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![]() |
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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