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HiZELS: The high redshift emission line survey with UKIRT. / Best, Philip; Smail, Ian
; Sobral, David et al.
Thirty Years of Astronomical Discovery with UKIRT . ed. / A. Adamson; J. Davies; I. Robson. Dordrecht: Springer Netherlands, 2013. p. 235-250 (Astrophysics and Space Science Proceedings ; Vol. 37).
Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSN › Chapter
Harvard
Best, P, Smail, I
, Sobral, D, Geach, J, Garn, T, Ivison, R, Kurk, J, Dalton, G, Cirasuolo, M & Casali, M 2013,
HiZELS: The high redshift emission line survey with UKIRT. in A Adamson, J Davies & I Robson (eds),
Thirty Years of Astronomical Discovery with UKIRT . Astrophysics and Space Science Proceedings , vol. 37, Springer Netherlands, Dordrecht, pp. 235-250.
https://doi.org/10.1007/978-94-007-7432-2_22APA
Best, P., Smail, I.
, Sobral, D., Geach, J., Garn, T., Ivison, R., Kurk, J., Dalton, G., Cirasuolo, M., & Casali, M. (2013).
HiZELS: The high redshift emission line survey with UKIRT. In A. Adamson, J. Davies, & I. Robson (Eds.),
Thirty Years of Astronomical Discovery with UKIRT (pp. 235-250). (Astrophysics and Space Science Proceedings ; Vol. 37). Springer Netherlands.
https://doi.org/10.1007/978-94-007-7432-2_22Vancouver
Best P, Smail I
, Sobral D, Geach J, Garn T, Ivison R et al.
HiZELS: The high redshift emission line survey with UKIRT. In Adamson A, Davies J, Robson I, editors, Thirty Years of Astronomical Discovery with UKIRT . Dordrecht: Springer Netherlands. 2013. p. 235-250. (Astrophysics and Space Science Proceedings ). Epub 2013 Oct 9. doi: 10.1007/978-94-007-7432-2_22
Author
Bibtex
@inbook{dd1e59ec722b469fa8338341bfd95c0b,
title = "HiZELS: The high redshift emission line survey with UKIRT",
abstract = "We report on HiZELS, the High-z Emission Line Survey, our successful panoramic narrow-band campaign survey using WFCAM on UKIRT to detect and study emission line galaxies at z ∼ 1–9. HiZELS employs the H2(S1) narrow-band filter together with custom-made narrow-band filters in the J and H-bands, with the primary aim of delivering large identically-selected samples of Hα emitting galaxies at redshifts of 0.84, 1.47 and 2.23. Comparisons between the luminosity function, the host galaxy properties, the clustering, and the variation with environment of these Hα-selected samples are yielding unique constraints on the nature and evolution of star-forming galaxies, across the peak epoch of star formation activity in the Universe. We provide a summary of the project status, and detail the main scientific results obtained so far: the measurement of the evolution of the cosmic star formation rate density out to z < 2 using a single star formation indicator, determination of the morphologies, environments and dust content of the star-forming galaxies, and a detailed investigation of the evolution of their clustering properties. We also summarise the on-going work and future goals of the project.",
author = "Philip Best and Ian Smail and David Sobral and Jim Geach and Tim Garn and Rob Ivison and Jaron Kurk and Gavin Dalton and Michele Cirasuolo and Mark Casali",
year = "2013",
doi = "10.1007/978-94-007-7432-2_22",
language = "English",
isbn = "9789400774315",
series = "Astrophysics and Space Science Proceedings ",
publisher = "Springer Netherlands",
pages = "235--250",
editor = "A. Adamson and J. Davies and I. Robson",
booktitle = "Thirty Years of Astronomical Discovery with UKIRT",
address = "Netherlands",
}
RIS
TY - CHAP
T1 - HiZELS
T2 - The high redshift emission line survey with UKIRT
AU - Best, Philip
AU - Smail, Ian
AU - Sobral, David
AU - Geach, Jim
AU - Garn, Tim
AU - Ivison, Rob
AU - Kurk, Jaron
AU - Dalton, Gavin
AU - Cirasuolo, Michele
AU - Casali, Mark
PY - 2013
Y1 - 2013
N2 - We report on HiZELS, the High-z Emission Line Survey, our successful panoramic narrow-band campaign survey using WFCAM on UKIRT to detect and study emission line galaxies at z ∼ 1–9. HiZELS employs the H2(S1) narrow-band filter together with custom-made narrow-band filters in the J and H-bands, with the primary aim of delivering large identically-selected samples of Hα emitting galaxies at redshifts of 0.84, 1.47 and 2.23. Comparisons between the luminosity function, the host galaxy properties, the clustering, and the variation with environment of these Hα-selected samples are yielding unique constraints on the nature and evolution of star-forming galaxies, across the peak epoch of star formation activity in the Universe. We provide a summary of the project status, and detail the main scientific results obtained so far: the measurement of the evolution of the cosmic star formation rate density out to z < 2 using a single star formation indicator, determination of the morphologies, environments and dust content of the star-forming galaxies, and a detailed investigation of the evolution of their clustering properties. We also summarise the on-going work and future goals of the project.
AB - We report on HiZELS, the High-z Emission Line Survey, our successful panoramic narrow-band campaign survey using WFCAM on UKIRT to detect and study emission line galaxies at z ∼ 1–9. HiZELS employs the H2(S1) narrow-band filter together with custom-made narrow-band filters in the J and H-bands, with the primary aim of delivering large identically-selected samples of Hα emitting galaxies at redshifts of 0.84, 1.47 and 2.23. Comparisons between the luminosity function, the host galaxy properties, the clustering, and the variation with environment of these Hα-selected samples are yielding unique constraints on the nature and evolution of star-forming galaxies, across the peak epoch of star formation activity in the Universe. We provide a summary of the project status, and detail the main scientific results obtained so far: the measurement of the evolution of the cosmic star formation rate density out to z < 2 using a single star formation indicator, determination of the morphologies, environments and dust content of the star-forming galaxies, and a detailed investigation of the evolution of their clustering properties. We also summarise the on-going work and future goals of the project.
U2 - 10.1007/978-94-007-7432-2_22
DO - 10.1007/978-94-007-7432-2_22
M3 - Chapter
AN - SCOPUS:85039057923
SN - 9789400774315
T3 - Astrophysics and Space Science Proceedings
SP - 235
EP - 250
BT - Thirty Years of Astronomical Discovery with UKIRT
A2 - Adamson, A.
A2 - Davies, J.
A2 - Robson, I.
PB - Springer Netherlands
CY - Dordrecht
ER -
