z-ph-REM: A photometric redshift code for the REM telescope
Astrophysics
2019-08-14 v1
Abstract
The REM telescope is being deployed these very days at the La Silla Observatory in Chile, and will be fully operational by the beginning of 2004. It is a very fast-slewing robotized telescope, endowed with optical and near-infrared capabilities, designed with the primary objective of performing rapid follow-up of GRB events. One of the key issues will be the prompt recognition of potentially interesting bursts (those happening at high redshift or peculiarly reddened). Here I present a sketch of z-ph-REM, the photometric redshift code designed for this mission.
Cite
@article{arxiv.astro-ph/0309492,
title = {z-ph-REM: A photometric redshift code for the REM telescope},
author = {A. Fernandez-Soto},
journal= {arXiv preprint arXiv:astro-ph/0309492},
year = {2019}
}
Comments
2 pages, to appear in Proceedings of the "Multi-Wavelength Cosmology" Conference held in Mykonos, Greece, June 2003, ed. M. Plionis (Kluwer)