Search Results - "Mann, Robert G."

Identification of low surface brightness tidal features in galaxies using convolutional neural networks by Walmsley, Mike, Ferguson, Annette M N, Mann, Robert G, Lintott, Chris J

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The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5 by Furnell, Kate E, Collins, Chris A, Kelvin, Lee S, Baldry, Ivan K, James, Phil A, Manolopoulou, Maria, Mann, Robert G, Giles, Paul A, Bermeo, Alberto, Hilton, Matthew, Wilkinson, Reese, Romer, A Kathy, Vergara, Carlos, Bhargava, Sunayana, Stott, John P, Mayers, Julian, Viana, Pedro

“…ABSTRACT We estimate the intracluster light (ICL) component within a sample of 18 clusters detected in the XMM Cluster Survey (XCS) data using the deep (∼26.8…”
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Early assembly of the most massive galaxies by Hilton, Matt, Collins, Chris A, Nichol, Robert C, Romer, A. Kathy, Stott, John P, Mann, Robert G, Kay, Scott T, Lloyd-Davies, Ed, Davidson, Michael, Liddle, Andrew, Hosmer, Mark, Mehrtens, Nicola, West, Michael J, Viana, Pedro T. P, Miller, Christopher J, Hoyle, Ben, Sahlén, Martin, Stanford, S. Adam

“…The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging…”
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The XMM Cluster Survey: X-ray analysis methodology by Lloyd-Davies, E. J., Romer, A. Kathy, Mehrtens, Nicola, Hosmer, Mark, Davidson, Michael, Sabirli, Kivanc, Mann, Robert G., Hilton, Matt, Liddle, Andrew R., Viana, Pedro T. P., Campbell, Heather C., Collins, Chris A., Dubois, E. Naomi, Freeman, Peter, Harrison, Craig D., Hoyle, Ben, Kay, Scott T., Kuwertz, Emma, Miller, Christopher J., Nichol, Robert C., Sahlén, Martin, Stanford, S. A., Stott, John P.

“…The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Its main aims…”
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High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey by Hughes, David H, Serjeant, Stephen, Dunlop, James, Rowan-Robinson, Michael, Blain, Andrew, Mann, Robert G, Ivison, Rob, Peacock, John, Efstathiou, Andreas, Gear, Walter, Oliver, Seb, Lawrence, Andy, Longair, Malcolm, Goldschmidt, Pippa, Jenness, Tim

“…In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of…”
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Uncovering tidal treasures: automated classification of faint tidal features in DECaLS data by Gordon, Alexander J, Ferguson, Annette M N, Mann, Robert G

“…ABSTRACT Tidal features are a key observable prediction of the hierarchical model of galaxy formation and contain a wealth of information about the properties…”
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The XMM Cluster Survey: testing chameleon gravity using the profiles of clusters by Wilcox, Harry, Bacon, David, Nichol, Robert C., Rooney, Philip J., Terukina, Ayumu, Romer, A. Kathy, Koyama, Kazuya, Zhao, Gong-Bo, Hood, Ross, Mann, Robert G., Hilton, Matt, Manolopoulou, Maria, Sahlén, Martin, Collins, Chris A., Liddle, Andrew R., Mayers, Julian A., Mehrtens, Nicola, Miller, Christopher J., Stott, John P., Viana, Pedro T. P.

“…The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would…”
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The XMM Cluster Survey: optical analysis methodology and the first data release by Mehrtens, Nicola, Romer, A. Kathy, Hilton, Matt, Lloyd-Davies, E. J., Miller, Christopher J., Stanford, S. A., Hosmer, Mark, Hoyle, Ben, Collins, Chris A., Liddle, Andrew R., Viana, Pedro T. P., Nichol, Robert C., Stott, John P., Dubois, E. Naomi, Kay, Scott T., Sahlén, Martin, Young, Owain, Short, C. J., Christodoulou, L., Watson, William A., Davidson, Michael, Harrison, Craig D., Baruah, Leon, Smith, Mathew, Burke, Claire, Mayers, Julian A., Deadman, Paul-James, Rooney, Philip J., Edmondson, Edward M., West, Michael, Campbell, Heather C., Edge, Alastair C., Mann, Robert G., Sabirli, Kivanc, Wake, David, Benoist, Christophe, da Costa, Luiz, Maia, Marcio A. G., Ogando, Ricardo

“…The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Its main aims…”
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The XMM Cluster Survey: Galaxy Morphologies and the Color-Magnitude Relation in XMMXCS J2215.9 – 1738 at z = 1.46 by Hilton, Matt, Stanford, S. Adam, Stott, John P, Collins, Chris A, Hoyle, Ben, Davidson, Michael, Hosmer, Mark, Kay, Scott T, Liddle, Andrew R, Lloyd-Davies, Ed, Mann, Robert G, Mehrtens, Nicola, Miller, Christopher J, Nichol, Robert C, Romer, A. Kathy, Sabirli, Kivanc, Sahlén, Martin, Viana, Pedro T. P, West, Michael J, Barbary, Kyle, Dawson, Kyle S, Meyers, Joshua, Perlmutter, Saul, Rubin, David, Suzuki, Nao

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The "Contact of Living Souls": Shepard Gilbert's Civics Education in Reconstruction South Carolina by MANN, ROBERT G.

“…Just after the Civil War, a Harvard graduate from Massachusetts receives a civics education from former slaves in South Carolina that radically transforms his…”
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The XMM Cluster Survey: evolution of the velocity dispersion–temperature relation over half a Hubble time by Wilson, Susan, Hilton, Matt, Rooney, Philip J., Caldwell, Caroline, Kay, Scott T., Collins, Chris A., McCarthy, Ian G., Romer, A. Kathy, Bermeo, Alberto, Bernstein, Rebecca, da Costa, Luiz, Gifford, Daniel, Hollowood, Devon, Hoyle, Ben, Jeltema, Tesla, Liddle, Andrew R., Maia, Marcio A. G, Mann, Robert G., Mayers, Julian A., Mehrtens, Nicola, Miller, Christopher J., Nichol, Robert C., Ogando, Ricardo, Sahlén, Martin, Stahl, Benjamin, Stott, John P., Thomas, Peter A., Viana, Pedro T. P., Wilcox, Harry

“…We measure the evolution of the velocity dispersion–temperature (σv–T X) relation up to z = 1 using a sample of 38 galaxy clusters drawn from the XMM Cluster…”
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The XMM Cluster Survey: A Massive Galaxy Cluster at z = 1.45 by Stanford, S. A, Romer, A. Kathy, Sabirli, Kivanc, Davidson, Michael, Hilton, Matt, Viana, Pedro T. P, Collins, Chris A, Kay, Scott T, Liddle, Andrew R, Mann, Robert G, Miller, Christopher J, Nichol, Robert C, West, Michael J, Conselice, Christopher J, Spinrad, Hyron, Stern, Daniel, Bundy, Kevin

“…We report the discovery of XMMXCS J2215.9-1738, a massive galaxy cluster at z = 1.45, which was found in the XMM Cluster Survey. The cluster candidate was…”
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The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters by Mehrtens, Nicola, Romer, A Kathy, Nichol, Robert C, Collins, Chris A, Sahlen, Martin, Rooney, Philip J, Mayers, Julian A, Bermeo-Hernandez, A, Bristow, Martyn, Capozzi, Diego, Christodoulou, L, Comparat, Johan, Hilton, Matt, Hoyle, Ben, Kay, Scott T, Liddle, Andrew R, Mann, Robert G, Masters, Karen, Miller, Christopher J, Parejko, John K, Prada, Francisco, Ross, Ashley J, Schneider, Donald P, Stott, John P, Streblyanska, Alina, Viana, Pedro TP, White, Martin, Wilcox, Harry, Zehavi, Idit

“…We present a direct measurement of the mean halo occupation distribution (HOD) of galaxies taken from the eleventh data release (DR11) of the Sloan Digital Sky…”
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The XMM Cluster Survey: evidence for energy injection at high redshift from evolution of the X-ray luminosity-temperature relation by Hilton, Matt, Romer, A. Kathy, Kay, Scott T., Mehrtens, Nicola, Lloyd-Davies, E. J., Thomas, Peter A., Short, Chris J., Mayers, Julian A., Rooney, Philip J., Stott, John P., Collins, Chris A., Harrison, Craig D., Hoyle, Ben, Liddle, Andrew R., Mann, Robert G., Miller, Christopher J., Sahlén, Martin, Viana, Pedro T. P., Davidson, Michael, Hosmer, Mark, Nichol, Robert C., Sabirli, Kivanc, Stanford, S. A., West, Michael J.

“…Abstract We measure the evolution of the X-ray luminosity-temperature (L X − T) relation since z ∼ 1.5 using a sample of 211 serendipitously detected galaxy…”
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The XMM Cluster Survey: forecasting cosmological and cluster scaling-relation parameter constraints by Sahlén, Martin, Viana, Pedro T. P., Liddle, Andrew R., Romer, A. Kathy, Davidson, Michael, Hosmer, Mark, Lloyd-Davies, Ed, Sabirli, Kivanc, Collins, Chris A., Freeman, Peter E., Hilton, Matt, Hoyle, Ben, Kay, Scott T., Mann, Robert G., Mehrtens, Nicola, Miller, Christopher J., Nichol, Robert C., Stanford, S. Adam, West, Michael J.

“…We forecast the constraints on the values of σ8, Ωm and cluster scaling-relation parameters which we expect to obtain from the XMM Cluster Survey (XCS). We…”
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A Serendipitous Galaxy Cluster Survey with XMM: Expected Catalog Properties and Scientific Applications by Romer, A. Kathy, Viana, Pedro T. P, Liddle, Andrew R, Mann, Robert G

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The XMM Cluster Survey: The Dynamical State of XMMXCS J2215.9–1738 at z = 1.457 by Hilton, Matt, Collins, Chris A, Stanford, S. Adam, Lidman, Chris, Dawson, Kyle S, Davidson, Michael, Kay, Scott T, Liddle, Andrew R, Mann, Robert G, Miller, Christopher J, Nichol, Robert C, Romer, A. Kathy, Sabirli, Kivanc, Viana, Pedro T. P, West, Michael J

“…We present new spectroscopic observations of the most distant X-ray-selected galaxy cluster currently known, XMMXCS J2215.9-1738 at z = 1.457, obtained with…”
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The European Large Area ISO Survey — II. Mid-infrared extragalactic source counts by Serjeant, Stephen, Oliver, Seb, Rowan-Robinson, Michael, Crockett, Hans, Missoulis, Vasilis, Sumner, Tim, Gruppioni, Carlotta, Mann, Robert G., Eaton, Nick, Elbaz, David, Clements, David L., Baker, Amanda, Efstathiou, Andreas, Cesarsky, Catherine, Danese, Luigi, Franceschini, Alberto, Genzel, Reinhardt, Lawrence, Andy, Lemke, Dietrich, McMahon, Richard G., Miley, George, Puget, Jean-Loup, Rocca-Volmerange, Brigitte

“…We present preliminary source counts at 6.7 and 15 μm from the preliminary analysis of the European Large Area ISO Survey, with limiting flux densities of ∼2…”
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Dust and Gas Obscuration in ELAIS Deep X-Ray Survey Reddened Quasars by Willott, Chris J, Simpson, Chris, Almaini, Omar, Johnson, Olivia, Lawrence, Andrew, Dunlop, James S, Roche, Nathan D, Mann, Robert G, Manners, James C, González-Solares, Eduardo, Pérez-Fournon, Ismael, Ivison, Rob J, Serjeant, Stephen, Oliver, Seb J, McMahon, Richard G, Rowan-Robinson, Michael

“…Hard X-ray surveys have uncovered a large population of heavily obscured AGNs. They also reveal a population of quasars with moderate obscuration at both…”
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THE XMM CLUSTER SURVEY: GALAXY MORPHOLOGIES AND THE COLOR-MAGNITUDE RELATION IN XMMXCS J2215.9―1738 AT z = 1.46 by HILTON, Matt, STANFORD, S. Adam, MANN, Robert G, MEHRTENS, Nicola, MILLER, Christopher J, NICHOL, Robert C, ROMER, A. Kathy, SABIRLI, Kivanc, SAHLEN, Martin, VIANA, Pedro T. P, WEST, Michael J, BARBARY, Kyle, STOTT, John P, DAWSON, Kyle S, MEYERS, Joshua, PERLMUTTER, Saul, RUBIN, David, SUZUKI, Nao, COLLINS, Chris A, HOYLE, Ben, DAVIDSON, Michael, HOSMER, Mark, KAY, Scott T, LIDDLE, Andrew R, LLOYD-DAVIES, E. D

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