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Identifier

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

Doi

10.21938/v3tmOOzxQ3cZx4apXSQWJQ

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Description

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

Galaxy clusters

Creator

Lisker, T.
Wittmann, C.
Pasquali, A.
Hilker, M.
Grebel, E.K.
Venhola, A.

Created

2015-09-22T12:42:00Z

Data updated

2021-05-27T17:43:21Z

Metadata updated

2024-08-15T15:16:57Z

Rights

the Fornax VST Survey is licensed under the Creative Commons Attribution 4.0 License
https://spdx.org/licenses/CC-BY-4.0.html

Source

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

Reference URL

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Deep Mosaic of the Fornax cluster core

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.