Search Results - "Stephenson, H M O"

Quasar Sightline and Galaxy Evolution (QSAGE) – III. The mass–metallicity and fundamental metallicity relation of z ≈ 2.2 galaxies by Stephenson, H M O, Stott, J P, Cullen, F, Bielby, R M, Amos, N, Dutta, R, Fumagalli, M, Tejos, N, Burchett, J N, Crain, R A, Prochaska, J X

“…ABSTRACT We present analysis of the mass–metallicity relation (MZR) for a sample of 67 [O iii]-selected star-forming (SF) galaxies at a redshift range of z =…”
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Quasar Sightline and Galaxy Evolution (QSAGE) -- III. The mass-metallicity and fundamental metallicity relation of $z \approx$ 2.2 galaxies by Stephenson, H. M. O, Stott, J. P, Cullen, F, Bielby, R. M, Amos, N, Dutta, R, Fumagalli, M, Tejos, N, Burchett, J. N, Crain, R. A, Prochaska, J. X

“…We present analysis of the mass-metallicity relation (MZR) for a sample of 67 [OIII]-selected star-forming galaxies at a redshift range of $z=1.99 - 2.32$…”
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The JWST Emission Line Survey (JELS): An untargeted search for H$\alpha$ emission line galaxies at $z > 6$ and their physical properties by Pirie, C. A, Best, P. N, Duncan, K. J, McLeod, D. J, Cochrane, R. K, Clausen, M, Dunlop, J. S, Flury, S. R, Geach, J. E, Hale, C. L, Ibar, E, Kondapally, R, Li, Zefeng, Matthee, J, McLure, R. J, Ossa-Fuentes, L, Patrick, A. L, Smail, Ian, Sobral, D, Stephenson, H. M. O, Stott, J. P, Swinbank, A. M

“…We present the first results of the JWST Emission Line Survey (JELS). Utilising the first NIRCam narrow-band imaging at 4.7$\mu$m, over 63 arcmin$^{2}$ in the…”
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The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization by Duncan, K. J, McLeod, D. J, Best, P. N, Pirie, C. A, Clausen, M, Cochrane, R. K, Dunlop, J. S, Flury, S. R, Geach, J. E, Grogin, N. A, Hale, C. L, Ibar, E, Kondapally, R, Li, Zefeng, Matthee, J, McLure, R. J, Ossa-Fuentes, Luis, Patrick, A. L, Smail, Ian, Sobral, D, Stephenson, H. M. O, Stott, J. P, Swinbank, A. M

“…We present the JWST Emission Line Survey (JELS), a Cycle 1 JWST imaging programme exploiting the wavelength coverage and sensitivity of NIRCam to extend…”
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