- ID:
- ivo://bira-iasb/tap
- Title:
- VESPA PA team server TAP service
- Short Name:
- BIRA-IASB TAP
- Date:
- 08 Oct 2024 09:26:16
- Publisher:
- bira-iasb
- Description:
- The VESPA PA team server's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: epn_core from the gem_mars schema, epn_core from the nomad schema, epn_core from the soir schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
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Search Results
442. vespa-vu Registry
- ID:
- ivo://vovu.vu/__system__/services/registry
- Title:
- vespa-vu Registry
- Short Name:
- VOVU Reg
- Date:
- 09 Feb 2018 11:44:20
- Publisher:
- The staff at the vespa-vu
- Description:
- The publishing registry for the vespa-vu.
- 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.
