Hi, thanks for your question. The ls_dr10.apflux table does not have RA/Dec columns, so it cannot be used directly with our crossmatch service. However, it does include a column named ls_id, which you can use to join with other LS DR10 tables.
A recommended workflow would be:
Crossmatch your input table with ls_dr10.tractor to get the corresponding ls_id values.
Save the results to your MyDB (for example, as "my_ls_dr10_xmatch").
In a Jupyter notebook on our notebook server, run a query that joins your saved table with ls_dr10.apflux using ls_id to retrieve the desired aperture flux columns. For example:
SELECT X.ra, X.dec, X.ls_id, A.apflux_g_1, A.apflux_r_1
FROM mydb://my_ls_dr10_xmatch AS X
JOIN ls_dr10.apflux AS A ON X.ls_id = A.ls_id
We also have a notebook with similar examples here: https://github.com/astro-datalab/notebooks-latest/blob/master/04_HowTos/CrossmatchTables/Examples_using_pre_crossmatched_tables.ipynb