Showing 1 - 20 results of 211 for search '"Analyse ', query time: 0.15s Refine Results
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    Diminished diversity-of-thought in a standard large language model by Park, Peter S., Schoenegger, Philipp, Zhu, Chongyang

    Published 2024
    “…Based on our pre-registered analyses, we find that among the eight studies we could analyse, our GPT sample replicated 37.5% of the original results and 37.5% of the Many Labs 2 results. …”
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  4. 4

    DAQExpert the service to increase CMS data-taking efficiency by Paus, Christoph

    Published 2022
    “…It pinpoints data flow problems, and recovers them automatically or after given operator approval. We analyse the CMS downtime in the 2018 run focusing on what was improved with the introduction of automated recovery; present challenges and design of encoding the expert knowledge into automated recovery jobs. …”
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  5. 5

    Simulating the dust content of galaxies: successes and failures by McKinnon, Ryan, Torrey, Paul, Vogelsberger, Mark, Hayward, Christopher C, Marinacci, Federico

    Published 2021
    “…Moreover, we estimate the 850 μm number density functions for simulated galaxies and analyse the relation between dust-to-stellar flux and mass ratios at z = 0. …”
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    Top-quark physics at the CLIC electron-positron linear collider by The CLICdp Collaboration

    Published 2021
    “…Operation above 1 TeV leads to more highly collimated jet environments where dedicated methods are used to analyse the jet constituents. These techniques enable studies of the top-quark pair production, and hence the sensitivity to BSM physics, to be extended to higher energies. …”
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    Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts by Safarzadeh, Mohammadtaher, Ji, Alexander P, Dooley, Gregory Alan, Frebel, Anna L., Scannapieco, Evan, Gómez, Facundo A, O'Shea, Brian W

    Published 2019
    “…To find such candidates, we analyse the merger trees of Milky Way type haloes from the high-resolution Caterpillar suite of dark matter only simulations. …”
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    X-ray signatures of black hole feedback: hot galactic atmospheres in IllustrisTNG and X-ray observations by Truong, Nhut, Pillepich, Annalisa, Werner, Norbert, Nelson, Dylan, Lakhchaura, Kiran, Weinberger, Rainer, Springel, Volker, Vogelsberger, Mark, Hernquist, Lars

    Published 2022
    “…In this work, we study the properties of this hot X-ray emitting medium using the IllustrisTNG cosmological simulations. We analyse their mock X-ray spectra, obtained from the diffuse and metal-enriched gas in TNG100 and TNG50, and compare the results with X-ray observations of nearby early-type galaxies. …”
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  10. 10

    On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies by Suresh, Joshua, Rubin, Kate HR, Kannan, Rahul, Werk, Jessica K, Hernquist, Lars, Vogelsberger, Mark

    Published 2021
    “…© 2016 The Authors. We analyse the mass, temperature, metal enrichment, and OVI abundance of the circumgalactic medium (CGM) around z ~ 0.2 galaxies of mass 109M⊙ < M* < 1011.5M⊙ in the Illustris simulation. …”
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    Galaxy formation with BECDM – I. Turbulence and relaxation of idealized haloes by Mocz, Philip, Vogelsberger, Mark, Robles, Victor H, Zavala, Jesús, Boylan-Kolchin, Michael, Fialkov, Anastasia, Hernquist, Lars

    Published 2021
    “…The haloes also exhibit a conspicuous turbulent behaviour driven by the continuous reconnection of vortex lines due to wave interference. We analyse the turbulence 1D velocity power spectrum and find a k-1.1 power law. …”
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    The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation by Genel, Shy, Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Pakmor, Rüdiger, Weinberger, Rainer, Hernquist, Lars, Naiman, Jill, Vogelsberger, Mark, Marinacci, Federico, Torrey, Paul

    Published 2021
    “…Published by Oxford University Press on behalf of the Royal Astronomical Society. We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the IllustrisTNG simulation suite. …”
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    Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2 by Ricker, George R, Seager, Sara

    Published 2022
    “…We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic chemically peculiar A-type stars. We analyse TESS 2-min cadence data from sectors 1 and 2 on a sample of 83 stars. …”
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    Shock finding on a moving-mesh – II. Hydrodynamic shocks in the Illustris universe by Schaal, Kevin, Springel, Volker, Pakmor, Rüdiger, Pfrommer, Christoph, Nelson, Dylan, Vogelsberger, Mark, Genel, Shy, Pillepich, Annalisa, Sijacki, Debora, Hernquist, Lars

    Published 2017
    “…In this work, we identify and analyse shocks in the Illustris simulation, and contrast the results with those of non-radiative runs. …”
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    First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium by Naiman, Jill P, Pillepich, Annalisa, Springel, Volker, Ramirez-Ruiz, Enrico, Torrey, Paul A., Vogelsberger, Mark, Pakmor, Rüdiger, Nelson, Dylan, Marinacci, Federico, Hernquist, Lars, Weinberger, Rainer, Genel, Shy

    Published 2022
    “…Here we investigate the elemental distributions of stars in the IllustrisTNG simulations. We analyse the abundance ratios of magnesium and europium in Milky Way-like galaxies from the TNG100 simulation (stellar masses log (M*/M⊙) ~ 9.7-11.2). …”
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    Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG by Habouzit, Mélanie, Genel, Shy, Somerville, Rachel S, Kocevski, Dale, Hirschmann, Michaela, Dekel, Avishai, Choi, Ena, Nelson, Dylan, Pillepich, Annalisa, Hernquist, Lars, Vogelsberger, Mark, Weinberger, Rainer, Springel, Volker, Vogelsberger, Mark, Torrey, Paul A.

    Published 2019
    “…We study galaxy star formation activity and structural properties, and design sample-dependent criteria to identify different galaxy types (star-forming/quiescent, extended/compact) that we apply both to the simulations and observations from the candels fields. We analyse how the simulated and observed galaxies populate the specific star formation rate - stellar mass surface density diagram. …”
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    Halo mass and assembly history exposed in the faint outskirts: the stellar and dark matter haloes of Illustris galaxies by Pillepich, Annalisa, Vogelsberger, Mark, Deason, Alis, Rodriguez-Gomez, Vicente, Genel, Shy, Nelson, Dylan, Torrey, Paul, Sales, Laura V., Marinacci, Federico, Springel, Volker, Sijacki, Debora, Hernquist, Lars

    Published 2015
    “…We characterize the stellar haloes by means of the logarithmic slope of the spherically averaged stellar density profiles, α[subscript STARS] at z = 0, and we relate these slopes to the properties of the underlying dark matter (DM) haloes, their central galaxies, and their assembly histories. We analyse a sample of ∼5000 galaxies resolved with more than 5 × 10[superscript 4] particles each, and spanning a variety of morphologies and halo masses (3 × 10[superscript 11] ≤ M[subscript vir] ≲ 10[superscript 14]M[subscript ⊙]). …”
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    Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample by Percival, Will J., Reid, Beth A., Eisenstein, Daniel J., Bahcall, Neta A., Budavari, Tamas, Frieman, Joshua A., Fukugita, Masataka, Gunn, James E., Ivezic, Zeljko, Knapp, Gillian R., Kron, Richard G., Loveday, Jon, Lupton, Robert H., McKay, Timothy A., Meiksin, Avery, Nichol, Robert C., Pope, Adrian C., Schlegel, David J., Schneider, Donald P., Spergel, David N., Stoughton, Chris, Strauss, Michael A., Szalay, Alexander S., Tegmark, Max Erik, Vogeley, Michael S., Weinberg, David H., York, Donald G., Zehavi, Idit

    Published 2013
    “…The spectroscopic Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) galaxy sample represents the final set of galaxies observed using the original SDSS target selection criteria. We analyse the clustering of galaxies within this sample, including both the luminous red galaxy and main samples, and also include the 2-degree Field Galaxy Redshift Survey data. …”
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    A roadmap for HEP software and computing R&D for the 2020s by Albrecht, Johannes, Alves, Antonio A, Amadio, Guilherme, Andronico, Giuseppe, Anh-Ky, Nguyen, Aphecetche, Laurent, Apostolakis, John, Asai, Makoto, Atzori, Luca, Babik, Marian, Bagliesi, Giuseppe, Bandieramonte, Marilena, Banerjee, Sunanda, Barisits, Martin, Bauerdick, Lothar A T, Belforte, Stefano, Benjamin, Douglas, Bernius, Catrin, Bhimji, Wahid, Bianchi, Riccardo M, Bird, Ian, Biscarat, Catherine, Blomer, Jakob, Bloom, Kenneth, Boccali, Tommaso, Bockelman, Brian, Bold, Tomasz, Bonacorsi, Daniele, Boveia, Antonio, Bozzi, Concezio, Bracko, Marko, Britton, David, Buckley, Andy, Buncic, Predrag, Calafiura, Paolo, Campana, Simone, Canal, Philippe, Canali, Luca, Carlino, Gianpaolo, Castro, Nuno, Cattaneo, Marco, Cerminara, Gianluca, Cervantes Villanueva, Javier, Chang, Philip, Chapman, John, Chen, Gang, Childers, Taylor, Clarke, Peter, Clemencic, Marco, Cogneras, Eric, Coles, Jeremy, Collier, Ian, Colling, David, Corti, Gloria, Cosmo, Gabriele, Costanzo, Davide, Couturier, Ben, Cranmer, Kyle, Cranshaw, Jack, Cristella, Leonardo, Crooks, David, Crépé-Renaudin, Sabine, Currie, Robert, Dallmeier-Tiessen, Sünje, De, Kaushik, De Cian, Michel, De Roeck, Albert, Delgado Peris, Antonio, Derue, Frédéric, Di Girolamo, Alessandro, Di Guida, Salvatore, Dimitrov, Gancho, Doglioni, Caterina, Dotti, Andrea, Duellmann, Dirk, Duflot, Laurent, Dykstra, Dave, Dziedziniewicz-Wojcik, Katarzyna, Dziurda, Agnieszka, Egede, Ulrik, Elmer, Peter, Elmsheuser, Johannes, Elvira, V. D, Eulisse, Giulio, Farrell, Steven, Ferber, Torben, Filipcic, Andrej, Fisk, Ian, Fitzpatrick, Conor, Flix, José, Formica, Andrea, Forti, Alessandra, Franzoni, Giovanni, Frost, James, Fuess, Stu, Gaede, Frank, Ganis, Gerardo, Gardner, Robert, Garonne, Vincent, Gellrich, Andreas, Genser, Krzysztof, George, Simon, Geurts, Frank, Gheata, Andrei, Gheata, Mihaela, Giacomini, Francesco, Giagu, Stefano, Giffels, Manuel, Gingrich, Douglas, Girone, Maria, Gligorov, Vladimir V, Glushkov, Ivan, Gohn, Wesley, Gonzalez Lopez, Jose B, González Caballero, Isidro, González Fernández, Juan R, Govi, Giacomo, Grandi, Claudio, Grasland, Hadrien, Gray, Heather, Grillo, Lucia, Guan, Wen, Gutsche, Oliver, Gyurjyan, Vardan, Hanushevsky, Andrew, Hariri, Farah, Hartmann, Thomas, Harvey, John, Hauth, Thomas, Hegner, Benedikt, Heinemann, Beate, Heinrich, Lukas, Heiss, Andreas, Hernández, José M, Hildreth, Michael, Hodgkinson, Mark, Hoeche, Stefan, Holzman, Burt, Hristov, Peter, Huang, Xingtao, Ivanchenko, Vladimir N, Ivanov, Todor, Iven, Jan, Jashal, Brij, Jayatilaka, Bodhitha, Jones, Roger, Jouvin, Michel, Jun, Soon Y, Kagan, Michael, Kalderon, Charles W, Kane, Meghan, Karavakis, Edward, Katz, Daniel S, Kcira, Dorian, Keeble, Oliver, Kersevan, Borut P, Kirby, Michael, Klimentov, Alexei, Klute, Markus, Komarov, Ilya, Konstantinov, Dmitri, Koppenburg, Patrick, Kowalkowski, Jim, Kreczko, Luke, Kuhr, Thomas, Kutschke, Robert, Kuznetsov, Valentin, Lampl, Walter, Lancon, Eric, Lange, David, Lassnig, Mario, Laycock, Paul, Leggett, Charles, Letts, James, Lewendel, Birgit, Li, Teng, Lima, Guilherme, Linacre, Jacob, Linden, Tomas, Livny, Miron, Lo Presti, Giuseppe, Lopienski, Sebastian, Love, Peter, Lyon, Adam, Magini, Nicolò, Marshall, Zachary L, Martelli, Edoardo, Martin-Haugh, Stewart, Mato, Pere, Mazumdar, Kajari, McCauley, Thomas, McFayden, Josh, McKee, Shawn, McNab, Andrew, Mehdiyev, Rashid, Meinhard, Helge, Menasce, Dario, Mendez Lorenzo, Patricia, Mete, Alaettin S, Michelotto, Michele, Mitrevski, Jovan, Moneta, Lorenzo, Morgan, Ben, Mount, Richard, Moyse, Edward, Murray, Sean, Nairz, Armin, Neubauer, Mark S, Norman, Andrew, Novaes, Sérgio, Novak, Mihaly, Oyanguren, Arantza, Ozturk, Nurcan, Pacheco Pages, Andres, Paganini, Michela, Pansanel, Jerome, Pascuzzi, Vincent R, Patrick, Glenn, Pearce, Alex, Pearson, Ben, Pedro, Kevin, Perdue, Gabriel, Perez-Calero Yzquierdo, Antonio, Perrozzi, Luca, Petersen, Troels, Petric, Marko, Petzold, Andreas, Piedra, Jónatan, Piilonen, Leo, Piparo, Danilo, Pivarski, Jim, Pokorski, Witold, Polci, Francesco, Potamianos, Karolos, Psihas, Fernanda, Puig Navarro, Albert, Quast, Günter, Raven, Gerhard, Reuter, Jürgen, Ribon, Alberto, Rinaldi, Lorenzo, Ritter, Martin, Robinson, James, Rodrigues, Eduardo, Roiser, Stefan, Rousseau, David, Roy, Gareth, Rybkine, Grigori, Sailer, Andre, Sakuma, Tai, Santana, Renato, Sartirana, Andrea, Schellman, Heidi, Schovancová, Jaroslava, Schramm, Steven, Schulz, Markus, Sciabà, Andrea, Seidel, Sally, Sekmen, Sezen, Serfon, Cedric, Severini, Horst, Sexton-Kennedy, Elizabeth, Seymour, Michael, Sgalaberna, Davide, Shapoval, Illya, Shiers, Jamie, Shiu, Jing-Ge, Short, Hannah, Siroli, Gian P, Skipsey, Sam, Smith, Tim, Snyder, Scott, Sokoloff, Michael D, Spentzouris, Panagiotis, Stadie, Hartmut, Stark, Giordon, Stewart, Gordon, Stewart, Graeme A, Sánchez, Arturo, Sánchez-Hernández, Alberto, Taffard, Anyes, Tamponi, Umberto, Templon, Jeff, Tenaglia, Giacomo, Tsulaia, Vakhtang, Tunnell, Christopher, Vaandering, Eric, Valassi, Andrea, Vallecorsa, Sofia, Valsan, Liviu, Van Gemmeren, Peter, Vernet, Renaud, Viren, Brett, Vlimant, Jean-Roch, Voss, Christian, Votava, Margaret, Vuosalo, Carl, Vázquez Sierra, Carlos, Wartel, Romain, Watts, Gordon T, Wenaus, Torre, Wenzel, Sandro, Williams, Michael, Winklmeier, Frank, Wissing, Christoph, Wuerthwein, Frank, Wynne, Benjamin, Xiaomei, Zhang, Yang, Wei, Yazgan, Efe

    Published 2020
    “…Similarly, it requires commensurate investment in the R&D of software to acquire, manage, process, and analyse the shear amounts of data to be recorded. …”
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