PDS_VERSION_ID = PDS3 /* File Characteristics */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 50 FILE_RECORDS = 50 /* Data Object Pointers */ ^TABLE = "smasseig.tab" /* Identification Keywords */ DATA_SET_ID = "EAR-A-M3SPEC-3-RDR-SMASS-V1.0" PRODUCT_NAME = "SMASS PCA Eigenvectors Table" PRODUCT_ID = "SMASS-SMASSEIG-199604" INSTRUMENT_HOST_NAME = "MICHIGAN-DARTMOUTH-MIT OBSERVATORY" INSTRUMENT_NAME = "MARK III SPECTROGRAPH" TARGET_NAME = ASTEROID START_TIME = 1990 STOP_TIME = 1994 PRODUCT_CREATION_TIME = 1996-03-29 /* Peer Review Date */ RECORD_FORMAT = "(i5,2x,4(2x,f8.5))" /* Data Object Descriptions */ OBJECT = TABLE ROWS = 50 ROW_BYTES = 50 INTERCHANGE_FORMAT = ASCII COLUMNS = 5 DESCRIPTION = " ----------------------------------------------------------------------------- SMALL MAIN-BELT ASTEROID SPECTROSCOPIC SURVEY (SMASS) Principal component eigenvectors used in Xu et al. (1995), Icarus 115, 1-35, Table I and Figure 3. The principal components PC1 and PC2 for each asteroid are calculated from the observed reflectances (normalized to unity at 5500 A), at 50 equally spaced wavelengths from 4800 - 9700 A. At the ith wavelength: lambda(i) = Wavelength E1(i) = ith Eigenvector coefficient for PC1 E2(i) = ith Eigenvector coefficient for PC2 R(i) = Asteroid reflectance at lambda(i) (normalized to unity at 5500A) m(i) = mean value of R(i) for the entire set of asteroid spectra s(i) = standard deviation of R(i) for the entire set of asteroid spectra PC1 and PC2 are calculated as follows: 50 PC1 = SUM E1(i)*{[R(i)-m(i)]/s(i)} i=1 50 PC2 = SUM E2(i)*{[R(i)-m(i)]/s(i)} i=1 (where 'SUM' represents the standard mathematical summation notation) ----------------------------------------------------------------------------- " OBJECT = COLUMN COLUMN_NUMBER = 1 NAME = "WAVELENGTH" DESCRIPTION = "lambda(i); the ith wavelength where i is the record number." UNIT = ANGSTROM DATA_TYPE = ASCII_INTEGER START_BYTE = 1 BYTES = 5 FORMAT = I5 END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 2 NAME = "EIGENVECTOR ONE" DESCRIPTION = "E1(i); ith coefficient of the eigenvector for the first principal component, where i is the record number." DATA_TYPE = ASCII_REAL START_BYTE = 10 BYTES = 8 FORMAT = "F8.5" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 3 NAME = "EIGENVECTOR TWO" DESCRIPTION = "E2(i); ith coefficient of the eigenvector for the second principal component, where i is the record number." DATA_TYPE = ASCII_REAL START_BYTE = 20 BYTES = 8 FORMAT = "F8.5" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 4 NAME = "REFLECTANCE MEAN" DESCRIPTION = "m(i); mean value of R(i) for the entire set of asteroid spectra, where i is the record number. R(i) is the asteroid reflectance at lambda(i) normalized to unity at 5500A." DATA_TYPE = ASCII_REAL START_BYTE = 30 BYTES = 8 FORMAT = "F8.5" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 5 NAME = "REFLECTANCE STANDARD DEVIATION" DESCRIPTION = "s(i); standard deviation of R(i) for the entire set of asteroid spectra, where i is the record number. R(i) is the asteroid reflectance at lambda(i) normalized to unity at 5500A." DATA_TYPE = ASCII_REAL START_BYTE = 40 BYTES = 8 FORMAT = "F8.5" END_OBJECT = COLUMN END_OBJECT = TABLE END