Search Results - "Honscheid,  K."

Image analysis for cosmology: results from the GREAT10 Galaxy Challenge by Kitching, T. D., Balan, S. T., Bridle, S., Cantale, N., Courbin, F., Eifler, T., Gentile, M., Gill, M. S. S., Harmeling, S., Heymans, C., Hirsch, M., Honscheid, K., Kacprzak, T., Kirkby, D., Margala, D., Massey, R. J., Melchior, P., Nurbaeva, G., Patton, K., Rhodes, J., Rowe, B. T. P., Taylor, A. N., Tewes, M., Viola, M., Witherick, D., Voigt, L., Young, J., Zuntz, J.

“…In this paper, we present results from the weak-lensing shape measurement GRavitational lEnsing Accuracy Testing 2010 (GREAT10) Galaxy Challenge. This marks an…”
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DAHe white dwarfs from the DESI Survey by Manser, Christopher J, Gänsicke, Boris T, Inight, Keith, Robert, Akshay, Ahlen, S, Allende Prieto, C, Brooks, D, Cooper, A P, de la Macorra, A, Font-Ribera, A, Honscheid, K, Kisner, T, Landriau, M, Meisner, Aaron M, Miquel, R, Nie, Jundan, Poppett, C, Tarlé, Gregory, Zhou, Zhimin

“…ABSTRACT A new class of white dwarfs, dubbed DAHe, that present Zeeman-split Balmer lines in emission has recently emerged. However, the physical origin of…”
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Planting a Lyman alpha forest on AbacusSummit by Hadzhiyska, Boryana, Font-Ribera, A, Cuceu, A, Chabanier, S, Aguilar, J, Brooks, D, de la Macorra, A, Doel, P, Eisenstein, D J, Forero-Romero, J E, Gontcho A Gontcho, S, Honscheid, K, Kehoe, R, Landriau, M, Miquel, R, Nie, Jundan, Percival, W J, Rossi, G, Tarlé, Gregory, Zhou, Zhimin

“…ABSTRACT The full-shape correlations of the Lyman alpha (Ly α) forest contain a wealth of cosmological information through the Alcock–Paczyński effect…”
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The frequency of metal enrichment of cool helium-atmosphere white dwarfs using the DESI early data release by Manser, Christopher J, Gänsicke, Boris T, Izquierdo, Paula, Swan, Andrew, Najita, Joan, Rockosi, C, Carrillo, Andreia, Kim, Bokyoung, Xu, Siyi, Dey, Arjun, Aguilar, J, Ahlen, S, Blum, R, Brooks, D, Claybaugh, T, Dawson, K, de la Macorra, A, Doel, P, Gaztañaga, E, Gontcho A Gontcho, S, Honscheid, K, Kehoe, R, Kremin, A, Landriau, M, Le Guillou, L, Levi, Michael E, Li, T S, Meisner, A, Miquel, R, Nie, J, Rezaie, M, Rossi, G, Sanchez, E, Schubnell, M, Tarlé, G, Weaver, B A, Zhou, Z, Zou, H

“…ABSTRACT There is an overwhelming evidence that white dwarfs host planetary systems; revealed by the presence, disruption, and accretion of planetary bodies. A…”
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A Large Sample of Extremely Metal-poor Galaxies at z < 1 Identified from the DESI Early Data by Zou, Hu, Sui, Jipeng, Saintonge, Amélie, Scholte, Dirk, Moustakas, John, Siudek, Malgorzata, Dey, Arjun, Juneau, Stephanie, Guo, Weijian, Canning, Rebecca, Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., Dawson, K., de la Macorra, A., Doel, P., Forero-Romero, J. E., Gontcho A Gontcho, S., Honscheid, K., Landriau, M., Le Guillou, L., Manera, M., Meisner, A., Miquel, R., Nie, Jundan, Poppett, C., Rezaie, M., Rossi, G., Sanchez, E., Schubnell, M., Seo, H., Tarlé, G., Zhou, Zhimin, Zou, Siwei

“…Abstract Extremely metal-poor galaxies (XMPGs) at relatively low redshift are excellent laboratories for studying galaxy formation and evolution in the early…”
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New Measurements of the Lyα Forest Continuum and Effective Optical Depth with LyCAN and DESI Y1 Data by Turner, Wynne, Martini, Paul, Karaçaylı, Naim Göksel, Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., de la Macorra, A., Dey, A., Doel, P., Fanning, K., Forero-Romero, J . E., Gontcho A Gontcho, S., Gonzalez-Morales, A. X., Gutierrez, G., Guy, J., Herrera-Alcantar, H. K., Honscheid, K., Juneau, S., Kisner, T., Kremin, A., Lambert, A., Landriau, M., Le Guillou, L., Meisner, A., Miquel, R., Moustakas, J., Mueller, E., Muñoz-Gutiérrez, A., Myers, A. D., Nie, J., Niz, G., Poppett, C., Prada, F., Rezaie, M., Rossi, G., Sanchez, E., Schlafly, E. F., Schlegel, D., Schubnell, Michael F., Seo, H., Sprayberry, D., Tarlé, G., Weaver, B. A., Zou, H.

“…Abstract We present the Ly α Continuum Analysis Network (LyCAN), a convolutional neural network that predicts the unabsorbed quasar continuum within the…”
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Correcting Turbulence-induced Errors in Fiber Positioning for the Dark Energy Spectroscopic Instrument by Schlafly, E. F., Guy, J., Honscheid, K., Kent, S., Koposov, S. E., Aguilar, J., Ahlen, S., Bailey, S., Brooks, D., Claybaugh, T., Dawson, K., Doel, P., Fanning, K., Finkbeiner, D. P., Font-Ribera, A., Forero-Romero, J. E., Gontcho A Gontcho, S., Gutierrez, G., Kirkby, D., Kisner, T., Kremin, A., Landriau, M., Lasker, J., Le Guillou, L., Levi, M. E., de la Macorra, A., Martini, P., Meisner, A., Miquel, R., Moustakas, J., Niz, G., Prada, F., Rossi, G., Sanchez, E., Schubnell, M., Sharples, R., Sprayberry, D., Tarlé, G., Weaver, B. A., Zou, H.

“…Abstract Highly multiplexed, robotic, fiber-fed spectroscopic surveys are observing tens of millions of stars and galaxies. For many systems, accurate…”
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A striking relationship between dust extinction and radio detection in DESI QSOs: evidence for a dusty blow-out phase in red QSOs by Fawcett, V A, Alexander, D M, Brodzeller, A, Edge, A C, Rosario, D J, Myers, A D, Aguilar, J, Ahlen, S, Alfarsy, R, Brooks, D, Canning, R, Circosta, C, Dawson, K, de la Macorra, A, Doel, P, Fanning, K, Font-Ribera, A, Forero-Romero, J E, Gontcho A Gontcho, S, Guy, J, Harrison, C M, Honscheid, K, Juneau, S, Kehoe, R, Kisner, T, Kremin, A, Landriau, M, Manera, M, Meisner, A M, Miquel, R, Moustakas, J, Nie, J, Percival, W J, Poppett, C, Pucha, R, Rossi, G, Schlegel, D, Siudek, M, Tarlé, G, Weaver, B A, Zhou, Z, Zou, H

“…ABSTRACT We present the first eight months of data from our secondary target programme within the ongoing Dark Energy Spectroscopic Instrument (DESI) survey…”
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The BTeV experiment: Physics and detector by Honscheid, K.

“…AbstractExploring the large number of heavy quarks produced at Fermilab’s Tevatron collider, the BTeV experiment is designed to make precision measurements of…”
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Silicon as an unconventional detector in positron emission tomography by Clinthorne, Neal, Brzezinski, Karol, Chesi, Enrico, Cochran, Eric, Grkovski, Milan, Grošičar, Borut, Honscheid, Klaus, Huh, Sam, Kagan, Harris, Lacasta, Carlos, Linhart, Vladimir, Mikuž, Marko, Smith, D. Shane, Stankova, Vera, Studen, Andrej, Weilhammer, Peter, Žontar, Dejan

“…Positron emission tomography (PET) is a widely used technique in medical imaging and in studying small animal models of human disease. In the conventional…”
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Silicon detectors for combined MR–PET and MR–SPECT imaging by Studen, A., Brzezinski, K., Chesi, E., Cindro, V., Clinthorne, N.H., Cochran, E., Grošičar, B., Grkovski, M., Honscheid, K., Kagan, H., Lacasta, C., Llosa, G., Mikuž, M., Stankova, V., Weilhammer, P., Žontar, D.

“…Silicon based devices can extend PET–MR and SPECT–MR imaging to applications, where their advantages in performance outweigh benefits of high statistical…”
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AX-PET: A novel PET detector concept with full 3D reconstruction by Braem, A., Joram, C., Séguinot, J., Dissertori, G., Djambazov, L., Lustermann, W., Nessi-Tedaldi, F., Pauss, F., Schinzel, D., Solevi, P., Lacasta, C., Oliver, J.F., Rafecas, M., De Leo, R., Nappi, E., Vilardi, I., Chesi, E., Cochran, E., Honscheid, K., Kagan, H., Rudge, A., Smith, S., Weilhammer, P., Johnson, I., Renker, D., Clinthorne, N., Huh, S., Bolle, E., Stapnes, S., Meddi, F.

“…We describe the concept and first experimental tests of a novel 3D axial Positron Emission Tomography (PET) geometry. It allows for a new way of measuring the…”
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A device to measure the effects of strong magnetic fields on the image resolution of PET scanners by Burdette, D., Albani, D., Chesi, E., Clinthorne, N.H., Cochran, E., Honscheid, K., Huh, S.S., Kagan, H., Knopp, M., Lacasta, C., Mikuz, M., Schmalbrock, P., Studen, A., Weilhammer, P.

“…Very high resolution images can be achieved in small animal PET systems utilizing solid state silicon pad detectors. As these systems approach sub-millimeter…”
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Construction and tests of demonstrator modules for a 3-D axial PET system for brain or small animal imaging by Beltrame, P., Bolle, E., Braem, A., Casella, C., Chesi, E., Clinthorne, N., Cochran, E., De Leo, R., Dissertori, G., Djambazov, G., Fanti, V., Honscheid, K., Huh, S., Johnson, I., Joram, C., Kagan, H., Lustermann, W., Meddi, F., Nappi, E., Nessi-Tedaldi, F., Oliver, J.F., Pauss, P., Rafecas, M., Renker, D., Rudge, A., Schinzel, D., Schneider, T., Seguinot, J., Smith, S., Solevi, P., Stapnes, S., Weilhammer, P.

“…The design and construction of a PET camera module with high sensitivity, full 3-D spatial reconstruction and very good energy resolution is presented. The…”
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Last Results of a First Compton Probe Demonstrator by Llosa, G., Bernabeu, J., Burdette, D., Chesi, E., Clinthorne, N.H., Honscheid, K., Kagan, H., Lacasta, C., Mikuz, M., Modesto, P., Rogers, W.L., Studen, A., Weilhammer, P.

“…A first prostate probe prototype based on the Compton imaging technique has been developed, with a scatter detector composed of a stack of five thick silicon…”
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The AX-PET project: Demonstration of a high resolution axial 3D PET by Bolle, E., Braem, A., Casella, C., Chesi, E., Clinthorne, N., Cochran, E., De Leo, R., Dissertori, G., Djambazov, G., Fanti, V., Honscheid, K., Huh, S., Johnson, I., Joram, C., Kagan, H., Lustermann, W., Meddi, F., Nappi, E., Nessi-Tedaldi, F., Oliver, J.F., Pauss, P., Rafecas, M., Renker, D., Rudge, A., Schinzel, D., Schneider, T., Seguinot, J., Smith, S., Solevi, P., Stapnes, S., Weilhammer, P.

“…The AX-PET is a new geometrical concept for a high resolution 3D PET scanner, based on matrices of axially oriented LYSO crystals interleaved by stacks of WLS,…”
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STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408−5354 by Shajib, A J, Birrer, S, Treu, T, Agnello, A, Buckley-Geer, E J, Chan, J H H, Christensen, L, Lemon, C, Lin, H, Millon, M, Poh, J, Rusu, C E, Sluse, D, Spiniello, C, Chen, G C-F, Collett, T, Courbin, F, Fassnacht, C D, Frieman, J, Galan, A, Gilman, D, More, A, Anguita, T, Auger, M W, Bonvin, V, McMahon, R, Meylan, G, Wong, K C, Abbott, T M C, Annis, J, Avila, S, Bechtol, K, Brooks, D, Brout, D, Burke, D L, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, F J, Costanzi, M, da Costa, L N, De Vicente, J, Desai, S, Dietrich, J P, Doel, P, Drlica-Wagner, A, Evrard, A E, Finley, D A, Flaugher, B, Fosalba, P, García-Bellido, J, Gerdes, D W, Gruen, D, Gruendl, R A, Gschwend, J, Gutierrez, G, Hollowood, D L, Honscheid, K, Huterer, D, James, D J, Jeltema, T, Krause, E, Kuropatkin, N, Li, T S, Lima, M, MacCrann, N, Maia, M A G, Marshall, J L, Melchior, P, Miquel, R, Ogando, R L C, Palmese, A, Paz-Chinchón, F, Plazas, A A, Romer, A K, Roodman, A, Sako, M, Sanchez, E, Santiago, B, Scarpine, V, Schubnell, M, Scolnic, D, Serrano, S, Sevilla-Noarbe, I, Smith, M, Soares-Santos, M, Suchyta, E, Tarle, G, Thomas, D, Walker, A R, Zhang, Y

“…ABSTRACT We present a blind time-delay cosmographic analysis for the lens system DES J0408−5354. This system is extraordinary for the presence of two sets of…”
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Dark Energy Survey Year 3 results: redshift calibration of the weak lensing source galaxies by Myles, J, Alarcon, A, Amon, A, Sánchez, C, DeRose, J, McCullough, J, Gruen, D, Bernstein, G M, Troxel, M A, Dodelson, S, MacCrann, N, Yin, B, Raveri, M, Amara, A, Becker, M R, Choi, A, Cordero, J, Eckert, K, Gatti, M, Giannini, G, Gschwend, J, Gruendl, R A, Harrison, I, Hartley, W G, Huff, E M, Lin, H, Masters, D, Miquel, R, Prat, J, Roodman, A, Rykoff, E S, Sevilla-Noarbe, I, Sheldon, E, Wechsler, R H, Yanny, B, Abbott, T M C, Aguena, M, Allam, S, Annis, J, Bacon, D, Bertin, E, Bhargava, S, Bridle, S L, Brooks, D, Burke, D L, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Conselice, C, Costanzi, M, Crocce, M, da Costa, L N, Pereira, M E S, Desai, S, Diehl, H T, Eifler, T F, Elvin-Poole, J, Evrard, A E, Ferrero, I, Ferté, A, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gaztanaga, E, Giannantonio, T, Hinton, S R, Honscheid, K, Hoyle, B, Huterer, D, James, D J, Krause, E, Kuehn, K, Lahav, O, Lima, M, Maia, M A G, Marshall, J L, Martini, P, Melchior, P, Menanteau, F, Mohr, J J, Muir, J, Ogando, R L C, Palmese, A, Paz-Chinchón, F, Plazas, A A, Rodriguez-Monroy, M, Samuroff, S, Sanchez, E, Scarpine, V, Secco, L F, Serrano, S, Smith, M, Soares-Santos, M, Swanson, M E C, Tarle, G, Thomas, D, To, C, Weller, J, Wester, W

“…ABSTRACT Determining the distribution of redshifts of galaxies observed by wide-field photometric experiments like the Dark Energy Survey (DES) is an essential…”
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Target Selection and Validation of DESI Emission Line Galaxies by Raichoor, A., Moustakas, J., Newman, Jeffrey A., Karim, T., Ahlen, S., Alam, Shadab, Bailey, S., Brooks, D., Dawson, K., de la Macorra, A., de Mattia, A., Dey, A., Dey, Biprateep, Dhungana, G., Eftekharzadeh, S., Eisenstein, D. J., Fanning, K., Font-Ribera, A., García-Bellido, J., Gaztañaga, E., A Gontcho, S. Gontcho, Guy, J., Honscheid, K., Ishak, M., Kehoe, R., Kisner, T., Kremin, Anthony, Lan, Ting-Wen, Landriau, M., Le Guillou, L., Levi, Michael E., Magneville, C., Manera, M., Martini, P., Meisner, Aaron M., Myers, Adam D., Nie, Jundan, Palanque-Delabrouille, N., Percival, W. J., Poppett, C., Prada, F., Ross, A. J., Ruhlmann-Kleider, V., Sabiu, C. G., Schlafly, E. F., Schlegel, D., Tarlé, Gregory, Weaver, B. A., Yèche, Christophe, Zhou, Rongpu, Zhou, Zhimin, Zou, H.

“…Abstract The Dark Energy Spectroscopic Instrument (DESI) will precisely constrain cosmic expansion and the growth of structure by collecting ∼40 million…”
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Dark Energy Survey Y3 results: blending shear and redshift biases in image simulations by MacCrann, N, Becker, M R, McCullough, J, Amon, A, Gruen, D, Jarvis, M, Choi, A, Troxel, M A, Sheldon, E, Yanny, B, Herner, K, Dodelson, S, Zuntz, J, Eckert, K, Rollins, R P, Varga, T N, Bernstein, G M, Gruendl, R A, Harrison, I, Hartley, W G, Sevilla-Noarbe, I, Pieres, A, Bridle, S L, Myles, J, Alarcon, A, Everett, S, Sánchez, C, Huff, E M, Tarsitano, F, Gatti, M, Secco, L F, Abbott, T M C, Aguena, M, Allam, S, Annis, J, Bacon, D, Bertin, E, Brooks, D, Burke, D L, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Costanzi, M, Crocce, M, Pereira, M E S, De Vicente, J, Desai, S, Diehl, H T, Dietrich, J P, Doel, P, Eifler, T F, Ferrero, I, Ferté, A, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gaztanaga, E, Gerdes, D W, Giannantonio, T, Gschwend, J, Gutierrez, G, Hinton, S R, Hollowood, D L, Honscheid, K, James, D J, Lahav, O, Lima, M, Maia, M A G, March, M, Marshall, J L, Martini, P, Melchior, P, Menanteau, F, Miquel, R, Mohr, J J, Morgan, R, Muir, J, Ogando, R L C, Palmese, A, Paz-Chinchón, F, Plazas, A A, Rodriguez-Monroy, M, Roodman, A, Samuroff, S, Sanchez, E, Scarpine, V, Serrano, S, Smith, M, Soares-Santos, M, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, To, C, Wilkinson, R D

“…ABSTRACT As the statistical power of galaxy weak lensing reaches per cent level precision, large, realistic, and robust simulations are required to calibrate…”
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