- 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.
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- 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/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/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/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.
