About the LSST science preparation seminar series: Each seminar will start with a very brief overview of the LSST science goals and planned data products that are relevant to each week’s topic, and then move into a hands-on demonstration of how to access and analyze simulated versions of those data products via the Rubin Science Platform (RSP). The focus of these seminars is on how to access Rubin data, rather than how to do the science. These seminars use the simulated Data Preview 0 datasets (dp0.lsst.io ).
All are welcome, with students particularly encouraged to attend. There will be time for Q&A.
Prior to attending it is recommended to get an account in the Rubin Science Platform: rsp.lsst.io .
Douglas and Christina, thank you both for this helpful talk (and for recording it)! Nicely presented and it addressed a lot of questions I’ve had. It sounds like the _gaap??Flux type calculations will be deprecated, so some of these questions may not get resolved until DP1 is out, but I’m wondering if you have some thoughts at this point. I get that _cModelFlux is best for individual fluxes and magnitudes of galaxies (whereas psf is best for stars), but should I be using the _ap??Flux measurements for color calculations and, if so, what determines the best aperture size to use? I’m sure the various size options are calculated for specific reasons. I liked Christine’s comparison plots, but I’m not sure how to determine which aperture is best. Also, for a flux density g_ap35Flux - is that 35 pixels?
For the best (r - i) color, should I set m_r - m_i = -2.5 * log(r_ap??Flux / i_ap??Flux)? When would I use the Kron flux?
Hi Bob! Good question! Although it is true that it appears that the _gaapOptimalFlux measurements will be deprecated, it is our understanding that the fixed aperture _gaap??Flux measurements are recommended for use for galaxy colors. Which _gaap??Flux to use depends a little bit on one’s science: smaller apertures for the central regions of galaxies, and larger apertures for colors that better approximate a total galaxy color. The number associated with an aperture flux (e.g., the “35” in g_ap35Flux is indeed the aperture size in pixels. Finally, it is our understanding that the Kron flux should basically never be used but has been included for completeness and for comparison with other surveys that utilize Kron fluxes.