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Authors:
Kewley, Lisa J
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Yuan, Tiantian
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Labbé, Ivo
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Tomczak, Adam
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Nanayakkara, Themiya
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Kacprzak, Glenn G
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Tran, Kim-Vy H
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Glazebrook, Karl
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Spitler, Lee
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Cowley, Michael
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Dopita, Michael
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Straatman, Caroline
Date: 2016
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1200354
Description:
We investigate the ISM properties of 13 star-forming galaxies within the z ~ 2 COSMOS cluster. We show that the cluster members have [N II]/Hα and [O III]/Hβ emission-line ratios similar to z ~ 2 fiel
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Authors:
Kacprzak, Glenn G
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Yuan, Tiantian
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Labbe, Ivo
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Straatman, Caroline
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Tomczak, Adam
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Nanayakkara, Themiya
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Kobayashi, Chiaki
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Tran, Kim-Vy H
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Kewley, Lisa J
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Glazebrook, Karl
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Spitler, Lee
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Taylor, Philip
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Cowley, Michael
Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/357554
Description:
We investigate the environmental dependence of the mass–metallicity relation at z = 2 with MOSFIRE/Keck as part of the ZFIRE survey. Here, we present the chemical abundance of a Virgo-like progenitor
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Authors:
Tran, Kim-Vy H
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Nanayakkara, Themiya
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Saintonge, Amélie
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Spitler, Lee R
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Straatman, Caroline
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Tomczak, Adam
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Yuan, Tiantian
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Kacprzak, Glenn G
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Glazebrook, Karl
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Kewley, Lisa J
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Momcheva, Ivelina
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Papovich, Casey J
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Quadri, Ryan
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Rudnick, Greg
Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1044558
Description:
We spectroscopically survey the galaxy cluster XMM-LSS J02182-05102 (hereafter IRC 0218) using LRIS (optical) and MOSFIRE (near-infrared) on Keck I as part of the ZFIRE survey. IRC 0218 has a narrow r
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Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/261862
Description:
We demonstrate that the space formed by the star formation rate (SFR), gas-phase metallicity (Z), and stellar mass (M) can be reduced to a plane, as first proposed by Lara-López et al. We study three
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Date: 2012
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/216009
Description:
A full appreciation of the role played by gas metallicity (Z), star-formation rate (SFR), and stellar mass (M*) is fundamental to understanding how galaxies form and evolve. Using data from the SDSS-D
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Authors:
Foster, C
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Hopkins, A. M
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Liske, J
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Loveday, J
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Norberg, P
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Peacock, J. A
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Alpaslan, M
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Bauer, A. E
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Bland-Hawthorn, J
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Brough, S
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Cameron, E
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Colless, M
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Gunawardhana, M
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Conselice, C. J
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Croom, S. M
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Frenk, C. S
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Hill, D. T
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Jones, D. H
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Kelvin, L. S
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Kuijken, K
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Nichol, R. C
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Owers, M. S
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Parkinson, H. R
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Lara-López, M. A
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Pimbblet, K. A
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Popescu, C. C
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Prescott, M
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Robotham, A. S. G
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López-Sánchez, Á. R
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Sutherland, W. J
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Thomas, D
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Tuffs, R. J
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van Kampen, E
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Wijesinghe, D
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Sharp, R. G
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Steele, O
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Taylor, E. N
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Driver, S. P
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Baldry, I. K
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Bamford, S. P
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/210680
Description:
Context. The mass-metallicity relationship (MMR) of star-forming galaxies is well-established, however there is still some disagreement with respect to its exact shape and its possible dependence on o
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