUES, WUPPE. High Level Science Products (HLSPs) available include: 3D-DASH, 3DHST, CDIPS, CLASSY, DIAMANTE, ELEANOR, EVEREST, GSFC-ELEANOR-LITE, HALO, HFF-DEEPSPACE, hlsp_3cr, hlsp_acsggct, hlsp_andromeda, hlsp_angrrr, hlsp_angst, hlsp_appp, hlsp_borg, hlsp_candels, hlsp_carina, hlsp_clash, hlsp_coma, hlsp_cosmos, hlsp_frontier, hlsp_gems, hlsp_ghosts, hlsp_goods, hlsp_goodsnic, hlsp_heritage, hlsp_hippies, hlsp_hlastarclusters, hlsp_hudf09, hlsp_hudf12, hlsp_ison, hlsp_legus, hlsp_m82, hlsp_m83mos, hlsp_orion, hlsp_phat, hlsp_sgal, hlsp_sm4ero, hlsp_stages, hlsp_starcat, hlsp_udf, hlsp_uvudf, hlsp_wfc3ers, hlsp_wisp, hlsp_xdf, IRIS, K2SC, K2SFF, K2VARCAT, KBONUS-APEXBA, KEPSEISMIC, PATHOS, PSFK2, QLP, TASOC, TESS-SPOC, ULLYSES Tables exposed through this endpoint include the ObsCore (version 1.1) view of our CAOM (version 2.4) database, as well as all other CAOM tables
- ID:
- ivo://archive.stsci.edu/tap/hlsp_classy
- Title:
- MAST STScI CLASSY HLSP TAP service
- Short Name:
- HLSP CLASSY TAP
- Date:
- 10 Mar 2022 21:11:46
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The COS Legacy Archive Spectroscopic SurveY (CLASSY): A UV Treasury of Star-Forming Galaxies is a High Level Science Product hosted at the Mikulski Archive for Space Telescopes. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/hscv3tap
- Title:
- MAST STScI Hubble Source Catalog Version 3 (HSCv3) TAP service
- Short Name:
- HSCv3 TAP
- Date:
- 08 Aug 2023 17:46:27
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The MAST Archive at STScI TAP end point for the Hubble Source Catalog, version 3.1. 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 version 3.1 also provides proper motions for over 400,00 stars in the augmented Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) HST field, and the Hubble Catalog of Variables (HCV). The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/hsctap
- Title:
- MAST STScI Hubble Source Catalog Version 3 (HSCv3) TAP service
- Short Name:
- HSC TAP
- Date:
- 08 Aug 2023 17:42:44
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The MAST Archive at STScI TAP end point for the Hubble Source Catalog, version 3.1. 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 version 3.1 also provides proper motions for over 400,00 stars in the augmented Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) HST field, and the Hubble Catalog of Variables (HCV). The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/MissionMAST
- Title:
- MAST STScI MissionMAST TAP service for HST Science Data
- Short Name:
- MissionMAST TAP
- Date:
- 12 Aug 2021 16:27:28
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/ps1dr2tap
- Title:
- MAST STScI PanSTARRS 1 DR2 TAP service
- Short Name:
- PS1DR2 TAP
- Date:
- 03 Mar 2023 17:21:59
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS or PS1) is a wide-field imaging facility developed at the University of Hawaii's Institute for Astronomy for a variety of scientific studies from the nearby to the very distant Universe. The PS1 catalog includes measurements in five filters (grizy) covering 30,000 square degrees of the sky north of declination -30 degrees, with typically ~12 epochs for each filter. This interface allows searches for the mean measurements and the deeper stacked measurements from images combining all the epochs. The DR2 release also includes the detection catalog containing all the multi-epoch observations. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/regtap
- Title:
- MAST STScI Registry TAP service
- Short Name:
- STScI RegTAP
- Date:
- 03 Mar 2023 16:58:32
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The MAST Archive at STScI TAP end point for registry metadata. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. Tables exposed through this endpoint include are only for the Registry Relational database
- ID:
- ivo://archive.stsci.edu/tap/tic
- Title:
- MAST STScI TESS Input Catalog TAP service
- Short Name:
- TIC TAP
- Date:
- 08 Aug 2023 17:29:26
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The MAST Archive at STScI TAP end point for the TESS Input Catalog. The TIC is used to help identify two-minute cadence target selection for the TESS mission, and to calculate physical and observational properties of planet candidates. It is for use by both the TESS science team and the public, and it is periodically updated – the current version is TIC-8. TIC-8 uses the GAIA DR2 catalog as a base and merges a large number of other photometric catalogs, including 2MASS, UCAC4, APASS, SDSS, WISE, etc. There are roughly 1.5 billion stellar and extended sources in TIC-8, containing compiled magnitudes including B, V, u, g, r, i, z, J, H, K, W1-W4, and G. The TIC can be directly accessed through the Mikulski Archive for Space Telescopes (MAST), using either queries or bulk download. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- ID:
- ivo://archive.stsci.edu/tap/hlsp_ullyses
- Title:
- MAST STScI ULLYSES HLSP TAP service
- Short Name:
- HLSP ULLYSES TAP
- Date:
- 05 Oct 2022 14:57:15
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hubble Space Telescope’s (HST) Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES) program is an ultraviolet spectroscopic library of young high- and low-mass stars in the local universe. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
- 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/catalogs/HLSP_PHAT
- Title:
- Panchromatic Hubble Andromeda Treasury ConeSearch
- Short Name:
- PHAT CS
- Date:
- 23 Jul 2020 20:42:13
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared. With HST's resolution and sensitivity, the disk of M31 will be resolved into more than 100 million stars, enabling a wide range of scientific endeavors. The PHAT observations are grouped into 23 "bricks", each listed under a different proposal ID. Each brick consists of a 3x6 array of pointings, producing complete coverage in the UV, optical, and NIR. Each brick is observed as two 3x3 "half bricks", with observations taken ~6 months apart. In the first observing season, a 3x3 half brick of WFC3 pointings is completed in primary, while parallel observations produce a highly overlapping 3x3 tile of ACS observations in the adjacent half brick. After 6 months, the telescope can be rotated by 180 degrees from the original orientation, such that the primary WFC3 pointings cover the area that was tiled by ACS in the first season, and vice versa. Each pointing is observed for 2 orbits, using the 2 WFC3 cameras for one orbit each. Filters: F275W+F336W (WFC3/UVIS), F475W+F814W (ACS/WFC), F110W+F160W (WFC3/IR) Depth: UVIS data reach a magnitude limit of ~25 in F275W and F336W. ACS data reach maximum depths of ~28 magnitudes in F475W and ~27 magnitudes in F814W in the uncrowded outer disk. In these same regions, WFC3/IR data reach maximum depths of ~26.5 and ~25.5 in F110W and F160W, respectively. However, the depth is crowding limited in the optical and NIR, and thus is a strong function of radius. As a result, photometry in the inner bulge fields is far shallower. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://mast.stsci/phat
- Title:
- Panchromatic Hubble Andromeda Treasury (PHAT)
- Short Name:
- PHAT
- Date:
- 23 Jul 2020 19:28:22
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared. With HST's resolution and sensitivity, the disk of M31 will be resolved into more than 100 million stars, enabling a wide range of scientific endeavors.
- ID:
- ivo://archive.stsci.edu/catalogs/PanSTARRS1DR1Best
- Title:
- Pan-STARRS DR1 "Best" Catalog ConeSearch
- Short Name:
- PS1DR1Cone
- Date:
- 13 Feb 2020 17:45:49
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1). The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera (GPC1; see PS1 GPC1 camera) to image the sky in five broadband filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries. The Pan-STARRS Data Release 1 Object Catalog "Best" filtered exists in the MAST holdings and is thus available through a cone search. The filtered data is a ~2billion row subset based on an object having more than 2 detections. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/PanSTARRS1
- Title:
- Pan-STARRS DR1 Catalog ConeSearch
- Short Name:
- PanSTARRS1
- Date:
- 13 Feb 2020 17:45:19
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1). The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera (GPC1; see PS1 GPC1 camera) to image the sky in five broadband filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries. The Pan-STARRS Data Release 1 Object Catalog v3 exists in the MAST holdings and is thus available through a cone search. All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
96. RC3 ConeSearch
- ID:
- ivo://archive.stsci.edu/catalogs/RC3
- Title:
- RC3 ConeSearch
- Short Name:
- RC3 CS
- Date:
- 13 Feb 2020 17:38:51
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. The Third Reference Catalog of Bright Galaxies (RC3) by G. and A. de Vaucouleurs, H.G. Corwin, R.J. Buta, G. Paturel, and P. Fouque. is included as held in a MAST local copy. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
97. SDSS ConeSearch
- ID:
- ivo://archive.stsci.edu/catalogs/SDSS
- Title:
- SDSS ConeSearch
- Short Name:
- SDSS CS
- Date:
- 13 Feb 2020 17:40:32
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via a ConeSearch endpoint. The Sloan Digital Sky Survey (SDSS) Data Release 12 (SDSS DR12) contains all SDSS observations through July 2014. The STScI mirror is available here. More information on SDSS and this data release are available at http://www.sdss.org/dr12/. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/skiff_spclass
- Title:
- Skiff Spectral Catalog
- Short Name:
- skiff_spclass
- Date:
- 08 Jun 2017 15:34:41
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- This service provides access to a modified version of the Skiff Spectral catalog. The full catalog is available from VizieR. The table includes the standard spectral classifications (with spaces removed) and their encoded values as described in the IVOA note titled "An Encoding system to Represent Stellar Spectral Classes in Archival Databases and Catalogs". The table contains roughly 450,000 targets. Note Skiff does not list novae or supernovae.
- ID:
- ivo://mast.stsci/siap/stages
- Title:
- Space Telescope A901/902 Galaxy Evolution Survey (STAGES)
- Short Name:
- HST.STAGES
- Date:
- 23 Jul 2020 19:41:16
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- STAGES is a large area (0.5x0.5 degree) survey of the complex Abell 901(a,b)/902 multiple-cluster system at z=0.165. An 80-tile imaging mosaic in F606W was conducted in HST cycle 13 with the HST/ACS instrument.
- 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.