2025A&A...693A.189D


Query : 2025A&A...693A.189D

2025A&A...693A.189D - Astronomy and Astrophysics, volume 693A189 (2025/1-1)

The ViCTORIA project Description of a multi-frequency radio survey of the Virgo galaxy cluster.

DE GASPERIN F., EDLER H.W., BOSELLI A., SERRA P., FOSSATI M., HEESEN V., MERLONI A., MURGIA M., REIPRICH T.H., SPASIC A. and ZABEL N.

Abstract (from CDS):

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.

Abstract Copyright: © The Authors 2025

Journal keyword(s): surveys - galaxies: clusters: individual: Virgo - radio continuum: galaxies - radio lines: galaxies - radio lines: general

Simbad objects: 30

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Number of rows : 30
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 3C 196 Sy1 08 13 36.0561170112 +48 13 02.644966020   18.36 17.79     ~ 578 2
2 NAME HYA SUPERCL SCG 08 57.9 +03 10           ~ 204 0
3 NAME North Polar Spur ISM 12 00 +00.0           ~ 405 1
4 M 86 GiG 12 26 11.814 +12 56 45.49 10.32 9.83 8.90   7.50 ~ 1126 1
5 NGC 4424 H2G 12 27 11.5741235616 +09 25 14.330453700   13.1       ~ 407 0
6 M 49 Sy2 12 29 46.8 +08 00 01   13.21 12.17     ~ 2174 2
7 NGC 4477 Sy2 12 30 02.1955766304 +13 38 11.543715888 11.98 11.38 10.42     ~ 419 2
8 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
9 NAME Virgo Region reg 12 30.8 +12 23           ~ 140 1
10 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
11 NAME Local Supercluster SCG 12 31 +12.4           ~ 566 0
12 IC 3453 H2G 12 31 37.742 +14 51 35.23   15.2       ~ 97 0
13 IC 797 GiC 12 31 54.752 +15 07 26.11   13.9       ~ 157 0
14 M 88 Sy2 12 31 59.1525062448 +14 25 13.148971824   14.33 13.18     ~ 843 1
15 NGC 4506 GiG 12 32 10.5232013544 +13 25 10.824935016   13.63       ~ 123 1
16 IC 3476 GiC 12 32 41.744 +14 03 05.81   13.5       ~ 221 0
17 NGC 4523 GiC 12 33 47.9911135872 +15 10 06.049286292   15.1       ~ 178 0
18 IC 800 LSB 12 33 56.715 +15 21 16.35   14.3       ~ 153 0
19 NGC 4540 GiG 12 34 50.8741239840 +15 33 06.116283900   12.5       ~ 220 1
20 M 91 LIN 12 35 26.4446761320 +14 29 46.760333748   14.63 13.57     ~ 639 0
21 M 90 Sy2 12 36 49.8009839880 +13 09 46.523813040 10.56 10.26 9.54     ~ 953 1
22 M 60 GiC 12 43 39.9708251934 +11 33 09.688174067   10.3       ~ 1395 1
23 ACO 3526 ClG 12 48 49.2 -41 18 17           ~ 1154 2
24 ACO 1656 ClG 12 59 44.40 +27 54 44.9           ~ 5141 2
25 ACO 3558 ClG 13 28 03.2 -31 31 35           ~ 476 2
26 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
27 3C 295 Sy1 14 11 20.6 +52 12 09   22.34 20.80 18.54   ~ 1021 4
28 NAME Loop I SR? 15 01 -38.7           ~ 414 2
29 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
30 NAME CFA Great Wall SCG ~ ~           ~ 142 0

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