2017
DOI: 10.1039/c7cc06083a
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Prebiotic synthesis of 2-deoxy-d-ribose from interstellar building blocks promoted by amino esters or amino nitriles

Abstract: COMMUNICATION

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Cited by 24 publications
(29 citation statements)
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“…1 H NMR (400 MHz, CDCl 3 ):  = 6.85 (1 H, s), 5.40-6.10 (1 H, m), 4.35-4.15 (1 H, m), 3.55-3.25 (2 H, m), 2.40-1.80 (4 H, m), 1.45 (9 H, s). HRMS (ESI): m/z [M + Na] + calcd for C 10 H 18 N 2 O 3 Na: 237.1210; found: 237.1209.Spectroscopic data are in agreement with the literature 8.…”
supporting
confidence: 85%
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“…1 H NMR (400 MHz, CDCl 3 ):  = 6.85 (1 H, s), 5.40-6.10 (1 H, m), 4.35-4.15 (1 H, m), 3.55-3.25 (2 H, m), 2.40-1.80 (4 H, m), 1.45 (9 H, s). HRMS (ESI): m/z [M + Na] + calcd for C 10 H 18 N 2 O 3 Na: 237.1210; found: 237.1209.Spectroscopic data are in agreement with the literature 8.…”
supporting
confidence: 85%
“…N. Vagkidis et al NMR (400 MHz, CDCl 3 ):  = 121.1, 49.7, 32.8, 18.8, 17.5. HRMS (ESI): m/z [M + H] + calcd for C 5 H 11 N 2 : 99.0917; found: 99.0919.Spectroscopic data are identical to that reported in the literature 8.…”
supporting
confidence: 72%
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“…Likewise, prebiotic routes to ribose involving borate minerals are proposed (Ricardo et al, 2004; Kim et al, 2011; Furukawa and Kakegawa, 2017). Also, the prebiotic synthesis of enantiomeric enriched carbohydrates (Breslow et al, 2013) and 2-deoxy ribose are reported (Steer et al, 2017).…”
Section: Introductionmentioning
confidence: 99%