# Title: Clustering of Local Group distances: publication bias or
# correlated measurements? II. M31 and beyond
# Authors: Richard de Grijs, Giuseppe Bono
# Journal: The Astronomical Journal, 148, 17 (2014)
# Table: ic10distbyyear.dat
#
# updated 27/01/2014
#
# Uncertainties
#MM YYYY (m-M)0 stat. syst. Reference; tracer
#
09 1962 25.5 0.4 # Roberts 1962, AJ, 67, 431; HII region sizes
08 1965 25.5 0. # de Vaucouleurs & Ables 1965, PASP, 77, 272; HII region sizes
04 1972 27.3 0.9 # Bottinelli et al. 1972, A&A, 18, 121; scaling of HI mass to Magellanic-type galaxies
02 1974 27.4 0.45 # Shostak 1974, A&A, 31, 97; from Tammann (priv. comm.), errors +0.8 -0.6 Mpc
12 1974 27.4 0. # Sandage & Tammann 1974, ApJ, 194, 559; HII region sizes
03 1975 25.6 0. # Dean & Davies 1975, MNRAS, 170, 503; HI mapping
11 1977 25.9 0. # Yahill et al. 1977, ApJ, 217, 903; based on the degree of resolution into indiv. stars (upper limit)
09 1978 26.5 0. # de Vaucouleurs 1978, ApJ, 224, 710; HII region sizes
04 1979 25.59 0. # Kraan-Korteweg & Tammann 1979, AN, 300, 181; velocity flows
05 1979 25.0 0. # Huchtmeier 1979, A&A, 75, 170; HI extent compared to other Magellanic-type galaxies
02 1981 26.28 0.45 # Jacoby & Lesser 1981, AJ, 86, 185; single PN
06 1984 26.45 0.15 1.7 # Bottinelli et al. 1984, A&AS, 56, 381; B-band TFR (significant extinction correction!)
04 1992 25.88 0. # Massey et al. 1992, AJ, 103, 1159; WR star brightnesses compared to the LMC
08 1993 25.20 0. # Karachentsev & Tikhonov 1993, A&AS, 100, 227; brightest red stars
08 1993 24.85 0. # Karachentsev & Tikhonov 1993, A&AS, 100, 227; brightest blue stars
08 1993 25.08 0.15 # Karachentsev & Tikhonov 1993, A&AS, 100, 227; weighted mean
00 1994 21.90 0.26 # Wilson 1994, ESOC, 51, 15; Cepheids
06 1994 24.61 0. # Karachentsev & Tikhonov 1994, A&A, 286, 718; brightest blue and red stars, matched to M31
06 1995 24.9 0. # Massey & Armandroff 1995, AJ, 109, 2470; bluest (WR) stars
01 1996 24.59 0.30 # Saha et al. 1996, AJ, 111, 197; Cepheids, optical
03 1996 24.57 0.21 # Wilson et al. 1996, AJ, 111, 1106; Cepheids, NIR
00 1999 24.0 0.13 # Georgiev et al. 1999, Proc. IAU Symp., 193, 762; brightest RSGs w.r.t. IC 1613
01 1999 23.8 0.1 # Tikhonov 1999, Proc. IAU Symp., 192, 244; CMD comparison of brightest stars
02 1999 24.1 0.2 # Sakai et al. 1999, ApJ, 511, 671; Population I = Cepheids
02 1999 23.5 0.2 # Sakai et al. 1999, ApJ, 511, 671; Population II = TRGB, lower limit
00 2000 24.60 0.12 # van den Bergh, S. 2000, The galaxies of the Local Group (Cambridge Univ. Press); unweighted average
02 2000 24.17 0.39 # Ferrarese et al. 2000, ApJ, 529, 745; TRGB
11 2000 23.86 0.12 # Borissova et al. 2000, A&A, 363, 130; RSGs w.r.t. IC 1613 (JHK)
09 2001 24.95 0.20 # Hunter 2001, ApJ, 559, 225; TRGB
09 2001 24.1 0. # Hunter 2001, ApJ, 559, 225; TRGB based on Sakai et al. (1999) for E(B-V) = 0.77: lower limit
08 2003 26.28 0. # Magrini et al. 2003, A&A, 407, 51; PNLF, upper limit
06 2004 24.3 0.3 # Ovcharov & Nedialkov 2005, Aerospace Research in Bulgaria, 20, 85, in Balkan Astronomical Meeting, BAM 2004; K-band LF of RSGs
09 2004 24.35 0.11 # Demers et al. 2004, A&A, 424, 125; Carbon stars
06 2007 24.48 0.08 0.16 # Vacca et al. 2007, ApJ, 662, 272; TRGB
06 2007 24.5 0.15 # Vacca et al. 2007, ApJ, 662, 272; Carbon stars
00 2008 24.75 0.1 # Sanna et al. 2008, Mem. Soc. Astron. It., 79, 747; TRGB
03 2008 24.10 0. # Tully et al. 2008, ApJ, 676, 184; Cepheids
03 2008 24.30 0.14 # Kniazev et al. 2008, MNRAS, 384, 1045; PNLF, errors +0.18 -0.10
12 2008 24.60 0.15 0.08 # Sanna et al. 2008, ApJ, 688, L69; TRGB, theory
12 2008 24.51 0.08 0.08 # Sanna et al. 2008, ApJ, 688, L69; TRGB, theory
12 2008 24.56 0.08 # Sanna et al. 2008, ApJ, 688, L69; TRGB, theory
00 2009 24.67 0. # Sanna et al. 2009, Mem Soc. Astron. It., 80, 79; TRGB - no error
08 2009 23.52 0.08 # Jacobs et al. 2009, AJ, 138, 332; TRGB, errors +0.12 -0.04
09 2009 24.27 0.03 0.18 # Kim et al. 2009, ApJ, 703, 816; TRGB, random/systematic uncertainties
11 2009 24.47 0.10 # Tikhonov & Galazudtdunova 2009, Astron. Lett. 35, 748 (arXiv:1002.2046); TRGB
10 2012 24.1 0.25 # Gonçalves et al. 2012, MNRAS, 425, 2557; PNLF