2023ApJ...944...94T


Query : 2023ApJ...944...94T

2023ApJ...944...94T - Astrophys. J., 944, 94 (2023/February-2)

Cosmicflows-4.

TULLY R.B., KOURKCHI E., COURTOIS H.M., ANAND G.S., BLAKESLEE J.P., BROUT D., DE JAEGER T., DUPUY A., GUINET D., HOWLETT C., JENSEN J.B., POMAREDE D., RIZZI L., RUBIN D., SAID K., SCOLNIC D. and STAHL B.E.

Abstract (from CDS):

With Cosmicflows-4, distances are compiled for 55,877 galaxies gathered into 38,065 groups. Eight methodologies are employed, with the largest numbers coming from the correlations between the photometric and kinematic properties of spiral galaxies (TF) and elliptical galaxies (FP). Supernovae that arise from degenerate progenitors (type Ia SNe) are an important overlapping component. Smaller contributions come from distance estimates from the surface brightness fluctuations of elliptical galaxies and the luminosities and expansion rates of core-collapse supernovae (SNe II). Cepheid period-luminosity relation and tip of the red giant branch observations founded on local stellar parallax measurements along with the geometric maser distance to NGC 4258 provide the absolute scaling of distances. The assembly of galaxies into groups is an important feature of the study in facilitating overlaps between methodologies. Merging between multiple contributions within a methodology and between methodologies is carried out with Bayesian Markov chain Monte Carlo procedures. The final assembly of distances is compatible with a value of the Hubble constant of H0 = 74.6 km s–1 Mpc–1 with the small statistical error of ±0.8 km s–1 Mpc–1 but a large potential systematic error of ∼3 km s–1 Mpc–1. Peculiar velocities can be inferred from the measured distances. The interpretation of the field of peculiar velocities is complex because of large errors on individual components and invites analyses beyond the scope of this study.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Distance indicators - Galaxy distances - Large-scale structure of the universe - Observational cosmology - Hubble constant

VizieR on-line data: <Available at CDS (J/ApJ/944/94): table2.dat table3.dat table4.dat>

Status at CDS : All or part of tables of objects will be ingested in SIMBAD with priority 1. // All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 25

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Number of rows : 25
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 NGC 147 GiG 00 33 12.120 +48 30 31.46   12.0 9.5     ~ 720 1
2 NGC 185 Sy2 00 38 57.9400026024 +48 20 15.035874648   9.10 9.2     ~ 840 1
3 IC 1613 GiC 01 04 48.4071 +02 07 10.185   10.42 10.01 9.77   ~ 1316 2
4 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
5 NGC 1316 rG 03 22 41.789 -37 12 29.52 9.81 9.15 8.53 7.66   ~ 1491 1
6 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
7 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
8 NGC 3417 Sy2 10 51 01.7276243088 +08 28 24.569095512   15.3       ~ 16 0
9 M 66 AGN 11 20 15.0 +12 59 29 9.85 9.65 8.92     ~ 1509 4
10 NAME Leo Cluster ClG 11 30.0 +15 00           ~ 71 0
11 ACO 1367 ClG 11 44 44.6 +19 41 59           ~ 1127 1
12 IC 3019 GiG 12 09 22.257 +13 59 32.73   15.0       ~ 114 0
13 M 106 Sy2 12 18 57.620 +47 18 13.39   9.14 8.41 8.11   ~ 2512 4
14 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
15 NGC 4874 LIN 12 59 35.7093764280 +27 57 33.293892204 13.01 13.7 12.71 12.27 11.386 ~ 814 3
16 ACO 1656 ClG 12 59 44.40 +27 54 44.9           ~ 5141 2
17 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
18 NGC 5253 rG 13 39 55.990 -31 38 24.11 11.48 10.94 10.49 10.33 13.47 ~ 1421 4
19 MCG+03-40-046 G 15 49 20.3077232400 +16 17 21.006028536           ~ 16 0
20 ACO 2147 ClG 16 02 11.96 +15 55 11.5           ~ 416 0
21 ACO 2151 ClG 16 05 15.0 +17 44 55           ~ 594 3
22 NGC 6814 Sy1 19 42 40.5862186152 -10 19 25.108718844   15.33 14.21 11.7 11.3 ~ 866 0
23 NAME SCP reg ~ ~           ~ 113 0
24 NAME Local Group GrG ~ ~           ~ 9325 0
25 NAME Sloan Great Wall ? ~ ~           ~ 191 0

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