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Start Over Publisher WFAU, Institute for Astronomy, University of Edinburgh
61. VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 2
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.
62. 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).
63. VMC DR4 - VISTA Magellanic System survey
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.
64. VMC DR3 - VISTA Magellanic System survey
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.
65. VMC DR2 - VISTA Magellanic System survey
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.
66. VMC DR1 - VISTA Magellanic System survey
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.
67. VMC DR4 - VISTA Magellanic System survey
ID:
ivo://wfau.roe.ac.uk/vmcDR4-dsa/ceaApplication
Title:
VMC DR4 - VISTA Magellanic System survey
Date:
10 Nov 2017 17:33:38
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.
68. VVV DR5 - VISTA Variables in the Via Lactea survey
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.
69. VVV DR5 - VISTA Variables in the Via Lactea survey
ID:
ivo://wfau.roe.ac.uk/vvvDR5-dsa/ceaApplication
Title:
VVV DR5 - VISTA Variables in the Via Lactea survey
Date:
24 Jan 2022 11:48:18
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.
70. VVV DR4 - VISTA Variables in the Via Lactea survey
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.