SUMMARY
The photometric data from the Sloan Digital Sky Survey (SDSS) is stored in the "PhotoObj" fits files, while the spectroscopic data is found in "SpecObjAll". To create photometric plots, users must match the object IDs from spectroscopic data (bestObjID) to the photometric objID. A new query can be run using the CAS tool to retrieve ugriz photometry by including a condition that links these IDs. For optimal results, users should consider the type of photometry needed, with Model magnitudes recommended for galaxy targets.
PREREQUISITES
- Familiarity with SDSS data structures, specifically spSpec and spAtlas files
- Understanding of SQL queries, particularly SELECT statements
- Knowledge of photometric measurement types: Petrosian, Model, Kron, and aperture
- Experience with CAS (Catalog Archive Server) for querying SDSS data
NEXT STEPS
- Learn how to construct SQL queries for SDSS data retrieval
- Research the differences between photometric measurement types in SDSS
- Explore the SDSS schema to understand data relationships between PhotoObj and SpecObjAll
- Investigate the use of extinction corrections in photometric data analysis
USEFUL FOR
Astronomers, data analysts, and researchers working with SDSS data who need to analyze and visualize photometric measurements alongside spectroscopic data.