GLAST LAT ProjectGround Software Workshop, July 15-18, 2003 1 L1 Database Contents Seth Digel, for LAT FITS definition group: Masa Hirayama, Sandhi Bansal,

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Presentation transcript:

GLAST LAT ProjectGround Software Workshop, July 15-18, L1 Database Contents Seth Digel, for LAT FITS definition group: Masa Hirayama, Sandhi Bansal, Jerry Bonnell, and Guillaume Dubus HEPL/Stanford Univ. 16 July 2003

GLAST LAT ProjectGround Software Workshop, July 15-18, Outline Why have this talk? Contents of L1 event summaries What might we need to add What we might do without

GLAST LAT ProjectGround Software Workshop, July 15-18, Why have this talk? The L1 database is intended to contain the summary information for each event, what might be useful for high-level analysis The needs for the standard analysis environment are simple –Event number, time, energy, direction, zenith angle, classification flags For use outside the SAE, some additional quantities can be anticipated as being useful –This is kind of a slippery slope – intent is not to facilitate second guessing the reconstruction, for example Current set is kind of a grab bag of ideas that have been floated over the last 3 years

GLAST LAT ProjectGround Software Workshop, July 15-18, Current contents of the L1 data Names and comments extracted from June 27 version by the LAT FITS group, posted by Masa Hirayama Highlighted in red are the must-have quantities (for DC1 and afterward) Quality parameters are not defined, or their application in higher-level analysis

GLAST LAT ProjectGround Software Workshop, July 15-18, What’s missing and might be needed? Geomagnetic coordinates, McIlwain L, B Particle identification (gamma ray, electron, etc.) Event classification –Bill Atwood’s work is currently classifiying events based on CAL (No, Low, High), conversion location (Thin, Thick), and tracking (Vertex, Single Track). –These basic distinctions already multiply up to 12 event classifications Coordinates in other systems –Moon-centered, sun-centered, for example (or face question of how to analyze a moving source – solar system-type – in general) –l,b?

GLAST LAT ProjectGround Software Workshop, July 15-18, What might be needed? (2) Measured quantities and uncertainties –Incorporating uncertainties is certainly desirable, especially for export of the data outside of the SAE –However, characterizing the uncertainties short of providing the response functions is perhaps problematic – errors are not gaussian

GLAST LAT ProjectGround Software Workshop, July 15-18, What can we omit? Information about secondaries? Information for multi-gamma events? –Will these really be reconstructed? –Will these be common enough to worry about? Hits not reconstructed? –Are there better ways to warn that an event was particularly noisy?