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HiZELS: The high redshift emission line survey with UKIRT

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HiZELS : The high redshift emission line survey with UKIRT. / Best, Philip; Smail, Ian; Sobral, David; Geach, Jim; Garn, Tim; Ivison, Rob; Kurk, Jaron; Dalton, Gavin; Cirasuolo, Michele; Casali, Mark.

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/ISSNChapter

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_22

APA

Best, P., Smail, I., Sobral, D., Geach, J., Garn, T., Ivison, R., ... 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). Dordrecht: Springer Netherlands. https://doi.org/10.1007/978-94-007-7432-2_22

Vancouver

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 ). https://doi.org/10.1007/978-94-007-7432-2_22

Author

Best, Philip ; Smail, Ian ; Sobral, David ; Geach, Jim ; Garn, Tim ; Ivison, Rob ; Kurk, Jaron ; Dalton, Gavin ; Cirasuolo, Michele ; Casali, Mark. / HiZELS : The high redshift emission line survey with UKIRT. Thirty Years of Astronomical Discovery with UKIRT . editor / A. Adamson ; J. Davies ; I. Robson. Dordrecht : Springer Netherlands, 2013. pp. 235-250 (Astrophysics and Space Science Proceedings ).

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

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 -