Rapid Reionization by the Oligarchs: The Case for Massive, UV-bright, Star-forming Galaxies with High Escape Fractions von Naidu, Rohan P., Tacchella, Sandro, Mason, Charlotte A., Bose, Sownak, Oesch, Pascal A., Conroy, Charlie

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All-sky dynamical response of the Galactic halo to the Large Magellanic Cloud von Conroy, Charlie, Naidu, Rohan P., Garavito-Camargo, Nicolás, Besla, Gurtina, Zaritsky, Dennis, Bonaca, Ana, Johnson, Benjamin D.

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Model-independent constraints on the hydrogen-ionizing emissivity at z > 6 von Mason, Charlotte A, Naidu, Rohan P, Tacchella, Sandro, Leja, Joel

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Evidence from the H3 Survey That the Stellar Halo Is Entirely Comprised of Substructure von Naidu, Rohan P., Conroy, Charlie, Bonaca, Ana, Johnson, Benjamin D., Ting, Yuan-Sen, Caldwell, Nelson, Zaritsky, Dennis, Cargile, Phillip A.

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Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys von Matthee, Jorryt, Naidu, Rohan P., Brammer, Gabriel, Chisholm, John, Eilers, Anna-Christina, Goulding, Andy, Greene, Jenny, Kashino, Daichi, Labbe, Ivo, Lilly, Simon J., Mackenzie, Ruari, Oesch, Pascal A., Weibel, Andrea, Wuyts, Stijn, Xiao, Mengyuan, Bordoloi, Rongmon, Bouwens, Rychard, van Dokkum, Pieter, Illingworth, Garth, Kramarenko, Ivan, Maseda, Michael V., Mason, Charlotte, Meyer, Romain A., Nelson, Erica J., Reddy, Naveen A., Shivaei, Irene, Simcoe, Robert A., Yue, Minghao

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Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWST von Naidu, Rohan P., Oesch, Pascal A., Dokkum, Pieter van, Nelson, Erica J., Suess, Katherine A., Brammer, Gabriel, Whitaker, Katherine E., Illingworth, Garth, Bouwens, Rychard, Tacchella, Sandro, Matthee, Jorryt, Allen, Natalie, Bezanson, Rachel, Conroy, Charlie, Labbe, Ivo, Leja, Joel, Leonova, Ecaterina, Magee, Dan, Price, Sedona H., Setton, David J., Strait, Victoria, Stefanon, Mauro, Toft, Sune, Weaver, John R., Weibel, Andrea

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Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey von Conroy, Charlie, Naidu, Rohan P., Zaritsky, Dennis, Bonaca, Ana, Cargile, Phillip, Johnson, Benjamin D., Caldwell, Nelson

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What Is Missing from the Local Stellar Halo? von Sharpe, Katherine, Naidu, Rohan P., Conroy, Charlie

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EIGER IV. The Cool 104 K Circumgalactic Environment of High-redshift Galaxies Reveals Remarkably Efficient Intergalactic Medium Enrichment von Bordoloi, Rongmon, Simcoe, Robert A., Matthee, Jorryt, Kashino, Daichi, Mackenzie, Ruari, Lilly, Simon J., Eilers, Anna-Christina, Liu, Bin, DePalma, David, Yue, Minghao, P. Naidu, Rohan

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UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5 von Greene, Jenny E., Labbe, Ivo, Goulding, Andy D., Furtak, Lukas J., Chemerynska, Iryna, Kokorev, Vasily, Dayal, Pratika, Volonteri, Marta, Williams, Christina C., Wang, Bingjie, Setton, David J., Burgasser, Adam J., Bezanson, Rachel, Atek, Hakim, Brammer, Gabriel, Cutler, Sam E., Feldmann, Robert, Fujimoto, Seiji, Glazebrook, Karl, de Graaff, Anna, Khullar, Gourav, Leja, Joel, Marchesini, Danilo, Maseda, Michael V., Matthee, Jorryt, Miller, Tim B., Naidu, Rohan P., Nanayakkara, Themiya, Oesch, Pascal A., Pan, Richard, Papovich, Casey, Price, Sedona H., van Dokkum, Pieter, Weaver, John R., Whitaker, Katherine E., Zitrin, Adi

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Evolution of the UV LF from z ∼ 15 to z ∼ 8 using new JWST NIRCam medium-band observations over the HUDF/XDF von Bouwens, Rychard J, Stefanon, Mauro, Brammer, Gabriel, Oesch, Pascal A, Herard-Demanche, Thomas, Illingworth, Garth D, Matthee, Jorryt, Naidu, Rohan P, van Dokkum, Pieter G, van Leeuwen, Ivana F

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The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: what makes a galaxy a Lyman α emitter? von Matthee, Jorryt, Sobral, David, Hayes, Matthew, Pezzulli, Gabriele, Gronke, Max, Schaerer, Daniel, Naidu, Rohan P, Röttgering, Huub, Calhau, João, Paulino-Afonso, Ana, Santos, Sérgio, Amorín, Ricardo

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The synchrony of production and escape: half the bright Lyα emitters at z ≈ 2 have Lyman continuum escape fractions ≈50 von Naidu, Rohan P, Matthee, Jorryt, Oesch, Pascal A, Conroy, Charlie, Sobral, David, Pezzulli, Gabriele, Hayes, Matthew, Erb, Dawn, Amorín, Ricardo, Gronke, Max, Schaerer, Daniel, Tacchella, Sandro, Kerutt, Josephine, Paulino-Afonso, Ana, Calhau, João, Llerena, Mario, Röttgering, Huub

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The Poor Old Heart of the Milky Way von Rix, Hans-Walter, Chandra, Vedant, Andrae, René, Price-Whelan, Adrian M., Weinberg, David H., Conroy, Charlie, Fouesneau, Morgan, Hogg, David W, De Angeli, Francesca, Naidu, Rohan P., Xiang, Maosheng, Ruz-Mieres, Daniela

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A low Lyman Continuum escape fraction of <10 per cent for extreme [O iii] emitters in an overdensity at z ∼ 3.5 von Naidu, Rohan P, Forrest, Ben, Oesch, Pascal A, Tran, Kim-Vy H, Holden, Bradford P

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Early galaxies and early dark energy: a unified solution to the hubble tension and puzzles of massive bright galaxies revealed by JWST von Shen, Xuejian, Vogelsberger, Mark, Boylan-Kolchin, Michael, Tacchella, Sandro, Naidu, Rohan P

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Orbital Clustering Identifies the Origins of Galactic Stellar Streams von Bonaca, Ana, Naidu, Rohan P., Conroy, Charlie, Caldwell, Nelson, Cargile, Phillip A., Han, Jiwon Jesse, Johnson, Benjamin D., Kruijssen, J. M. Diederik, Myeong, G. C., Speagle, Joshua S., Ting, Yuan-Sen, Zaritsky, Dennis

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Mapping the Stellar Halo with the H3 Spectroscopic Survey von Conroy, Charlie, Bonaca, Ana, Cargile, Phillip, Johnson, Benjamin D., Caldwell, Nelson, Naidu, Rohan P., Zaritsky, Dennis, Fabricant, Daniel, Moran, Sean, Rhee, Jaehyon, Szentgyorgyi, Andrew, Berlind, Perry, Calkins, Michael L., Kattner, ShiAnne, Ly, Chun

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EIGER. V. Characterizing the Host Galaxies of Luminous Quasars at z ≳ 6 von Yue, Minghao, Eilers, Anna-Christina, Simcoe, Robert A., Mackenzie, Ruari, Matthee, Jorryt, Kashino, Daichi, Bordoloi, Rongmon, Lilly, Simon J., Naidu, Rohan P.

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Reconstructing the Last Major Merger of the Milky Way with the H3 Survey von Naidu, Rohan P., Conroy, Charlie, Bonaca, Ana, Zaritsky, Dennis, Weinberger, Rainer, Ting, Yuan-Sen, Caldwell, Nelson, Tacchella, Sandro, Han, Jiwon Jesse, Speagle, Joshua S., Cargile, Phillip A.

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