pith. sign in

arxiv: 1903.02476 · v2 · pith:VEV64U7Inew · submitted 2019-03-06 · 🌌 astro-ph.IM

4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES)

classification 🌌 astro-ph.IM
keywords surveytransientsextragalacticspectroscopictidesactivefollow-upgalactic
0
0 comments X
read the original abstract

The Time-Domain Extragalactic Survey (TiDES) is focused on the spectroscopic follow-up of extragalactic optical transients and variable sources selected from forthcoming large sky surveys such as that from the Large Synoptic Survey Telescope (LSST). TiDES contains three sub-surveys: (i) spectroscopic observations of supernova-like transients; (ii) comprehensive follow-up of transient host galaxies to obtain redshift measurements for cosmological applications; and (iii) repeat spectroscopic observations to enable the reverberation mapping of active galactic nuclei. Our simulations predict we will be able to classify transients down to $r = 22.5$ magnitudes (AB) and, over five years of 4MOST operations, obtain spectra for up to 30,000 live transients to redshift $z \sim 0.5$, measure redshifts for up to 50,000 transient host galaxies to $z \sim 1$ and monitor around 700 active galactic nuclei to $z \sim 2.5$.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Impact of Host Galaxy Properties on Supernova Classification with Hierarchical Labels

    astro-ph.IM 2026-06 unverdicted novelty 6.0

    Host galaxy properties enable >90% pure Type Ia samples from photometry alone and improve classification accuracy when redshift is unavailable, via a new hierarchical cross-entropy objective.