Open Access

Table A.1

Observed line parameters of molecular anions in interstellar clouds.

Species Transition Frequency (MHz) VLSR (km s−1) Δυ (km s−1) (mK) (mK km s−1) Telescope Reference

TMC-1 CP


C6H 4-3 11014.896 +5.80(2) 0.38(4) 25(3) 10.1(33) GBT McCarthy et al. (2006)
5-4 13768.614 +5.80(11) 0.44(7) 24(3) 11.2(43) GBT McCarthy et al. (2006)
10-9 27537.130 41.6(90)b,c Cordiner et al. (2013)
11-10 30290.813
12-11 33044.488 +5.78(1) 0.73(1) 22.3(23) 17.4(18) Yebes 40 m This work
13-12 35798.153 +5.78(1) 0.70(1) 20.9(22) 15.5(17) Yebes 40 m This work
14-13 38551.808 +5.78(1) 0.64(2) 18.9(20) 12.8(14) Yebes 40 m This work
15-14 41305.453 +5.79(2) 0.56(3) 17.2(19) 10.3(12) Yebes 40 m This work
16-15 44059.085 +5.79(2) 0.57(3) 12.8(15) 7.7(10) Yebes 40 m This work
17-16 46812.706 +5.81(2) 0.59(4) 9.6(13) 6.0(8) Yebes 40 m This work
18-17 49566.313 +5.84(3) 0.56(5) 5.4(10) 3.2(5) Yebes 40 m This work

C4H 2-1 18619.761 +5.70(5) 0.43(13) 1.0(3)b,d GBT Cordiner et al. (2013)
4-3 37239.410 +5.81(2) 0.71(2) 6.0(7) 4.5(6) Yebes 40 m This work
5-4 46549.156 +5.81(2) 0.55(3) 5.8(8) 3.4(4) Yebes 40 m This work

C8H 11-10 12833.460 +5.71(5) 0.36(4) 8(1) 3.1(10) GBT Brünken et al. (2007a)
12-11 14000.134 +5.86(5) 0.37(4) 7(1) 2.8(10) GBT Brünken et al. (2007a)
13-12 15166.806 +5.84(6) 0.45(4) 6(1) 2.9(10) GBT Brünken et al. (2007a)
16-15 18666.814 +5.80(7) 0.34(5) 10(2) 3.6(16) GBT Brünken et al. (2007a)
27-26 31500.029 +5.82(4) 0.63(10) 1.28(28) 0.86(20) Yebes 40 m This work
28-27 32666.670 +5.76(3) 0.76(6) 1.08(26) 0.87(15) Yebes 40 m This work
29-28 33833.309 +5.90(12) 0.68(17) 0.78(19) 0.56(18) Yebes 40 m This work
30-29 34999.944 +5.86(6) 0.60(10) 0.87(20) 0.56(14) Yebes 40 m This work
31-30 36166.576 +5.83(8) 0.32(20) 1.01(24) 0.34(10) Yebes 40 m This work
32-31 37333.205 +5.73(5) 0.66(11) 0.87(23) 0.61(16) Yebes 40 m This work
33-32 38499.831 +5.81(9) 0.82(17) 0.68(20) 0.60(18) Yebes 40 m This work
34-33 39666.453 +5.93(10) 0.40(12) 0.44(21) 0.19(7)e Yebes 40 m This work

C3N 4-3 38812.797 +5.78(1) 0.88(2) 4.2(2) 3.95) Yebes 40 m This work
5-4 48515.872 +5.86(2) 0.61(4) 6.3(9) 4.1(6) Yebes 40 m This work
8-7 77624.540 +5.88(3) 0.52(8) 7.1(17) 3.9(9) IRAM 30m This work
10-9 97029.687 +5.77(4) 0.38(6) 2.7(8) 1.1(3) IRAM 30m This work

C5N 12-11 33332.570 +5.83(1) 0.71(3) 6.5(7) 4.9(6) Yebes 40 m This work
13-12 36110.238 +5.80(1) 0.64(2) 6.1(7) 4.1(5) Yebes 40 m This work
14-13 38887.896 +5.81(1) 0.63(2) 6.5(8) 4.4(5) Yebes 40 m This work
15-14 41665.541 +5.82(2) 0.58(2) 5.7(7) 3.5(5) Yebes 40 m This work
16-15 44443.173 +5.79(2) 0.56(2) 4.7(6) 2.8(4) Yebes 40 m This work
17-16 47220.793 +5.81(2) 0.50(4) 3.6(6) 1.9(3) Yebes 40 m This work


Lupus-1A


C6H 7-6 19276.037 +5.046(8) 0.16(2) 85(8)b 14(2)b GBT Sakai et al. (2010)
8-7 22029.741 +5.034(10) 0.17(2) 94(11)b 15(3)b GBT Sakai et al. (2010)
12-11 33044.488 +5.06(2) 0.59(3) 30.1(37) 18.9(24) Yebes 40 m This work
13-12 35798.153 +5.08(2) 0.51(3) 32.9(40) 17.8(25) Yebes 40 m This work
14-13 38551.808 +5.05(2) 0.48(4) 30.4(38) 15.7(20) Yebes 40 m This work
15-14 41305.453 +5.09(3) 0.40(7) 32.7(42) 13.8(19) Yebes 40 m This work
16-15 44059.085 +5.07(3) 0.55(6) 24.2(35) 14.2(22) Yebes 40 m This work
17-16 46812.706 +5.10(6) 0.51(8) 17.1(33) 9.3(18) Yebes 40 m This work

C4H 4-3 37239.410 +5.078(13) 0.34(3) 59(5)b 19(5)b GBT Sakai et al. (2010)
4-3 37239.410 +5.04(4) 0.78(7) 7.4(14) 6.1(11) Yebes 40 m This work
5-4 46549.156 +5.05(9) 0.45(12) 9.8(27) 4.7(13) Yebes 40 m This work
9-8 83787.297 +5.23(6) 0.47(12) 10.4(31) 5.3(13) IRAM 30m This work

C8H 16-15 18666.814 0.09(3) 35(9) 4(1)b,c Sakai et al. (2010)
18-17 21000.145

C3N 4-3 38812.797 +5.16(15) 0.96(15) 2.8(10) 2.8(9) Yebes 40 m This work

C5N 12-11 33332.570 +5.11(7) 0.50(9) 8.4(16) 4.4(10) Yebes 40 m This work
13-12 36110.238 +5.11(7) 0.44(9) 6.5(13) 3.1(7) Yebes 40 m This work
14-13 38887.896 +5.13(7) 0.64(8) 8.0(17) 5.4(11) Yebes 40 m This work
15-14 41665.541 +5.14(9) 0.37(10) 9.2(19) 3.7(9) Yebes 40 m This work
16-15 44443.173 +5.09(10) 0.58(15) 6.1(18) 3.8(11) Yebes 40 m This work


L1527


C6H 7-6 19276.037 +5.93(9) 0.45(11) 14(3)b 7(2)b GBT Sakai et al. (2007)
8-7 22029.741 +5.89(3) 0.49(10) 26(4)b 18(4)b GBT Sakai et al. (2007)
12-11 33044.488 +5.90(5) 0.85(10) 9.6(14) 8.6(16) Yebes 40 m This work
13-12 35798.153 +5.85(4) 0.60(4) 11.4(20) 7.3(18) Yebes 40 m This work
14-13 38551.808 +5.84(3) 0.61(5) 12.0(18) 7.8(12) Yebes 40 m This work
15-14 41305.453 +5.90(3) 0.60(4) 16.4(25) 10.4(19) Yebes 40 m This work
16-15 44059.085 +5.90(3) 0.52(4) 14.5(23) 8.0(16) Yebes 40 m This work
17-16 46812.706 +5.83(5) 0.58(8) 11.1(23) 6.8(14) Yebes 40 m This work

C4H 4-3 37239.410 +5.92(12) 0.80(20) 3.2(10) 2.7(7) Yebes 40 m This work
5-4 46549.156 +6.05(15) 0.73(15) 4.9(19) 3.8(13) Yebes 40 m This work
9-8 83787.297 +5.80(3) 0.62(9) 13(2) 8(1) IRAM 30m Agúndez et al. (2008)
10-9 93096.550 +5.90(4) 0.59(9) 11(2) 7(1) IRAM 30m Agúndez et al. (2008)


L483


C6H 12-11 33044.488 +5.38(6) 0.66(8) 4.9(11) 3.4(8) Yebes 40 m This work
13-12 35798.153 +5.33(5) 0.70(7) 5.8(10) 4.3(8) Yebes 40 m This work
14-13 38551.808 +5.33(5) 0.78(7) 5.2(9) 4.3(9) Yebes 40 m This work
15-14 41305.453 +5.29(6) 0.46(9) 5.3(12) 2.6(6) Yebes 40 m This work
16-15 44059.085 +5.24(10) 0.75(12) 4.8(12) 3.8(10) Yebes 40 m This work
17-16 46812.706 +5.34(7) 0.63(9) 5.0(14) 3.4(9) Yebes 40 m This work

C4H 4-3 37239.410 +5.39(8) 0.73(12) 2.8(7) 2.2(5) Yebes 40 m This work
5-4 46549.156 +5.37(10) 0.44(15) 2.7(12) 1.3(5)e Yebes 40 m This work


L1495B


C6H 10-9 27537.130 9.6(20)b,c Cordiner et al. (2013)
11-10 30290.813
12-11 33044.488 +7.66(5) 0.80(7) 5.9(12) 5.0(9) Yebes 40 m This work
13-12 35798.153 +7.65(5) 0.50(8) 5.8(12) 3.1(6) Yebes 40 m This work
14-13 38551.808 +7.58(7) 0.39(10) 4.3(11) 1.8(4) Yebes 40 m This work
15-14 41305.453 +7.66(10) 0.36(14) 6.6(16) 2.6(6) Yebes 40 m This work
16-15 44059.085 +7.61(8) 0.49(12) 4.1(11) 2.1(6) Yebes 40 m This work


L1544


C6H 7-6 19276.037e 0.16(3) 16(2) 6.0(18) Gupta et al. (2009)
0.13(3) 26(2)
12-11 33044.488 +7.11(13) 0.67(28) 4.5(16) 3.2(14) Yebes 40 m This work
13-12 35798.153 +7.04(10) 0.48(16) 4.1(12) 2.1(9) Yebes 40 m This work
14-13 38551.808 +6.98(8) 0.50(13) 6.0(16) 3.2(12) Yebes 40 m This work
15-14 41305.453 +7.34(18) 0.76(36) 4.6(15) 3.7(16) Yebes 40 m This work


L1521F


C6H 7-6 19276.037e 0.18(3) 17(2) 7.0(17) Gupta et al. (2009)
0.35(9) 9(2)


L1251A


C6H 10-9 27537.130 6.5(17)b,c Cordiner et al. (2013)
11-10 30290.813


L1512


C6H 10-9 27537.130 4.3(8)b,c Cordiner et al. (2013)
11-10 30290.813


L1172


C6H 10-9 27537.130 6.7(15)b,c Cordiner et al. (2013)
11-10 30290.813


L1389


C6H 10-9 27537.130 5.9(14)b,c Cordiner et al. (2013)
11-10 30290.813


TMC-1 C


C6H 10-9 27537.130 13.6(25)b,c Cordiner et al. (2013)
11-10 30290.813

a Unless otherwise stated, the intensity scale is antenna temperature (). It can be converted to main beam brightness temperature (Tmb) by dividing by Beff/Feff, where Beff is the main beam efficiency and ieff is the telescope forward efficiency. For the Yebes 40 m telescope in the Q band Beff = 0.797exp[−(ν(GHz)/71.1)2] and Feff = 0.97 (https://rt40m.oan.es/rt40m_en.php), for the IRAM30m telescope Beff = 0.871 exp[−(ν(GHz)/359)2] and Feff = 0.95 (https://publicwiki.iram.es/Iram30mEfficiencies), and for the GBT telescope we adopt Feff = 1.0 and Beff = 1.32 × 0.71 exp[−(ν(GHz)/103.7)2] (Frayer et al. 2018). The error in includes the contributions from the Gaussian fit and from calibration (assumed to be 10%). b Intensity scale is Tmb. c Average of two lines. d Line neglected in the analysis. Intensity should be ~3 times larger to be consistent with the other lines.e Line detected marginally.

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