The ASTRO-H (Hitomi) x-ray astronomy satellite by Bulbul, Gul E, Miller, Eric D

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Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster by Bulbul, Gul E, Miller, Eric D, Bautz, Marshall W.

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HIGH-VELOCITY CLOUDS IN THE NEARBY SPIRAL GALAXY M 83 by Bregman, Joel N., Wakker, Bart P., Miller, Eric D

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THE REDSHIFT EVOLUTION OF THE MEAN TEMPERATURE, PRESSURE, AND ENTROPY PROFILES IN 80 SPT-SELECTED GALAXY CLUSTERS by McDonald, Michael A., Bautz, Marshall W., Miller, Eric D

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SPT-CL J2040–4451: AN SZ-SELECTED GALAXY CLUSTER AT z = 1.478 WITH SIGNIFICANT ONGOING STAR FORMATION by Bautz, Marshall W., McDonald, Michael A., Miller, Eric D

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SIMULATING ASTRO-H OBSERVATIONS OF SLOSHING GAS MOTIONS IN THE CORES OF GALAXY CLUSTERS by Simionescu, A., Bautz, Marshall W., ZuHone, John A., Miller, Eric D

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COOL CORE BIAS IN SUNYAEV–ZEL’DOVICH GALAXY CLUSTER SURVEYS by Lin, Henry W., Benson, Bradford A., McDonald, Michael A., Miller, Eric D

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OUTFLOW VERSUS INFALL IN SPIRAL GALAXIES: METAL ABSORPTION IN THE HALO OF NGC 891 by Bregman, Joel N., Seitzer, Patrick, Cowley, C. R., Miller, Matthew J., Miller, Eric D

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A VERY DEEP CHANDRA OBSERVATION OF A1795: THE COLD FRONT AND COOLING WAKE by Ehlert, Steven, David, Laurence P., McDonald, Michael A., Bautz, Marshall W., Miller, Eric D

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A massive, cooling-flow-induced starburst in the core of a highly luminous cluster of galaxies by McDonald, Michael A., Bautz, Marshall W., Simcoe, Robert A., Sullivan, Peter W., Miller, Eric D

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A ROBUST QUANTIFICATION OF GALAXY CLUSTER MORPHOLOGY USING ASYMMETRY AND CENTRAL CONCENTRATION by Nurgaliev, D., Benson, Bradford A., Stubbs, C. W., Vikhlinin, A., McDonald, Michael A., Miller, Eric D

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SEARCHING FOR THE 3.5 keV LINE IN THE STACKED SUZAKU OBSERVATIONS OF GALAXY CLUSTERS by Markevitch, Maxim, Foster, Adam, Loewenstein, Mike, Randall, Scott W., Smith, Randall K., Bulbul, Gul E, Miller, Eric D, Bautz, Mark

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IACHEC CROSS-CALIBRATION OF CHANDRA, NuSTAR, SWIFT, SUZAKU, XMM-NEWTON WITH 3C 273 ANDPKS 2155-304 by Madsen, Kristin K., Beardmore, Andrew P., Forster, Karl, Guainazzi, Matteo, Page, Kim L., Stuhlinger, Martin, Marshall, Herman, Miller, Eric D

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Heavy Ion radiation assessment of a 100G/200G commercial optical coherent DSP ASIC by Aniceto, Raichelle J., Milanowski, Randall, McClure, Steve, Aguilar, Alexa, Moro, Slaven, Miller, Eric D., Cahoy, Kerri, Nicholson, Neal, Greene, Daniel

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Uniform Contribution of Supernova Explosions to the Chemical Enrichment of Abell 3112 out to R[subscript 200] by Ezer, Cemile, Bulbul, Esra, Ercan, E. Nihal, Smith, Randall K., Loewenstein, Mike, McDonald, Michael A., Miller, Eric D, Bautz, Marshall W.

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Arcus: the x-ray grating spectrometer explorer by Grant, Catherine E, Heilmann, Ralf K, Miller, Eric D, Bautz, Marshall W., Huenemoerder, David P., Nowak, Michael A., Schattenburg, Mark Lee, Schulz, Norbert S.

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The SMC SNR 1E0102.2-7219 as a calibration standard for X-ray astronomy in the 0.3-2.5 keV bandpass by Plucinsky, Paul P., Haberl, F., Dewey, Dan, Beardmore, Andrew P., DePasquale, Joseph M., Godet, Olivier, Grinberg, Victoria, Pollock, A. M. T., Sembay, Steven, Smith, Randall K., Miller, Eric D

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FINDING FOSSIL GROUPS: OPTICAL IDENTIFICATION AND X-RAY CONFIRMATION by Rykoff, Eli S., Dupke, Renato A., Mendes de Oliveira, Claudia, Lopes de Oliveira, Raimundo, Proctor, Robert N., Garmire, Gordon P., Koester, Benjamin P., McKay, Timothy A., Miller, Eric D

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RADIAL PROFILE OF THE 3.5 keV LINE OUT TO R[subscript 200] IN THE PERSEUS CLUSTER by Franse, Jeroen, Foster, Adam, Boyarsky, Alexey, Markevitch, Maxim, Iakubovskyi, Dmytro, Loewenstein, Mike, Miller, Eric, Randall, Scott W., Ruchayskiy, Oleg, Smith, Randall K., Bulbul, Gul E, Bautz, Mark, McDonald, Michael A., Miller, Eric D

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Astro-H data analysis, processing and archive by Angelini, Lorella, Terada, Yukitatsu, Loewenstein, Michael, Yamaguchi, Hiroya, Yaqoob, Tahir, Krimm, Hans, Harrus, Ilana, Takahashi, Hiromitsu, Nobukawa, Masayoshi, Sawada, Makoto, Witthoeft, Michael, Rutkowski, Kristin, Sargent, Andrew, Hill, Robert S., Dutka, Michael, Eggen, Joseph, Miller, Eric D

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