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Table A.1

Massive ATLASGAL clumps that have Jy fluxes and are located between 2 kpc and 5.5 kpc from the Sun.

ATLASGAL & common1 d Ref.2 Evolutionary ALMA Molecular
names [kpc] d stage3 [Jy] projects 4 complex5
G049.4888−0.3882 / W51-E / W51 Main 5.4±0.3 (1) IR-bright 113.2 (1), (8a,b), (9) (10), (11), (12) W51
G333.6036−0.2130 / G333.60 / IRAS 16183-4958 4.2±0.7 (2) IR-bright 97.4 (1) RCW106
G012.8057−0.1994 / G012.80 / W33-IRS3 2.4±0.2 (3) IR-bright 92.4 (1), (5a) W33
G351.7747−0.5369 / G351.77 / IRAS 17233-3606 2.0±0.7 (4) IR-bright 81.8 (1), (3), (13), (14) G353
G327.2921−0.5792 / G327.29 / RCW97 2.5 ±0.5 (2) IR-bright 71.2 (1), (15) G327
G353.4102−0.3611 /G353.41 / IRAS 17271-3439 2.0±0.7 (4) IR-bright 68.4 (1), (3) G353
G010.6237−0.3833 / G010.62 / W31 4.95 ±0.5 (5) IR-bright 54.9 (1), (5a), (14b) (16), (17) W31
G333.1341−0.4314/IRAS 16172-5028 4.2±0.7 (2) IR-bright 54.2 (2), (3), (4) RCW106
G338.9249+0.5539 / G338.92 3.9±1.0 (2) IR-quiet 53.3 (1), (2), (18)
G049.4897−0.3697 / W51-IRS2 / IRAS 19213+1424 5.4±0.3 (1) IR-bright 52.0 (1), (8a,b), (10) W51
G332.8262−0.5493 / IRAS 16164-5046 4.2±0.7 (2) IR-bright 51.4 (2), (5a), (3) RCW106
G348.7260−1.0391 /IRAS 17167-3854 3.4±0.3 (6) IR-bright 43.4 (2) RCW122
G030.8166−0.0561 /W43-MM1 5.5±0.4 (7) IR-quiet 42.3 (1), (19a,b) (20a,b), (21) W43
G328.8087+0.6328/IRAS 15520-5234 2.5±0.5 (2) IR-bright 40.6 G327
G333.2841−0.3868 4.2±0.7 (2) IR-bright 37.5 (2), (4) RCW106
G049.4908−0.3792 /W51-Main 5.4±0.3 (1) IR-bright 36.9 (1)in W51-E field W51
G337.9154−0.4773 / G337.92 / IRAS16274−4701 2.7±0.7 (4) IR-bright 36.6 (1), (5a), (5b), (6), G337
G301.1365−0.2256/IRAS 12326−6245 4.2±0.7 (2) IR-bright 34.5 (2), (5), (3)
G327.3005−0.5509 / IRAS 15492−5426 2.5±0.5 (2) IR-bright 32.3 G327
G337.4052−0.4024 / IRAS 16351−4722 2.7±0.7 (5) IR-bright 31.7 (2), (5b), (3), (6) G337
G008.6702−0.3557 / G008.67 3.4±0.3 (2) IR-quiet 30.6 (1), (5b), (22)
G322.1581+0.6354 / RCW92 3.2±1.1 (2) IR-bright 30.3
G329.0303−0.2022/IRAS 15566−5304 2.5±0.5 (2) IR-quiet 29.4 (3) G327
G330.8788−0.3681 / IRAS 16065−5158 4.2±0.7 (2) IR-quiet 28.1 RCW106
G019.6084−0.2346 /IRAS 18248−1158 3.6±0.8 (2) IR-bright 27.6 (7)
G326.6577+0.5941 / IRAS 15408−5356 / RCW95 2.5±0.5 (2) IR-bright 26.2 G327
G305.2083+0.2063 / IRAS 13079−6218 3.5±2.0 (8) IR-bright 26.1 (2), (3), (4)
G030.7016−0.0672 / W43−MM2 5.5±0.4 (7) IR-quiet 25.1 (1), (20c) W43

G328.2551−0.5321 /G328.25 2.5±0.5 (2) IR-quiet 15.0 (1), (23) G327
G030.7173−0.0822 / W43-MM3 5.5±0.4 (7) IR-bright 11.7 (1), (2), (20c) W43

1 ATLASGAL name (underlying their Galactic coordinates) from Csengeri et al. (2017) together with adopted name for ALMA-IMF (underlined names) as well as other most common names.

2 References for the distance to the Sun: (1) Sato et al. (2010); (2) Csengeri et al. (2017); (3) Immer et al. (2013); (4) This paper; (5) Sanna et al. (2014); (6) Reid et al. (2014); (7) Zhang et al. (2014); (8) Russeil (2003).

3 Evolutionary stage and 870 μm integrated fluxes, taken from Csengeri et al. (2017).

4 Observed as part of the: (1) ALMA-IMF Large Program #2017.1.01355.L, by Motte, Ginsburg, Louvet, Sanhueza et al. (B6+B3 mosaics); (2) Large Program #2019.1.00195.L (B6) by Molinari, Schilke et al.; (3) Program by Liu et al. #2019.1.00685.S (B3); (4) Program by Barnes et al. #2019.1.01031.S (B3, mosaic); (5) Programs by Leurini et al. a) #2016.1.01347.S, b) #2017.1.00377.S (B6+B3, mosaics); (6) Program by Hacar et al. #2018.1.00697.S (B3, mosaic); (7) Program by Se-Hyung et al. #2013.1.00266.S (B3); (8) Programs by Ginsburg et al. a) #2013.1.00308.S (B6, mosaic) and b) #2017.1.00293.S (B3); (9) Program by Kim et al. #2015.1.01571.S (B6); (10) Program by Goddi et al. #2015.1.01596.S (B6); (11) Program by Su et al. #2016.1.00268.S (B3); (12) Program by Rivilla et al. #2016.1.01071.S (B3); (13) Program by Beuther et al. #2015.1.00496.S (B6); (14) Program by Sanhueza et al. a) #2017.1.00237.S and b) #2016.1.01036.S (B6); (15) Program by Schilke et al. #2016.1.00168.S (B6, mosaic); (16) Program by Gerin et al. #2013.1.01194.S (B3); (17) Program by Zhang et al. #2015.1.00106.S (B6); (18) Program by Fuller et al. #2015.1.01312.S (B6); (19) Program by Motte et al. a) #2013.1.01365.S (B6, mosaic) and b) #2015.1.01273.S (B6, mosaic); (20) Program by Louvet et al. a) #2015.1.01020.S (B6), b) #2018.1.01787.S (B3) and c) #2017.1.00226; (21) Program by Kim et al. #2018.1.01288.S (B6); (22) Program by Shirley et al. #2017.1.01116.S (B3, B6); (23) Program by Csengeri et al. #2019.2.00093.S (B3).

5 Name of the molecular cloud complex hosting the ATLASGAL clump.

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