Table 2.

Description of the spectroscopic samples from the cross-match between S-PLUS DR2, SDSS DR14Q (quasars), SDSS DR16 (stars and galaxies) and AllWISE catalogues. Selection criteria are |$\texttt {zWarning}=0$| for galaxies, and r > 13 for stars. For all classes, the criteria are |$\texttt {PhotoFlag}_r=0$| and an upper limit of 22 magnitudes in r. After the selection criteria, we applied a 4-sigma clipping of the difference between r magnitudes from SDSS and S-PLUS.

Total matchesNumber of lost objects from criteriaNumber of lost objects from 4-sigma clippingwith_WISE sampleno_WISE sampleFinal sample
QSO28 2759 2176915 5383 45118 989
STAR78 21722 4641 70239 59514 45654 051
GALAXY154 52987 6695160 0595 55365 612
Total matchesNumber of lost objects from criteriaNumber of lost objects from 4-sigma clippingwith_WISE sampleno_WISE sampleFinal sample
QSO28 2759 2176915 5383 45118 989
STAR78 21722 4641 70239 59514 45654 051
GALAXY154 52987 6695160 0595 55365 612
Table 2.

Description of the spectroscopic samples from the cross-match between S-PLUS DR2, SDSS DR14Q (quasars), SDSS DR16 (stars and galaxies) and AllWISE catalogues. Selection criteria are |$\texttt {zWarning}=0$| for galaxies, and r > 13 for stars. For all classes, the criteria are |$\texttt {PhotoFlag}_r=0$| and an upper limit of 22 magnitudes in r. After the selection criteria, we applied a 4-sigma clipping of the difference between r magnitudes from SDSS and S-PLUS.

Total matchesNumber of lost objects from criteriaNumber of lost objects from 4-sigma clippingwith_WISE sampleno_WISE sampleFinal sample
QSO28 2759 2176915 5383 45118 989
STAR78 21722 4641 70239 59514 45654 051
GALAXY154 52987 6695160 0595 55365 612
Total matchesNumber of lost objects from criteriaNumber of lost objects from 4-sigma clippingwith_WISE sampleno_WISE sampleFinal sample
QSO28 2759 2176915 5383 45118 989
STAR78 21722 4641 70239 59514 45654 051
GALAXY154 52987 6695160 0595 55365 612
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close