Deep Mosaic of the Fornax cluster core

DOI

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.

Identifier
DOI http://doi.org/10.21938/v3tmOOzxQ3cZx4apXSQWJQ
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/fornax/q/c
Related Identifier http://dc.g-vo.org/fornax/q/c/info
Related Identifier http://dc.g-vo.org/fornax
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/fornax/q/c
Provenance
Creator Lisker, T.; Wittmann, C.; Pasquali, A.; Hilker, M.; Grebel, E.K.; Venhola, A.
Instrument ESO/MPG 2.2m
Publisher The GAVO DC team
Publication Year 2015
Rights the Fornax VST Survey is licensed under the `Creative Commons Attribution 4.0 License <http://creativecommons.org/licenses/by/4.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY]; https://spdx.org/licenses/CC-BY-4.0.html
OpenAccess true
Contact GAVO Data Centre Team <gavo(at)ari.uni-heidelberg.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Physics
Temporal Coverage 2009-07-19T12:00:00Z 2009-07-19T12:00:00Z