2018A&A...611A..21C


Query : 2018A&A...611A..21C

2018A&A...611A..21C - Astronomy and Astrophysics, volume 611A, 21-21 (2018/3-1)

A VST and VISTA study of globular clusters in NGC 253.

CANTIELLO M., GRADO A., REJKUBA M., ARNABOLDI M., CAPACCIOLI M., GREGGIO L., IODICE E. and LIMATOLA L.

Abstract (from CDS):


Context. Globular clusters (GCs) are key to our understanding of the Universe, as laboratories of stellar evolution, fossil tracers of the past formation epoch of the host galaxy, and effective distance indicators from local to cosmological scales. Aim. We analyze the properties of the sources in the NGC 253 with the aim of defining an up to date catalog of GC candidates in the galaxy. Given the distance of the galaxy, GCs in NGC 253 are ideal targets for resolved color-magnitude diagram studies of extragalactic GCs with next-generation diffraction limited ground-based telescopes.
Methods. Our analysis is based on the science verification data of two ESO survey telescopes, VST and VISTA. Using ugri photometry from VST and JKs from VISTA, GC candidates were selected using as reference the morpho-photometric and color properties of spectroscopically confirmed GCs available in the literature. The strength of the results was verified against available archival HST/ACS data from the GHOSTS survey: all but two of the selected GC candidates appear as star clusters in HST footprints.
Results. The adopted GC selection leads to the definition of a sample of ∼350GC candidates. At visual inspection, we find that 82 objects match all the requirements for selecting GC candidates and 155 are flagged as uncertain GC candidate; however, 110 are unlikely GCs, which are most likely background galaxies. Furthermore, our analysis shows that four of the previously spectroscopically confirmed GCs, i.e., ∼20% of the total spectroscopic sample, are more likely either background galaxies or high-velocity Milky Way stars. The radial density profile of the selected best candidates shows the typically observed r1/4-law radial profile. The analysis of the color distributions reveals only marginal evidence of the presence of color bimodality, which is normally observed in galaxies of similar luminosity. The GC luminosity function does not show the typical symmetry, mainly because of the lack of bright GCs. Part of the bright GCs missing might be at very large galactocentric distances or along the line of sight of the galaxy dusty disk. As an alternative possibility, we speculate that a fraction of low luminosity GC candidates might instead be metal-rich, intermediate age clusters, but fall in a similar color interval of old, metal-poor GCs.
Conclusions. Defining a contaminant-free sample of GCs in extragalactic systems is not a straight forward exercise. Using optical and near-IR photometry we purged the list of GCs with spectroscopic membership and photometric GC candidates in NGC 253. Our results show that the use of either spectroscopic or photometric data only does not generally ensure a contaminant-free sample and a combination of both spectroscopy and photometry is preferred.

Abstract Copyright: © ESO 2018

Journal keyword(s): galaxies: star clusters: general - galaxies: individual: NGC 253 - galaxies: stellar content - galaxies: evolution - catalogs - galaxies: photometry

VizieR on-line data: <Available at CDS (J/A+A/611/A21): table3.dat>

Nomenclature: Table 3: [CGR2018] NNN (Nos 1-347).

Simbad objects: 247

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Number of rows : 247
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 [CGR2018] 268 Gl? 00 45 18.623 -24 53 26.78           ~ 1 0
2 [CGR2018] 81 GlC 00 45 19.408 -25 29 19.50           ~ 1 0
3 [CGR2018] 114 Gl? 00 45 20.134 -25 25 31.74           ~ 1 0
4 [CGR2018] 244 GlC 00 45 20.493 -25 01 08.69           ~ 1 0
5 [CGR2018] 309 GlC 00 45 24.671 -25 07 57.62           ~ 1 0
6 [CGR2018] 300 Gl? 00 45 28.6955897808 -25 37 37.776749160           ~ 1 0
7 [CGR2018] 88 Gl? 00 45 29.010 -25 28 35.99           ~ 1 0
8 [CGR2018] 119 GlC 00 45 30.021 -25 24 21.87           ~ 1 0
9 [CGR2018] 66 Gl? 00 45 33.668 -25 32 41.37           ~ 1 0
10 [CGR2018] 132 Gl? 00 45 36.808 -25 21 58.60           ~ 1 0
11 [CGR2018] 35 GlC 00 45 37.8232369632 -25 42 22.412696364           ~ 1 0
12 [CGR2018] 93 Gl? 00 45 37.826 -25 27 39.77           ~ 1 0
13 [CGR2018] 302 GlC 00 45 40.173 -25 17 28.01           ~ 1 0
14 [CGR2018] 48 Gl? 00 45 40.346 -25 36 21.75           ~ 1 0
15 [CGR2018] 263 Gl? 00 45 40.692 -24 54 15.58           ~ 1 0
16 [CGR2018] 55 Gl? 00 45 43.3244740968 -25 35 03.906504096           ~ 1 0
17 [CGR2018] 276 Gl? 00 45 45.5958412536 -24 50 04.175330604           ~ 1 0
18 [CGR2018] 252 Gl? 00 45 46.407 -24 58 49.50           ~ 1 0
19 [CGR2018] 193 Gl? 00 45 48.108 -25 10 41.98           ~ 1 0
20 [CGR2018] 223 GlC 00 45 48.268 -25 06 04.86           ~ 1 0
21 [CGR2018] 308 Gl? 00 45 49.490 -25 40 22.87           ~ 1 0
22 [CGR2018] 53 Gl? 00 45 52.634 -25 35 19.51           ~ 1 0
23 [CGR2018] 174 Gl? 00 45 53.685 -25 15 02.93           ~ 1 0
24 [CGR2018] 289 Gl? 00 45 55.729 -24 48 16.70           ~ 1 0
25 [CGR2018] 65 Gl? 00 45 56.030 -25 32 57.07           ~ 1 0
26 [CGR2018] 117 Gl? 00 45 56.272 -25 24 24.17           ~ 1 0
27 [CGR2018] 297 Gl? 00 45 57.6683558136 -24 45 26.882278488           ~ 1 0
28 [CGR2018] 242 Gl? 00 45 57.794 -25 01 37.37           ~ 1 0
29 [CGR2018] 134 Gl? 00 45 59.052 -25 21 44.87           ~ 1 0
30 [CGR2018] 290 Gl? 00 46 04.228 -24 48 02.70           ~ 1 0
31 [BS2000] NGC 253 46 GlC 00 46 04.6634319720 -25 09 38.432964024   19.92       ~ 2 0
32 [CGR2018] 180 Gl? 00 46 07.329 -25 13 58.25           ~ 1 0
33 [CGR2018] 100 Gl? 00 46 07.9803459072 -25 27 00.629821836           ~ 1 0
34 [CGR2018] 74 GlC 00 46 09.083 -25 31 16.73           ~ 1 0
35 [CGR2018] 127 Gl? 00 46 09.581 -25 22 14.10           ~ 1 0
36 [CGR2018] 197 Gl? 00 46 11.279 -25 09 43.46           ~ 1 0
37 [CGR2018] 144 GlC 00 46 15.3495476160 -25 20 06.171581112   17.6       ~ 3 0
38 [CGR2018] 254 GlC 00 46 21.295 -24 57 27.87           ~ 1 0
39 [CGR2018] 135 Gl? 00 46 23.481 -25 21 39.27           ~ 1 0
40 [CGR2018] 194 Gl? 00 46 27.295 -25 10 41.29           ~ 1 0
41 [CGR2018] 145 Gl? 00 46 28.273 -25 19 53.46           ~ 1 0
42 [CGR2018] 285 Gl? 00 46 29.741 -24 49 01.42           ~ 1 0
43 [BS2000] NGC 253 72 GlC 00 46 32.216 -25 17 34.00   20.26       ~ 2 0
44 [CGR2018] 32 GlC 00 46 33.4139898240 -25 43 03.317990736           ~ 1 0
45 [CGR2018] 179 GlC 00 46 34.005 -25 14 26.52           ~ 1 0
46 [CGR2018] 315 Gl? 00 46 35.857 -24 58 15.69           ~ 1 0
47 [CGR2018] 27 Gl? 00 46 36.111 -25 44 24.29           ~ 1 0
48 [CGR2018] 41 GlC 00 46 37.3703608632 -25 39 15.730385184           ~ 1 0
49 [CGR2018] 225 Gl? 00 46 39.110 -25 05 48.02           ~ 1 0
50 [CGR2018] 231 GlC 00 46 40.660 -25 04 29.44   20.3       ~ 3 0
51 [CGR2018] 8 Gl? 00 46 41.670 -25 47 11.95           ~ 1 0
52 [CGR2018] 237 Gl? 00 46 43.093 -25 03 11.08           ~ 1 0
53 [CGR2018] 249 Gl? 00 46 44.679 -24 59 39.29           ~ 1 0
54 [CGR2018] 241 Gl? 00 46 45.162 -25 02 00.16           ~ 1 0
55 [CGR2018] 287 Gl? 00 46 45.5150251824 -24 48 31.244263632           ~ 1 0
56 [B86c] 15 GlC 00 46 45.5630004288 -25 17 43.674915768   21.0       ~ 4 0
57 [CGR2018] 47 Gl? 00 46 46.4912749824 -25 36 40.508271684           ~ 1 0
58 [CGR2018] 20 Gl? 00 46 47.231 -25 45 01.98           ~ 1 0
59 [CGR2018] 319 Gl? 00 46 47.473 -25 44 22.28           ~ 1 0
60 [CGR2018] 87 Gl? 00 46 47.572 -25 28 40.74           ~ 1 0
61 [CGR2018] 94 Gl? 00 46 49.402 -25 27 28.18           ~ 1 0
62 [CGR2018] 40 Gl? 00 46 50.438 -25 39 54.24           ~ 1 0
63 [CGR2018] 24 GlC 00 46 50.573 -25 44 34.40           ~ 1 0
64 [CGR2018] 105 GlC 00 46 50.734 -25 26 38.79           ~ 2 0
65 [CGR2018] 347 GlC 00 46 50.995 -25 24 21.12           ~ 1 0
66 [CGR2018] 86 Gl? 00 46 52.737 -25 28 41.15           ~ 1 0
67 [CGR2018] 108 Gl? 00 46 53.866 -25 26 20.10           ~ 1 0
68 [CGR2018] 272 Gl? 00 46 54.101 -24 51 38.34           ~ 1 0
69 [CGR2018] 233 GlC 00 46 55.558 -25 03 51.27           ~ 1 0
70 [CGR2018] 279 Gl? 00 46 57.732 -24 49 50.72           ~ 1 0
71 [CGR2018] 30 Gl? 00 47 00.353 -25 43 26.20           ~ 1 0
72 [CGR2018] 320 Gl? 00 47 02.428 -25 06 25.51           ~ 1 0
73 [CGR2018] 312 Gl? 00 47 02.450 -25 04 53.07           ~ 1 0
74 [CGR2018] 104 GlC 00 47 02.467 -25 26 43.60           ~ 1 0
75 [CGR2018] 79 GlC 00 47 03.141 -25 30 16.24           ~ 1 0
76 [CGR2018] 75 GlC 00 47 03.194 -25 31 14.30           ~ 1 0
77 [CGR2018] 120 Gl? 00 47 03.550 -25 24 11.84           ~ 1 0
78 [CGR2018] 321 Gl? 00 47 06.901 -24 51 41.16           ~ 1 0
79 [CGR2018] 303 Gl? 00 47 07.600 -25 17 55.18           ~ 1 0
80 [CGR2018] 121 GlC 00 47 07.932 -25 23 45.97           ~ 1 0
81 [CGR2018] 155 Gl? 00 47 09.558 -25 17 54.92           ~ 1 0
82 [CGR2018] 345 GlC 00 47 09.7486955016 -25 32 08.354183496           ~ 1 0
83 [CGR2018] 160 Gl? 00 47 09.897 -25 16 54.45           ~ 1 0
84 [CGR2018] 243 Gl? 00 47 09.978 -25 01 17.19           ~ 1 0
85 [CGR2018] 116 GlC 00 47 11.0337189336 -25 24 34.717240620           ~ 1 0
86 [CGR2018] 80 GlC 00 47 11.498 -25 29 38.84           ~ 1 0
87 [CGR2018] 49 GlC 00 47 12.582 -25 36 13.87           ~ 1 0
88 [CGR2018] 17 Gl? 00 47 13.797 -25 45 45.93           ~ 1 0
89 [CGR2018] 181 GlC 00 47 14.355 -25 13 35.62           ~ 1 0
90 [CGR2018] 123 Gl? 00 47 15.238 -25 23 40.17           ~ 1 0
91 [CGR2018] 54 GlC 00 47 15.715 -25 35 26.21           ~ 1 0
92 [CGR2018] 278 Gl? 00 47 16.507 -24 49 49.05           ~ 1 0
93 [CGR2018] 215 GlC 00 47 17.7464478120 -25 07 03.126372564   19.3       ~ 4 0
94 [CGR2018] 277 GlC 00 47 17.784 -24 49 50.94           ~ 1 0
95 [CGR2018] 280 Gl? 00 47 18.10 -24 49 38.7           ~ 1 0
96 [CGR2018] 283 GlC 00 47 18.376 -24 49 28.72           ~ 1 0
97 [CGR2018] 273 GlC 00 47 18.940 -24 50 52.30           ~ 1 0
98 [CGR2018] 99 GlC 00 47 19.7449465728 -25 27 07.513119828           ~ 1 0
99 [CGR2018] 221 GlC 00 47 20.137 -25 06 26.79           ~ 1 0
100 [B86c] 13 Gl? 00 47 23.0515288464 -25 16 23.049461424   21.4       ~ 3 0
101 [B86c] 12 GlC 00 47 23.3817085728 -25 15 41.560137360   20.6       ~ 3 0
102 [B86c] 14 Gl? 00 47 23.3976622992 -25 16 41.490996996   20.2       ~ 3 0
103 [CGR2018] 111 Gl? 00 47 23.763 -25 25 49.53           ~ 1 0
104 [CGR2018] 31 Gl? 00 47 25.135 -25 43 24.80           ~ 1 0
105 [CGR2018] 43 GlC 00 47 25.861 -25 37 26.94           ~ 1 0
106 [CGR2018] 85 Gl? 00 47 27.414 -25 29 05.50           ~ 1 0
107 [CGR2018] 328 Gl? 00 47 27.543 -25 16 41.15           ~ 1 0
108 [CGR2018] 232 Gl? 00 47 28.8215121936 -25 03 53.725410252           ~ 1 0
109 [CGR2018] 109 GlC 00 47 30.286 -25 25 51.62           ~ 1 0
110 [CGR2018] 173 Gl? 00 47 31.763 -25 15 08.82           ~ 1 0
111 [B86c] 24 GlC 00 47 32.5188086760 -25 21 34.691849460   21.0       ~ 3 0
112 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3177 2
113 [CGR2018] 342 GlC 00 47 33.2206463064 -25 23 31.923569328   19.4       ~ 2 0
114 [CGR2018] 313 Gl? 00 47 34.605 -24 49 29.06           ~ 1 0
115 [CGR2018] 57 Gl? 00 47 34.695 -25 34 57.23           ~ 1 0
116 [CGR2018] 33 Gl? 00 47 38.18 -25 43 05.4           ~ 1 0
117 [CGR2018] 52 Gl? 00 47 38.204 -25 35 49.31           ~ 1 0
118 [CGR2018] 201 Gl? 00 47 38.948 -25 09 20.83           ~ 1 0
119 [CGR2018] 115 Gl? 00 47 39.169 -25 25 32.20           ~ 1 0
120 [CGR2018] 11 Gl? 00 47 39.274 -25 46 52.47           ~ 1 0
121 [CGR2018] 72 Gl? 00 47 39.2944949256 -25 31 20.389861632           ~ 1 0
122 [CGR2018] 267 GlC 00 47 39.468 -24 53 48.30           ~ 1 0
123 [CGR2018] 23 Gl? 00 47 40.2138122904 -25 44 35.881053108           ~ 1 0
124 [CGR2018] 327 Gl? 00 47 40.6528744368 -25 17 42.941094936           ~ 1 0
125 [CGR2018] 270 GlC 00 47 40.7475154680 -24 51 41.333245056           ~ 1 0
126 [CGR2018] 184 Gl? 00 47 41.400 -25 12 38.47           ~ 1 0
127 [CGR2018] 316 Gl? 00 47 42.651 -25 04 24.47           ~ 1 0
128 [CGR2018] 326 Gl? 00 47 43.145 -25 16 59.30           ~ 1 0
129 [B86c] 4 GlC 00 47 43.174 -25 12 04.69   21.19 20.40     ~ 2 0
130 [CGR2018] 152 Gl? 00 47 43.840 -25 18 25.51           ~ 1 0
131 [CGR2018] 296 Gl? 00 47 46.3788796776 -24 46 18.795036864           ~ 1 0
132 [CGR2018] 151 Gl? 00 47 46.509 -25 18 39.65           ~ 1 0
133 [B86c] 29 Gl? 00 47 47.96 -25 17 42.1   22.3       ~ 3 0
134 [CGR2018] 157 Gl? 00 47 48.385 -25 17 43.76           ~ 1 0
135 [CGR2018] 186 Gl? 00 47 48.782 -25 12 08.28           ~ 1 0
136 [CGR2018] 141 Gl? 00 47 48.903 -25 20 44.36           ~ 1 0
137 [CGR2018] 206 GlC 00 47 49.170 -25 08 35.22           ~ 1 0
138 [CGR2018] 305 GlC 00 47 49.713 -25 05 54.83           ~ 1 0
139 [CGR2018] 330 Gl? 00 47 50.560 -25 15 21.20           ~ 1 0
140 [CGR2018] 128 GlC 00 47 50.862 -25 22 12.50           ~ 1 0
141 [CGR2018] 64 Gl? 00 47 51.210 -25 33 02.08           ~ 1 0
142 [BS2000] NGC 253 76 GlC 00 47 51.4757201256 -25 11 16.918756224   20.30       ~ 2 0
143 [CGR2018] 331 Gl? 00 47 53.072 -25 14 47.08           ~ 1 0
144 [CGR2018] 199 Gl? 00 47 54.570 -25 09 36.06           ~ 1 0
145 [CGR2018] 329 Gl? 00 47 55.254 -25 15 26.84           ~ 1 0
146 [CGR2018] 203 Gl? 00 47 56.151 -25 09 03.63           ~ 1 0
147 [CGR2018] 271 Gl? 00 47 56.258 -24 51 43.42           ~ 1 0
148 [CGR2018] 250 Gl? 00 47 56.9382357600 -24 59 11.630991372           ~ 1 0
149 [CGR2018] 245 Gl? 00 47 57.604 -25 00 51.19           ~ 1 0
150 [CGR2018] 178 GlC 00 47 57.835 -25 14 26.93           ~ 1 0
151 [CGR2018] 102 Gl? 00 47 58.255 -25 26 47.90           ~ 1 0
152 [CGR2018] 68 Gl? 00 47 58.353 -25 32 40.78           ~ 1 0
153 [CGR2018] 318 Gl? 00 47 58.584 -25 42 32.32           ~ 1 0
154 [CGR2018] 92 Gl? 00 47 58.971 -25 27 48.84           ~ 1 0
155 [CGR2018] 89 Gl? 00 47 59.362 -25 28 32.83           ~ 1 0
156 [CGR2018] 83 Gl? 00 47 59.657 -25 29 19.62           ~ 1 0
157 [CGR2018] 62 GlC 00 47 59.820 -25 33 24.27           ~ 1 0
158 [CGR2018] 101 Gl? 00 48 00.9070367208 -25 26 56.770893240           ~ 1 0
159 [CGR2018] 71 Gl? 00 48 01.002 -25 32 22.13           ~ 1 0
160 [CGR2018] 106 GlC 00 48 01.743 -25 26 39.69           ~ 1 0
161 [B86c] 1 Cl* 00 48 02.471 -25 10 37.37   21.1       ~ 3 0
162 [CGR2018] 96 Gl? 00 48 04.547 -25 27 23.12           ~ 1 0
163 [BS2000] NGC 253 66 GlC 00 48 04.6552710096 -25 07 18.692962428   20.17       ~ 2 0
164 [CGR2018] 146 GlC 00 48 04.722 -25 19 38.67           ~ 1 0
165 [CGR2018] 113 Gl? 00 48 05.073 -25 25 37.97           ~ 1 0
166 [CGR2018] 335 GlC 00 48 05.231 -25 12 01.23           ~ 1 0
167 [CGR2018] 265 Gl? 00 48 06.4352003880 -24 54 07.720924968           ~ 1 0
168 [CGR2018] 323 Gl? 00 48 07.079 -25 34 17.88           ~ 1 0
169 [CGR2018] 301 Gl? 00 48 07.458 -24 59 08.16           ~ 1 0
170 [CGR2018] 334 GlC 00 48 07.503 -25 12 01.89           ~ 1 0
171 [CGR2018] 274 Gl? 00 48 07.717 -24 50 47.41           ~ 1 0
172 [CGR2018] 256 GlC 00 48 08.399 -24 57 13.74           ~ 1 0
173 [CGR2018] 332 Gl? 00 48 08.6915800776 -25 12 21.808816236           ~ 1 0
174 [CGR2018] 147 Gl? 00 48 08.826 -25 18 57.50           ~ 1 0
175 [CGR2018] 56 GlC 00 48 09.507 -25 35 05.18           ~ 1 0
176 [CGR2018] 333 GlC 00 48 09.6774857976 -25 12 07.784937360           ~ 1 0
177 [CGR2018] 336 Gl? 00 48 10.110 -25 11 46.15           ~ 1 0
178 [CGR2018] 7 Gl? 00 48 10.422 -25 47 16.75           ~ 1 0
179 [CGR2018] 148 GlC 00 48 11.018 -25 18 58.68           ~ 1 0
180 [CGR2018] 207 Gl? 00 48 12.037 -25 08 36.49           ~ 1 0
181 [CGR2018] 209 GlC 00 48 12.298 -25 08 21.41           ~ 1 0
182 [CGR2018] 112 Gl? 00 48 12.454 -25 25 41.16           ~ 1 0
183 [CGR2018] 205 GlC 00 48 12.809 -25 08 48.91           ~ 1 0
184 [CGR2018] 224 GlC 00 48 13.1426703816 -25 05 57.050160252   20.0       ~ 2 0
185 [CGR2018] 211 GlC 00 48 13.7186376168 -25 08 05.885860236           ~ 1 0
186 [CGR2018] 251 Gl? 00 48 14.104 -24 59 11.70           ~ 1 0
187 [CGR2018] 200 Gl? 00 48 16.249 -25 09 33.53           ~ 1 0
188 [CGR2018] 246 Gl? 00 48 16.785 -25 00 47.58           ~ 1 0
189 [CGR2018] 204 GlC 00 48 16.910 -25 09 03.09           ~ 1 0
190 [CGR2018] 325 GlC 00 48 17.150 -25 10 36.06           ~ 1 0
191 [CGR2018] 166 Gl? 00 48 17.272 -25 16 06.29           ~ 1 0
192 [CGR2018] 210 GlC 00 48 18.414 -25 08 07.35           ~ 1 0
193 [CGR2018] 129 Gl? 00 48 19.811 -25 22 08.05           ~ 1 0
194 [CGR2018] 259 GlC 00 48 20.901 -24 55 39.27           ~ 1 0
195 [CGR2018] 140 Gl? 00 48 23.901 -25 21 08.46           ~ 1 0
196 [CGR2018] 176 GlC 00 48 24.4866024960 -25 14 48.035662260           ~ 1 0
197 [CGR2018] 288 Gl? 00 48 24.725 -24 48 38.15           ~ 1 0
198 [CGR2018] 235 Gl? 00 48 24.876 -25 03 41.73           ~ 1 0
199 [CGR2018] 275 Gl? 00 48 26.850 -24 50 18.38           ~ 1 0
200 [CGR2018] 260 Gl? 00 48 27.088 -24 55 13.99           ~ 1 0
201 [CGR2018] 298 Gl? 00 48 28.2002450640 -24 59 52.348802856           ~ 1 0
202 [CGR2018] 219 Gl? 00 48 28.985 -25 06 19.74           ~ 1 0
203 [CGR2018] 6 Gl? 00 48 29.838 -25 47 50.24           ~ 1 0
204 [CGR2018] 2 Gl? 00 48 30.113 -25 48 52.16           ~ 1 0
205 [CGR2018] 84 GlC 00 48 32.1301072944 -25 28 57.562172220   19.7       ~ 2 0
206 [CGR2018] 227 GlC 00 48 32.868 -25 05 23.71           ~ 1 0
207 [CGR2018] 191 Gl? 00 48 33.311 -25 11 22.46           ~ 1 0
208 [CGR2018] 311 Gl? 00 48 34.409 -25 16 25.01           ~ 1 0
209 [CGR2018] 163 Gl? 00 48 36.598 -25 16 33.95           ~ 1 0
210 [CGR2018] 218 GlC 00 48 37.232 -25 06 35.24           ~ 1 0
211 [CGR2018] 262 Gl? 00 48 37.893 -24 54 22.03           ~ 1 0
212 [CGR2018] 39 GlC 00 48 38.924 -25 40 01.32           ~ 1 0
213 [CGR2018] 149 Gl? 00 48 41.113 -25 18 57.81           ~ 1 0
214 [CGR2018] 299 GlC 00 48 42.9591709032 -24 58 46.728370740           ~ 1 0
215 [CGR2018] 42 GlC 00 48 43.940 -25 38 41.77           ~ 1 0
216 [LA83] NGC 253 11 Gl? 00 48 45.09 -25 18 27.6   20.1       ~ 2 0
217 [CGR2018] 264 Gl? 00 48 45.313 -24 54 15.61           ~ 1 0
218 [BS2000] NGC 253 79 GlC 00 48 46.511 -25 00 19.38   20.34       ~ 2 0
219 [CGR2018] 324 Gl? 00 48 46.878 -25 10 41.31           ~ 1 0
220 [CGR2018] 257 GlC 00 48 47.809 -24 55 59.43           ~ 1 0
221 [CGR2018] 4 Gl? 00 48 50.562 -25 48 35.13           ~ 1 0
222 [CGR2018] 239 GlC 00 48 51.121 -25 02 16.25           ~ 1 0
223 [CGR2018] 29 Gl? 00 48 52.7094421104 -25 43 47.934453900           ~ 1 0
224 [CGR2018] 226 GlC 00 48 52.715 -25 05 27.64           ~ 1 0
225 [CGR2018] 228 Gl? 00 48 55.095 -25 04 55.00           ~ 1 0
226 [CGR2018] 171 Gl? 00 48 56.965 -25 15 38.28           ~ 1 0
227 [CGR2018] 314 Gl? 00 48 57.726 -25 39 02.53           ~ 1 0
228 [CGR2018] 238 Gl? 00 49 04.574 -25 02 25.24           ~ 1 0
229 [CGR2018] 230 Gl? 00 49 09.338 -25 04 36.48           ~ 1 0
230 [CGR2018] 322 Gl? 00 49 10.044 -25 40 25.73           ~ 1 0
231 [CGR2018] 310 GlC 00 49 10.161 -25 44 19.79           ~ 1 0
232 [CGR2018] 346 Gl? 00 49 16.4626206240 -25 03 01.644597072           ~ 1 0
233 [CGR2018] 213 GlC 00 49 19.0346776296 -25 07 20.537527008           ~ 1 0
234 [CGR2018] 78 Gl? 00 49 23.466 -25 30 12.68           ~ 1 0
235 [CGR2018] 51 Gl? 00 49 25.5593745312 -25 35 45.399978852           ~ 1 0
236 [CGR2018] 45 Gl? 00 49 26.983 -25 37 20.69           ~ 1 0
237 [CGR2018] 304 Gl? 00 49 29.380 -25 17 20.33           ~ 1 0
238 [CGR2018] 306 Gl? 00 49 33.8643304560 -25 37 06.147308172           ~ 1 0
239 [CGR2018] 162 Gl? 00 49 38.154 -25 16 41.68           ~ 1 0
240 [CGR2018] 222 GlC 00 49 39.4041460896 -25 06 04.118258916           ~ 1 0
241 NAME Scl Group GrG 01 00 06 -33 44.2           ~ 493 0
242 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 6503 1
243 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 16411 1
244 M 82 IG 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 5658 6
245 NGC 3115 GiG 10 05 13.9270507008 -07 43 06.982712292   11   9.37   ~ 978 2
246 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 6785 3
247 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 2752 2

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2022.12.07-04:04:16

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