« Previous |
1 - 100 of 118
|
Next »
Number of results to display per page
Search Results
- ID:
- ivo://wfau.roe.ac.uk/atlasDR1-dsa
- Title:
- ATLAS DR1 - VST ATLAS Survey
- Date:
- 23 Jan 2024 09:42:24
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 1 of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.
- ID:
- ivo://wfau.roe.ac.uk/atlasDR1-dsa/ceaApplication
- Title:
- ATLAS DR1 - VST ATLAS Survey
- Date:
- 05 Dec 2013 00:07:16
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 1 of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.
- ID:
- ivo://wfau.roe.ac.uk/denis-dsa
- Title:
- Deep Near Infrared Survey of the Southern Sky (DENIS)
- Date:
- 04 Dec 2019 13:34:37
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Catalog of astrometry and photometry of detected point sources in the Far red optical (0.82-micron I-band) and near-infrared (1.25-micron J- and 2.15-micron Ks bands). ~16,700 square degrees of the southern sky
- ID:
- ivo://wfau.roe.ac.uk/denis-dsa/ceaApplication
- Title:
- Deep Near Infrared Survey of the Southern Sky (DENIS)
- Date:
- 30 May 2013 15:19:48
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Catalog of astrometry and photometry of detected point sources in the Far red optical (0.82-micron I-band) and near-infrared (1.25-micron J- and 2.15-micron Ks bands). ~16,700 square degrees of the southern sky
- ID:
- ivo://wfau.roe.ac.uk/6dF-ssap
- Title:
- 6dF DR3 Simple Spectra Access
- Short Name:
- 6dF Spectra
- Date:
- 18 Sep 2013 16:43:53
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75). This is the Data Release 3 version.
- ID:
- ivo://wfau.roe.ac.uk/6df-dsa
- Title:
- 6dF Galaxy Survey Data Release 2
- Short Name:
- 6dF DR2
- Date:
- 23 Jan 2024 09:39:52
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75).
- ID:
- ivo://wfau.roe.ac.uk/6dfdr3-dsa
- Title:
- 6dF Galaxy Survey Data Release 3
- Short Name:
- 6dF DR3
- Date:
- 23 Jan 2024 09:38:59
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75). This is the Data Release 3 version.
- ID:
- ivo://wfau.roe.ac.uk/6dfdr3-dsa/ceaApplication
- Title:
- 6dF Galaxy Survey Data Release 3
- Date:
- 15 Feb 2010 00:08:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75). This is the Data Release 3 version.
- ID:
- ivo://wfau.roe.ac.uk/FastKDA
- Title:
- Fast Kernel Density Analysis Classifier
- Date:
- 15 Feb 2010 14:29:30
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Classify objects using kernel density estimation. Cached sufficient statistics are used to speed up the process.
- ID:
- ivo://wfau.roe.ac.uk/first-dsa
- Title:
- FIRST Survey Catalogue (03Apr11 Version)
- Short Name:
- FIRST
- Date:
- 04 Dec 2019 13:34:53
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- FIRST (Faint Images of the Radio Sky at Twenty-cm) is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North and South Galactic Caps. The catalogue covers a total of about 9033 square degrees of sky (8422 square degrees in the north Galactic cap and 611 square degrees in the south Galactic cap.)
- ID:
- ivo://wfau.roe.ac.uk/first-dsa/ceaApplication
- Title:
- FIRST Survey Catalogue (03Apr11 Version)
- Date:
- 15 Feb 2010 00:11:08
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- FIRST (Faint Images of the Radio Sky at Twenty-cm) is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North and South Galactic Caps. The catalogue covers a total of about 9033 square degrees of sky (8422 square degrees in the north Galactic cap and 611 square degrees in the south Galactic cap.)
13. GALEX Release 6
- ID:
- ivo://wfau.roe.ac.uk/galexgr6-dsa
- Title:
- GALEX Release 6
- Date:
- 23 Jan 2024 09:43:10
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy
14. GALEX Release 6
- ID:
- ivo://wfau.roe.ac.uk/galexgr6-dsa/ceaApplication
- Title:
- GALEX Release 6
- Date:
- 30 May 2013 15:17:15
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy
- ID:
- ivo://wfau.roe.ac.uk/iras-dsa
- Title:
- Infrared Astronomical Satellite Archive (IRAS)
- Short Name:
- IRAS
- Date:
- 04 Dec 2019 13:35:12
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Infrared Astronomical Satellite Archive is an implementation of the IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986). This is a catalogue of some 250,000 well-confirmed infrared point sources observed by the Infrared Astronomical Satellite, i.e., sources with angular extents less than approximately 0.5, 0.5, 1.0, and 2.0 arcmin in the in-scan direction at 12, 25, 60, and 100 microns, respectively.
- ID:
- ivo://wfau.roe.ac.uk/iras-dsa/ceaApplication
- Title:
- Infrared Astronomical Satellite Archive (IRAS)
- Date:
- 15 Feb 2010 00:16:12
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Infrared Astronomical Satellite Archive is an implementation of the IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986). This is a catalogue of some 250,000 well-confirmed infrared point sources observed by the Infrared Astronomical Satellite, i.e., sources with angular extents less than approximately 0.5, 0.5, 1.0, and 2.0 arcmin in the in-scan direction at 12, 25, 60, and 100 microns, respectively.
- 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.
- ID:
- ivo://wfau.roe.ac.uk/twompz-dsa/ceaApplication
- Title:
- 2MASS Photometric Redshift catalogue (2MPZ)
- Date:
- 17 Dec 2013 13:59:49
- 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.
- ID:
- ivo://wfau.roe.ac.uk/mgc-dsa
- Title:
- Millennium Galaxy Catalogue (MGC)
- Date:
- 04 Dec 2019 13:35:24
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Millennium Galaxy Catalogue (MGC) is a 37.5 deg2, medium-deep, B-band imaging survey obtained with the Wide Field Camera on the INT. The survey region is a long, 35 arcmin wide strip along the equator, covering from 10h 00m to 14h 45m and is fully contained within the regions of both the Two Degree Field Galaxy Redshift Survey (2dFGRS) and the Sloan Digital Sky Survey (SDSS).
- ID:
- ivo://wfau.roe.ac.uk/mgc-dsa/ceaApplication
- Title:
- Millennium Galaxy Catalogue (MGC)
- Date:
- 30 May 2013 15:10:58
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Millennium Galaxy Catalogue (MGC) is a 37.5 deg2, medium-deep, B-band imaging survey obtained with the Wide Field Camera on the INT. The survey region is a long, 35 arcmin wide strip along the equator, covering from 10h 00m to 14h 45m and is fully contained within the regions of both the Two Degree Field Galaxy Redshift Survey (2dFGRS) and the Sloan Digital Sky Survey (SDSS).
- ID:
- ivo://wfau.roe.ac.uk/osa-tap
- Title:
- OSA VST ATLAS Survey
- Short Name:
- WFAU OSA TAP
- Date:
- 28 May 2018 17:35:25
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This service hosts the public releases of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh, as well as a number of other external datasets for which WFAU has neighbour tables, that can be cross matched with ATLAS. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.
- ID:
- ivo://wfau.roe.ac.uk/pssa-dsa
- Title:
- Personal SuperCOSMOS Science Archive (SSA)
- Date:
- 23 Jan 2024 09:43:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Small subset of the SuperCOSMOS Science Archive, useful for testing queries. The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/pssa-dsa/ceaApplication
- Title:
- Personal SuperCOSMOS Science Archive (SSA)
- Date:
- 15 Feb 2010 00:18:55
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Small subset of the SuperCOSMOS Science Archive, useful for testing queries. The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/rosat-dsa
- Title:
- Rontgen Satellite Archive (ROSAT)
- Short Name:
- ROSAT
- Date:
- 04 Dec 2019 13:35:43
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Rontgen Satellite Archive is an implementation of the ROSAT All-Sky Survey Bright Source Catalogue (RASS-BSC, revision 1RXS) and the ROSAT All-Sky Survey Faint Source Catalogue (RASS-FSC, revision 1RXS). The RASS-BSC is derived from the all-sky survey performed during the first half year of the ROSAT mission in 1990/91. 18,811 sources are catalogued, with a limiting ROSAT PSPC countrate of 0.05 cts/s in the 0.1-2.4 keV energy band. The sources have a detection likelihood of at least 15 and contain at least 15 source photons. At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. The typical positional accuracy is 30 arcsec. The RASS-FSC is derived from the all-sky survey performed during the ROSAT mission in the energy band 0.1- 2.4 keV. 105,924 sources are catalogued and represent the faint extension to the RASS bright source catalogue. The sources have a detection likelihood of at least 7 and contain at least 6 source photons. (The likelihood of source detection is defined as L =-ln (1-P) , with P = probability of source detection).
- ID:
- ivo://wfau.roe.ac.uk/rosat-dsa/ceaApplication
- Title:
- Rontgen Satellite Archive (ROSAT)
- Date:
- 15 Feb 2010 00:21:30
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Rontgen Satellite Archive is an implementation of the ROSAT All-Sky Survey Bright Source Catalogue (RASS-BSC, revision 1RXS) and the ROSAT All-Sky Survey Faint Source Catalogue (RASS-FSC, revision 1RXS). The RASS-BSC is derived from the all-sky survey performed during the first half year of the ROSAT mission in 1990/91. 18,811 sources are catalogued, with a limiting ROSAT PSPC countrate of 0.05 cts/s in the 0.1-2.4 keV energy band. The sources have a detection likelihood of at least 15 and contain at least 15 source photons. At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. The typical positional accuracy is 30 arcsec. The RASS-FSC is derived from the all-sky survey performed during the ROSAT mission in the energy band 0.1- 2.4 keV. 105,924 sources are catalogued and represent the faint extension to the RASS bright source catalogue. The sources have a detection likelihood of at least 7 and contain at least 6 source photons. (The likelihood of source detection is defined as L =-ln (1-P) , with P = probability of source detection).
- ID:
- ivo://wfau.roe.ac.uk/sdssdr9-dsa
- Title:
- SDSS DR9 - Sloan Digital Sky Survey Data Release 9
- Date:
- 04 Dec 2019 13:36:43
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR9 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr3-dsa
- Title:
- SDSS DR3 - Sloan Digital Sky Survey Data Release 3
- Short Name:
- SDSS DR3
- Date:
- 04 Dec 2019 13:35:52
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR3 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr8-dsa
- Title:
- SDSS DR8 - Sloan Digital Sky Survey Data Release 8
- Short Name:
- SDSS DR8
- Date:
- 04 Dec 2019 13:36:31
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR8 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr7-dsa
- Title:
- SDSS DR7 - Sloan Digital Sky Survey Data Release 7
- Short Name:
- SDSS DR7
- Date:
- 04 Dec 2019 13:36:17
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR7 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr5-dsa
- Title:
- SDSS DR5 - Sloan Digital Sky Survey Data Release 5
- Short Name:
- SDSS DR5
- Date:
- 04 Dec 2019 13:36:06
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR5 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr9-dsa/ceaApplication
- Title:
- SDSS DR9 - Sloan Digital Sky Survey Data Release 9
- Date:
- 07 May 2013 16:05:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR9 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr7-dsa/ceaApplication
- Title:
- SDSS DR7 - Sloan Digital Sky Survey Data Release 7
- Date:
- 27 Oct 2011 17:45:27
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR7 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr8-dsa/ceaApplication
- Title:
- SDSS DR8 - Sloan Digital Sky Survey Data Release 8
- Date:
- 27 Oct 2011 17:17:51
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR8 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr5-dsa/ceaApplication
- Title:
- SDSS DR5 - Sloan Digital Sky Survey Data Release 5
- Date:
- 17 Feb 2010 17:34:48
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR5 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr3-dsa/ceaApplication
- Title:
- SDSS DR3 - Sloan Digital Sky Survey Data Release 3
- Date:
- 15 Feb 2010 14:03:59
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR3 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/ssa-dsa
- Title:
- SuperCOSMOS Science Archive (SSA)
- Short Name:
- SuperCOSMOS
- Date:
- 23 Jan 2024 09:44:26
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/ssa-dsa/ceaApplication
- Title:
- SuperCOSMOS Science Archive (SSA)
- Date:
- 17 Nov 2009 13:59:20
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/sss-siap
- Title:
- SuperCOSMOS Sky Surveys SSS SIAP Cutout Service
- Short Name:
- SuperCOSMOS SIAP
- Date:
- 09 Jul 2019 14:41:02
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to SuperCOSMOS Sky Surveys (SSS) images (scans of photographic survey plates)
- ID:
- ivo://wfau.roe.ac.uk/twomass-dsa
- Title:
- Two Micron All Sky Survey (2MASS)
- Short Name:
- 2MASS
- Date:
- 04 Dec 2019 13:36:55
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Two Micron All Sky Survey (2MASS) will provide a uniform survey of the entire sky at three near-infrared wavebands: J(lambdaeff = 1.25 micrometers), H(lambdaeff = 1.65 micrometers), and Ks(lambdaeff = 2.16 micrometers). A major goal of the survey is to probe large scale structures in the Milky Way and in the Local Universe, exploiting the relatively high transparency of the interstellar medium in the near-infrared, and the high near-infrared luminosities of evolved low- and intermediate-mass stars.Home page at http://pegasus.phast.umass.edu/
- ID:
- ivo://wfau.roe.ac.uk/twomass-dsa/ceaApplication
- Title:
- Two Micron All Sky Survey (2MASS)
- Date:
- 24 Nov 2009 00:41:40
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Two Micron All Sky Survey (2MASS) will provide a uniform survey of the entire sky at three near-infrared wavebands: J(lambdaeff = 1.25 micrometers), H(lambdaeff = 1.65 micrometers), and Ks(lambdaeff = 2.16 micrometers). A major goal of the survey is to probe large scale structures in the Milky Way and in the Local Universe, exploiting the relatively high transparency of the interstellar medium in the near-infrared, and the high near-infrared luminosities of evolved low- and intermediate-mass stars.Home page at http://pegasus.phast.umass.edu/
- ID:
- ivo://wfau.roe.ac.uk/uhsDR2-dsa
- Title:
- UHS DR2 - UKIRT Hemisphere Survey Data Release 2
- Date:
- 23 Jan 2024 09:45:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Hemisphere Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The UHS provides continuous J and K-band coverage in the northern hemisphere from a declination of 0 deg to 60 deg.
- ID:
- ivo://wfau.roe.ac.uk/uhsDR2-dsa/ceaApplication
- Title:
- UHS DR2 - UKIRT Hemisphere Survey Data Release 2
- Date:
- 15 Jun 2023 11:07:39
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Hemisphere Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The UHS provides continuous J and K-band coverage in the northern hemisphere from a declination of 0 deg to 60 deg.
43. UHS SIAP Service
- ID:
- ivo://wfau.roe.ac.uk/uhs-siap
- Title:
- UHS SIAP Service
- Short Name:
- UHS SIAP
- Date:
- 14 Jul 2023 11:31:11
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to all images from DR2 of the UKIRT Hemisphere Survey.
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR11-siap
- Title:
- UKIDSS DR11 SIAP Service
- Short Name:
- UKIDSS DR11 SIAP
- Date:
- 16 Feb 2021 09:44:32
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 11 images for the LAS, GCS, DXS, and UDS surveys.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr10-siap
- Title:
- UKIDSS DR10 SIAP Service
- Short Name:
- UKIDSS DR10 SIAP
- Date:
- 14 Aug 2019 10:48:18
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 10 images for the LAS, GCS, DXS, and UDS surveys.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr9-siap
- Title:
- UKIDSS DR9 SIAP Service
- Short Name:
- UKIDSS DR9 SIAP
- Date:
- 09 Jul 2019 14:44:16
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 9 images for the LAS, GCS, DXS, and UDS surveys.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr8-siap
- Title:
- UKIDSS DR8 SIAP Service
- Short Name:
- UKIDSS DR8 SIAP
- Date:
- 09 Jul 2019 14:44:01
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 9 images for the LAS, GCS, DXS, and UDS surveys. GPS images are from DR7.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr7-siap
- Title:
- UKIDSS DR7 SIAP Service
- Short Name:
- UKIDSS DR7 SIAP
- Date:
- 09 Jul 2019 14:43:29
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 7 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr6-siap
- Title:
- UKIDSS DR6 SIAP Service
- Short Name:
- UKIDSS DR6 SIAP
- Date:
- 09 Jul 2019 14:43:08
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 6 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr5-siap
- Title:
- UKIDSS DR5 SIAP Service
- Short Name:
- UKIDSS DR5 SIAP
- Date:
- 09 Jul 2019 14:42:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 5 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr4-siap
- Title:
- UKIDSS DR4 SIAP Service
- Short Name:
- UKIDSS DR4 SIAP
- Date:
- 09 Jul 2019 14:42:34
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 4 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr3-siap
- Title:
- UKIDSS DR3 SIAP Service
- Short Name:
- UKIDSS DR3 SIAP
- Date:
- 09 Jul 2019 14:42:18
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 3 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssdr2-siap
- Title:
- UKIDSS DR2 SIAP Service
- Short Name:
- UKIDSS DR2 SIAP
- Date:
- 09 Jul 2019 14:42:01
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 2 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidss-siap
- Title:
- UKIDSS DR1 SIAP Service
- Short Name:
- UKIDSS DR1 SIAP
- Date:
- 09 Jul 2019 14:41:43
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to UKIDSS data release 1 images.
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR10-dsa
- Title:
- UKIDSS DR10 - UKIRT Infrared Deep Sky Survey Data Release 10
- Short Name:
- UKIDSS DR10
- Date:
- 04 Dec 2019 13:39:25
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 10 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR9-dsa
- Title:
- UKIDSS DR9 - UKIRT Infrared Deep Sky Survey Data Release 9
- Short Name:
- UKIDSS DR9
- Date:
- 04 Dec 2019 13:39:14
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 9 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR8-dsa
- Title:
- UKIDSS DR8 - UKIRT Infrared Deep Sky Survey Data Release 8
- Short Name:
- UKIDSS DR8
- Date:
- 04 Dec 2019 13:39:04
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 8 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. The Galactic Plane Survey will be available in January 2014. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR7-dsa
- Title:
- UKIDSS DR7 - UKIRT Infrared Deep Sky Survey Data Release 7
- Short Name:
- UKIDSS DR7
- Date:
- 04 Dec 2019 13:38:39
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 7 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from three of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey. The Galactic Plane Survey will be available in march 2012. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR6-dsa
- Title:
- UKIDSS DR6 - UKIRT Infrared Deep Sky Survey Data Release 6
- Short Name:
- UKIDSS DR6
- Date:
- 04 Dec 2019 13:38:28
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 6 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Galactic Plane Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR5-dsa
- Title:
- UKIDSS DR5 - UKIRT Infrared Deep Sky Survey Data Release 5
- Short Name:
- UKIDSS DR5
- Date:
- 04 Dec 2019 13:38:15
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 5 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR4-dsa
- Title:
- UKIDSS DR4 - UKIRT Infrared Deep Sky Survey Data Release 4
- Short Name:
- UKIDSS DR4
- Date:
- 04 Dec 2019 13:38:02
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 4 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey. The data for the Galactic Plane Survey will not be available until April 22, 2010. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR3-dsa
- Title:
- UKIDSS DR3 - UKIRT Infrared Deep Sky Survey Data Release 3
- Short Name:
- UKIDSS DR3
- Date:
- 04 Dec 2019 13:37:44
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 3 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR2-dsa
- Title:
- UKIDSS DR2 - UKIRT Infrared Deep Sky Survey Data Release 2
- Short Name:
- UKIDSS DR2
- Date:
- 04 Dec 2019 13:37:33
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR1-dsa
- Title:
- UKIDSS DR1 - UKIRT Infrared Deep Sky Survey Data Release 1
- Short Name:
- UKIDSS DR1
- Date:
- 04 Dec 2019 13:37:23
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 1 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR8-dsa/ceaApplication
- Title:
- UKIDSS DR8 - UKIRT Infrared Deep Sky Survey Data Release 8
- Short Name:
- UKIDSS DR8
- Date:
- 02 Apr 2014 17:42:59
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 8 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. The Galactic Plane Survey will be available in January 2014. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR9-dsa/ceaApplication
- Title:
- UKIDSS DR9 - UKIRT Infrared Deep Sky Survey Data Release 9
- Date:
- 17 Dec 2013 11:47:17
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 9 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR6-dsa/ceaApplication
- Title:
- UKIDSS DR6 - UKIRT Infrared Deep Sky Survey Data Release 6
- Date:
- 11 May 2012 15:32:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 6 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Galactic Plane Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR7-dsa/ceaApplication
- Title:
- UKIDSS DR7 - UKIRT Infrared Deep Sky Survey Data Release 7
- Date:
- 11 May 2012 15:31:22
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 7 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from three of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey. The Galactic Plane Survey will be available in march 2012. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR5-dsa/ceaApplication
- Title:
- UKIDSS DR5 - UKIRT Infrared Deep Sky Survey Data Release 5
- Date:
- 15 Mar 2011 16:19:02
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 5 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR10-dsa/ceaApplication
- Title:
- UKIDSS DR10 - UKIRT Infrared Deep Sky Survey Data Release 10
- Date:
- 12 Dec 2014 11:22:23
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 10 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR4-dsa/ceaApplication
- Title:
- UKIDSS DR4 - UKIRT Infrared Deep Sky Survey Data Release 4
- Date:
- 27 Apr 2010 10:28:10
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 4 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey. The data for the Galactic Plane Survey will not be available until April 22, 2010. (see www.ukidss.org for survey descriptions)
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR3-dsa/ceaApplication
- Title:
- UKIDSS DR3 - UKIRT Infrared Deep Sky Survey Data Release 3
- Date:
- 15 Feb 2010 13:53:52
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR2-dsa/ceaApplication
- Title:
- UKIDSS DR2 - UKIRT Infrared Deep Sky Survey Data Release 2
- Date:
- 15 Feb 2010 13:50:03
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR1-dsa/ceaApplication
- Title:
- UKIDSS DR1 - UKIRT Infrared Deep Sky Survey Data Release 1
- Date:
- 15 Feb 2010 13:47:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 1 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions).
- ID:
- ivo://wfau.roe.ac.uk/vhsdr1-siap
- Title:
- VHS DR1 SIAP Service
- Short Name:
- VHS DR1 SIAP
- Date:
- 14 Aug 2019 10:49:59
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to VISTA Hemisphere Survey data release 1 images.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR4-dsa
- Title:
- VHS DR4 - VISTA Hemisphere Survey Data Release 4
- Date:
- 23 Jan 2024 09:46:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR3-dsa
- Title:
- VHS DR3 - VISTA Hemisphere Survey Data Release 3
- Short Name:
- VHS DR3
- Date:
- 04 Dec 2019 13:40:01
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR2-dsa
- Title:
- VHS DR2 - VISTA Hemisphere Survey Data Release 2
- Short Name:
- VHS DR2
- Date:
- 04 Dec 2019 13:39:51
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR1-dsa
- Title:
- VHS DR1 - VISTA Hemisphere Survey Data Release 1
- Short Name:
- VHS DR1
- Date:
- 04 Dec 2019 13:39:40
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR6-dsa
- Title:
- VHS DR6 - VISTA Hemisphere Survey Data Release 6
- Date:
- 20 Mar 2019 15:52:58
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR6-dsa/ceaApplication
- Title:
- VHS DR6 - VISTA Hemisphere Survey Data Release 6
- Date:
- 20 Mar 2019 15:27:39
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR2-dsa/ceaApplication
- Title:
- VHS DR2 - VISTA Hemisphere Survey Data Release 2
- Date:
- 05 Mar 2014 14:46:46
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR1-dsa/ceaApplication
- Title:
- VHS DR1 - VISTA Hemisphere Survey Data Release 1
- Date:
- 23 Feb 2012 11:45:57
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR3-dsa/ceaApplication
- Title:
- VHS DR3 - VISTA Hemisphere Survey Data Release 3
- Date:
- 06 May 2015 13:38:49
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/vhsDR4-dsa/ceaApplication
- Title:
- VHS DR4 - VISTA Hemisphere Survey Data Release 4
- Date:
- 10 Nov 2017 16:38:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The resulting data will be about 4 magnitudes deeper than 2MASS and DENIS. The 5000 square degrees covered by the Dark Energy Survey (DES), another imaging survey scheduled to begin in 2010 at the CTIO 4 metre Blanco telescope, will also be observed in H-band. The area around both of the Galactic Caps will be observed in Y- and H- band as well to be combined with the data from the VST ATLAS survey. The main science drivers of the VHS include: examining low mass and nearby stars, studying the merger history of the Galaxy, measuring the properties of Dark Energy through the examination of large-scale structure to a redshift of ~1, and searches for high redshift quasars.
- ID:
- ivo://wfau.roe.ac.uk/videoDR5-dsa
- Title:
- VIDEO DR5 - VISTA Deep Extragalactic Observations survey
- Date:
- 25 May 2021 15:50:06
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR4-dsa
- Title:
- VIDEO DR4 - VISTA Deep Extragalactic Observations survey
- Short Name:
- VIDEO DR4
- Date:
- 04 Dec 2019 13:40:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR3-dsa
- Title:
- VIDEO DR3 - VISTA Deep Extragalactic Observations survey
- Short Name:
- VIDEO DR3
- Date:
- 04 Dec 2019 13:40:40
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR2-dsa
- Title:
- VIDEO DR2 - VISTA Deep Extragalactic Observations survey
- Short Name:
- VIDEO DR2
- Date:
- 04 Dec 2019 13:40:29
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR3-dsa/ceaApplication
- Title:
- VIDEO DR3 - VISTA Deep Extragalactic Observations survey
- Date:
- 05 Mar 2014 15:03:47
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR2-dsa/ceaApplication
- Title:
- VIDEO DR2 - VISTA Deep Extragalactic Observations survey
- Date:
- 17 Jul 2012 15:58:34
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR4-dsa/ceaApplication
- Title:
- VIDEO DR4 - VISTA Deep Extragalactic Observations survey
- Date:
- 06 May 2015 00:45:51
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/videoDR5-dsa/ceaApplication
- Title:
- VIDEO DR5 - VISTA Deep Extragalactic Observations survey
- Date:
- 10 Nov 2017 17:06:48
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIDEO survey is a 30 sq. degree, Z,Y,J,H,K survey that is specifically designed to enable exploration of the main issues in observational cosmology. It allows galaxy and cluster/structure evolution to be traced as a function of both epoch and environment from the present day out to z=4 and AGN/QSO evolution up to and into the epoch of reionization at z > 6. The multi-band nature of the survey ensures many key science drivers can be tackled using the survey alone, without recourse to data from other wavebands.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR4-dsa
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 4
- Short Name:
- VIKING DR4
- Date:
- 04 Dec 2019 13:41:34
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR3-dsa
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 3
- Short Name:
- VIKING DR3
- Date:
- 04 Dec 2019 13:41:21
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR2-dsa
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 2
- Short Name:
- VIKING DR2
- Date:
- 04 Dec 2019 13:41:10
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR3-dsa/ceaApplication
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 3
- Date:
- 17 Dec 2013 11:21:21
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR2-dsa/ceaApplication
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 2
- Date:
- 17 Jul 2012 14:09:16
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
- ID:
- ivo://wfau.roe.ac.uk/vikingDR4-dsa/ceaApplication
- Title:
- VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 4
- Date:
- 06 May 2015 16:46:18
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP, centred on Dec = -30). The matching VISTA survey will cover (almost) all of these stripes in Z,Y,J,H, Ks with ~ 400s exposures per band.
100. VISTA SIAP Service
- ID:
- ivo://wfau.roe.ac.uk/vista-siap
- Title:
- VISTA SIAP Service
- Short Name:
- VISTA SIAP
- Date:
- 09 Jul 2019 15:59:27
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Simple image access to all images from the latest releases of the VISTA public surveys (VHS, VMC, VVV, VIDEO, VIKING).