Search Results - "Narayanan, Desika"

The Dust Attenuation Law in Galaxies by Salim, Samir, Narayanan, Desika

“…Understanding the properties of dust attenuation curves in galaxies and the physical mechanisms that shape them are among the fundamental questions of…”
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The dust-to-gas and dust-to-metal ratio in galaxies from z = 0 to 6 by Li, Qi, Narayanan, Desika, Davé, Romeel

“…ABSTRACT We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-metal ratio (DTM) from z = 0 → 6, using a model for the…”
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A theory for the excitation of CO in star-forming galaxies by Narayanan, Desika, Krumholz, Mark R.

“…Observations of molecular gas in high-z star-forming galaxies typically rely on emission from CO lines arising from states with rotational quantum numbers…”
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Mergers, starbursts, and quenching in the simba simulation by Rodríguez Montero, Francisco, Davé, Romeel, Wild, Vivienne, Anglés-Alcázar, Daniel, Narayanan, Desika

“…ABSTRACT We use the simba cosmological galaxy formation simulation to investigate the relationship between major mergers ($\lesssim$4:1), starbursts, and…”
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A Theory for the Variation of Dust Attenuation Laws in Galaxies by Narayanan, Desika, Conroy, Charlie, Davé, Romeel, Johnson, Benjamin D., Popping, Gergö

“…In this paper, we provide a physical model for the origin of variations in the shapes and bump strengths of dust attenuation laws in galaxies by combining a…”
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How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting by Lower, Sidney, Narayanan, Desika, Leja, Joel, Johnson, Benjamin D., Conroy, Charlie, Davé, Romeel

“…Abstract The primary method for inferring the stellar mass ( M * ) of a galaxy is through spectral energy distribution (SED) modeling. However, the technique…”
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FIRE-2 simulations: physics versus numerics in galaxy formation by Hopkins, Philip F, Wetzel, Andrew, Kereš, Dušan, Faucher-Giguère, Claude-André, Quataert, Eliot, Boylan-Kolchin, Michael, Murray, Norman, Hayward, Christopher C, Garrison-Kimmel, Shea, Hummels, Cameron, Feldmann, Robert, Torrey, Paul, Ma, Xiangcheng, Anglés-Alcázar, Daniel, Su, Kung-Yi, Orr, Matthew, Schmitz, Denise, Escala, Ivanna, Sanderson, Robyn, Grudić, Michael Y, Hafen, Zachary, Kim, Ji-Hoon, Fitts, Alex, Bullock, James S, Wheeler, Coral, Chan, T K, Elbert, Oliver D, Narayanan, Desika

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Galaxy cold gas contents in modern cosmological hydrodynamic simulations by Davé, Romeel, Crain, Robert A, Stevens, Adam R H, Narayanan, Desika, Saintonge, Amelie, Catinella, Barbara, Cortese, Luca

“…ABSTRACT We present a comparison of galaxy atomic and molecular gas properties in three recent cosmological hydrodynamic simulations, namely SIMBA, EAGLE, and…”
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Discovery of a Dark, Massive, ALMA-only Galaxy at z ∼ 5-6 in a Tiny 3 mm Survey by Williams, Christina C., Labbe, Ivo, Spilker, Justin, Stefanon, Mauro, Leja, Joel, Whitaker, Katherine, Bezanson, Rachel, Narayanan, Desika, Oesch, Pascal, Weiner, Benjamin

“…We report the serendipitous detection of two 3 mm continuum sources found in deep ALMA Band 3 observations to study intermediate-redshift galaxies in the…”
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Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization by Lower, Sidney, Narayanan, Desika, Li, Qi, Davé, Romeel

“…Abstract We present the Cosmic Sands suite of cosmological zoom-in simulations based on the simba galaxy formation model in order to study the buildup of the…”
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Interacting galaxies on FIRE-2: the connection between enhanced star formation and interstellar gas content by Moreno, Jorge, Torrey, Paul, Ellison, Sara L, Patton, David R, Hopkins, Philip F, Bueno, Michael, Hayward, Christopher C, Narayanan, Desika, Kereš, Dušan, Bluck, Asa F L, Hernquist, Lars

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The formation of submillimetre-bright galaxies from gas infall over a billion years by Narayanan, Desika, Turk, Matthew, Feldmann, Robert, Robitaille, Thomas, Hopkins, Philip, Thompson, Robert, Hayward, Christopher, Ball, David, Faucher-Giguère, Claude-André, Kereš, Dušan

“…Submillimetre-bright galaxies at high redshift are the most luminous, heavily star-forming galaxies in the Universe, but cosmological simulations of such…”
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ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ∼ 1.5 by Williams, Christina C., Spilker, Justin S., Whitaker, Katherine E., Davé, Romeel, Woodrum, Charity, Brammer, Gabriel, Bezanson, Rachel, Narayanan, Desika, Weiner, Benjamin

“…Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) CO(2–1) spectroscopy of six massive (log 10 / > 11.3) quiescent galaxies at z  ∼ 1.5…”
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Tracing the History of Obscured Star Formation with the SIMBA Cosmological Galaxy Evolution Simulation by Zimmerman, Dhruv T., Narayanan, Desika, Whitaker, Katherine E., Davé, Romeel

“…Abstract We explore the cosmic evolution of the fraction of dust-obscured star formation predicted by the simba cosmological hydrodynamic simulations featuring…”
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The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral Atomic Carbon [C i] by Valentino, Francesco, Magdis, Georgios E., Daddi, Emanuele, Liu, Daizhong, Aravena, Manuel, Bournaud, Frédéric, Cortzen, Isabella, Gao, Yu, Jin, Shuowen, Juneau, Stéphanie, Kartaltepe, Jeyhan S., Kokorev, Vasily, Lee, Min-Young, Madden, Suzanne C., Narayanan, Desika, Popping, Gergö, Puglisi, Annagrazia

“…We report Atacama Large Millimeter Array observations of the neutral atomic carbon transitions [C i] and multiple CO lines in a sample of ∼30 main-sequence…”
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slick: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations by Garcia, Karolina, Narayanan, Desika, Popping, Gergö, Anirudh, R., Sutherland, Sagan, Kaasinen, Melanie

“…Abstract We present slick (the Scalable Line Intensity Computation Kit), a software package that calculates realistic CO, [C i ], and [C ii ] luminosities for…”
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Galaxy gas fractions at high redshift: the tension between observations and cosmological simulations by Narayanan, Desika, Bothwell, Matt, Davé, Romeel

“…ABSTRACT CO measurements of z ∼ 1–4 galaxies have found that their baryonic gas fractions are significantly higher than those for galaxies at z = 0, with…”
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Dark Molecular Gas in Simulations of z ∼ 0 Disk Galaxies by Li, Qi, Narayanan, Desika, Davè, Romeel, Krumholz, Mark R.

“…The H2 mass of molecular clouds has traditionally been traced by the CO(J = 1−0) rotational transition line. This said, CO is relatively easily…”
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Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution and implications for the IMF by Hayward, Christopher C., Narayanan, Desika, Kereš, Dušan, Jonsson, Patrik, Hopkins, Philip F., Cox, T. J., Hernquist, Lars

“…High-redshift submillimetre galaxies (SMGs) are some of the most rapidly star-forming galaxies in the Universe. Historically, galaxy formation models have had…”
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Quenching of star formation from a lack of inflowing gas to galaxies by Whitaker, Katherine E., Williams, Christina C., Mowla, Lamiya, Spilker, Justin S., Toft, Sune, Narayanan, Desika, Pope, Alexandra, Magdis, Georgios E., van Dokkum, Pieter G., Akhshik, Mohammad, Bezanson, Rachel, Brammer, Gabriel B., Leja, Joel, Man, Allison, Nelson, Erica J., Richard, Johan, Pacifici, Camilla, Sharon, Keren, Valentino, Francesco

“…Star formation in half of massive galaxies was quenched by the time the Universe was 3 billion years old 1 . Very low amounts of molecular gas seem to be…”
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