justinlittman
commented
5 years ago Only editors I'm finding are book editors. For example:
{
"UID": "WOS:000313272200020",
"static_data": {
"summary": {
"pub_info": {
"coverdate": 2012,
"vol": 1480,
"pubyear": 2012,
"sortdate": "2012-01-01",
"has_abstract": "Y",
"pubtype": "Book in series",
"page": {
"end": 128,
"begin": 123,
"page_count": 6,
"content": "123-128"
}
},
"names": {
"count": 7,
"name": [{
"seq_no": 1,
"role": "author",
"full_name": "Wise, John H.",
"reprint": "Y",
"addr_no": 1,
"last_name": "Wise",
"display_name": "Wise, John H.",
"wos_standard": "Wise, JH",
"daisng_id": 357368,
"first_name": "John H."
}, {
"seq_no": 2,
"role": "author",
"full_name": "Abel, Tom",
"addr_no": 2,
"last_name": "Abel",
"display_name": "Abel, Tom",
"wos_standard": "Abel, T",
"daisng_id": 155315,
"first_name": "Tom"
}, {
"seq_no": 3,
"orcid_id": "0000-0002-5294-0198",
"role": "author",
"full_name": "Turk, Matthew J.",
"addr_no": 3,
"last_name": "Turk",
"display_name": "Turk, Matthew J.",
"wos_standard": "Turk, MJ",
"daisng_id": 159039,
"first_name": "Matthew J."
}, {
"seq_no": 4,
"role": "author",
"full_name": "Norman, Michael L.",
"addr_no": 4,
"last_name": "Norman",
"display_name": "Norman, Michael L.",
"wos_standard": "Norman, ML",
"daisng_id": 26363,
"first_name": "Michael L."
}, {
"seq_no": 5,
"role": "author",
"full_name": "Smith, Britton D.",
"addr_no": 5,
"last_name": "Smith",
"display_name": "Smith, Britton D.",
"wos_standard": "Smith, BD",
"daisng_id": 1018500,
"first_name": "Britton D."
}, {
"seq_no": 6,
"role": "book_editor",
"full_name": "Umemura, M",
"last_name": "Umemura",
"display_name": "Umemura, M",
"wos_standard": "Umemura, M",
"first_name": "M"
}, {
"seq_no": 7,
"role": "book_editor",
"full_name": "Omukai, K",
"last_name": "Omukai",
"display_name": "Omukai, K",
"wos_standard": "Omukai, K",
"first_name": "K"
}]
},
"doctypes": {
"doctype": "Proceedings Paper",
"count": 1
},
"publishers": {
"publisher": {
"names": {
"count": 1,
"name": {
"seq_no": 1,
"role": "publisher",
"full_name": "AMER INST PHYSICS",
"addr_no": 1,
"display_name": "AMER INST PHYSICS"
}
},
"address_spec": {
"city": "MELVILLE",
"addr_no": 1,
"full_address": "2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA"
}
}
},
"EWUID": {
"WUID": {
"coll_id": "WOS"
},
"edition": {
"value": "WOS.ISTP"
}
},
"titles": {
"count": 7,
"title": [{
"type": "source",
"content": "FIRST STARS IV - FROM HAYASHI TO THE FUTURE"
}, {
"type": "series",
"content": "AIP Conference Proceedings"
}, {
"type": "source_abbrev",
"content": "AIP CONF PROC"
}, {
"type": "abbrev_11",
"content": "AIP CONF PR"
}, {
"type": "abbrev_29",
"content": "AIP CONF PROC"
}, {
"type": "item",
"content": "The Imprint of Pop III Stars on the First Galaxies"
}, {
"translated": "N",
"type": "book_series",
"content": "AIP Conference Proceedings"
}]
},
"conferences": {
"conference": {
"conf_dates": {
"conf_date": {
"conf_start": 20120521,
"conf_end": 20120525,
"content": "MAY 21-25, 2012"
},
"count": 1
},
"conf_id": 279963,
"sponsors": {
"sponsor": ["Univ Tsukuba, Ctr Computat Sci", "Kyoto Univ, Yukawa Inst Theoret Phys", "Univ Tokyo, Kavli Inst Phys & Math Universe", "Japan Soc Promot Sci"],
"count": 4
},
"conf_infos": {
"count": 1,
"conf_info": "Conference on FIRST STARS IV - From Hayashi to the Future, MAY 21-25, 2012, Kyoto, JAPAN"
},
"conf_locations": {
"count": 1,
"conf_location": {
"conf_state": "JAPAN",
"conf_city": "Kyoto"
}
},
"conf_titles": {
"count": 1,
"conf_title": "Conference on FIRST STARS IV - From Hayashi to the Future"
}
},
"count": 1
}
},
"item": {
"book_pages": 458,
"xsi:type": "itemType_wos",
"coll_id": "WOS",
"ids": {
"avail": "N",
"content": "BDH60"
},
"xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance",
"bib_pagecount": {
"type": "Book",
"content": 458
},
"keywords_plus": {
"count": 5,
"keyword": ["COSMOLOGICAL SIMULATIONS", "INTERGALACTIC MEDIUM", "STELLAR POPULATIONS", "ENRICHMENT", "CHEMISTRY"]
},
"book_notes": {
"book_note": "Figures",
"count": 1
},
"bib_id": "1480: 123-128 2012",
"book_desc": {
"bk_publisher": "AMER INST PHYSICS, 2 HUNTINGTON QUADRANGLE, STE 1NO1 D, MELVILLE, NY 11747-4501 USA",
"bk_binding": "P",
"bk_prepay": "Y"
}
},
"fullrecord_metadata": {
"addresses": {
"count": 5,
"address_name": [{
"names": {
"count": 1,
"name": {
"seq_no": 1,
"role": "author",
"full_name": "Wise, John H.",
"reprint": "Y",
"addr_no": 1,
"last_name": "Wise",
"display_name": "Wise, John H.",
"wos_standard": "Wise, JH",
"daisng_id": 357368,
"first_name": "John H."
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 30332
},
"country": "USA",
"city": "Atlanta",
"addr_no": 1,
"organizations": {
"organization": ["Georgia Inst Technol", {
"pref": "Y",
"content": "University System of Georgia"
}, {
"pref": "Y",
"content": "Georgia Institute of Technology"
}],
"count": 3
},
"full_address": "Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA",
"state": "GA",
"suborganizations": {
"count": 1,
"suborganization": "Ctr Relativist Astrophys"
}
}
}, {
"names": {
"count": 1,
"name": {
"seq_no": 2,
"role": "author",
"full_name": "Abel, Tom",
"addr_no": 2,
"last_name": "Abel",
"display_name": "Abel, Tom",
"wos_standard": "Abel, T",
"daisng_id": 155315,
"first_name": "Tom"
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 94025
},
"country": "USA",
"city": "Menlo Pk",
"addr_no": 2,
"organizations": {
"organization": ["Stanford Univ", {
"pref": "Y",
"content": "Stanford University"
}],
"count": 2
},
"full_address": "Stanford Univ, kavli Inst Partic Astrophy&Cosmol, Menlo Pk, CA 94025 USA",
"state": "CA",
"suborganizations": {
"count": 1,
"suborganization": "kavli Inst Partic Astrophy&Cosmol"
}
}
}, {
"names": {
"count": 1,
"name": {
"seq_no": 3,
"role": "author",
"full_name": "Turk, Matthew J.",
"addr_no": 3,
"last_name": "Turk",
"display_name": "Turk, Matthew J.",
"wos_standard": "Turk, MJ",
"daisng_id": 159039,
"first_name": "Matthew J."
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 10027
},
"country": "USA",
"city": "New York",
"addr_no": 3,
"organizations": {
"organization": ["Columbia Univ", {
"pref": "Y",
"content": "Columbia University"
}],
"count": 2
},
"full_address": "Columbia Univ, Dept Astron, New York, NY 10027 USA",
"state": "NY",
"suborganizations": {
"count": 1,
"suborganization": "Dept Astron"
}
}
}, {
"names": {
"count": 1,
"name": {
"seq_no": 4,
"role": "author",
"full_name": "Norman, Michael L.",
"addr_no": 4,
"last_name": "Norman",
"display_name": "Norman, Michael L.",
"wos_standard": "Norman, ML",
"daisng_id": 26363,
"first_name": "Michael L."
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 92093
},
"country": "USA",
"city": "La Jolla",
"addr_no": 4,
"organizations": {
"organization": ["Univ Calif San Diego", {
"pref": "Y",
"content": "University of California San Diego"
}, {
"pref": "Y",
"content": "University of California System"
}],
"count": 3
},
"full_address": "Univ Calif San Diego, Ctr Astrophy&Space Sci, La Jolla, CA 92093 USA",
"state": "CA",
"suborganizations": {
"count": 1,
"suborganization": "Ctr Astrophy&Space Sci"
}
}
}, {
"names": {
"count": 1,
"name": {
"seq_no": 5,
"role": "author",
"full_name": "Smith, Britton D.",
"addr_no": 5,
"last_name": "Smith",
"display_name": "Smith, Britton D.",
"wos_standard": "Smith, BD",
"daisng_id": 1018500,
"first_name": "Britton D."
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 48824
},
"country": "USA",
"city": "E Lansing",
"addr_no": 5,
"organizations": {
"organization": ["Michigan State Univ", {
"pref": "Y",
"content": "Michigan State University"
}],
"count": 2
},
"full_address": "Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA",
"state": "MI",
"suborganizations": {
"count": 1,
"suborganization": "Dept Phys & Astron"
}
}
}]
},
"category_info": {
"subheadings": {
"count": 1,
"subheading": "Physical Sciences"
},
"subjects": {
"subject": [{
"ascatype": "traditional",
"code": "BU",
"content": "Astronomy & Astrophysics"
}, {
"ascatype": "extended",
"content": "Astronomy & Astrophysics"
}],
"count": 2
},
"headings": {
"heading": "Science & Technology",
"count": 1
}
},
"normalized_languages": {
"count": 1,
"language": {
"type": "primary",
"content": "English"
}
},
"languages": {
"count": 1,
"language": {
"type": "primary",
"content": "English"
}
},
"keywords": {
"count": 4,
"keyword": ["cosmology", "hydrodynamics", "radiative transfer", "star formation"]
},
"refs": {
"count": 24
},
"reprint_addresses": {
"count": 1,
"address_name": {
"names": {
"count": 1,
"name": {
"seq_no": 1,
"role": "author",
"full_name": "Wise, John H.",
"reprint": "Y",
"addr_no": 1,
"last_name": "Wise",
"display_name": "Wise, John H.",
"wos_standard": "Wise, JH",
"first_name": "John H."
}
},
"address_spec": {
"zip": {
"location": "AP",
"content": 30332
},
"country": "USA",
"city": "Atlanta",
"addr_no": 1,
"organizations": {
"organization": ["Georgia Inst Technol", {
"pref": "Y",
"content": "University System of Georgia"
}, {
"pref": "Y",
"content": "Georgia Institute of Technology"
}],
"count": 3
},
"full_address": "Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA",
"state": "GA",
"suborganizations": {
"count": 1,
"suborganization": "Ctr Relativist Astrophys"
}
}
}
},
"abstracts": {
"count": 1,
"abstract": {
"abstract_text": {
"p": "Here we present three adaptive mesh refinement radiation hydrodynamics simulations that illustrate the impact of momentum transfer from ionising radiation to the absorbing gas on star formation in high-redshift dwarf galaxies. Momentum transfer is calculated by solving the radiative transfer equation with a ray tracing algorithm that is adaptive in spatial and angular coordinates. We find that momentum input partially affects star formation by increasing the turbulent support to a three-dimensional rms velocity equal to the circular velocity of early haloes. Compared to a calculation that neglects radiation pressure, the star formation rate is decreased by a factor of five to 1.8x10(-2) M-circle dot yr(-1) in a dwarf galaxy with a dark matter and stellar mass of 2.0x10(8)M(circle dot) and 4.5x10(5)M(circle dot), respectively, when radiation pressure is included. Its mean metallicity of 10(-2.1) Z(circle dot) is consistent with the observed dwarf galaxy luminosity-metallicity relation. In addition to photoheating in H II regions, radiation pressure further drives dense gas from star forming regions, so supernovae feedback occurs in a warmer and more diffuse medium, launching metal-rich outflows.",
"count": 1
}
}
},
"fund_ack": {
"grants": {
"count": 3,
"grant": [{
"grant_ids": {
"grant_id": "SMD-11-2258",
"count": 1
},
"grant_agency": "NASA/ NCCS"
}, {
"grant_ids": {
"grant_id": "NNX08AH26G",
"count": 1
},
"grant_agency": "NASA ATFP"
}, {
"grant_ids": {
"grant_id": ["AST-0807312", "AST-1109243"],
"count": 2
},
"grant_agency": "NSF"
}]
},
"fund_text": {
"p": "We thank the local and scientific organising committees for a wonderful conference. Computational resources were provided by NASA/ NCCS award SMD-11-2258 and a director's discretionary allocation on SDSC Trestles. This work was partially supported by NASA ATFP grant NNX08AH26G, NSF AST-0807312, and NSF AST-1109243. The majority of the analysis and plots were done with yt [ 24]."
}
},
"normalized_doctypes": {
"doctype": "Meeting",
"count": 1
}
},
"contributors": {
"contributor": {
"name": {
"seq_no": 1,
"orcid_id": "0000-0002-5294-0198",
"role": "researcher_id",
"full_name": "Turk, Matthew",
"last_name": "Turk",
"display_name": "Turk, Matthew",
"first_name": "Matthew"
}
},
"count": 1
}
},
"r_id_disclaimer": "ResearcherID data provided by Clarivate Analytics",
"dynamic_data": {
"citation_related": {
"tc_list": {
"silo_tc": {
"coll_id": "WOS",
"local_count": 1
}
}
},
"cluster_related": {
"identifiers": {
"identifier": [{
"type": "issn",
"value": "0094-243X"
}, {
"type": "eisbn",
"value": "978-0-7354-1092-3"
}, {
"type": "doi",
"value": "10.1063/1.4754341"
}]
}
}
}
}
Supersedes #26
Use the entity resolver service to determine if editors already exist as agents in RIALTO Core.
vivo:Positionentity (position could be something generic like "employee")vivo:Editorshipentity