The ViCTORIA project

The Virgo cluster is the closest and richest nearby galaxy cluster. It is still in the formation process, with a number of sub-clusters undergoing merging and interactions. Although a great laboratory to study galaxy evolution and cluster formation, its large apparent size and the severe dynamic range limitations due to the presence of the bright radio source Virgo A (M 87) reduced the ability of past wide-area radio surveys to image the region with high levels of sensitivity and fidelity. In this paper we describe the Virgo Cluster multi-Telescope Observations in Radio of Interacting galaxies and AGN (ViCTORIA) project. The survey and its data reduction strategy are designed to mitigate the challenges of this field and deliver images from 42 MHz to 1.7 GHz frequencies of the Virgo cluster about 60 times deeper than existing data; final deliberables will include polarisation images and a blind H I survey aimed at mapping seven times more galaxies than previous experiments without selection biases. Data have been collected with the Low-Frequency Array (LOFAR) using both the Low Band Antenna (LBA) and the High Band Antenna (HBA) systems and with MeerKAT in L -band, including polarisation and enough frequency resolution to conduct local H I studies. At the distance of Virgo, current radio instruments have the resolution to probe scales of ∼500 pc and the sensitivity to study dwarf galaxies, which are the most fragile systems given their shallow gravitational potential wells, making Virgo a unique laboratory to study galaxy evolution and AGN feedback in a rich environment. In this work, we present some preliminary results including the highest resolution images of the radio emission surrounding M 87 ever captured that show that the lobes are filled with filamentary structures. The combination of the presented radio surveys with state-of-the-art optical (NGVS, VESTIGE), UV (GUViCS), and X-ray (eROSITA) surveys will massively increase the scientific output from the studies of the Virgo cluster, making the ViCTORIA Project’s legacy value outstanding.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-12-19
DOI
https://doi.org/10.1051/0004-6361/202452060
Citations
2
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
0.66

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article

The ViCTORIA project

T. H. Reiprich, H. W. Edler, Matteo Fossati, V. Heesen et al.
2 citations
Astronomy and Astrophysics
Radio Astronomy Observations and Technology
0.66
article

The ViCTORIA project

T. H. Reiprich, H. W. Edler, Matteo Fossati, V. Heesen, A. Merloni, P. Serra, F. de Gasperin, Nikki Zabel, M. Murgia, Ana Spasić, A. Boselli
article en
2 citations

Abstract

The Virgo cluster is the closest and richest nearby galaxy cluster. It is still in the formation process, with a number of sub-clusters undergoing merging and interactions. Although a great laboratory to study galaxy evolution and cluster formation, its large apparent size and the severe dynamic range limitations due to the presence of the bright radio source Virgo A (M 87) reduced the ability of past wide-area radio surveys to image the region with high levels of sensitivity and fidelity. In this paper we describe the Virgo Cluster multi-Telescope Observations in Radio of Interacting galaxies and AGN (ViCTORIA) project. The survey and its data reduction strategy are designed to mitigate the challenges of this field and deliver images from 42 MHz to 1.7 GHz frequencies of the Virgo cluster about 60 times deeper than existing data; final deliberables will include polarisation images and a blind H I survey aimed at mapping seven times more galaxies than previous experiments without selection biases. Data have been collected with the Low-Frequency Array (LOFAR) using both the Low Band Antenna (LBA) and the High Band Antenna (HBA) systems and with MeerKAT in L -band, including polarisation and enough frequency resolution to conduct local H I studies. At the distance of Virgo, current radio instruments have the resolution to probe scales of ∼500 pc and the sensitivity to study dwarf galaxies, which are the most fragile systems given their shallow gravitational potential wells, making Virgo a unique laboratory to study galaxy evolution and AGN feedback in a rich environment. In this work, we present some preliminary results including the highest resolution images of the radio emission surrounding M 87 ever captured that show that the lobes are filled with filamentary structures. The combination of the presented radio surveys with state-of-the-art optical (NGVS, VESTIGE), UV (GUViCS), and X-ray (eROSITA) surveys will massively increase the scientific output from the studies of the Virgo cluster, making the ViCTORIA Project’s legacy value outstanding.

Astronomy and AstrophysicsVol. 693
Centre National de la Recherche Scientifique (FR), University of Bonn (DE), Universität Hamburg (DE), University of Groningen (NL), Aix-Marseille Université (FR), Max Planck Institute for Extraterrestrial Physics (DE), Laboratoire d’Astrophysique de Marseille (FR), Istituto di Radioastronomia di Bologna (IT), Château Gombert (FR), Osservatorio Astronomico di Cagliari (IT), University of Milano-Bicocca (IT)
European Research Council
Openalex Percentile: Top 27%
Radio Astronomy Observations and Technology
0.66
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