- ID:
- ivo://archive.stsci.edu/cs/tic
- Title:
- TIC (TESS Input Catalog ConeSearch)
- Short Name:
- TIC ConeSearch
- Date:
- 03 May 2024 19:58:43
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The TESS Input Catalog is a comprehensive collection of 1.73 billion sources on the sky, providing stellar parameters for evaluation of potential planetary transit signals. It combines sources from many other catalogs, including 2MASS, LAMOST, SuperBlink, HSOY, RAVE, APOGEE, UCAC, KIC, EPIC, Tycho-2, APASS, AllWISE, SDSS, Gaia DR2, and Hipparcos. It was constructed for the TESS mission to serve as a source for selecting targets to observe with the TESS two-minute cadence, and to provide stellar parameter information for evaluating the properties of transit candidates. MAST catalog holdings are available via Cone Search endpoints. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html. This service provides access to the TESS input catalog (TIC), currently version 8.2
Number of results to display per page
Search Results
- ID:
- ivo://mast.stsci/ssap/tues
- Title:
- Tubingen Echelle Spectra
- Short Name:
- TUES
- Date:
- 22 Jul 2020 21:57:14
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Tübingen Echelle Spectrograph (TUES), designed and managed at the University of Tübingen, flew on the Orbiting and Retrievable Far and Extreme Ultraviolet Spectrograph (ORFEUS)-SPAS II space shuttle mission in 1996, returning spectra in the 900 Å to 1400 Å wavelength range. The instrument was designed to achieve a spectral resolution of /=10000 when used with an entrance aperture of 10" diameter. During the 17.7 day flight, TUES returned 239 spectra of 62 targets. Note each file contains one echelle order.
- ID:
- ivo://archive.stsci.edu/tues
- Title:
- Tubingen Echelle Spectrograph
- Short Name:
- TUES
- Date:
- 22 Jul 2020 21:31:05
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Tübingen Echelle (TUES) obtained moderate dispersion observations (R=13,000) using an echelle grating including orders 40 - 61 from 910 - 1410 Angstroms. The instrument was designed and built by the University of Tübingen (PI: M. Grewing) and flew as one of three spectrographs on the ORFEUS/SPAS-2 mission for 14 days in November/December 1996. The instrumental resolution was about 10,000 and the effective aperture peaks at 1.3 cm2 near 1100 Angstroms. Objects were observed in a 10 arcsec entrance aperture. The wavelength calibration was established by means of interstellar molecular hydrogen lines.
- ID:
- ivo://archive.stsci.edu/uit
- Title:
- Ultraviolet Imaging Telescope
- Short Name:
- UIT
- Date:
- 22 Jul 2020 21:32:30
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Ultraviolet Imaging Telescope UIT was one of three ultraviolet telescopes on the ASTRO-1 mission flown on the space shuttle Columbia during 2-10 December 1990. The same three instruments were later flown on the space shuttle Endeavour from 3-17 March 1995, as part of the ASTRO-2 mission. Exposures were obtained on 70-mm photographic film in the 1200-3300 Å range using broadband filters and later digitized using a Perkin-Elmer microdensitometer. Image resolution was 3" over a 40' field of view. Overall, UIT-1 obtained 821 exposures of 66 targets, and UIT-2 obtained 758 images of 193 targets.
- ID:
- ivo://mast.stsci/siap/uit
- Title:
- Ultraviolet Imaging Telescope (UIT)
- Short Name:
- UIT
- Date:
- 23 Jul 2020 19:44:25
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Ultraviolet Imaging Telescope UIT was one of three ultraviolet telescopes on the ASTRO-1 mission flown on the space shuttle Columbia during 2-10 December 1990. The same three instruments were later flown on the space shuttle Endeavour from 3-17 March 1995, as part of the ASTRO-2 mission. Exposures were obtained on 70-mm photographic film in the 1200-3300 Å range using broadband filters and later digitized using a Perkin-Elmer microdensitometer. Image resolution was 3" over a 40' field of view. Overall, UIT-1 obtained 821 exposures of 66 targets, and UIT-2 obtained 758 images of 193 targets.
- ID:
- ivo://archive.stsci.edu/catalogs/ultravista
- Title:
- UltraVISTA ConeSearch
- Short Name:
- UltraVISTA CS
- Date:
- 23 Jul 2020 20:36:35
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the UltraVISTA survey: This is the deepest and narrowest VISTA survey. It is imaging one patch of sky over and over again to unprecedented depths. The science goals of UltraVISTA include studying the first galaxies, understanding the stellar mass build-up during the peak epoch of star formation activity and dust-obscured star formation. All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://archive.stsci.edu/catalogs/USNOB
- Title:
- USNO-B Catalog ConeSearch
- Short Name:
- USNOB CS
- Date:
- 13 Feb 2020 17:42:39
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- USNO-B is an all-sky catalog that presents positions, proper motions, magnitudes in various optical passbands, and star/galaxy estimators for 1,042,618,261 objects derived from 3,643,201,733 separate observations. The data were obtained from scans of 7435 Schmidt plates taken for the various sky surveys during the last 50 years. USNO-B1.0 is believed to provide all-sky coverage, completeness down to V = 21, 0>2 astrometric accuracy at J2000, 0.3 mag photometric accuracy in up to five colors, and 85% accuracy for distinguishing stars from nonstellar objects. A more detailed description of the construction and contents of the USNO-B1 catalog can be found in Monet et al. (2003, "The USNO-B Catalog", AJ, 125, 984), http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/usno-b1.0/resolveuid/41be0c1a4d1a8372289bad3baf27cde5. A mirror of USNOB 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/vistavhs
- Title:
- Vista Hemisphere Survey ConeSearch
- Short Name:
- VISTA VHS CS
- Date:
- 13 Feb 2020 17:43:47
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- All MAST catalog holdings are available via Cone Search endpoints. This service provides access to the MAST copy of the VISTA Hemisphere Survey All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
- ID:
- ivo://mast.stsci/siap/al218
- Title:
- VLA-A Array AL218 Texas Survey Source Snapshots (AL218)
- Short Name:
- VLA.AL218
- Date:
- 23 Jul 2020 19:30:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The VLA-A Texas Survey consists of a sample of objects extracted from the earlier Texas Interferometer 365 MHz Survey of radio sources covering a strip of sky from approximately -35.5 degrees declination to +71.5 degrees declination, and complete to flux densities of 0.25 Jy, with positional accuracies of ~1 arcsecond in RA and DEC. The sample is a subset of 71 sources drawn from the area of one optical Schmidt sky survey plate (covering ~6.5x6.5 degrees), Region S861, centered at approximately RA=190.640822109, DEC=-0.273834224277 (J2000), from the UK Schmidt SRC-J Survey. The Region S861 was initially chosen because it represented the combination of the deepest UK Schmidt plate material (the best optical survey material available at the time of the sample definition in 1989) and the highest galactic latitude, thereby emphasizing the extragalactic nature of the survey and also maximizing the likelihood of having more optical detections. Much more recently, the area of this plate has been covered by a number of important sky surveys including 2MASS, NRAO VLA FIRST, and the Sloan Digital Sky Survey (SDSS) which is now public. In particular, the availability of the Sloan Survey data provides 5-band ugriz color information at optical wavelengths, to depth of g,r=22.2.
- ID:
- ivo://mast.stsci/siap/vla-first
- Title:
- VLA Faint Images of the Radio Sky at Twenty Centimeters (FIRST)
- Short Name:
- VLA-FIRST
- Date:
- 23 Jul 2020 19:41:49
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Faint Images of the Radio Sky at Twenty-cm (FIRST) is a systematic survey of the North and South Galactic caps begun in 1993, using the NRAO Very Large Array (VLA) . Typical images are comprised of 1150x1550 1.8" pixels with 5" resolution. Source catalogs are also available including peak and integrated flux densities generated from the high resolution coadded images. The survey yields very accurate (<1 arcsec rms) radio positions of faint (>1 mJy/beam) compact sources. The areas observed were chosen to coincide with the Sloan Digital Sky Survey.
