Search Results - "Mao, Yao"

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  1. 1

    The Aemulus Project. II. Emulating the Halo Mass Function by McClintock, Thomas, Rozo, Eduardo, Becker, Matthew R., DeRose, Joseph, Mao, Yao-Yuan, McLaughlin, Sean, Tinker, Jeremy L., Wechsler, Risa H., Zhai, Zhongxu

    Published in The Astrophysical journal (10-02-2019)
    “…Existing models for the dependence of the halo mass function on cosmological parameters will become a limiting source of systematic uncertainty for cluster…”
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  2. 2

    THE CONCENTRATION DEPENDENCE OF THE GALAXY-HALO CONNECTION: MODELING ASSEMBLY BIAS WITH ABUNDANCE MATCHING by Lehmann, Benjamin V., Mao, Yao-Yuan, Becker, Matthew R., Skillman, Samuel W., Wechsler, Risa H.

    Published in The Astrophysical journal (01-01-2017)
    “…ABSTRACT Empirical methods for connecting galaxies to their dark matter halos have become essential for interpreting measurements of the spatial statistics of…”
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  3. 3

    Modeling the Connection between Subhalos and Satellites in Milky Way-like Systems by Nadler, Ethan O., Mao, Yao-Yuan, Green, Gregory M., Wechsler, Risa H.

    Published in The Astrophysical journal (01-03-2019)
    “…We develop a comprehensive and flexible model for the connection between satellite galaxies and dark matter subhalos in dark matter-only zoom-in simulations of…”
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  4. 4

    The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way–like Galaxies by Mao, Yao-Yuan, Geha, Marla, Wechsler, Risa H., Weiner, Benjamin, Tollerud, Erik J., Nadler, Ethan O., Kallivayalil, Nitya

    Published in The Astrophysical journal (01-02-2021)
    “…Abstract We present the Stage II results from the ongoing Satellites Around Galactic Analogs (SAGA) Survey. Upon completion, the SAGA Survey will…”
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  5. 5

    Beyond assembly bias: exploring secondary halo biases for cluster-size haloes by Mao, Yao-Yuan, Zentner, Andrew R, Wechsler, Risa H

    “…Abstract Secondary halo bias, commonly known as ‘assembly bias’, is the dependence of halo clustering on a halo property other than mass. This prediction of…”
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  6. 6

    The Aemulus Project. I. Numerical Simulations for Precision Cosmology by DeRose, Joseph, Wechsler, Risa H., Tinker, Jeremy L., Becker, Matthew R., Mao, Yao-Yuan, McClintock, Thomas, McLaughlin, Sean, Rozo, Eduardo, Zhai, Zhongxu

    Published in The Astrophysical journal (10-04-2019)
    “…The rapidly growing statistical precision of galaxy surveys has led to a need for ever more precise predictions of the observables used to constrain…”
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  7. 7

    The Aemulus Project. III. Emulation of the Galaxy Correlation Function by Zhai, Zhongxu, Tinker, Jeremy L., Becker, Matthew R., DeRose, Joseph, Mao, Yao-Yuan, McClintock, Thomas, McLaughlin, Sean, Rozo, Eduardo, Wechsler, Risa H.

    Published in The Astrophysical journal (20-03-2019)
    “…Using the N-body simulations of the Aemulus Project, we construct an emulator for the nonlinear clustering of galaxies in real and redshift space. We construct…”
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  8. 8

    The SAGA Survey. I. Satellite Galaxy Populations around Eight Milky Way Analogs by Geha, Marla, Wechsler, Risa H., Mao, Yao-Yuan, Tollerud, Erik J., Weiner, Benjamin, Bernstein, Rebecca, Hoyle, Ben, Marchi, Sebastian, Marshall, Phil J., Muñoz, Ricardo, Lu, Yu

    Published in The Astrophysical journal (20-09-2017)
    “…We present the survey strategy and early results of the "Satellites Around Galactic Analogs" (SAGA) Survey. The SAGA Survey's goal is to measure the…”
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  9. 9

    Modeling the Impact of Baryons on Subhalo Populations with Machine Learning by Nadler, Ethan O., Mao, Yao-Yuan, Wechsler, Risa H., Garrison-Kimmel, Shea, Wetzel, Andrew

    Published in The Astrophysical journal (01-06-2018)
    “…We identify subhalos in dark matter-only (DMO) zoom-in simulations that are likely to be disrupted due to baryonic effects by using a random forest classifier…”
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  10. 10

    Signatures of Velocity-dependent Dark Matter Self-interactions in Milky Way-mass Halos by Nadler, Ethan O., Banerjee, Arka, Adhikari, Susmita, Mao, Yao-Yuan, Wechsler, Risa H.

    Published in The Astrophysical journal (01-06-2020)
    “…We explore the impact of elastic, anisotropic, velocity-dependent dark matter (DM) self-interactions on the host halo and subhalos of Milky Way (MW)-mass…”
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  11. 11

    On the galaxy–halo connection in the EAGLE simulation by Desmond, Harry, Mao, Yao-Yuan, Wechsler, Risa H., Crain, Robert A., Schaye, Joop

    “…Abstract Empirical models of galaxy formation require assumptions about the correlations between galaxy and halo properties. These may be calibrated against…”
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  12. 12

    THE DEPENDENCE OF SUBHALO ABUNDANCE ON HALO CONCENTRATION by Mao, Yao-Yuan, Williamson, Marc, Wechsler, Risa H.

    Published in The Astrophysical journal (01-09-2015)
    “…ABSTRACT Hierarchical structure formation implies that the number of subhalos within a dark matter halo depends not only on halo mass, but also on the…”
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  13. 13

    The clustering of DESI-like luminous red galaxies using photometric redshifts by Zhou, Rongpu, Newman, Jeffrey A, Mao, Yao-Yuan, Meisner, Aaron, Moustakas, John, Myers, Adam D, Prakash, Abhishek, Zentner, Andrew R, Brooks, David, Duan, Yutong, Landriau, Martin, Levi, Michael E, Prada, Francisco, Tarle, Gregory

    “…ABSTRACT We present measurements of the redshift-dependent clustering of a DESI-like luminous red galaxy (LRG) sample selected from the Legacy Survey imaging…”
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  14. 14

    Monitoring of volatile organic compounds (VOCs) from an oil and gas station in northwest China for 1 year by Zheng, Huang, Kong, Shaofei, Xing, Xinli, Mao, Yao, Hu, Tianpeng, Ding, Yang, Li, Gang, Liu, Dantong, Li, Shuanglin, Qi, Shihua

    Published in Atmospheric chemistry and physics (05-04-2018)
    “…Oil and natural gas are important for energy supply around the world. The exploring, drilling, transportation and processing in oil and gas regions can release…”
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  15. 15
  16. 16

    The Aemulus Project. V. Cosmological Constraint from Small-scale Clustering of BOSS Galaxies by Zhai, Zhongxu, Tinker, Jeremy L., Banerjee, Arka, DeRose, Joseph, Guo, Hong, Mao, Yao-Yuan, McLaughlin, Sean, Storey-Fisher, Kate, Wechsler, Risa H.

    Published in The Astrophysical journal (01-05-2023)
    “…Abstract We analyze clustering measurements of BOSS galaxies using a simulation-based emulator of two-point statistics. We focus on the monopole and quadrupole…”
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  17. 17

    Adaptive stochastic parallel gradient descent approach for efficient fiber coupling by Hu, Qintao, Zhen, Liangli, Mao, Yao, Zhu, Shiwei, Zhou, Xi, Zhou, Guozhong

    Published in Optics express (27-04-2020)
    “…In high-speed free-space optical communication systems, the received laser beam must be coupled into a single-mode fiber at the input of the receiver module…”
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  18. 18

    UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations by Wang, Yunchong, Nadler, Ethan O., Mao, Yao-Yuan, Adhikari, Susmita, Wechsler, Risa H., Behroozi, Peter

    Published in The Astrophysical journal (01-07-2021)
    “…Abstract We apply the empirical galaxy–halo connection model UniverseMachine to dark-matter-only zoom-in simulations of isolated Milky Way (MW)–mass halos,…”
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  19. 19

    Spread of airborne antibiotic resistance from animal farms to the environment: Dispersal pattern and exposure risk by Bai, Hong, He, Liang-Ying, Wu, Dai-Ling, Gao, Fang-Zhou, Zhang, Min, Zou, Hai-Yan, Yao, Mao-Sheng, Ying, Guang-Guo

    Published in Environment international (01-01-2022)
    “…[Display omitted] •Abundant airborne ARGs were found in animal farms and surrounding environment.•Airborne bacteria can disperse from the animal houses to a…”
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  20. 20

    The Importance of Preventive Feedback: Inference from Observations of the Stellar Masses and Metallicities of Milky Way Dwarf Galaxies by Lu, Yu, Benson, Andrew, Wetzel, Andrew, Mao, Yao-Yuan, Tonnesen, Stephanie, Peter, Annika H. G., Boylan-Kolchin, Michael, Wechsler, Risa H.

    Published in The Astrophysical journal (01-09-2017)
    “…Dwarf galaxies are known to have remarkably low star formation efficiency due to strong feedback. Adopting the dwarf galaxies of the Milky Way (MW) as a…”
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