Katalog Plus
Bibliothek der Frankfurt UAS
Bald neuer Katalog: sichern Sie sich schon vorab Ihre persönlichen Merklisten im Nutzerkonto: Anleitung.
Dieses Ergebnis aus BASE kann Gästen nicht angezeigt werden.  Login für vollen Zugriff.

TiDES: The 4MOST Time Domain Extragalactic Survey

Title: TiDES: The 4MOST Time Domain Extragalactic Survey
Authors: Frohmaier, C; Vincenzi, M; Sullivan, M; Hönig, SF; Smith, M; Addison, H; Collett, T; Dimitriadis, G; Ellis, RS; Gandhi, P; Graur, O; Hook, I; Kelsey, L; Kim, Y-L; Lidman, C; Maguire, K; Makrygianni, L; Martin, B; Möller, A; Nichol, RC; Nicholl, M; Schady, P; Simmons, BD; Smartt, SJ; Tempel, E; Wiseman, P; Collaboration, the LSST Dark Energy Science
Publisher Information: American Astronomical Society; //doi.org/10.3847/1538-4357/adff4e
Publication Year: 2025
Collection: Apollo - University of Cambridge Repository
Subject Terms: 5109 Space Sciences; 51 Physical Sciences
Description: The Time Domain Extragalactic Survey (TiDES) conducted on the 4 m Multi-Object Spectroscopic Telescope will perform spectroscopic follow-up of extragalactic transients discovered in the era of the NSF-DOE Vera C. Rubin Observatory. TiDES will conduct a 5 yr survey, covering >14,000squaredegrees , and use around 250,000 fibre hours to address three main science goals: (i) spectroscopic observations of >30,000 live transients, (ii) comprehensive follow-up of >200,000 host galaxies to obtain redshift measurements, and (iii) repeat spectroscopic observations of active galactic nuclei to enable reverberation mapping studies. The live spectra from TiDES will be used to reveal the diversity and astrophysics of both normal and exotic supernovae across the luminosity-timescale plane. The extensive host-galaxy redshift campaign will allow exploitation of the larger sample of supernovae and improve photometric classification, providing the largest-ever sample of SNe Ia, capable of a sub-2% measurement of the equation-of-state of dark energy. Finally, the TiDES reverberation mapping experiment of 700–1000 AGN will complement the SN Ia sample and extend the Hubble diagram to z ∼ 2.5.
Document Type: article in journal/newspaper
File Description: text/xml; application/pdf
Language: English
Relation: apjadff4e; adff4e; aas63672; https://www.repository.cam.ac.uk/handle/1810/390820
Availability: https://www.repository.cam.ac.uk/handle/1810/390820
Accession Number: edsbas.EA0CE822
Database: BASE