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

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4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES). / Swann, E.; Sullivan, M.; Carrick, J. et al.
In: The Messenger, Vol. 175, 03.2019, p. 58-61.

Research output: Contribution to specialist publication › Article

Harvard

Swann, E, Sullivan, M, Carrick, J, Hoenig, S, Hook, I, Kotak, R, Maguire, K, McMahon, R, Nichol, R & Smartt, S 2019, '4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES)' The Messenger, vol. 175, pp. 58-61. https://doi.org/10.18727/0722-6691/5129

APA

Swann, E., Sullivan, M., Carrick, J., Hoenig, S., Hook, I., Kotak, R., Maguire, K., McMahon, R., Nichol, R., & Smartt, S. (2019). 4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES). The Messenger, 175, 58-61. https://doi.org/10.18727/0722-6691/5129

Vancouver

Swann E, Sullivan M, Carrick J, Hoenig S, Hook I, Kotak R et al. 4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES). The Messenger. 2019 Mar;175:58-61. doi: 10.18727/0722-6691/5129

Author

Swann, E. ; Sullivan, M. ; Carrick, J. et al. / 4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES). In: The Messenger. 2019 ; Vol. 175. pp. 58-61.

Bibtex

@misc{9cbbf396fbae49c0bfb1340a37efe8fa,
title = "4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES)",
abstract = "The Time-Domain Extragalactic Survey (TiDES) is focused on the spectro-scopic 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 0.5, measure redshifts for up to 50 000 transient host galaxies to z 1 and monitor around 700 active galactic nuclei to z 2.5....",
author = "E. Swann and M. Sullivan and J. Carrick and S. Hoenig and I. Hook and R. Kotak and K. Maguire and R. McMahon and R. Nichol and S. Smartt",
year = "2019",
month = mar,
doi = "10.18727/0722-6691/5129",
language = "English",
volume = "175",
pages = "58--61",
journal = "The Messenger",
issn = "0722-6691",

}

RIS

TY - GEN

T1 - 4MOST Consortium Survey 10: The Time-Domain Extragalactic Survey (TiDES)

AU - Swann, E.

AU - Sullivan, M.

AU - Carrick, J.

AU - Hoenig, S.

AU - Hook, I.

AU - Kotak, R.

AU - Maguire, K.

AU - McMahon, R.

AU - Nichol, R.

AU - Smartt, S.

PY - 2019/3

Y1 - 2019/3

N2 - The Time-Domain Extragalactic Survey (TiDES) is focused on the spectro-scopic 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 0.5, measure redshifts for up to 50 000 transient host galaxies to z 1 and monitor around 700 active galactic nuclei to z 2.5....

AB - The Time-Domain Extragalactic Survey (TiDES) is focused on the spectro-scopic 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 0.5, measure redshifts for up to 50 000 transient host galaxies to z 1 and monitor around 700 active galactic nuclei to z 2.5....

U2 - 10.18727/0722-6691/5129

DO - 10.18727/0722-6691/5129

M3 - Article

VL - 175

SP - 58

EP - 61

JO - The Messenger

JF - The Messenger

SN - 0722-6691

ER -