| 22 | | The ForcedMeanObjectView only has fluxes. Since this was my first set of queries in awhile I decided not to convert the fluxes to magnitudes in the query. I simply grabbed the objects and ran the results through |
| 23 | | various iterations of a [http://www.star.bristol.ac.uk/~mbt/stilts/ STILTS] program to convert to magnitudes.at I used this [wiki:forcedFluxToMagsExaample perl script] to facitiate the conversions |
| | 22 | The !ForcedMeanObjectView only has fluxes. Since this was my first set of queries in awhile I decided not to convert the fluxes to magnitudes in the query. I simply grabbed the objects and ran the results through |
| | 23 | various iterations of a [http://www.star.bristol.ac.uk/~mbt/stilts/ STILTS] program to convert to magnitudes.at I used this [wiki:forcedFluxToMagsExaample perl script] to facitiate the conversions. Adding |
| | 24 | entries like |
| | 25 | {{{ |
| | 26 | 8.9-2.5*log10(gFPSFFlux) |
| | 27 | }}} |
| | 28 | to the list of columns in the query would allow us to avoid the stilts step. However the database is going to be busy and keeping the math done there to a minimum seems like a reasonable thing to do. |
| | 29 | |
| | 30 | |