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--- molecules:extragalactic:formamid_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1
+++ molecules:extragalactic:formamid_extragalactic [2019/10/22 16:27] (current) – mueller
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 S. Muller, A. Beelen, J. H. Black, S. J. Curran, C. Horellou, S. Aalto, F. Combes, M. Guélin, and C. Henkel\\
 reported on\\
-**[[http://dx.doi.org/10.1051/0004-6361/201220613|A precise and accurate determination of the cosmic microwave background temperature at //z// = 0.89]]**\\
+**[[https://doi.org/10.1051/0004-6361/201220613|A precise and accurate determination of the cosmic microwave background temperature at //z// = 0.89]]**\\
 //Astron. Astrophys.// **551**, (2013) Art. No. A109.\\
 The famous, but unnamed foreground galaxy in direction of the quasar PKS 1830–211 was studied with the Australia Telecope Compact Array and the Plateau de Bure Interferometer. ATCA observations at 7 mm revealed 2 significant lines of formamide, 4<sub>04</sub> – 3<sub>03</sub> near 44.8 GHz (restfrequency near 84.5 GHz) and 4<sub>13</sub> – 3<sub>12</sub> near 46.6 GHz (restfrequency near 87.8 GHz). Even though rather few transitions have been observed, the detection is probably secure because of the limited line density.
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 Contributor(s): H. S. P. Müller; 04, 2013
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