The expected spins of gravitational wave sources with isolated field binary progenitors von Zaldarriaga, Matias, Kushnir, Doron, Kollmeier, Juna A.

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Evidence for Cocoon Emission from the Early Light Curve of SSS17a von Piro, Anthony L., Kollmeier, Juna A.

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GW150914: spin-based constraints on the merger time of the progenitor system von Kushnir, Doron, Zaldarriaga, Matias, Kollmeier, Juna A., Waldman, Roni

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Radiation pressure clear-out of dusty photoevaporating discs von Owen, James E, Kollmeier, Juna A

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Cosmological perturbation theory using the FFTLog: formalism and connection to QFT loop integrals von Simonović, Marko, Baldauf, Tobias, Zaldarriaga, Matias, Carrasco, John Joseph, Kollmeier, Juna A.

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Evidence for a Hard Ionizing Spectrum from a z = 6.11 Stellar Population von Mainali, Ramesh, Kollmeier, Juna A., Stark, Daniel P., Simcoe, Robert A., Walth, Gregory, Newman, Andrew B., Miller, Daniel R.

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THE COS-DWARFS SURVEY: THE CARBON RESERVOIR AROUND SUB- L GALAXIES von BORDOLOI, RONGMON, Tumlinson, Jason, Werk, Jessica K, Oppenheimer, Benjamin D, Peeples, Molly S, Prochaska, J Xavier, Tripp, Todd M, Katz, Neal, Dave, Romeel, Fox, Andrew J, Thom, Christopher, d, Amanda Brady, Weinberg, David H, Burchett, Joseph N, Kollmeier, Juna A

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ULTRAHIGH-ENERGY COSMIC RAYS FROM THE “EN CAUL” BIRTH OF MAGNETARS von Piro, Anthony L, Kollmeier, Juna A

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Feedback and recycled wind accretion: assembling the z= 0 galaxy mass function von Oppenheimer, Benjamin D., Davé, Romeel, Kereš, Dušan, Fardal, Mark, Katz, Neal, Kollmeier, Juna A., Weinberg, David H.

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The neutral hydrogen content of galaxies in cosmological hydrodynamic simulations von Davé, Romeel, Katz, Neal, Oppenheimer, Benjamin D., Kollmeier, Juna A., Weinberg, David H.

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Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry von Monson, Andrew J., Beaton, Rachael L., Scowcroft, Victoria, Freedman, Wendy L., Madore, Barry F., Rich, Jeffrey A., Seibert, Mark, Kollmeier, Juna A., Clementini, Gisella

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THE CARNEGIE-CHICAGO HUBBLE PROGRAM. I. AN INDEPENDENT APPROACH TO THE EXTRAGALACTIC DISTANCE SCALE USING ONLY POPULATION II DISTANCE INDICATORS von Beaton, Rachael L., Freedman, Wendy L., Madore, Barry F., Bono, Giuseppe, Carlson, Erika K., Clementini, Gisella, Durbin, Meredith J., Garofalo, Alessia, Hatt, Dylan, Jang, In Sung, Kollmeier, Juna A., Lee, Myung Gyoon, Monson, Andrew J., Rich, Jeffrey A., Scowcroft, Victoria, Seibert, Mark, Sturch, Laura, Yang, Soung-Chul

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Tracing inflows and outflows with absorption lines in circumgalactic gas von Ford, Amanda Brady, Davé, Romeel, Oppenheimer, Benjamin D., Katz, Neal, Kollmeier, Juna A., Thompson, Robert, Weinberg, David H.

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Baryon cycling in the low-redshift circumgalactic medium: a comparison of simulations to the COS-Halos survey von Ford, Amanda Brady, Werk, Jessica K., Davé, Romeel, Tumlinson, Jason, Bordoloi, Rongmon, Katz, Neal, Kollmeier, Juna A., Oppenheimer, Benjamin D., Peeples, Molly S., Prochaska, Jason X., Weinberg, David H.

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DIFFUSE Lyα EMITTING HALOS: A GENERIC PROPERTY OF HIGH-REDSHIFT STAR-FORMING GALAXIES von STEIDEL, Charles C, BOGOSAVLJEVIC, Milan, SHAPLEY, Alice E, KOLLMEIER, Juna A, REDDY, Naveen A, ERB, Dawn K, PETTINI, Max

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The intergalactic medium over the last 10 billion years - II. Metal-line absorption and physical conditions von Oppenheimer, Benjamin D., Davé, Romeel, Katz, Neal, Kollmeier, Juna A., Weinberg, David H.

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H α emission in the nebular spectrum of the Type Ia supernova ASASSN-18tb von Kollmeier, Juna A, Chen, Ping, Dong, Subo, Morrell, Nidia, Phillips, M M, Kushnir, Doron, Prieto, J L, Piro, Anthony L, Simon, Joshua D

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Probing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα Forest von Tonnesen, Stephanie, Smith, Britton D., Kollmeier, Juna A., Cen, Renyue

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Can moons have moons? von Kollmeier, Juna A, Raymond, Sean N

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Hydrogen and metal line absorption around low-redshift galaxies in cosmological hydrodynamic simulations von Ford, Amanda Brady, Oppenheimer, Benjamin D., Davé, Romeel, Katz, Neal, Kollmeier, Juna A., Weinberg, David H.

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