Search Results - "Nanayakkara, T."

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    Newly Discovered Bright z ∼ 9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS Area by Bouwens, R. J., Stefanon, M., Oesch, P. A., Illingworth, G. D., Nanayakkara, T., Roberts-Borsani, G., Labbé, I., Smit, R.

    Published in The Astrophysical journal (20-07-2019)
    “…We report the results of an expanded search for z ∼ 9-10 candidates over the ∼883 arcmin2 CANDELS+ERS fields. This study adds 147 arcmin2 to the search area we…”
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    Journal Article
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    On the lack of correlation between [O  iii ]/[O  ii ] and Lyman continuum escape fraction by Bassett, R, Ryan-Weber, E V, Cooke, J, Diaz, C G, Nanayakkara, T, Yuan, T-T, Spitler, L R, Meštrić, U, Garel, T, Sawicki, M, Gwyn, S, Golob, A

    “…We present the first results of our pilot study of eight photometrically selected Lyman-continuum (LyC) emitting galaxy candidates from the COSMOS field and…”
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    Journal Article
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    The origin of large emission line widths in massive galaxies at redshifts z ∼ 3 − 4 by Martínez-Marín, M, Glazebrook, K, Nanayakkara, T, Jacobs, C, Labbé, I, Kacprzak, G G, Papovich, C, Schreiber, C

    “…Abstract We present a sample of 22 massive galaxies with stellar masses >1010M⊙ at 3 < z < 4 with deep H and K-band high resolution spectra (R=3500-3000) from…”
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    Journal Article
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    Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z ≈ 1 by Patrício, V, Richard, J, Carton, D, Péroux, C, Contini, T, Brinchmann, J, Schaye, J, Weilbacher, P M, Nanayakkara, T, Maseda, M, Mahler, G, Wisotzki, L

    “…ABSTRACT The existence of a spatially resolved star-forming main sequence (rSFMS) and a spatially resolved mass–metallicity relation (rMZR) is now well…”
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    Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra by Gunawardhana, M L P, Brinchmann, J, Weilbacher, P M, Norberg, P, Monreal-Ibero, A, Nanayakkara, T, den Brok, M, Boogaard, L, Kollatschny, W

    “…ABSTRACT We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high…”
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    Journal Article
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