Deep Mosaic of the Fornax cluster core Virtual Observatory Resource

Authors

1. Lisker, T.
2. Wittmann, C.
3. Pasquali, A.
4. Hilker, M.
5. Grebel, E.K.
6. Venhola, A.

Published by

The GAVO DC team

Abstract

 This is a deep optical mosaic of the Fornax cluster’s core, covering
1.6 square degrees. The data were acquired with ESO/MPG 2.2m/WFI,
using a transparent filter that nearly equals the no-filter throughput
and thus provides a high signal-to-noise ratio. Based on an
approximate conversion to V-band magnitudes, the unbinned and binned
mosaics (0.24 and 0.71 arcsec/pixel) reach a median depth of 26.6 and
27.8 mag/sq.arcsec, respectively.

Keywords

1. galaxy-clusters

Bibliographic source

Lisker, T., and the Fornax Deep Survey with VST, private communication

See also HTML

http://dc.zah.uni-heidelberg.de/fornax/q/c/info

IVOA Identifier IVOID

ivo://org.gavo.dc/fornax/q/c

Document Object Identifer DOI

doi:10.21938/v3tmOOzxQ3cZx4apXSQWJQ

Access

Web browser access HTML

http://dc.zah.uni-heidelberg.de/fornax
https://dc.zah.uni-heidelberg.de/fornax

IVOA Simple Image Search SIAP

For use with a VO-enabled image processor (e.g., Aladin).
http://dc.zah.uni-heidelberg.de/fornax/q/c/siap.xml?
https://dc.zah.uni-heidelberg.de/fornax/q/c/siap.xml?

Unknown endpoint

Capability for unknown standard ivo://ivoa.net/std/hips#hips-1.0. The VO Registry may have more details; look for IVOID ivo://org.gavo.dc/fornax/q/c.

IVOA Table Access TAP

http://dc.zah.uni-heidelberg.de/tap
https://dc.zah.uni-heidelberg.de/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

Unknown endpoint

Capability for unknown standard ivo://ivoa.net/std/soda#sync-1.0. The VO Registry may have more details; look for IVOID ivo://org.gavo.dc/fornax/q/c.

Unknown endpoint

Capability for unknown standard ivo://ivoa.net/std/datalink#links-1.1. The VO Registry may have more details; look for IVOID ivo://org.gavo.dc/fornax/q/c.