EGS/master_catalogue_egs_20180501_photoz_20180608.fits
dmu1/dmu1_ml_EGS/data/master_catalogue_egs_20180501.fits
dmu23/dmu23_EGS/data/EGS-specz-v2.1_hedam.csv
- EAZY Default
- Atlas of Galaxy SEDs (Brown et al. 2014)
- XMM-COSMOS Template library
"Available" corresponds to aperture magnitudes. Additional total magnitudes are present in the masterlist but not used during photo-z fitting.
| Telescope / Instrument | Filter | Available | Used |
|---|---|---|---|
| Subaru/HSC | suprime_g | Yes | Yes |
| Subaru/HSC | suprime_g | Yes | Yes |
| Subaru/HSC | suprime_i | Yes | Yes |
| Subaru/HSC | suprime_z | Yes | Yes |
| Subaru/HSC | suprime_y | Yes | Yes |
| CFHT/Megacam | megacam_u | Yes | Yes |
| CFHT/Megacam | megacam_g | Yes | Yes |
| CFHT/Megacam | megacam_r | Yes | Yes |
| CFHT/Megacam | megacam_i | Yes | Yes |
| CFHT/Megacam | megacam_z | Yes | Yes |
| HST/ACS | acs_f606w | Yes | Yes |
| HST/ACS | acs_f814w | Yes | Yes |
| HST/WFC3 | wfc3_f125w | Yes | Yes |
| HST/WFC3 | wfc3_f160w | Yes | Yes |
| Bok/90prime | 90prime_g | Yes | Yes |
| Bok/90prime | 90prime_r | Yes | Yes |
| Mayall/MOSAIC | mosaic_z | Yes | Yes |
| Pan-STARRS1/Pan-STARRS1 | gpc1_g | Yes | No |
| Pan-STARRS1/Pan-STARRS1 | gpc1_r | Yes | No |
| Pan-STARRS1/Pan-STARRS1 | gpc1_i | Yes | No |
| Pan-STARRS1/Pan-STARRS1 | gpc1_z | Yes | No |
| Pan-STARRS1/Pan-STARRS1 | gpc1_y | Yes | No |
| CFHT/WIRCam | wircam_j | Yes | Yes |
| CFHT/WIRCam | wircam_h | Yes | Yes |
| CFHT/WIRCam | wircam_ks | Yes | Yes |
| Palomar/WIRCS | wircs_j | Yes | Yes |
| Palomar/WIRCS | wircs_k | Yes | Yes |
| UKIDSS/WFCAM | ukidss_j | Yes | Yes |
For the main galaxy population, three additional Gaussian Process machine learning estimates were also incorporated into the Bayesian combination estimates. These were training using the combined spectroscopic sample - with cost-sensitive learning weights calibrated for the full field. The two sets of filters used were:
- Megacam u, g, r, i, z
- HSC g, r, i, z, y
- In order to have a fully calibrated redshift estimate, sources must have a magnitude measurement in any of the optical r-bands.
- Sources must also be detected in 4 bands at different wavelengths for a redshift to have been estimated (i.e. multiple r-band detections count only as one), including 3 optical bands (b -> y). Multiple detections in similar optical bands are not counted.
