USM Photometric Redshifts
for Astro-wise

Introduction

Spectral Energy Distributions (model input)

Method:

Assigning a redshift and SED to each source

Slide 6

Slide 7

Slide 8

Comparison with zspec

Limitations of this method

Slide 11

Slide 12

Present Implementation of Photometric Redshift Routine

Integration into Astro-Wise Pipeline