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. Author manuscript; available in PMC: 2016 Mar 22.
Published in final edited form as: Mon Not R Astron Soc. 2016 Mar 11;456(4):4101–4110. doi: 10.1093/mnras/stv2866

Table 2.

Observed line parameters.

Source Molecule Transition Frequency (MHz) Eup (K) Aul (s−1) HPBW (″) BeffFeff VLSR (km s−1) Δv (km s−1) TAdv(Kkms1)
TMC-1 HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +5.72(5) 0.39(13) 0.006(2)
HCCCHO 51,5 – 40,4 107556.726 9.6 8.58 × 10−6 22.6 0.83 +5.86(4) 0.48(8) 0.007(1)
c-C3H2O 71,7 – 61,6 92517.434 17.2 8.11 × 10−5 26.3 0.85 +5.65(6) 0.43(13) 0.004(1)

B1-b HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +6.43(6) 0.60(12) 0.012(2)
c-C3H2O 71,6 – 61,5 103069.924 19.2 1.12 × 10−4 23.6 0.84 +6.49(4) 0.44(9) 0.006(1)

L483 HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +5.24(4) 0.34(12) 0.009(2)
c-C3H2O 71,6 – 61,5 103069.924 19.2 1.12 × 10−4 23.6 0.84 +5.27(3) 0.26(6) 0.008(2)

Lupus-1A HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +5.03(4) 0.38(10) 0.007(1)
c-C3H2O 71,6 – 61,5 103069.924 19.2 1.12 × 10−4 23.6 0.84 +4.98(4) 0.34(10) 0.005(1)

L1495B HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +7.60(4) 0.25(5) 0.005(1)

L1521F HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +6.38(6) 0.46(11) 0.005(1)

Serpens South 1a HCCCHO 90,9 – 80,8 83775.832 20.1 1.80 × 10−5 29.0 0.86 +7.51(5) 0.74(13) 0.020(3)

Numbers in parentheses are 1σ uncertainties in units of the last digits. Antenna temperature (TA) can be converted to main beam brightness temperature (TMB) by dividing by (Beff/Feff).