ner_tags: O O O O O B-Model O O O O O O O O O O O B-Model O O O O O O O O O O O O O B-Model O O B-Citation I-Citation I-Citation I-Citation I-Citation O O O O O O O O B-Model O O O O O O O O O O O O O B-Model O O B-Citation I-Citation I-Citation I-Citation O O O O O O O O B-Model O O O O O O O O O O O B-Citation I-Citation O O O B-Model O O O O O O B-Survey O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O O B-Formula I-Formula I-Formula O B-Citation I-Citation I-Citation I-Citation O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-Model O O O O O O O O O O O O O B-Model O O O O O B-Survey O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O O B-Formula I-Formula I-Formula O B-Citation I-Citation I-Citation I-Citation O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-CelestialObjectRegion I-CelestialObjectRegion O O O O O O O O O O B-Model O O O O O O O O O O O O B-Model O O O O O B-Survey O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O B-Formula I-Formula I-Formula O O O B-Formula I-Formula I-Formula O B-Citation I-Citation I-Citation I-Citation O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-CelestialObjectRegion I-CelestialObjectRegion O O O O O O O O O O B-Model I-Model O O O O O O O O O O O O B-Model O O B-Citation I-Citation I-Citation I-Citation O O O O O O O O O B-Model O O O O O O O O O O O O O B-Model O O O O O O O O O O O O O O O O B-Model O O O O O O O O O O O O O O O O O O B-Model O O O O O O O O O O O O O O O
tokens: and best detections. Table D20 StackModelFitExp: Contains the Exponential Fit Parameters to Extended Sources Note. See the StackObjectThin table for a discussion of the primary, secondary, and best detections. Table D21 StackModelFitDeV: Contains the de Vaucouleurs ( 1948 ) Fit Parameters to Extended Sources Note. See the StackObjectThin table for a discussion of the primary, secondary, and best detections. Table D22 StackModelFitSer: Contains the Sérsic ( 1963 ) Fit Parameters to Extended Sources Note. See the StackObjectThin table for a discussion of the primary, secondary, and best detections (Sérsic 1963 ). Table D23 StackApFlxExGalUnc: Contains the Unconvolved Fluxes within the SDSS R3 ( r = 103), R4 ( r = 176), R5 ( r = 300), R6 ( r = 463), R7 ( r = 743), R8 ( r = 1142), R9 ( r = 1820), R10 ( r = 2820), and R11 ( r = 4421) Apertures (Stoughton et al. 2002 ) for Extended Sources Note. These measurements are only provided for objects in the extragalactic sky, i.e., they are not provided for objects in the Galactic plane because they are not useful in crowded areas. See the StackObjectThin table for a discussion of the primary, secondary, and best detections. Table D24 StackApFlxExGalCon6: Contains the Fluxes within the SDSS R3 ( r = 103), R4 ( r = 176), R5 ( r = 300), R6 ( r = 463), R7 ( r = 743), R8 ( r = 1142), R9 ( r = 1820), R10 ( r = 2820), and R11 ( r = 4421) Apertures (Stoughton et al. 2002 ) for Extended Sources after the Images Have Been Convolved to a Target of 6 Sky Pixels (15) Note. These measurements are only provided for objects in the extragalactic sky, i.e., they are not provided for objects in the Galactic plane because they are not useful in crowded areas. See the StackObjectThin table for a discussion of primary, secondary, and best detections. Table D25 StackApFlxExGalCon8: Contains the Fluxes within the SDSS R3 ( r = 103), R4 ( r = 176), R5 ( r = 300), R6 ( r = 463), R7 ( r = 743), R8 ( r = 1142), R9 ( r = 1820), R10 ( r = 2820), and R11 ( r = 4421) Apertures (Stoughton et al. 2002 ) for Extended Sources after the Images Have Been Convolved to a Target of 8 Sky Pixels (20) Note. These measurements are only provided for objects in the extragalactic sky, i.e., they are not provided for objects in the Galactic plane because they are not useful in crowded areas. See the StackObjectThin table for a discussion of the primary, secondary, and best detections. Table D26 StackPetrosian: Contains the Petrosian ( 1976 ) Magnitudes and Radii for Extended Sources Note. See the StackObjectThin table for a discussion of the primary, secondary, and best detections. Table D27 StackToImage: Contains the Mapping of Which Input Images Were Used to Construct a Particular Stack Table D28 StackToFrame: Contains the Mapping of Input Frames Used to Construct a Particular stack along with Processing Statistics Table D29 StackDetEffMeta: Contains the Detection Efficiency Information for a Given Stacked Image Note. Provides the number of