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Table A.1.

Literature distances.

ID Distance Target Description Ref.
(pc)
O-001 9490 NGC 3603 Gaia DR2 parallax, no covariance term C18
7600 NGC 3603 Visible spectro-photometry M08
6900 NGC 3603 Visible CMD S04
7900 H II gas Kinematic distance R03
7700 H II gas Kinematic distance N02
7200 NGC 3603 Visible CMD S01
6300 NGC 3603 Visible CMD P00a
6100 H II gas Kinematic distance d99
10 100 NGC 3603 Visible spectro-photometry C98
7200 NGC 3603 Visible CMD M89
8600 H II gas Kinematic distance S83a
7000 NGC 3603 Visible spectro-photometry M83
5300 NGC 3603 Visible CMD M82
7200 H II gas Kinematic distance v78
8100 NGC 3603 Visible CMD M74
8400 H II gas Kinematic distance G72
5720 NGC 3603 Visible CMD B71
3500 NGC 3603 Visible CMD S65
O-002 + O-003 2500 Molecular clouds Gaia DR2 parallax Z20
2400 Car OB1 Gaia DR2 parallax L19
2640 Trumpler 14 Gaia DR2 parallax K19
2610 Trumpler 16 Gaia DR2 parallax K19
2680 Trumpler 14 Gaia DR2 parallax S19
2550 Trumpler 16 Gaia DR2 parallax S19
O-002 + O-003 2690 Car OB1 Gaia DR2 parallax B18
(continued) 305 Trumpler 14 Gaia DR2 parallax D18
2600 Trumpler 16 Gaia DR2 parallax D18
2414 Trumpler 14 Gaia DR2 parallax, no covariance term C18
2395 Trumpler 16 Gaia DR2 parallax, no covariance term C18
2900 Trumpler 14 + Trumpler 16 Visible + NIR CMD H12
4200 Trumpler 16 Ca II ISM lines M09a
2350 η Car Geometric distance from Homunculus expansion S06
2500 Trumpler 14 Visible CMD C04a
4000 Trumpler 16 Visible CMD C04a
2800 Trumpler 14 Visible + NIR CMD T03
2500 Trumpler 16 Visible + NIR CMD T03
2580 Car OB1 Statistical parallaxes R99
2800 Car OB1 Visible spectro-photometry with R5495 = 3.0 W95
2250 Car OB1 Visible spectro-photometry with R5495 = 4.0 W95
3610 Trumpler 14 Visible spectro-photometry M93
3150 Trumpler 16 Visible spectro-photometry M93
3960 Trumpler 14 Visible spectro-photometry M88
2400 Car OB1 Visible + NIR CMD T88
2750 Trumpler 14 Visible CMD F83
2700 H II gas Kinematic distance S83a
2800 Trumpler 16 Visible spectro-photometry W82
2800 Car OB1 Visible CMD with R5495 = 3.3 T80
2350 Car OB1 Visible CMD with R5495 = 4.0 T80
3600 Trumpler 14 Visible spectro-photometry H78
2690 Trumpler 16 Visible spectro-photometry H78
2400 Car OB1 Visible CMD F78
3500 Trumpler 14 Visible spectro-photometry W73a
2600 Trumpler 16 Visible spectro-photometry W73a
3390 Trumpler 14 + Trumpler 16 Visible CMD with R5495 = 3.0 F73
2650 Trumpler 14 + Trumpler 16 Visible CMD with R5495 = 4.0 F73
1650 Trumpler 14 Visible CMD B71
2950 Trumpler 16 Visible CMD B71
2000 Trumpler 14 Visible CMD T71
2500 Trumpler 16 Visible CMD T71
O-004 4400 Westerlund 2 Gaia DR2 parallax B18
4208 Westerlund 2 Gaia DR2 parallax, no covariance term C18
4000 Westerlund 2 Visible CMD Z15
6000 Westerlund 2 Visible CMD H15
6500 Molecular clouds Kinematic distance B13
4469 Westerlund 2 Visible + NIR CMD K13
2850 Westerlund 2 Visible spectro-photometry C13
4160 Westerlund 2 Visible CMD V13
6698 Westerlund 2 Visible spectro-photometry K12
8000 Three EBs Spectroscopic eclipsing binaries R11
5400 Molecular clouds Kinematic distance F09
6000 Molecular clouds Kinematic distance D07
2800 Westerlund 2 NIR CMD A07
6400 Westerlund 2 Visible CMD C04b
5700 Westerlund 2 Visible CMD P98
7900 Westerlund 2 Visible CMD M91a
5100 H II gas Kinematic distance S83a
5000 Westerlund 2 Visible CMD M75
4680 H II gas Kinematic distance G73
6000 Westerlund 2 Association with spiral arm W61
O-005 1770 NGC 6357 Gaia DR2 parallax R20
1790 Pismis 24 Gaia DR2 parallax K19
1780 NGC 6357 Gaia DR2 parallax B18
1678 NGC 6357 Gaia DR2 parallax, no covariance term C18
2460 Pismis 24 Visible spectro-photometry R17
1780 NGC 6357 NIR CMD L14
1900 NGC 6357 Visible + NIR CMD R12a
1700 Pismis 24 Visible + NIR CMD F12
1700 Pismis 24 Visible + NIR CMD G11
2500 Pismis 24 Visible spectro-photometry M01
1200 H II gas Kinematic distance S83a
1740 NGC 6357 + NGC 6334 Visible CMD N78
1580 NGC 6357 Visible spectro-photometry J73
770 H II gas Kinematic distance G73
1000 H II gas Kinematic distance W70
920 H II gas Kinematic distance D67
O-006 7000 H II gas Kinematic distance M17a
8000 H II gas Kinematic distance G00
6000 H II gas Kinematic distance A89
9100 H II gas Kinematic distance C87
O-007 + O-008 1600 Cyg OB2 Gaia DR2 parallax L19
1760 Cyg OB2 Gaia DR2 parallax, foreground group at 1350 pc B19a
1330 Four EBs Spectroscopic eclipsing binaries K15
1400 Four masers VLBI parallaxes R12b
1220 Cyg OB2 Visible spectro-photometry H03
1800 Bica 1 + 2 NIR CMD B03
1740 Cyg OB2 Visible spectro-photometry M91b
1700 Cyg OB2 Visible + NIR CMD T91
1790 Cyg OB2 Visible spectro-photometry H78
1800 Cyg OB2 Visible spectro-photometry W73b
2100 Cyg OB2 Visible spectro-photometry R66
1500 Cyg OB2 Visible spectro-photometry J54
O-009 1500 Molecular clouds Gaia DR2 parallax Z20
1680 M 17 Gaia DR2 parallax K19
1820 M 17 Gaia DR2 parallax B18
2390 H II gas Kinematic distance W18
2040 One maser VLBI parallax C16
1308 M 17 Visible + NIR CMD K13
1980 One maser VLBI parallax X11
2100 M 17 Visible + NIR spectro-photometry H08
1600 M 17 Luminosity budget P07
14 550 H II gas Kinematic distance Q06
2400 H II gas Kinematic distance R03
1600 M 17 Visible + NIR spectro-photometry N01
1300 M 17 Visible + NIR spectro-photometry H97
2200 Molecular clouds Kinematic distance S89a
2200 Molecular clouds Kinematic distance F84
2200 Molecular clouds Kinematic distance S84
2400 H II gas Kinematic distance S83a
2200 M 17 Visible CMD C80
1300 M 17 Visible CMD O76
1780 M 17 Visible spectro-photometry J73
2200 H II gas Kinematic distance G73
2460 H II gas Kinematic distance G70
2250 H II gas Kinematic distance D67
O-010 1046 Southern molecular cloud Gaia DR2 parallax Z20
1190 NGC 6193 Gaia DR2 parallax, no covariance term C18
1096 HD 150 136 Spectroastrometric orbit M18
1380 NGC 6193 Visible + NIR CMD B11a
1410 NGC 6193 Visible CMD V92
1340 Ara OB1 Visible spectro-photometry F87
1460 Ara OB1a Visible spectro-photometry H78
1320 Ara OB1 Visible CMD H77
1360 NGC 6193 Visible CMD M73b
1390 NGC 6193 Visible CMD B71
1880 H II gas Kinematic distance G70
1400 Ara OB1 Visible CMD W63
O-011 3016 Berkeley 90 Gaia DR2 parallax, no covariance term C18
3500 Berkeley 90 Visible CMD M17b
2670 Berkeley 90 CHORIZOS analysis of LS III +46 11 and LS III +46 12 M15
2430 Berkeley 90 NIR CMD T08
1500 LS III +46 11 Visible spectro-photometry M97
3000 Molecular clouds Kinematic distance F84
2320 LS III +46 12 Visible spectro-photometry M73a
O-012 5050 Haffner 19 Gaia DR2 parallax, no covariance term C18
4673 Haffner 18 Gaia DR2 parallax, no covariance term C18
4810 Two EBs Spectroscopic eclipsing binaries L17
5700 Haffner 19 Visible + NIR CMD Y15
11 200 Haffner 18 Visible + NIR CMD Y15
1313 Villafranca O-012 Visible + NIR CMD K13
5300 H II gas Kinematic distance B11b
5400 H II gas Kinematic distance Q06
6400 Haffner 19 Visible CMD G06
5900 Haffner 18 Visible CMD G06
4800 Haffner 19 Visible CMD M02
4090 Haffner 19 Statistical parallaxes R99
4570 Haffner 18 Statistical parallaxes R99
4100 Molecular clouds Kinematic distance F84
3900 H II gas Kinematic distance S83a
4200 H II gas Kinematic distance P76
6900 Villafranca O-012 Visible CMD F74
3510 H II gas Kinematic distance G73
2500 Villafranca O-012 Visible CMD B71
3830 H II gas Kinematic distance G70
3370 Villafranca O-012 Visible CMD L66
O-013 4880 H II gas Kinematic distance W18
2700 Villafranca O-013 NIR spectro-photometry P10
2650 Two masers VLBI parallaxes M09b
2270 Villafranca O-013 Visible spectro-photometry R07
6400 H II gas Kinematic distance Q06
2200 Villafranca O-013 NIR CMD M86
3700 H II gas Kinematic distance M86
2800 Molecular clouds Kinematic distance F84
2800 Two stars Visible spectro-photometry C78
4750 H II gas Kinematic distance G73
4230 H II gas Kinematic distance G70
O-014 800 Molecular clouds Gaia DR2 parallax Z20
858 Pelican nebula stars Gaia DR2 parallax B19b
605 Molecular clouds Visible CMD D17
700 North America nebula Kinematic distance C07
560 Molecular clouds Visible CMD L06
610 Bajamar star Visible + NIR spectro-photometry C05
600 Molecular clouds Visible CMD L02
485 Molecular clouds Star counts C02
550 Molecular clouds Visible spectro-photometry S93
800 Molecular clouds Kinematic distance S89a
550 Molecular clouds Visible CMD S89b
1000 Molecular clouds Kinematic distance S84
800 Molecular clouds Kinematic distance F84
970 Molecular clouds Star counts A81
150 2MASS J20535282+4424015 Stellar parameters estimation N80
1200 HD 199 579 Visible spectro-photometry M68
1980 H II gas Kinematic distance D67
1130 HD 199 579 Visible spectro-photometry B63
500 Molecular clouds Visible CMD H58
910 HD 199 579 Visible spectro-photometry S52
O-015 1019 Collinder 419 Gaia DR2 parallax, no covariance term C18
741 Collinder 419 Visible + NIR CMD R10
1400 Collinder 419 Visible CMD H87
O-016 750 Molecular clouds Gaia DR2 parallax Z20
738 NGC 2244 Gaia DR2 parallax, no covariance term K19
723 NGC 2244 Gaia DR2 parallax C18
738 Two masers VLBI parallaxes K14
913 NGC 2244 v sin i and rotation periods B09
759 NGC 2244 Visible CMD P00b
720 NGC 2244 Statistical parallaxes R99
764 NGC 2244 Visible CMD S97
910 NGC 2244 Visible + NIR CMD N93
700 NGC 2244 Visible CMD F91
800 Molecular clouds Kinematic distance S89a
950 NGC 2244 Visible spectro-photometry P87
800 Molecular clouds Kinematic distance S84
800 Molecular clouds Kinematic distance F84
798 NGC 2244 Visible CMD S83b
875 NGC 2244 Visible CMD M80
715 NGC 2244 Visible CMD B71
715 NGC 2244 Visible spectro-photometry B63
800 NGC 2244 Visible spectro-photometry W56

Notes. The specific target and a brief description of the method is given. Note that “spectro-photometry” indicates a combination of spectroscopic and photometric methods. For simplicity, random and systematic uncertainties have been combined.

References. A81: Armandroff & Herbst (1981), A89: Avedisova & Palous (1989), A07: Ascenso et al. (2007b), B63: Becker & Fenkart (1963), B71: Becker & Fenkart (1971), B03: Bica et al. (2003), B09: Baxter et al. (2009), B11a: Baume et al. (2011), B11b: Balser et al. (2011), B13: Benaglia et al. (2013), B18: Binder & Povich (2018), B19a: Berlanas et al. (2019), B19b: Bhardwaj et al. (2019), C05: Comerón & Pasquali (2005), C78: Crampton et al. (1978), C80: Chini et al. (1980), C87: Caswell & Haynes (1987), C98: Crowther & Dessart (1998), C02: Cambrésy et al. (2002), C04a: Carraro et al. (2004), C04b: Carraro & Munari (2004), C07: Cersosimo et al. (2007), C13: Carraro et al. (2013), C16: Chibueze et al. (2016), C18: Cantat-Gaudin et al. (2018), D67: Dieter (1967), d99: de Pree et al. (1999), D07: Dame (2007), D17: Damiani et al. (2017b), D18: Davidson et al. (2018), F73: Feinstein et al. (1973), F74: Fitzgerald & Moffat (1974), F78: Forte (1978), F83: Feinstein (1983), F84: Fich & Blitz (1984), F87: Fitzgerald (1987), F91: Feldbrugge & van Genderen (1991), F09: Furukawa et al. (2009), F12: Fang et al. (2012), G70: Georgelin & Georgelin (1970), G72: Goss et al. (1972), G73: Georgelin et al. (1973), G00: Georgelin et al. (2000), G06: Gamen et al. (2006), G11: Gvaramadze et al. (2011), H58: Herbig (1958), H77: Herbst & Havlen (1977), H78: Humphreys (1978), H87: Hron (1987), H97: Hanson et al. (1997), H03: Hanson (2003), H08: Hoffmeister et al. (2008), H12: Hur et al. (2012), H15: Hur et al. (2015), J54: Johnson & Morgan (1954), J73: Johnson (1973), K12: Kaltcheva & Golev (2012), K13: Kharchenko et al. (2013), K14: Kamezaki et al. (2014), K15: Kiminki et al. (2015), K19: Kuhn et al. (2019), L66: Lodén (1966), L02: Laugalys & Straižys (2002), L06: Laugalys et al. (2006), L14: Lima et al. (2014), L17: Lorenzo et al. (2017), L19: Lim et al. (2019), M68: Miller (1968), M73a: Mayer & Macák (1973), M73b: Moffat & Vogt (1973), M74: Moffat (1974), M75: Moffat & Vogt (1975), M80: Mendoza V. & Gómez (1980), M82: Melnick & Grosbol (1982), M83: Moffat (1983), M86: Moreno & Chavarría-K. (1986), M88: Morrell et al. (1988), M89: Melnick et al. (1989), M91a: Moffat et al. (1991), M91b: Massey & Thompson (1991), M93: Massey & Johnson (1993), M97: Motch et al. (1997), M01: Massey et al. (2001), M02: Moreno-Corral et al. (2002), M08: Melena et al. (2008), M09a: Megier et al. (2009), M09b: Moscadelli et al. (2009), M15: Maíz Apellániz et al. (2015a), M17a: Mohr-Smith et al. (2017), M17b: Marco & Negueruela (2017), M18: Mahy et al. (2018), N78: Neckel (1978), N80: Neckel et al. (1980), N01: Nielbock et al. (2001), N02: Nürnberger et al. (2002), N93: Neri et al. (1993), O76: Ogura & Ishida (1976), P76: Pišmiš & Moreno (1976), P87: Pérez et al. (1987), P98: Piatti et al. (1998), P00a: Pandey et al. (2000), P00b: Park et al. (2000), P07: Povich et al. (2007), P10: Puga et al. (2010), Q06: Quireza et al. (2006), R66: Reddish et al. (1966), R99: Rastorguev et al. (1999), R03: Russeil (2003), R07: Russeil et al. (2007), R10: Roberts et al. (2010), R11: Rauw et al. (2011), R12a: Russeil et al. (2012), R12b: Rygl et al. (2012), R17: Russeil et al. (2017), R20: Ramírez-Tannus et al. (2020), S52: Sharpless & Osterbrock (1952), S65: Sher (1965), S83a: Shaver et al. (1983), S83b: Sagar & Joshi (1983), S84: Stark (1984), S89a: Stark & Brand (1989), S89b: Straizys et al. (1989), S93: Straizys et al. (1993), S97: Sung et al. (1997), S01: Sagar et al. (2001), S04: Sung & Bessell (2004), S06: Smith (2006b), S19: Shull & Danforth (2019), T71: Thé & Vleeming (1971), T80: Thé et al. (1980), T88: Tapia et al. (1988), T91: Torres-Dodgen et al. (1991), T03: Tapia et al. (2003), T08: Tadross (2008), v78: van den Bergh (1978), V92: Vazquez & Feinstein (1992), V13: Vargas Álvarez et al. (2013), W56: Walker (1956), W61: Westerlund (1961), W63: Whiteoak (1963), W70: Wilson et al. (1970), W73a: Walborn (1973b), W73b: Walborn (1973c), W82: Walborn (1982b), W95: Walborn (1995), W18: Wenger et al. (2018), X11: Xu et al. (2011), Y15: Yadav et al. (2015), Z15: Zeidler et al. (2015), Z20: Zucker et al. (2020).

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