Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Williams, Christina C."'
Autor:
Maseda, Michael V., van der Wel, Arjen, Franx, Marijn, Bell, Eric F., Bezanson, Rachel, Muzzin, Adam, Sobral, David, D'Eugenio, Francesco, Gallazzi, Anna, de Graaff, Anna, Leja, Joel, Straatman, Caroline, Whitaker, Katherine E., Williams, Christina C., Wu, Po-Feng
Using deep rest-frame optical spectroscopy from the Large Early Galaxy Astrophysical Census (LEGA-C) survey, conducted using VIMOS on the ESO Very Large Telescope, we systematically search for low-ionization [OII] 3726,3729 emission in the spectra of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36195b6ca16f66692ae166cfa94ce594
Autor:
Akhshik, Mohammad, Whitaker, Katherine E., Brammer, Gabriel, Mahler, Guillaume, Sharon, Keren, Leja, Joel, Bayliss, Matthew B., Bezanson, Rachel, Gladders, Michael D., Man, Allison, Nelson, Erica J., Rigby, Jane R., Rizzo, Francesca, Toft, Sune, Wellons, Sarah, Williams, Christina C.
We present a novel Bayesian methodology to jointly model photometry and deep Hubble Space Telescope (HST) 2d grism spectroscopy of high-redshift galaxies. Our requiem2d code measures both unresolved and resolved stellar populations, ages, and star-fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1903e28cf7d9b5799b8f38da458afd0d
http://arxiv.org/abs/2008.02276
http://arxiv.org/abs/2008.02276
Autor:
Behroozi, Peter, Conroy, Charlie, Wechsler, Risa H., Hearin, Andrew, Williams, Christina C., Moster, Benjamin P., Yung, L. Y. Aaron, Somerville, Rachel S., Gottl��ber, Stefan, Yepes, Gustavo, Endsley, Ryan
The James Webb Space Telescope (JWST) is expected to observe galaxies at $z>10$ that are presently inaccessible. Here, we use a self-consistent empirical model, the UniverseMachine, to generate mock galaxy catalogues and lightcones over the redshift
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ebd2d6b10ed8deeeb0e5d148caf1f1b3
Autor:
Lee, Bomee, Giavalisco, Mauro, Whitaker, Katherine, Williams, Christina C., Ferguson, Henry C., Acquaviva, Viviana, Koekemoer, Anton M., Straughn, Amber N., Guo, Yicheng, Kartaltepe, Jeyhan S., Lotz, Jennifer, Pacifici, Camilla, Croton, Darren J., Somerville, Rachel S., Lu, Yu
We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass (M_*), star formation rate (SFR) and morphology, and to introduce a fourth dimension, the mass-weighted stellar age, in galaxies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::ce498aa557c1db35ec513c6b968f317e
https://resolver.caltech.edu/CaltechAUTHORS:20180201-112824988
https://resolver.caltech.edu/CaltechAUTHORS:20180201-112824988
Autor:
Williams, Christina C., Curtis-Lake, Emma, Hainline, Kevin N., Chevallard, Jacopo, Robertson, Brant E., Charlot, Stephane, Endsley, Ryan, Stark, Daniel P., Willmer, Christopher N. A., Alberts, Stacey, Amorin, Ricardo, Arribas, Santiago, Baum, Stefi, Bunker, Andrew, Carniani, Stefano, Crandall, Sara, Egami, Eiichi, Eisenstein, Daniel J., Ferruit, Pierre, Husemann, Bernd, Maseda, Michael V., Maiolino, Roberto, Rawle, Timothy D., Rieke, Marcia, Smit, Renske, Tacchella, Sandro, Willott, Chris J.
We present an original phenomenological model to describe the evolution of galaxy number counts, morphologies, and spectral energy distributions across a wide range of redshifts (0.26]. Our model follows observed mass and luminosity functions of both
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb22849ad31521facbfab8e250eeb493
Autor:
Kocevski, Dale D., Barro, Guillermo, Faber, S.M., Dekel, Avishai, Somerville, Rachel S., Young, Joshua A., Williams, Christina C., McIntosh, Daniel H., Georgakakis, Antonis, Hasinger, Guenther, Nandra, Kirpal, Civano, Francesca, Alexander, David M., Almaini, Omar, Conselice, Christopher J., Donley, Jennifer L., Ferguson, Harry C., Giavalisco, Mauro, Grogin, Norman A., Hathi, Nimish, Hawkins, Matthew, Koekemoer, Anton M., Koo, David C., McGrath, Elizabeth J., Mobasher, Bahram, Pforr, Janine, Primack, Joel R., Santini, Paola, Stefanon, Mauro, Trump, Jonathan R., van der Wel, Arjen, Wuyts, Stijn, Yan, Haojing
We examine the fraction of massive (M* > 1010 M) compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at z ~ 2. These cSFGs are likely the direct progenitors of the compact quiescent galaxies observed at this epoch, which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::352297612de682e118879978821dec86
https://nottingham-repository.worktribe.com/file/882131/1/Kocevski_2017_ApJ_846_112.pdf
https://nottingham-repository.worktribe.com/file/882131/1/Kocevski_2017_ApJ_846_112.pdf
Autor:
Lee, Bomee, Giavalisco, Mauro, Whitaker, Katherine, Williams, Christina C., Ferguson, Henry C., Acquaviva, Viviana, Koekemoer, Anton M., Straughn, Amber N., Guo, Yicheng, Kartaltepe, Jeyhan S., Lotz, Jennifer, Pacifici, Camilla, Croton, Darren J., Somerville, Rachel S., Lu, Yu
We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass ($M_*$), star--formation rate (SFR) and morphology, and to introduce a fourth dimension, the mass-weighted stellar age, in galax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_______::4041b4fee9a320fb8cecebd0cb9e4531
http://arxiv.org/abs/1706.02311
http://arxiv.org/abs/1706.02311
Autor:
Pope, Alexandra, Montana, Alfredo, Battisti, Andrew, Limousin, Marceau, Marchesini, Danilo, Wilson, Grant W., Alberts, Stacey, Aretxaga, Itziar, Avila-Reese, Vladimir, Bermejo-Climent, Jose Ramon, Brammer, Gabriel, Bravo-Alfaro, Hector, Calzetti, Daniela, Chary, Ranga-Ram, Cybulski, Ryan, Giavalisco, Mauro, Hughes, David, Kado-Fong, Erin, Keller, Erica, Kirkpatrick, Allison, Labbe, Ivo, Lange-Vagle, Daniel, Lowenthal, James, Murphy, Eric, Oesch, Pascal, Gonzalez, Daniel Rosa, Sanchez-Arguelles, David, Shipley, Heath, Stefanon, Mauro, Vega, Olga, Whitaker, Katherine, Williams, Christina C., Yun, Min, Zavala, Jorge A., Zeballos, Milagros
We directly detect dust emission in an optically-detected, multiply-imaged galaxy lensed by the Frontier Fields cluster MACSJ0717.5+3745. We detect two images of the same galaxy at 1.1mm with the AzTEC camera on the Large Millimeter Telescope leaving
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f5b98d2e47040f077e959b9e4f6e868b