Item talk:Q328926

{

 "DOI": {
   "doi": "10.5066/p9a03d91",
   "prefix": "10.5066",
   "suffix": "p9a03d91",
   "identifiers": [],
   "alternateIdentifiers": [],
   "creators": [
     {
       "name": "Croke, Mary R",
       "nameType": "Personal",
       "givenName": "Mary R",
       "familyName": "Croke",
       "affiliation": [],
       "nameIdentifiers": [
         {
           "schemeUri": "https://orcid.org",
           "nameIdentifier": "https://orcid.org/0000-0001-8965-9722",
           "nameIdentifierScheme": "ORCID"
         }
       ]
     },
     {
       "name": "Jubb, Aaron M",
       "nameType": "Personal",
       "givenName": "Aaron M",
       "familyName": "Jubb",
       "affiliation": [],
       "nameIdentifiers": [
         {
           "schemeUri": "https://orcid.org",
           "nameIdentifier": "https://orcid.org/0000-0001-6875-1079",
           "nameIdentifierScheme": "ORCID"
         }
       ]
     },
     {
       "name": "Hackley, Paul C",
       "nameType": "Personal",
       "givenName": "Paul C",
       "familyName": "Hackley",
       "affiliation": [],
       "nameIdentifiers": [
         {
           "schemeUri": "https://orcid.org",
           "nameIdentifier": "https://orcid.org/0000-0002-5957-2551",
           "nameIdentifierScheme": "ORCID"
         }
       ]
     },
     {
       "name": "Birdwell, Justin E",
       "nameType": "Personal",
       "givenName": "Justin E",
       "familyName": "Birdwell",
       "affiliation": [],
       "nameIdentifiers": [
         {
           "schemeUri": "https://orcid.org",
           "nameIdentifier": "https://orcid.org/0000-0001-8263-1452",
           "nameIdentifierScheme": "ORCID"
         }
       ]
     },
     {
       "name": "Hatcherian, Javin J",
       "nameType": "Personal",
       "givenName": "Javin J",
       "familyName": "Hatcherian",
       "affiliation": [],
       "nameIdentifiers": [
         {
           "schemeUri": "https://orcid.org",
           "nameIdentifier": "https://orcid.org/0000-0001-9151-6798",
           "nameIdentifierScheme": "ORCID"
         }
       ]
     },
     {
       "name": "Qu, Jing",
       "nameType": "Personal",
       "givenName": "Jing",
       "familyName": "Qu",
       "affiliation": [],
       "nameIdentifiers": []
     }
   ],
   "titles": [
     {
       "title": "Atomic Force Microscopy-based Infrared Spectroscopy Data within Immature Eagle Ford Shale at the Nanometer-scale"
     }
   ],
   "publisher": "U.S. Geological Survey",
   "container": {},
   "publicationYear": 2020,
   "subjects": [
     {
       "subject": "Energy Resources, Geochemistry"
     }
   ],
   "contributors": [],
   "dates": [
     {
       "date": "2020",
       "dateType": "Issued"
     }
   ],
   "language": null,
   "types": {
     "ris": "DATA",
     "bibtex": "misc",
     "citeproc": "dataset",
     "schemaOrg": "Dataset",
     "resourceType": "Dataset",
     "resourceTypeGeneral": "Dataset"
   },
   "relatedIdentifiers": [
     {
       "relationType": "IsCitedBy",
       "relatedIdentifier": "10.1016/j.coal.2020.103608",
       "relatedIdentifierType": "DOI"
     }
   ],
   "relatedItems": [],
   "sizes": [],
   "formats": [],
   "version": null,
   "rightsList": [],
   "descriptions": [
     {
       "description": "The nanoscale molecular composition of kerogen is a challenging parameter to characterize given the chemical and structural complexity exhibited by this important biopolymer. However, kerogen composition will strongly impact its reactivity and so is a critical parameter to understand petroleum generation processes during kerogen catagenesis. The recent advent of tip-enhanced analytical methods, such as atomic force microscopy-based infrared spectroscopy (AFM-IR), has allowed for the major compositional features of kerogen to be elucidated at spatial resolutions at or below 50 nm. Here we apply AFM-IR to examine inertinite, an important kerogen maceral type, from an immature Eagle Ford Shale sample. Our data show that the nanoscale molecular composition of the examined inertinite is: (i) less heterogeneous than other organic matter types from the Eagle Ford Shale and (ii) more hydrogen- and oxygen-rich than inertinite from the New Albany Shale at a similar stage of thermal maturity.",
       "descriptionType": "Abstract"
     }
   ],
   "geoLocations": [],
   "fundingReferences": [],
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