Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach von Calderon, Victor F, Berlind, Andreas A

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The Impact of Baryonic Physics on the Abundance, Clustering, and Concentration of Halos von Beltz-Mohrmann, Gillian D., Berlind, Andreas A.

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Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies von Zheng, Zheng, Berlind, Andreas A, Weinberg, David H, Benson, Andrew J, Baugh, Carlton M, Cole, Shaun, Davé, Romeel, Frenk, Carlos S, Katz, Neal, Lacey, Cedric G

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The lensing and temperature imprints of voids on the cosmic microwave background von Cai, Yan-Chuan, Neyrinck, Mark, Mao, Qingqing, Peacock, John A., Szapudi, Istvan, Berlind, Andreas A.

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Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension von Beltz-Mohrmann, Gillian D., Szewciw, Adam O., Berlind, Andreas A., Sinha, Manodeep

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The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass von Berlind, Andreas A, Weinberg, David H

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The Physics of Galaxy Clustering. I. A Model for Subhalo Populations von Zentner, Andrew R, Berlind, Andreas A, Bullock, James S, Kravtsov, Andrey V, Wechsler, Risa H

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SHAM beyond clustering: new tests of galaxy-halo abundance matching with galaxy groups von Hearin, Andrew P., Zentner, Andrew R., Berlind, Andreas A., Newman, Jeffrey A.

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Testing the accuracy of halo occupation distribution modelling using hydrodynamic simulations von Beltz-Mohrmann, Gillian D, Berlind, Andreas A, Szewciw, Adam O

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A noninteracting low-mass black hole-giant star binary system von Thompson, Todd A, Kochanek, Christopher S, Stanek, Krzysztof Z, Badenes, Carles, Post, Richard S, Jayasinghe, Tharindu, Latham, David W, Bieryla, Allyson, Esquerdo, Gilbert A, Berlind, Perry, Calkins, Michael L, Tayar, Jamie, Lindegren, Lennart, Johnson, Jennifer A, Holoien, Thomas W-S, Auchettl, Katie, Covey, Kevin

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The Luminosity and Color Dependence of the Galaxy Correlation Function von Zehavi, Idit, Zheng, Zheng, Weinberg, David H, Frieman, Joshua A, Berlind, Andreas A, Blanton, Michael R, Scoccimarro, Roman, Sheth, Ravi K, Strauss, Michael A, Kayo, Issha, Suto, Yasushi, Fukugita, Masataka, Nakamura, Osamu, Bahcall, Neta A, Brinkmann, Jon, Gunn, James E, Hennessy, Greg S, Ivezić, Željko, Knapp, Gillian R, Loveday, Jon, Meiksin, Avery, Schlegel, David J, Schneider, Donald P, Szapudi, Istvan, Tegmark, Max, Vogeley, Michael S, York, Donald G

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Reversing arrested development: a new method to address halo assembly bias von Smith, William J, Berlind, Andreas A, Sinha, Manodeep

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Small- and large-scale galactic conformity in SDSS DR7 von Calderon, Victor F, Berlind, Andreas A, Sinha, Manodeep

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The secondary spin bias of dark matter haloes von Johnson, James W, Maller, Ariyeh H, Berlind, Andreas A, Sinha, Manodeep, Holley-Bockelmann, J Kelly

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What Aspects of Galaxy Environment Matter? von Blanton, Michael R, Berlind, Andreas A

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Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog von Florez, Jonathan, Berlind, Andreas A., Kannappan, Sheila J., Stark, David V., Eckert, Kathleen D., Calderon, Victor F., Moffett, Amanda J., Campbell, Duncan, Sinha, Manodeep

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THE Hα EMISSION OF NEARBY M DWARFS AND ITS RELATION TO STELLAR ROTATION von Newton, Elisabeth R., Irwin, Jonathan, Charbonneau, David, Berlind, Perry, Calkins, Michael L., Mink, Jessica

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A Cosmic Void Catalog of SDSS DR12 BOSS Galaxies von Mao, Qingqing, Berlind, Andreas A., Scherrer, Robert J., Neyrinck, Mark C., Scoccimarro, Román, Tinker, Jeremy L., McBride, Cameron K., Schneider, Donald P., Pan, Kaike, Bizyaev, Dmitry, Malanushenko, Elena, Malanushenko, Viktor

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The Dark Side of the Halo Occupation Distribution von Kravtsov, Andrey V, Berlind, Andreas A, Wechsler, Risa H, Klypin, Anatoly A, Gottlöber, Stefan, Allgood, Brandon, Primack, Joel R

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THE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE von Blondin, S, Matheson, T, Kirshner, R P, Mandel, K S, Berlind, P, Calkins, M, Challis, P, Garnavich, P M, Jha, S W, Modjaz, M, Riess, A G, Schmidt, B P

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