The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are a Major Reservoir of Galactic Metals von Tumlinson, J., Thom, C., Werk, J. K., Prochaska, J. X., Tripp, T. M., Weinberg, D. H., Peeples, M. S., O'Meara, J. M., Oppenheimer, B. D., Meiring, J. D., Katz, N. S., Davé, R., Ford, A. B., Sembach, K. R.

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Non-equilibrium chemistry and cooling in the diffuse interstellar medium – II. Shielded gas von Richings, A. J., Schaye, J., Oppenheimer, B. D.

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Non-equilibrium chemistry and cooling in the diffuse interstellar medium – I. Optically thin regime von Richings, A. J., Schaye, J., Oppenheimer, B. D.

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How is star formation quenched in massive galaxies? von Gabor, J. M., Davé, R., Finlator, K., Oppenheimer, B. D.

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Quenching massive galaxies with on-the-fly feedback in cosmological hydrodynamic simulations von Gabor, J. M., Davé, R., Oppenheimer, B. D., Finlator, K.

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The host haloes of O i absorbers in the reionization epoch von Finlator, Kristian, Muñoz, Joseph A., Oppenheimer, B. D., Oh, S. Peng, Özel, Feryal, Davé, Romeel

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The soft, fluctuating UVB at z ∼ 6 as traced by C iv, Si iv, and C ii von Finlator, Kristian, Oppenheimer, B. D., Davé, Romeel, Zackrisson, E., Thompson, Robert, Huang, Shuiyao

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The reionization of carbon von Finlator, Kristian, Thompson, Robert, Huang, Shuiyao, Dave, Romeel, Zackrisson, E, Oppenheimer, B D

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The minimum halo mass for star formation at z  = 6–8 von Finlator, Kristian, Prescott, Moire KM, Oppenheimer, B D, Dave, Romeel, Zackrisson, E, Livermore, R C, Finkelstein, S L, Thompson, Robert, Huang, Shuiyao

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The enrichment history of baryons in the Universe von Davé, Romeel, Oppenheimer, Benjamin D.

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The physical properties and detectability of reionization-epoch galaxies von Davé, Romeel, Finlator, Kristian, Oppenheimer, Benjamin D.

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High-Resolution Mid-Infrared Imaging of the Asymptotic Giant Branch Star RV Bootis with the Steward Observatory Adaptive Optics System von Biller, B. A, Close, L. M, Li, A, Bieging, J. H, Hoffmann, W. F, Hinz, P. M, Miller, D, Brusa, G, Lloyd-Hart, M, Wildi, F, Potter, D, Oppenheimer, B. D

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The Approaching Death of the OH/IR star IRAS 18455+0448 von Lewis, B. M, Oppenheimer, B. D, Daubar, I. J

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Optical Spectropolarimetry of Asymptotic Giant Branch and Post-Asymptotic Giant Branch Stars von Bieging, John H, Schmidt, Gary D, Smith, Paul S, Oppenheimer, Benjamin D

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Spectropolarimetry and Radiative Transfer Modeling of Three Proto-Planetary Nebulae von Oppenheimer, Benjamin Darwin, Bieging, John H, Schmidt, Gary D, Gordon, Karl D, Misselt, Karl A, Smith, Paul S

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The simulated H I sky at low redshift von Popping, A., Davé, R., Braun, R., Oppenheimer, B. D.

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The soft, fluctuating UVB at z similar to 6 as traced by C IV, Si IV, and C II von Finlator, Kristian, Oppenheimer, B. D., Dave, Romeel, Zackrisson, Erik, Thompson, Robert, Huang, Shuiyao

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Quenching massive galaxies with on-the-fly feedback in cosmological hydrodynamic simulations: Quenching in cosmological simulations von Gabor, J. M., Davé, R., Oppenheimer, B. D., Finlator, K.

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How is star formation quenched in massive galaxies? von Gabor, J. M., Davé, R., Finlator, K., Oppenheimer, B. D.

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How is star formation quenched in massive galaxies?: Star formation quenching von Gabor, J. M., Davé, R., Finlator, K., Oppenheimer, B. D.

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