Search Results - "Bosman, Sarah"

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    Reionization and galaxy inference from the high-redshift Ly α forest by Qin, Yuxiang, Mesinger, Andrei, Bosman, Sarah E I, Viel, Matteo

    “…ABSTRACT The transmission of Lyman α (Ly α) in the spectra of distant quasars depends on the density, temperature, and ionization state of the intergalactic…”
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    Large Ly α opacity fluctuations and low CMB τ in models of late reionization with large islands of neutral hydrogen extending to z < 5.5 by Kulkarni, Girish, Keating, Laura C, Haehnelt, Martin G, Bosman, Sarah E I, Puchwein, Ewald, Chardin, Jonathan, Aubert, Dominique

    “…Abstract High-redshift quasi-stellar object (QSO) spectra show large spatial fluctuations in the Ly α opacity of the intergalactic medium on surprisingly large…”
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    Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation by Gronke, Max, Ocvirk, Pierre, Mason, Charlotte, Matthee, Jorryt, Bosman, Sarah E I, Sorce, Jenny G, Lewis, Joseph, Ahn, Kyungjin, Aubert, Dominique, Dawoodbhoy, Taha, Iliev, Ilian T, Shapiro, Paul R, Yepes, Gustavo

    “…ABSTRACT The decline in abundance of Lyman-α (Lyα) emitting galaxies at z ≳ 6 is a powerful and commonly used probe to constrain the progress of cosmic…”
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    New constraints on quasar evolution: broad-line velocity shifts over 1.5 ≲ z ≲ 7.5 by Meyer, Romain A, Bosman, Sarah E I, Ellis, Richard S

    “…ABSTRACT We present the results of a model-independent investigation of the rest-frame UV spectra from a comprehensive sample of 394 quasars in the redshift…”
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    A comparison of quasar emission reconstruction techniques for z ≥ 5.0 Lyman α and Lyman β transmission by Bosman, Sarah E I, Ďurovčíková, Dominika, Davies, Frederick B, Eilers, Anna-Christina

    “…ABSTRACT Reconstruction techniques for intrinsic quasar continua are crucial for the precision study of Lyman α (Ly α) and Lyman β (Ly β) transmission at z >…”
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    Studying the Lyman α optical depth fluctuations at z ∼ 5.5 using fast semi-numerical methods by Choudhury, T Roy, Paranjape, Aseem, Bosman, Sarah E I

    “…ABSTRACT We present a computationally efficient and fast semi-numerical technique for simulating the Lyman α (Ly α) absorption optical depth in presence of…”
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    Constraining IGM enrichment and metallicity with the C iv forest correlation function by Tie, Suk Sien, Hennawi, Joseph F, Kakiichi, Koki, Bosman, Sarah E I

    “…ABSTRACT The distribution and abundance of metals in the diffuse intergalactic medium (IGM) have implications for galaxy formation and evolution models, and…”
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    Measuring the Density Fields around Bright Quasars at z ∼ 6 with XQR-30 Spectra by Chen, Huanqing, Eilers, Anna-Christina, Bosman, Sarah E. I., Gnedin, Nickolay Y., Fan, Xiaohui, Wang, Feige, Yang, Jinyi, D’Odorico, Valentina, Becker, George D., Bischetti, Manuela, Mazzucchelli, Chiara, Mesinger, Andrei, Pallottini, Andrea

    Published in The Astrophysical journal (01-05-2022)
    “…Abstract Measuring the density of the intergalactic medium using quasar sight lines in the epoch of reionization is challenging due to the saturation of Ly α…”
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    Three Lyα Emitting Galaxies within a Quasar Proximity Zone at z ∼ 5.8 by Bosman, Sarah E. I., Kakiichi, Koki, Meyer, Romain A., Gronke, Max, Laporte, Nicolas, Ellis, Richard S.

    Published in The Astrophysical journal (01-06-2020)
    “…Abstract Quasar proximity zones at correspond to overdense and overionized environments. Galaxies found inside proximity zones can therefore display features…”
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    Reionization history constraints from neural network based predictions of high-redshift quasar continua by Ďurovčíková, Dominika, Katz, Harley, Bosman, Sarah E I, Davies, Frederick B, Devriendt, Julien, Slyz, Adrianne

    “…ABSTRACT Observations of the early Universe suggest that reionization was complete by z ∼ 6, however, the exact history of this process is still unknown. One…”
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    Re-examining the case for neutral gas near the redshift 7 quasar ULAS J1120+0641 by Bosman, Sarah E. I., Becker, George D.

    “…Signs of damping-wing absorption attenuating the Lyman α emission line of the first known z ∼ 7 quasar, ULAS J1120+0641, recently provided exciting evidence of…”
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