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Start Over Subject infrared, survey, galaxy, marellanic cloud Publisher WFAU, Institute for Astronomy, University of Edinburgh
1. 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.
2. 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.
3. 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.
4. 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.
5. VMC DR2 - VISTA Magellanic System survey
ID:
ivo://wfau.roe.ac.uk/vmcDR2-dsa/ceaApplication
Title:
VMC DR2 - VISTA Magellanic System survey
Date:
05 Mar 2014 15:07:59
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.
6. VMC DR1 - VISTA Magellanic System survey
ID:
ivo://wfau.roe.ac.uk/vmcDR1-dsa/ceaApplication
Title:
VMC DR1 - VISTA Magellanic System survey
Date:
17 Jul 2012 14:15:55
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.
7. VMC DR3 - VISTA Magellanic System survey
ID:
ivo://wfau.roe.ac.uk/vmcDR3-dsa/ceaApplication
Title:
VMC DR3 - VISTA Magellanic System survey
Date:
06 May 2015 16:22:28
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.
8. 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.

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