Add to ORKGWe have constructed a mass-selected sample of M*>1011 M⊙ galaxies at 1<z<3 in the CANDELS UKIDSS UDS and COSMOS fields and have decomposed these systems into their separate bulge and disc components according to their H160-band morphologies. By extending this analysis to multiple bands, we have been able to conduct individual bulge and disc component SED fitting which has provided us with stellar-mass and star formation rate estimates for the separate bulge and disc components. Having utilized the new decomposed stellar-mass estimates, we confirm that the bulge components display a stronger size evolution than the discs. The median sizes of the bulge components is 3.09±0.20times smaller than similarly massive local galaxies over the full 1<...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We quantify the morphological evolution of z ~ 0 massive galaxies (M_*/M_∼ ∼10^11.2 +/- 0.3) from z ...
We have constructed a mass-selected sample of M* \u3e 1011 M⊙ galaxies at 1 \u3c z \u3c 3 in the CAN...
We have constructed a mass-selected sample of M ∗> 1011 M galaxies at 1 < z < 3 in the CAND...
We present the results of a new and improved study of the morphological and spectral evolution of ma...
© 2019 The Author(s). We study the rest-frame optical mass-size relation of bulges and discs from z ...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high‐resolution, Hubble Space Telescope , near‐infrared imaging to conduct a detailed ...
We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two-compone...
We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two-compone...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We explore the evolution of the stellar mass-size relation of galaxies of different morphological ty...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We quantify the morphological evolution of z ~ 0 massive galaxies (M_*/M_∼ ∼10^11.2 +/- 0.3) from z ...
We have constructed a mass-selected sample of M* \u3e 1011 M⊙ galaxies at 1 \u3c z \u3c 3 in the CAN...
We have constructed a mass-selected sample of M ∗> 1011 M galaxies at 1 < z < 3 in the CAND...
We present the results of a new and improved study of the morphological and spectral evolution of ma...
© 2019 The Author(s). We study the rest-frame optical mass-size relation of bulges and discs from z ...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed an...
We have used high‐resolution, Hubble Space Telescope , near‐infrared imaging to conduct a detailed ...
We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two-compone...
We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two-compone...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We explore the evolution of the stellar mass-size relation of galaxies of different morphological ty...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We study the rest-frame optical mass-size relation of bulges and discs from z similar to 2 to z simi...
We quantify the morphological evolution of z ~ 0 massive galaxies (M_*/M_∼ ∼10^11.2 +/- 0.3) from z ...