Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Noble, Allison G."'
Autor:
Calzadilla, Michael S., McDonald, Michael, Benson, Bradford A., Bleem, Lindsey E., Croston, Judith H., Donahue, Megan, Edge, Alastair C., Floyd, Benjamin, Garmire, Gordon P., Hlavacek-Larrondo, Julie, Huynh, Minh T., Khullar, Gourav, Kraft, Ralph P., McNamara, Brian R., Noble, Allison G., Romero, Charles E., Ruppin, Florian, Somboonpanyakul, Taweewat, Voit, G. Mark
We present a multi-wavelength study of the brightest cluster galaxies (BCGs) in a sample of the 95 most massive galaxy clusters selected from South Pole Telescope (SPT) Sunyaev-Zeldovich (SZ) survey. Our sample spans a redshift range of 0.3 < z < 1.7
Externí odkaz:
http://arxiv.org/abs/2311.00396
Autor:
Kim, Keunho J., Bayliss, Matthew B., Noble, Allison G., Khullar, Gourav, Cronk, Ethan, Roberson, Joshua, Ansarinejad, Behzad, Bleem, Lindsey E., Floyd, Benjamin, Grandis, Sebastian, Mahler, Guillaume, McDonald, Michael A., Reichardt, Christian L., Saro, Alexandro, Sharon, Keren, Somboonpanyakul, Taweewat, Strazzullo, Veronica
The environments where galaxies reside crucially shape their star formation histories. We investigate a large sample of 1626 cluster galaxies located within 105 galaxy clusters spanning a large range in redshift ($0.26 < z < 1.13)$. The galaxy cluste
Externí odkaz:
http://arxiv.org/abs/2207.12491
Autor:
Barfety, Capucine, Valin, Félix-Antoine, Webb, Tracy M. A., Yun, Min, Shipley, Heath, Boone, Kyle, Hayden, Brian, Hlavacek-Larrondo, Julie, Muzzin, Adam, Noble, Allison G., Perlmutter, Saul, Rhea, Carter, Wilson, Gillian, Yee, H. K. C
The formation of the stellar mass within galaxy cluster cores is a poorly understood process. It features the complicated physics of cooling flows, AGN feedback, star formation and more. Here, we study the growth of the stellar mass in the vicinity o
Externí odkaz:
http://arxiv.org/abs/2203.13764
Autor:
Williams, Christina C., Alberts, Stacey, Spilker, Justin S., Noble, Allison G., Stefanon, Mauro, Willmer, Christopher N. A., Bezanson, Rachel, Narayanan, Desika, Whitaker, Katherine E.
We report the serendipitous discovery of an overdensity of CO emitters in an X-ray-identified cluster (Log$_{10}$M$_{\rm halo}/M_{\odot}\sim13.6$ at z=1.3188) using ALMA. We present spectroscopic confirmation of 6 new cluster members exhibiting CO(2-
Externí odkaz:
http://arxiv.org/abs/2201.01304
Autor:
Matharu, Jasleen, Muzzin, Adam, Brammer, Gabriel B., Nelson, Erica J., Auger, Matthew W., Hewett, Paul C., van der Burg, Remco, Balogh, Michael, Demarco, Ricardo, Marchesini, Danilo, Noble, Allison G., Rudnick, Gregory, van der Wel, Arjen, Wilson, Gillian, Yee, Howard K. C.
We present and publicly release (https://www.gclasshst.com) the first spatially resolved H$\alpha$ maps of star-forming cluster galaxies at $z\sim1$, made possible with the Wide Field Camera 3 (WFC3) G141 grism on the Hubble Space Telescope (HST). Us
Externí odkaz:
http://arxiv.org/abs/2109.06186
Autor:
Matharu, Jasleen, Muzzin, Adam, Brammer, Gabriel B., van der Burg, Remco F. J., Auger, Matthew W., Hewett, Paul C., Chan, Jeffrey C. C., Demarco, Ricardo, van Dokkum, Pieter, Marchesini, Danilo, Nelson, Erica J., Noble, Allison G., Wilson, Gillian
Minor mergers have been proposed as the driving mechanism for the size growth of quiescent galaxies with decreasing redshift. The process whereby large star-forming galaxies quench and join the quiescent population at the large size end has also been
Externí odkaz:
http://arxiv.org/abs/1912.05551
Autor:
Webb, Tracy, Lowenthal, James, Yun, Min, Noble, Allison G., Muzzin, Adam, Wilson, Gillian, Yee, H. K. C., Cybulski, Ryan
We report the detection of CO(2-1) emission coincident with the brightest cluster galaxy (BCG) of the high-redshift galaxy cluster SpARCS1049+56, with the Redshift Search Receiver (RSR) on the Large Millimetre Telescope (LMT). We confirm a spectrosco
Externí odkaz:
http://arxiv.org/abs/1706.01366
Autor:
Noble, Allison G.
Written for the Dept. of Physics. Title from title page of PDF (viewed 2010/04/07). Includes bibliographical references.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astron.J.135:326-332,2008
A subgroup of dwarf galaxies have characteristics of a possible evolutionary transition between star-forming systems and dwarf ellipticals. These systems host significant starbursts in combination with smooth, elliptical outer envelopes and small HI
Externí odkaz:
http://arxiv.org/abs/0710.4094