Recoverable Identifier
advisory
doi_compliance
recoverable_identifier
DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1175/1520-0450(1981) was visible in the surrounding text but could not be confirmed against doi.org as printed.
Paper page Integrity report arXiv Try DOI
Evidence text
Benzene on the giant planets. Icarus 154, 492– 500. Bierson, C., Zhang, X., 2020. Chemical cycling in the venusian atmosphere: a full photochemical model from the surface to 110 km. Journal of Geophysical Research: Planets 125, e2019JE006159. Bittner, J., Howard, J., 1981. Composition profiles and reaction mechanisms in a near-sooting premixed ben- zene/oxygen/argon flame, in: Symposium (Interna- tional) on Combustion, Elsevier. pp. 1105–1116. Bolovinos, A., Tsekeris, P., Philis, J., Pantos, E., An- dritsopoulos, G., 1984. Absolute vacuum ultravio- let absorption spectra of some gaseous azabenzenes. Journal of Molecular Spectroscopy 103, 240–256. Bonnet, J.Y ., Thissen, R., Frisari, M., Vuitton, V ., Quirico, É., Orthous-Daunay, F.R., Dutuit, O., Le Roy, L., Fray, N., Cottin, H., et al., 2013. Com- positional and structural investigation of hcn polymer through high resolution mass spectrometry. Interna- tional Journal of Mass Spectrometry 354, 193–203. Buck, A.L., 1981. New equations for comput- ing vapor pressure and enhancement factor. Journal of Applied Meteorology and Clima- tology 20, 1527 – 1532. doi:10.1175/1520- 0450(1981)020<1527:NEFCVP>2.0.CO;2. Burkholder, J., Sander, S., Abbatt, J., Barker, J., Cappa, C., Crounse, J., Dibble, T., Huie, R., Kolb, C., Kurylo, M., et al., 2020. Chemical kinetics and pho- tochemical data for use in atmospheric studies; eval- uation number 19. Technical Report. Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space . .
Evidence payload
{
"printed_excerpt": "Benzene on the giant planets. Icarus 154, 492\u2013 500. Bierson, C., Zhang, X., 2020. Chemical cycling in the venusian atmosphere: a full photochemical model from the surface to 110 km. Journal of Geophysical Research: Planets 125, e2019JE00615",
"reconstructed_doi": "10.1175/1520-0450(1981",
"ref_index": 4,
"resolved_title": null,
"verdict_class": "incontrovertible"
}