@article{wilkins_properties_2017,
	title = {The properties of the first galaxies in the {BlueTides} simulation},
	volume = {469},
	issn = {0035-8711},
	url = {http://adsabs.harvard.edu/abs/2017MNRAS.469.2517W},
	doi = {10.1093/mnras/stx841},
	abstract = {We employ the very large cosmological hydrodynamical simulation BlueTides to investigate the predicted properties of the galaxy
population during the epoch of reionization (z {\textgreater} 8). BlueTides has a resolution and volume ((400/h ≈ 577)3 cMpc3) providing a population of galaxies that is well matched to depth and area of current observational surveys targeting the high-redshift Universe. At z = 8, BlueTides includes almost 160 000 galaxies with stellar masses {\textgreater}108 M⊙. The population of
galaxies predicted by BlueTides closely matches observational
constraints on both the galaxy stellar mass function and far-UV (150 nm) luminosity function. Galaxies in BlueTides are characterized by rapidly increasing star formation histories. Specific star formation rates decrease with redshift though remain largely insensitive to stellar mass. As a result of the enhanced surface density of metals, more massive galaxies are predicted to have higher dust attenuation resulting in a significant steepening of the observed far-UV luminosity function at high luminosities. The contribution of active supermassive black holes (SMBHs) to the UV luminosities of galaxies with stellar masses 109-10 M⊙ is around 3 per cent on average. Approximately 25 per cent of galaxies with M* ≈
1010 M⊙ are predicted to have active SMBHs that contribute {\textgreater}10 per cent of the total UV luminosity.},
	urldate = {2020-03-26},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Wilkins, Stephen M. and Feng, Yu and Di Matteo, Tiziana and Croft, Rupert and Lovell, Christopher C. and Waters, Dacen},
	month = aug,
	year = {2017},
	keywords = {Astrophysics - Astrophysics of Galaxies, galaxies: high-redshift, galaxies: luminosity function, galaxies: photometry, mass function, methods: numerical},
	pages = {2517--2530},
}

{"_id":"wGzQkWw8X5ppK7GGK","bibbaseid":"wilkins-feng-dimatteo-croft-lovell-waters-thepropertiesofthefirstgalaxiesinthebluetidessimulation-2017","author_short":["Wilkins, S. M.","Feng, Y.","Di Matteo, T.","Croft, R.","Lovell, C. C.","Waters, D."],"bibdata":{"bibtype":"article","type":"article","title":"The properties of the first galaxies in the BlueTides simulation","volume":"469","issn":"0035-8711","url":"http://adsabs.harvard.edu/abs/2017MNRAS.469.2517W","doi":"10.1093/mnras/stx841","abstract":"We employ the very large cosmological hydrodynamical simulation BlueTides to investigate the predicted properties of the galaxy population during the epoch of reionization (z \\textgreater 8). BlueTides has a resolution and volume ((400/h ≈ 577)3 cMpc3) providing a population of galaxies that is well matched to depth and area of current observational surveys targeting the high-redshift Universe. At z = 8, BlueTides includes almost 160 000 galaxies with stellar masses \\textgreater108 M⊙. The population of galaxies predicted by BlueTides closely matches observational constraints on both the galaxy stellar mass function and far-UV (150 nm) luminosity function. Galaxies in BlueTides are characterized by rapidly increasing star formation histories. Specific star formation rates decrease with redshift though remain largely insensitive to stellar mass. As a result of the enhanced surface density of metals, more massive galaxies are predicted to have higher dust attenuation resulting in a significant steepening of the observed far-UV luminosity function at high luminosities. The contribution of active supermassive black holes (SMBHs) to the UV luminosities of galaxies with stellar masses 109-10 M⊙ is around 3 per cent on average. Approximately 25 per cent of galaxies with M* ≈ 1010 M⊙ are predicted to have active SMBHs that contribute \\textgreater10 per cent of the total UV luminosity.","urldate":"2020-03-26","journal":"Monthly Notices of the Royal Astronomical Society","author":[{"propositions":[],"lastnames":["Wilkins"],"firstnames":["Stephen","M."],"suffixes":[]},{"propositions":[],"lastnames":["Feng"],"firstnames":["Yu"],"suffixes":[]},{"propositions":[],"lastnames":["Di","Matteo"],"firstnames":["Tiziana"],"suffixes":[]},{"propositions":[],"lastnames":["Croft"],"firstnames":["Rupert"],"suffixes":[]},{"propositions":[],"lastnames":["Lovell"],"firstnames":["Christopher","C."],"suffixes":[]},{"propositions":[],"lastnames":["Waters"],"firstnames":["Dacen"],"suffixes":[]}],"month":"August","year":"2017","keywords":"Astrophysics - Astrophysics of Galaxies, galaxies: high-redshift, galaxies: luminosity function, galaxies: photometry, mass function, methods: numerical","pages":"2517–2530","bibtex":"@article{wilkins_properties_2017,\n\ttitle = {The properties of the first galaxies in the {BlueTides} simulation},\n\tvolume = {469},\n\tissn = {0035-8711},\n\turl = {http://adsabs.harvard.edu/abs/2017MNRAS.469.2517W},\n\tdoi = {10.1093/mnras/stx841},\n\tabstract = {We employ the very large cosmological hydrodynamical simulation BlueTides to investigate the predicted properties of the galaxy\npopulation during the epoch of reionization (z {\\textgreater} 8). BlueTides has a resolution and volume ((400/h ≈ 577)3 cMpc3) providing a population of galaxies that is well matched to depth and area of current observational surveys targeting the high-redshift Universe. At z = 8, BlueTides includes almost 160 000 galaxies with stellar masses {\\textgreater}108 M⊙. The population of\ngalaxies predicted by BlueTides closely matches observational\nconstraints on both the galaxy stellar mass function and far-UV (150 nm) luminosity function. Galaxies in BlueTides are characterized by rapidly increasing star formation histories. Specific star formation rates decrease with redshift though remain largely insensitive to stellar mass. As a result of the enhanced surface density of metals, more massive galaxies are predicted to have higher dust attenuation resulting in a significant steepening of the observed far-UV luminosity function at high luminosities. The contribution of active supermassive black holes (SMBHs) to the UV luminosities of galaxies with stellar masses 109-10 M⊙ is around 3 per cent on average. Approximately 25 per cent of galaxies with M* ≈\n1010 M⊙ are predicted to have active SMBHs that contribute {\\textgreater}10 per cent of the total UV luminosity.},\n\turldate = {2020-03-26},\n\tjournal = {Monthly Notices of the Royal Astronomical Society},\n\tauthor = {Wilkins, Stephen M. and Feng, Yu and Di Matteo, Tiziana and Croft, Rupert and Lovell, Christopher C. and Waters, Dacen},\n\tmonth = aug,\n\tyear = {2017},\n\tkeywords = {Astrophysics - Astrophysics of Galaxies, galaxies: high-redshift, galaxies: luminosity function, galaxies: photometry, mass function, methods: numerical},\n\tpages = {2517--2530},\n}\n\n","author_short":["Wilkins, S. M.","Feng, Y.","Di Matteo, T.","Croft, R.","Lovell, C. C.","Waters, D."],"key":"wilkins_properties_2017","id":"wilkins_properties_2017","bibbaseid":"wilkins-feng-dimatteo-croft-lovell-waters-thepropertiesofthefirstgalaxiesinthebluetidessimulation-2017","role":"author","urls":{"Paper":"http://adsabs.harvard.edu/abs/2017MNRAS.469.2517W"},"keyword":["Astrophysics - Astrophysics of Galaxies","galaxies: high-redshift","galaxies: luminosity function","galaxies: photometry","mass function","methods: numerical"],"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://api.zotero.org/users/2650003/collections/2GYAYTB9/items?key=HjJ9T6LSEhBUjY15bMA811su&format=bibtex&limit=100","dataSources":["CxJmmGJKTkqa9B6aM","7gvjSdWrEu7z5vjjj"],"keywords":["astrophysics - astrophysics of galaxies","galaxies: high-redshift","galaxies: luminosity function","galaxies: photometry","mass function","methods: numerical"],"search_terms":["properties","first","galaxies","bluetides","simulation","wilkins","feng","di matteo","croft","lovell","waters"],"title":"The properties of the first galaxies in the BlueTides simulation","year":2017}