- ID:
- ivo://org.gavo.dc/mcextinct/q/cone
- Title:
- Magellanic Clouds Extinction Values
- Short Name:
- MC extinctions
- Date:
- 27 Dec 2024 08:31:03
- Publisher:
- The GAVO DC team
- Description:
- A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.
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262. Magic Public Spectra
- ID:
- ivo://org.gavo.dc/magic/q/ssa
- Title:
- Magic Public Spectra
- Short Name:
- Magic SSAP
- Date:
- 27 Dec 2024 08:31:04
- Publisher:
- The GAVO DC team
- Description:
- The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. This service re-publishes the data with homogeneized in flux units (given here in 'erg/(s.cm2)'). Photon energy values in are transfomred to frequencies.
- ID:
- ivo://bsdc.icranet.org/magic/q/ssa
- Title:
- Magic Public Spectra SSAP Interface
- Short Name:
- Magic SSAP
- Date:
- 17 May 2017 10:12:24
- Publisher:
- BSDC
- Description:
- The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. Our goal here is to provide the same kind of service with the difference that the data is transformed and homogeneized in its flux units, to values in 'erg/(s.cm2)', and photon energy values in equivalent 'Hz' frequency values.
- ID:
- ivo://wfau.roe.ac.uk/twompz-dsa
- Title:
- 2MASS Photometric Redshift catalogue (2MPZ)
- Date:
- 23 Jan 2024 09:45:12
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 2MASS Photometric Redshift catalogue (2MPZ) is constructed by cross-matching 2MASS XSC, WISE and SuperCOSMOS all-sky samples and employing the artificial neural network approach (the ANNz algorithm, Collister & Lahav 2004), trained on several redshift surveys (2MRS, SDSS, 6dFGS, 2dFGRS and ZCAT). The derived photometric redshifts have errors nearly independent of distance, with an all-sky accuracy of Ïz = 0.015, and a very small percentage of outliers. These redshift estimates have a typical precision of 12% for all the 2MASS XSC galaxies that lack spectroscopy. The resulting 2MPZ sample contains almost 1 million galaxies with a median redshift of z=0.07. This catalogue is described in Bilicki et al. 2014, ApJS, 210, 9.
265. 2Mass Query
- ID:
- ivo://org.gavo.dc/2mass/res/2mass/q
- Title:
- 2Mass Query
- Short Name:
- twomass_q
- Date:
- 27 Dec 2024 08:31:04
- Publisher:
- The GAVO DC team
- Description:
- The 2MASS Point Source Catalogue, short a couple of exotic fields. We provide this data mainly for matching with other catalogs within our TAP service.
- 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/tap/hlsp_candels
- Title:
- MAST STScI CANDELS HLSP TAP service
- Short Name:
- HLSP CANDELS TAP
- Date:
- 27 Jan 2025 22:34:44
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (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. 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/caomtap
- Title:
- MAST STScI CAOM and ObsCore TAP service
- Short Name:
- STScI CAOMTAP
- Date:
- 06 Aug 2024 14:14:53
- 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:
- 27 Jan 2025 22:13:33
- 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/tap/hlsp_3DHST
- Title:
- MAST STScI 3D-HST HLSP TAP service
- Short Name:
- HLSP 3D-HST TAP
- Date:
- 27 Jan 2025 22:30:25
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- 3D-HST is a near-infrared spectroscopic survey with the Hubble Space Telescope designed to study the physical processes that shape galaxies in the distant Universe (GO-12177 and GO-12328; PI: Pieter van Dokkum). This Treasury program was allocated 248 orbits of HST time during Cycles 18 and 19. 3D-HST is surveying ~600 square arcminutes of well-studied extragalactic survey fields (AEGIS, COSMOS, GOODS-S, UKIDSS-UDS) with two orbits of primary WFC3/G141 grism coverage and two to four orbits with ACS/G800L coverage. 3D-HST now provides the critical third dimension - redshift - for ~10,000 galaxies at z>1. This is the epoch when ~60% of the star formation in the Universe took place, the number density of quasars peaked, the first galaxies stopped forming stars and the structural regularity that we see in galaxies today emerged. The 3D-HST project details can be found in "3D-HST: A Wide-Field Grism Spectroscopic Survey with the Hubble Space Telescope", Brammer et al., 2012, ApJ, 758L. The survey is optimally designed for the study of galaxy evolution over 1 < < 3.5. The science objectives include: disentangling the processes that regulate star-formation in massive galaxies, evaluating the role of environment and mergers in shaping the galaxy population, and resolving the growth of disks and bulges, spatially and spectrally. The Table Access Protocol (TAP) lets you execute queries against our database tables, and inspect various metadata. Upload is not currently supported.
