2024ApJS..271...40J

Query : 2024ApJS..271...40J

2024ApJS..271...40J - Astrophys. J., Suppl. Ser., 271, 40 (2024/April-0)

Toward Precision Cosmology with Improved Planetary Nebula Luminosity Function Distances Using VLT-MUSE. II. A Test Sample from Archival Data.

JACOBY G.H., CIARDULLO R., ROTH M.M., ARNABOLDI M. and WEILBACHER P.M.

Abstract (from CDS):

Thanks to the MUSE integral field spectrograph on board the Very Large Telescope (VLT), extragalactic distance measurements with the [O III] λ5007 planetary nebula luminosity function (PNLF) are now possible out to ∼40 Mpc. Here we analyze the VLT/MUSE data for 20 galaxies from the ESO public archive to identify the systems' planetary nebulae (PNe) and determine their PNLF distances. Three of the galaxies do not contain enough PNe for a robust measure of the PNLF, and the results for one other system are compromised of the galaxy's internal extinction. However, we obtain robust PNLF distances for the remaining 16 galaxies, two of which are isolated and beyond 30 Mpc in a relatively unperturbed Hubble flow. From these data, we derive a Hubble constant of 74.2 ± 7.2 (stat) ±3.7 (sys) km s–1 Mpc–1, a value that is very similar to that found from other quality indicators (e.g., Cepheids, the tip of the red giant branch, and surface brightness fluctuations). At present, the uncertainty is dominated by the small number of suitable galaxies in the ESO archive and their less-than-ideal observing conditions and calibrations. Based on our experience with these systems, we identify the observational requirements necessary for the PNLF to yield a competitive value for H0 that is independent of the Type Ia supernova distance scale.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxies - Distance indicators - Hubble constant - Planetary nebulae

VizieR on-line data: <Available at CDS (J/ApJS/271/40): table3.dat table2.dat>

Status at CDS : Examining the need for a new acronym. // All or part of tables of objects will be ingested in SIMBAD with priority 1.

Simbad objects: 53

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Number of rows : 53
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 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
4 NGC 300 GiG 00 54 53.4465638304 -37 41 03.168402396 8.83 8.69 8.13 7.46   ~ 1614 2
5 NAME Scl Group GrG 01 00 06 -33 44.2           ~ 526 0
6 NGC 474 GiP 01 20 06.6870520512 +03 24 55.861973100 12.75 12.37 11.51 11.42 10.56 ~ 371 1
7 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
8 M 74 G 01 36 41.7451236624 +15 47 01.107512304 10.52 10.00 9.46 9.16   ~ 1934 1
9 SMDG J0239150-080657 LSB 02 39 15.11 -08 06 58.6     16.5   16.2 ~ 116 0
10 NGC 1052 Bla 02 41 04.79849989 -08 15 20.7519527 11.84 11.41 10.47 10.71   ~ 1397 2
11 LEDA 3097693 LSB 02 41 46.80 -08 24 09.3     16.2   15.8 ~ 183 0
12 NGC 1297 EmG 03 19 14.2293540312 -19 06 00.356560524   14.97 13.98 13.43 12.71 ~ 90 0
13 NGC 1326 Sy1 03 23 56.3657298384 -36 27 52.322333040 11.69 11.43 10.54 10.02 10.9 ~ 279 2
14 NGC 1332 GiP 03 26 17.321 -21 20 07.33   11.45   9.84   ~ 378 0
15 NGC 1351 GiG 03 30 34.9598617824 -34 51 14.242996620   12.30   10.85   ~ 190 0
16 MCG-06-08-024 Sy2 03 31 08.2735132152 -36 17 24.787136976   14.60       ~ 78 1
17 NGC 1366 Sy2 03 33 53.6940996096 -31 11 38.966332632   12.94   11.49   ~ 102 0
18 NGC 1380 Sy2 03 36 27.590 -34 58 34.68 11.32 10.94 9.93 9.37   ~ 460 1
19 NGC 1385 EmG 03 37 28.323 -24 30 04.60 11.28 11.50 10.94 10.45 11.7 ~ 318 2
20 NGC 1399 rG 03 38 29.083 -35 27 02.67 11.05 9.74 9.59 8.12   ~ 1636 1
21 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
22 NGC 1395 SyG 03 38 29.789 -23 01 39.69   10.71   8.99   ~ 289 0
23 NAME Eridanus ClG GrG 03 38 32.00 -22 18 51.0           ~ 200 0
24 2MASS J03385017-3535311 * 03 38 50.1708223056 -35 35 31.156261260           ~ 2 0
25 SN 2007on SN* 03 38 50.90 -35 34 30.0       14.9   SNIa 153 1
26 SN 2011iv SN* 03 38 51.4 -35 35 32           SNIa-norm 96 1
27 NGC 1404 rG 03 38 51.917 -35 35 39.81 11.53 10.69 10.00 9.03   ~ 787 1
28 NGC 1407 rG 03 40 11.904 -18 34 49.36   10.64 9.67 9.13   ~ 613 2
29 NGC 1419 GiG 03 40 42.1036600944 -37 30 38.778564456   13.56   12.07   ~ 146 0
30 NGC 1433 Sy2 03 42 01.4847418992 -47 13 18.929092656   10.84 9.99 9.61 10.2 ~ 447 0
31 NGC 1426 GiG 03 42 49.0997091480 -22 06 30.173615028   12.21 11.44 10.90   ~ 205 0
32 NGC 1439 GiG 03 44 49.9398454104 -21 55 14.341002960   12.23   10.86   ~ 179 0
33 NGC 1512 GiP 04 03 54.281 -43 20 55.86 11.30 11.43 10.54 10.37   ~ 457 1
34 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
35 NGC 2207 AG? 06 16 22.0336889136 -21 22 21.759218400   11.48 10.65 10.21 11.9 ~ 301 4
36 SN 1975A SN* 06 16 26 -21 21.4   14.6       SNIa 39 1
37 IC 2163 AG? 06 16 27.9671433048 -21 22 33.133211832   12.55   11.28   ~ 172 2
38 [KWB2002] 1 X 08 19 12 +70 46.0           ~ 20 0
39 NAME M 96 Group GrG 10 46 45 +11 49.1           ~ 330 0
40 NGC 3501 GiP 11 02 47.307 +17 59 22.31   13.8       ~ 152 0
41 SN 2007sr SN* 12 01 52.80 -18 58 21.7     12.79     SNIa 100 1
42 NGC 4038 EmG 12 01 53.002 -18 52 03.32   10.91   9.74 11.0 ~ 1364 1
43 NAME Antennae IG 12 01 53.170 -18 52 37.92           ~ 1749 0
44 NGC 4039 GiP 12 01 53.51 -18 53 10.3   11.08   9.77   ~ 1173 1
45 M 106 Sy2 12 18 57.620 +47 18 13.39   9.14 8.41 8.11   ~ 2512 4
46 NGC 4365 GiG 12 24 28.228 +07 19 03.07   11.5       ~ 871 0
47 NGC 4355 Sy2 12 26 54.6206739120 -00 52 39.421212996   14.21 13.37     ~ 527 2
48 NAME RZ01 2109 GlC 12 29 39.689 +07 53 32.99   21.67 20.99 20.61   ~ 28 2
49 M 49 Sy2 12 29 46.8 +08 00 01   13.21 12.17     ~ 2174 2
50 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
51 NAME Local Supercluster SCG 12 31 +12.4           ~ 566 0
52 NGC 5248 G 13 37 32.0145074088 +08 53 06.496982448   11.4       ~ 554 0
53 NGC 6958 AG? 20 48 42.6064604520 -37 59 50.876997504 12.79 12.27 11.42 10.83   ~ 168 1

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