The Measurement of Atomic Transition Probabilities of Metal Atoms and Ions of Astrophysical Interest
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Edward G. Schmidt', 'PO_EMAI': None, 'PO_PHON': None}
Atomic and ionic transition data are fundamental to much of                     astrophysical research.  For example, this data is crucial for                  computing stellar atmosphere models and for deriving stellar                    elemental abundances.  This data needs to be obtained experimen-                tally, which the Principal Investigator proposes to do.  There                  will be two emphases:  apply existing techniques to measuring                   lifetimes and branching ratios of atomic and ionic transitions                  and extend current techniques to measuring at shorter wavelengths               and on higher excitation and ionization states.
{'FirstName': 'James', 'LastName': 'Lawler', 'PI_MID_INIT': 'E', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'James E Lawler', 'EmailAddress': 'jelawler@wisc.edu', 'NSF_ID': '000394942', 'StartDate': '01/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of Wisconsin-Madison', 'CityName': 'MADISON', 'ZipCode': '537151218', 'PhoneNumber': '6082623822', 'StreetAddress': '21 North Park Street', 'StreetAddress2': 'Suite 6301', 'CountryName': 'United States', 'StateName': 'Wisconsin', 'StateCode': 'WI', 'CONGRESSDISTRICT': '02', 'CONGRESS_DISTRICT_ORG': 'WI02', 'ORG_DUNS_NUM': '161202122', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF WISCONSIN SYSTEM', 'ORG_PRNT_DUNS_NUM': '041188822'}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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