ID |
![]() |
![]() |
sd |
![]() |
Skew | ![]() |
![]() |
![]() |
![]() |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
No colour selection, no magnitude limit | |||||||||
AI | 693 | 1457 ![]() |
312 | 309 ![]() |
-0.16 ![]() |
0.12 ![]() |
0.10 | 0.08 | 0.10 |
AII |
670 | 1446 ![]() |
306 | 302 ![]() |
-0.18 ![]() |
0.21 ![]() |
0.07 | 0.07 | 0.08 |
AV |
729 | 1438 ![]() |
294 | 290 ![]() |
-0.33 ![]() |
0.16 ![]() |
0.01 | 0.06 | 0.01 |
Faint (mR<21.1) GCs, no colour selection | |||||||||
FII | 493 | 1449 ![]() |
309 | 304 ![]() |
-0.07 ![]() |
0.12 ![]() |
0.45 | 0.46 | 0.69 |
FIV |
297 | 1432 ![]() |
288 | 285 ![]() |
-0.23 ![]() |
-0.07 ![]() |
0.28 | 0.37 | 0.14 |
Bright (mR<21.1) GCs | |||||||||
BRI | 144 | 1435 ![]() |
307 | 305 ![]() |
-0.50 ![]() |
0.44 ![]() |
0.05 | 0.03 | 0.02 |
BRII | 140 | 1428 ![]() |
294 | 292 ![]() |
-0.59 ![]() |
0.61 ![]() |
0.03 | 0.03 | 0.01 |
BRIII |
137 | 1424 ![]() |
280 | 279 ![]() |
-0.67 ![]() |
0.72 ![]() |
0.02 | 0.04 | 0.01 |
BRIV | 127 | 1412 ![]() |
283 | 282 ![]() |
-0.63 ![]() |
0.67 ![]() |
0.03 | 0.02 | 0.01 |
Blue GCs
![]() |
|||||||||
BI |
256 | 1452 ![]() |
362 | 358 ![]() |
-0.06 ![]() |
-0.35 ![]() |
0.65 | 0.50 | 0.67 |
BII |
246 | 1435 ![]() |
356 | 351 ![]() |
-0.04 ![]() |
-0.27 ![]() |
0.72 | 0.55 | 0.81 |
BIII |
240 | 1415 ![]() |
337 | 333 ![]() |
-0.21 ![]() |
-0.42 ![]() |
0.22 | 0.14 | 0.09 |
BIV |
139 | 1426 ![]() |
338 | 334 ![]() |
-0.27 ![]() |
-0.49 ![]() |
0.10 | 0.06 | 0.07 |
BV |
336 | 1420 ![]() |
316 | 312 ![]() |
-0.3 ![]() |
-0.14 ![]() |
0.18 | 0.39 | 0.05 |
Red GCs |
|||||||||
RI |
256 | 1472 ![]() |
259 | 256 ![]() |
0.02 ![]() |
0.02 ![]() |
0.48 | 0.70 | 0.70 |
RII | 247 | 1463 ![]() |
254 | 251 ![]() |
0.02 ![]() |
0.09 ![]() |
0.37 | 0.60 | 0.63 |
RIII | 243 | 1463 ![]() |
242 | 239 ![]() |
0.04 ![]() |
-0.08 ![]() |
0.55 | 0.80 | 0.66 |
RIV | 158 | 1437 ![]() |
238 | 234 ![]() |
-0.02 ![]() |
-0.14 ![]() |
0.80 | 0.63 | 0.76 |
RV | 329 | 1453 ![]() |
254 | 251 ![]() |
-0.2 ![]() |
0.33 ![]() |
0.24 | 0.09 | 0.12 |
Notes. This
table summarise the basic statistical properties for
the velocity samples defined in Sect. 5.4. The
samples are identified in the first column while the second column
gives the corresponding number of GC velocities. Column 3
lists the mean
velocity, and the standard deviation is given Col. 4. The
dispersion
,
as returned by the Pryor & Meylan
(1993) estimator, is
given in Col. 5. The third and fourth moments of the velocity
distributions, the skewness and the (reduced) kurtosis
,
are
listed in Cols. 6 and 7, respectively, and the uncertainties
were
estimated using bootstrap resampling. Columns 8 through 10
give the
p-values returned by the Anderson-Darling,
Lilliefors
(Kolmogorov-Smirnov), and the Shapiro-Wilks (W-test) test for
normality, respectively. The Roman numerals refer to the sequence of
subsamples defined in Sect. 5.4,
where (I) is the full sample, prior to
interloper removal. (II): GCs within 3
of NGC 1404 removed,
(III): extreme velocities removed via TME
algorithm (Sect. 5.3);
(IV): restriction to Class A
velocity measurements, and (V)
includes the data from B+07.
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