Table A.1
Molecular cloud distances.
| Clouda | la | ba | Db |  |
 |
 |
Centerc | Extensionc | Noised | Signald | Cutoff | Ne | DSchlaflyf | Noteg |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (°) | (°) | (pc) | (mag) | (mag) | (mag) | (°, °) | (°, °) | (mJy sr−1) | (mJy sr−1) | (pc) | (pc) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
| MBM155 | 1.6 | −21.3 |  |
 |
 |
 |
(0.7, −20.8) | (5.0, 8.7) | 3.9 | 8.3 | 300 | 626 | Y | MBM154,153 |
| MBM35 | 6.6 | 38.1 |  |
 |
 |
 |
(5.4, 38.1) | (6.6, 8.2) | 4.2 | 8.2 | 300 | 617 |  |
MBM38,36,37,34, CB 63 |
| MBM145 | 8.5 | 21.9 |  |
 |
 |
 |
(11.3, 23.2) | (9.2, 7.1) | 10.8 | 16.4 | 300 | 677 |  |
MBM146,149,148,139,150 |
| MBM151 | 21.5 | 20.9 |  |
 |
 |
 |
(20.8, 21.8) | (6.4, 9.4) | 5.9 | 11.7 | 300 | 766 |  |
|
| MBM159 | 27.4 | −21.1 |  |
 |
 |
 |
(27.2, −21.3) | (6.5, 9.4) | 5.1 | 7.3 | 300 | 786 |  |
MBM158 |
| Aquila S | 38.0 | −17.0 |  |
 |
 |
 |
(38.0, −17.9) | (6.1, 7.7) | 5.0 | 8.9 | 300 | 732 | 114±18 | |
| MBM46 | 40.5 | −35.5 |  |
 |
 |
 |
(41.7, −35.4) | (8.6, 5.2) | 2.7 | 4.9 | 1000 | 5130 |  |
MBM47,48 |
| MBM160 | 44.0 | −23.3 |  |
 |
 |
 |
(45.9, −21.3) | (6.7, 10.2) | 3.4 | 5.0 | 1500 | 22411 | Y | |
| Hercules | 44.0 | 8.6 |  |
 |
 |
 |
(45.5, 9.1) | (6.0, 2.6) | 12.4 | 16.9 | 500 | 575 | 193±15 | |
| Pegasus | 92.2 | −34.7 |  |
 |
 |
 |
(91.6, −32.8) | (4.5, 6.8) | 2.5 | 5.4 | 500 | 1175 | 230±24 | MBM53 |
| MBM54 | 93.0 | −37.5 |  |
 |
 |
 |
(94.5, −37.8) | (5.8, 3.0) | 2.7 | 5.4 | 500 | 591 |  |
|
| Lacerta | 96.0 | −12.0 |  |
 |
 |
 |
(96.1, −12.3) | (3.1, 6.5) | 5.5 | 8.9 | 1000 | 2758 | 498±64 | |
| MBM56 | 103.1 | −26.1 |  |
 |
 |
 |
(102.5, −27.4) | (5.4, 5.2) | 2.9 | 4.5 | 1000 | 3122 |  |
G102-27 |
| MBM157 | 103.2 | 22.7 |  |
 |
 |
 |
(100.3, 23.8) | (9.5, 7.0) | 2.0 | 4.2 | 1000 | 8883 |  |
MBM156 |
| Cepheus(Far)h | 107.0 | 12.0 |  |
 |
 |
 |
(107.5, 13.1) | (8.7, 4.5) | 16.1 | 24.2 | 2000 | 9048 | 909±108 | |
| MBM162 | 111.7 | 20.1 |  |
 |
 |
 |
(111.7, 21.3) | (4.4, 5.1) | 4.8 | 9.1 | 1000 | 2523 |  |
|
| Cepheus | 113.0 | 17.0 |  |
 |
 |
 |
(113.8, 17.1) | (3.9, 6.1) | 8.4 | 14.5 | 1000 | 2347 | 351±50 | |
| MBM163 | 115.8 | 20.2 |  |
 |
 |
 |
(117.0, 21.8) | (7.2, 5.8) | 4.7 | 7.6 | 1000 | 4266 |  |
MBM161,166,165,164 |
| MBM2 | 117.4 | −52.3 |  |
 |
 |
 |
(111.5, −51.2) | (17.6, 7.2) | 2.8 | 4.2 | 1000 | 4791 |  |
|
| HSVMT 03 | 120.5 | 29.6 |  |
 |
 |
 |
(118.9, 29.0) | (5.7, 5.5) | 3.8 | 5.5 | 1000 | 2576 | Y | HSVMT 01 |
| HSVMT 5 | 121.1 | 21.8 |  |
 |
 |
 |
(119.4, 21.6) | (7.0, 4.7) | 4.6 | 7.5 | 1000 | 3549 | MBM166,165,164 | |
| HSVMT 08 | 122.5 | 29.0 |  |
 |
 |
 |
(122.3, 29.9) | (2.7, 3.3) | 4.8 | 7.0 | 1000 | 623 | Y | |
| HSVMT 12 | 125.2 | 32.5 |  |
 |
 |
 |
(127.7, 29.6) | (6.8, 9.1) | 1.4 | 4.1 | 1000 | 5868 | Y | HSVMT 14 |
| Polaris | 126.0 | 21.2 |  |
 |
 |
 |
(126.6, 20.7) | (4.7, 4.2) | 4.2 | 7.7 | 1000 | 2640 | 399±37 | |
| Ursa Major | 143.0 | 38.0 |  |
 |
 |
 |
(142.3, 36.1) | (4.9, 7.7) | 1.3 | 3.2 | 1000 | 2411 | 347±48 | MBM29,28,27,30 |
| MBM31 | 146.4 | 39.6 |  |
 |
 |
 |
(147.2, 39.2) | (4.0, 4.7) | 2.6 | 4.3 | 1000 | 1145 |  |
MBM32, HSVMT 24 |
| Cam | 147.5 | 17.8 |  |
 |
 |
 |
(146.6, 18.0) | (6.6, 4.1) | 4.5 | 6.4 | 500 | 995 | 263±88 | |
| MBM7 | 150.4 | −38.1 |  |
 |
 |
 |
(150.9, −39.6) | (14.0, 6.7) | 3.6 | 5.9 | 500 | 2080 |  |
MBM8,6, G154.7-39.8 |
| HSVMT 27 | 153.6 | 36.9 |  |
 |
 |
 |
(152.9, 37.4) | (6.0, 6.0) | 2.1 | 3.3 | 1000 | 2204 | Y | |
| MBM26 | 156.4 | 32.6 |  |
 |
 |
 |
(158.1, 33.8) | (6.1, 4.8) | 2.1 | 3.3 | 1000 | 1802 | Y | HSVMT 28 |
| California | 157.0 | −12.0 |  |
 |
 |
 |
(161.2, −8.2) | (8.2, 2.9) | 18.9 | 30.3 | 1000 | 1641 | 414±27 | |
| MBM11 | 158.0 | −35.1 |  |
 |
 |
 |
(159.3, −34.6) | (7.2, 7.4) | 4.5 | 8.9 | 500 | 1206 |  |
MBM13,12,14 |
| UT 8d | 158.2 | −26.3 |  |
 |
 |
 |
(158.1, −24.0) | (5.5, 7.8) | 7.1 | 13.0 | 1000 | 2628 | Y | MBM101,103,102,104 |
| Perseus | 160.0 | −20.0 |  |
 |
 |
 |
(159.8, −19.3) | (4.4, 4.9) | 10.2 | 25.1 | 1000 | 980 | 280±39 | MBM101,103,102,104, IC 348 |
| G161.9−43.3 | 161.9 | −43.3 |  |
 |
 |
 |
(164.0, −44.9) | (11.2, 6.3) | 4.0 | 6.7 | 1000 | 3314 | Y | |
| UT 4 | 165.3 | −26.4 |  |
 |
 |
 |
(164.0, −26.8) | (4.0, 2.0) | 6.2 | 9.0 | 1000 | 602 | Y | UT 3 |
| MBM17 | 167.5 | −26.6 |  |
 |
 |
 |
(169.3, −27.5) | (5.5, 4.0) | 7.1 | 9.7 | 1000 | 1855 |  |
UT 6, UT 5 |
| 3C 75.0 | 170.3 | −44.9 |  |
 |
 |
 |
(170.6, −45.8) | (9.0, 9.5) | 3.2 | 7.5 | 1000 | 3705 | Y | ir1 |
| MBM16 | 171.7 | −37.7 |  |
 |
 |
 |
(167.9, −36.9) | (10.6, 6.6) | 5.8 | 11.2 | 300 | 817 |  |
|
| Taurus | 175.3 | −16.2 |  |
 |
 |
 |
(170.2, −16.2) | (12.5, 6.7) | 9.1 | 19.1 | 300 | 828 | 138±15 | |
| MBM18 | 189.1 | −36.0 |  |
 |
 |
 |
(190.2, −37.1) | (8.5, 11.4) | 4.8 | 9.3 | 300 | 1268 |  |
3C 105.0 |
| Orion Lam | 195.5 | −13.7 |  |
 |
 |
 |
(196.0, −16.6) | (5.4, 8.7) | 5.4 | 13.2 | 1000 | 5616 | 418±34 | |
| Gemini | 200.0 | 12.0 |  |
 |
 |
 |
(198.4, 12.7) | (5.8, 5.9) | 3.2 | 5.2 | 1500 | 6351 | Y | |
| Mon OB1 | 201.0 | 1.0 |  |
 |
 |
 |
(201.4, 5.0) | (4.0, 10.6) | 4.8 | 18.0 | 1500 | 13448 | 886±13 | |
| NGC 2068 | 205.3 | −14.3 |  |
 |
 |
 |
(204.6, −14.1) | (2.5, 2.0) | 11.2 | 27.7 | 1000 | 403 | ||
| Rosette | 206.8 | −1.2 |  |
 |
 |
 |
(206.4, −2.3) | (4.7, 3.2) | 27.4 | 56.4 | 3000 | 6017 | 1483±80 | |
| L1641 | 212.5 | −19.0 |  |
 |
 |
 |
(213.5, −19.9) | (3.0, 3.2) | 7.5 | 30.0 | 1000 | 828 | ||
| Mon R2 | 215.3 | −12.9 |  |
 |
 |
 |
(214.0, −12.3) | (4.6, 4.4) | 13.7 | 26.2 | 1500 | 2204 | 933±125 | |
| ir2 | 235.0 | 37.0 |  |
 |
 |
 |
(236.4, 38.8) | (6.5, 5.7) | 1.7 | 3.1 | 1500 | 2877 | Y | 235.9+38.2 |
| Lupus | 342.5 | 9.0 |  |
 |
 |
 |
(342.3, 9.8) | (5.0, 6.5) | 14.7 | 25.7 | 500 | 1427 | ||
| Ophiuchus | 355.2 | 16.0 |  |
 |
 |
 |
(351.3, 16.5) | (7.3, 6.2) | 14.6 | 38.6 | 300 | 443 | 121±9 | |
| MBM128 | 355.6 | 20.6 |  |
 |
 |
 |
(357.0, 21.6) | (5.4, 5.9) | 11.6 | 21.8 | 300 | 395 |  |
MBM130,133,127, 126,125,129,131 |
Notes. (a) Molecular clouds (Col. 1) and their Galactic coordinates (Cols. 2 and 3), most of which are cataloged by Magnani et al. (1985, 1996) and Schlafly et al. (2014). (b)The mean and 95% HPD errors of the distance (Col. 4), the extinction AG dispersion of foreground stars (Col. 5), the extinction AG of background stars (Col. 6), and their dispersion (Col. 7). The distance systematic error is about 5%, which is not included in this table. (c) The center (Col. 8) and angular extinction (Col. 9) of region boxes in galactic coordinates, not their actual angular sizes. Those region boxes contain both on- and off-cloud Gaia DR2 stars. (d) The noise (Col. 10) and signal threshold (Col. 11) used to classified on- and off-molecular clouds. (e) The number of on-cloud Gaia stars (Col. 13) nearer than the distance cutoff (Col. 12). (f) Distances in Schlafly et al. (2014; Col. 14). Because distances of multiple positions are provided for molecular clouds in Table 1 of Schlafly et al. (2014), we averaged the distances of those molecular clouds weighted by their errors. Molecular clouds that not measured by Schlafly et al. (2014) or other reliable methods are marked with Y, 13 in total. (g) Other molecular clouds covered by the region box (Col. 15). (h)The far component towards the Cepheus molecular clouds.
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