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- ID:
- ivo://archive.stsci.edu/ps1dr1tap
- Title:
- MAST STScI PanSTARRS 1 DR1 TAP service
- Short Name:
- PS1DR1 TAP
- Date:
- 18 Oct 2024 17:46:18
- 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 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:
- 18 Oct 2024 17:25:59
- 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:
- 18 Oct 2024 17:23:56
- 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/skymapperdr4
- Title:
- MAST STScI SkyMapper DR4 TAP service
- Short Name:
- SkyMapperDR4 TAP
- Date:
- 18 Oct 2024 17:49:51
- 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. 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/tic
- Title:
- MAST STScI TESS Input Catalog TAP service
- Short Name:
- TIC TAP
- Date:
- 18 Oct 2024 17:27:00
- 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. The MAST Archive at STScI TAP end point for the TESS Input Catalog (TIC), currently version 8.2. 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:
- 18 Oct 2024 17:22:38
- 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.
