alphaFeedback
AM

Alice Mortlock

astro-ph.GAastro-ph.CO

On Valency

published · living versions
W_fq3jhe2k·v1 · currentpublished

Preprints & journals

24 papers in the corpus · 2010–2017
Stellar populations, stellar masses and the formation of galaxy bulges and discs at z<3z < 3 in CANDELS1710.03477v1 · Berta Margalef-Bentabol, Christopher J. Conselice, Alice Mortlock et al.2017 · 19 citationsarXiv
Characterising the evolving KK-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys1610.06574v1 · Alice Mortlock, Ross J. McLure, Rebecca A. A. Bowler et al.2016 · 24 citationsarXiv
Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS1610.03070v1 · B. D. Simmons, Chris Lintott, Kyle W. Willett et al.2016 · 110 citationsarXiv
Exploring the progenitors of brightest cluster galaxies at z~21609.07287v2 · Dongyao Zhao, Christopher J. Conselice, Alfonso Arag'on-Salamanca et al.2016 · 16 citationsarXiv
The Formation of Bulges, Discs and Two Component Galaxies in the CANDELS Survey at z < 31606.07405v1 · Berta Margalef-Bentabol, Christopher J. Conselice, Alice Mortlock et al.2016 · 50 citationsarXiv
The Evolution of Galaxies at Constant Number Density: A Less Biased View of Star Formation, Quenching, and Structural Formation1605.05741v1 · Jamie R. Ownsworth, Christopher J. Conselice, Carl J. Mundy et al.2016 · 26 citationsarXiv
The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field1604.00018v2 · Aaron Wilkinson, Omar Almaini, Chian-Chou Chen et al.2016 · 95 citationsarXiv
Deconstructing the Galaxy Stellar Mass Function with UKIDSS and CANDELS: the Impact of Colour, Structure and Environment1411.3339v1 · Alice Mortlock, Christopher. J. Conselice, William G. Hartley et al.2014 · 109 citationsarXiv
Minor vs Major Mergers: The Stellar Mass Growth of Massive Galaxies from z=3 using Number Density Selection Techniques1409.1582v1 · Jamie R. Ownsworth, Christopher J. Conselice, Alice Mortlock et al.2014 · 72 citationsarXiv
Galaxy Zoo: CANDELS Barred Disks and Bar Fractions1409.1214v1 · B. D. Simmons, Thomas Melvin, Chris Lintott et al.2014 · 111 citationsarXiv
Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters1407.3811v1 · Christopher J. Conselice, Asa F.L. Bluck, Alice Mortlock et al.2014 · 53 citationsarXiv
Properties of Submillimeter Galaxies in the CANDELS GOODS-S Field1402.3268v1 · Tommy Wiklind, Christopher J. Conselice, Tomas Dahlen et al.2014 · 55 citationsarXiv
Evidence for a correlation between the sizes of quiescent galaxies and local environment to z ~ 21307.3247v2 · Caterina Lani, Omar Almaini, William G. Hartley et al.2013 · 89 citationsarXiv
The Redshift and Mass Dependence on the Formation of The Hubble Sequence at z>1 from CANDELS/UDS1305.2204v2 · Alice Mortlock, Christopher J. Conselice, William G. Hartley et al.2013 · 164 citationsarXiv
Evolution of Massive Galaxy Structural Properties and Sizes via Star Formation1212.3504v1 · Jamie R. Ownsworth, Christopher J. Conselice, Alice Mortlock et al.2012 · 0 citationsarXiv
Evolution of Massive Galaxy Structural Properties and Sizes via Star Formation In the GOODS NICMOS Survey1207.3084v2 · Jamie R. Ownsworth, Christopher J. Conselice, Alice Mortlock et al.2012 · 16 citationsarXiv
Gas Accretion as a Dominant Formation Mode in Massive Galaxies from the GOODS NICMOS Survey1206.6995v2 · Christopher J. Conselice, Alice Mortlock, Asa F. L. Bluck et al.2012 · 75 citationsarXiv
A Deep Probe of the Galaxy Stellar Mass Functions at z~1-3 with the GOODS NICMOS Survey1101.2867v2 · Alice Mortlock, Christopher J. Conselice, Asa F. L. Bluck et al.2011 · 102 citationsarXiv
Galaxy properties in different environments up to z ~ 3 in the GOODS NICMOS Survey1011.4846v1 · Ruth Grutzbauch, Robert W. Chuter, Christopher J. Conselice et al.2010 · 50 citationsarXiv
Career total: 44 works. 24 are in this corpus.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.