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- 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://helio-vo.eu/uoc
- Title:
- Unified Observing Catalogue
- Short Name:
- UOC
- Date:
- 22 May 2015 10:34:39
- Publisher:
- HELIO
- Description:
- Database that resolves how to access records in problematic datasets. There are several distinct types of table: 1) Planetary observations stored in NASA's PDS and ESA's PSA; 2) Small FOV, pointed solar instruments; 3) Observations in the Global H-alpha Network.
- ID:
- ivo://helio-vo.eu/uoc/trieste
- Title:
- Unified Observing Catalogue in Trieste
- Date:
- 25 Feb 2014 14:25:21
- Publisher:
- Vineeth T Shetty
- Description:
- Unified Observing Catalogue Description
- ID:
- ivo://helio-vo.eu/uoc/turin
- Title:
- Unified Observing Catalogue in Turin
- Date:
- 29 Jul 2011 18:55:26
- Publisher:
- Vineeth T Shetty
- Description:
- Unified Observing Catalogue Description
- 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/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/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/vmcDR4-dsa
- Title:
- VMC DR4 - VISTA Magellanic System survey
- Date:
- 04 Dec 2019 13:42:27
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar population and allows us to determine the global spatially resolved star formation history with unprecedented quality and to construct a three-dimensional map of the system. A wide-area encompassing the D25 as well as major features delineated by the distribution of stars and HI gas, will both trace the structure of the galaxies and signatures of past and present interactions. Contemporary optical and kinematic observations of comparable sensitivity will provide the community with a superior database for future studies of the system and will give us an excellent insight as to what has happened elsewhere in the Universe.
- ID:
- ivo://wfau.roe.ac.uk/vmcDR3-dsa
- Title:
- VMC DR3 - VISTA Magellanic System survey
- Short Name:
- VMC DR3
- Date:
- 04 Dec 2019 13:42:19
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar population and allows us to determine the global spatially resolved star formation history with unprecedented quality and to construct a three-dimensional map of the system. A wide-area encompassing the D25 as well as major features delineated by the distribution of stars and HI gas, will both trace the structure of the galaxies and signatures of past and present interactions. Contemporary optical and kinematic observations of comparable sensitivity will provide the community with a superior database for future studies of the system and will give us an excellent insight as to what has happened elsewhere in the Universe.
- ID:
- ivo://wfau.roe.ac.uk/vmcDR2-dsa
- Title:
- VMC DR2 - VISTA Magellanic System survey
- Short Name:
- VMC DR2
- Date:
- 04 Dec 2019 13:42:10
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar population and allows us to determine the global spatially resolved star formation history with unprecedented quality and to construct a three-dimensional map of the system. A wide-area encompassing the D25 as well as major features delineated by the distribution of stars and HI gas, will both trace the structure of the galaxies and signatures of past and present interactions. Contemporary optical and kinematic observations of comparable sensitivity will provide the community with a superior database for future studies of the system and will give us an excellent insight as to what has happened elsewhere in the Universe.
- ID:
- ivo://wfau.roe.ac.uk/vmcDR1-dsa
- Title:
- VMC DR1 - VISTA Magellanic System survey
- Short Name:
- VMC DR1
- Date:
- 04 Dec 2019 13:41:53
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar population and allows us to determine the global spatially resolved star formation history with unprecedented quality and to construct a three-dimensional map of the system. A wide-area encompassing the D25 as well as major features delineated by the distribution of stars and HI gas, will both trace the structure of the galaxies and signatures of past and present interactions. Contemporary optical and kinematic observations of comparable sensitivity will provide the community with a superior database for future studies of the system and will give us an excellent insight as to what has happened elsewhere in the Universe.
- ID:
- ivo://wfau.roe.ac.uk/vvvDR5-dsa
- Title:
- VVV DR5 - VISTA Variables in the Via Lactea survey
- Date:
- 24 Jan 2022 11:52:51
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.
- ID:
- ivo://wfau.roe.ac.uk/vvvDR4-dsa
- Title:
- VVV DR4 - VISTA Variables in the Via Lactea survey
- Date:
- 04 Dec 2019 13:43:08
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.
- ID:
- ivo://wfau.roe.ac.uk/vvvDR1-dsa
- Title:
- VVV DR1 - VISTA Variables in the Via Lactea survey
- Short Name:
- VVV DR1
- Date:
- 04 Dec 2019 13:42:47
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.
- ID:
- ivo://wfau.roe.ac.uk/cea-server
- Title:
- WFAU CEA Commandline
- Date:
- 19 Mar 2008 13:49:03
- Publisher:
- WFAU
- Description:
- Applications deployed by WFAU.
84. WFAU Community
- ID:
- ivo://wfau.roe.ac.uk/community
- Title:
- WFAU Community
- Date:
- 24 Apr 2008 13:31:24
- Publisher:
- WFAU
- Description:
- This AstroGrid community is for users from the Univeristy of Edinburgh, as well as users from continental Europe who have requested AstroGrid access to UKIDSS data. It is also for those users who will be using UKIDSS heavily and would like to have their online data storage close to the actual database server.
- ID:
- ivo://wfau.roe.ac.uk/wise-dsa
- Title:
- WISE (Wide-field Infrared Survey Explorer)
- Date:
- 04 Dec 2019 13:43:24
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010) mapped the sky at 3.4, 4.6, 12, and 22 μm (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5Ï? point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.
- ID:
- ivo://wfau.roe.ac.uk/xmm_dsa
- Title:
- XMM-Newton Serendipitous Source Catalogue (2XMM)
- Short Name:
- 2XMM
- Date:
- 23 Jan 2024 09:36:54
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- XMM is the second comprehensive catalogue of serendipitous X-ray sources from the European Space Agency's (ESA) XMM-Newton observatory. The 2XMM catalogue is the largest X-ray source catalogue ever produced, containing almost twice as many discrete sources as either the ROSAT survey or pointed catalogues. 2XMM complements deeper Chandra and XMM-Newton small area surveys, probing a much larger sky area.
87. XMM SUSS
- ID:
- ivo://mssl.ucl.ac.uk/xmmsuss_dsa/XMMSUSS
- Title:
- XMM SUSS
- Date:
- 25 Apr 2012 11:27:46
- Publisher:
- XMM at MSSL
- Description:
- The XMM-OM Serendipitous Ultra-violet Source Survey (SUSS) is a catalog of UV sources detected serendipitously by the Optical Monitor (OM) on-board the European Space Agency's (ESA's) XMM-Newton observatory. It has been created at the University College London's (UCL's) Mullard Space Science Laboratory (MSSL) on behalf of ESA and is a partner resource to the 2XMM serendipitous X-ray source catalogue. The catalog contains source detections drawn from 2,417 XMM-OM observations in up to three broad band UV filters made between 2000 February 24 and 2007 March 29. All datasets included were publicly available by 2007 May 01 but note that, due to screening criteria, not all public observations are included in this catalog. Taking account of substantial overlaps between observations, the net sky area covered independently is 29 - 54 square degreees, depending on UV filter. The primary content of the catalog is filter-dependent source positions and magnitudes, and these are accompanied by profile diagnostics and variability statistics. The XMM-OM SUSS catalog contains 753,578 UV source detections above a signal-to-noise threshold limit of 3-sigma which relate to 624,049 unique objects. A significant fraction of sources (12% - UVW2, 11% - UVM2, 11.% - UVW1) are visited more than once during XMM operation, and a large fraction of sources (38% - UVW2, 23% - UVM2, 22% - UVW1) are observed more than once per filter during an individual visit. UVW2, UVM2 and UVW1 refer to the filter bandpasses defined in the Source Properties: Filter Set section of the MSSL documentation for this catalog: <a href="http://www.mssl.ucl.ac.uk/~mds/XMM-OM-SUSS/SourcePropertiesFilters.shtml">http://www.mssl.ucl.ac.uk/~mds/XMM-OM-SUSS/SourcePropertiesFilters.shtml</a>. Consequently, the scope for science based on temporal source variability on timescales of hours to years is broad. The positional accuracy of the catalog detections is typically 1.0 arcsec (1-sigma confidence radius) with a median positional error of 0.67 arcsec. The median AB magnitude of the catalog detections in the three UV bands is 19.56 (UVW2), 20.23 (UVM2) and 20.69 (UVW1). 20% of sources have AB magnitudes fainter than 20.28 (UVW2), 20.97 (UVM2) and 21.54 (UVW1). As part of quality evaluation for the catalog, each field has been tested for astrometric accuracy and visually screened for cosmetic problems, compromising aspect anomalies, stray light, large extended sources and telemetry dropouts. Observations affected by these issues (11.2%) have been removed from the catalog sample. Furthermore, 2% of all observations were selected at random where each source in this sample was tested for falsehood, spuriousness and accuracy of quality flagging. The results of this detailed screening are included in the full documentation. The processing used to generate the catalog is based on the SAS8.0 pipeline developed for the pipeline reduction of all XMM observations. This version includes a number of significant improvements over the previous data processing system (as used by the SSC in routine processing of XMM-Newton data on behalf of ESA). These improvements include a more robust detection scheme for sources close to the limit of sky background, refined quality flagging and a higher success rate (90%) for refined aspect corrections.