Search Results - "Tacchella, Sandro"

Quantitative evaluation of gender bias in astronomical publications from citation counts by Caplar, Neven, Tacchella, Sandro, Birrer, Simon

“…Numerous studies across different research fields have shown that both male and female referees consistently give higher scores to work done by men than to…”
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A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4 by Tacchella, Sandro, Bose, Sownak, Conroy, Charlie, Eisenstein, Daniel J., Johnson, Benjamin D.

“…We explore the connection between the UV luminosity functions (LFs) of high-z galaxies and the distribution of stellar masses and star formation histories…”
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The galaxy–halo connection of emission-line galaxies in IllustrisTNG by Hadzhiyska, Boryana, Tacchella, Sandro, Bose, Sownak, Eisenstein, Daniel J

“…ABSTRACT We employ the hydrodynamical simulation IllustrisTNG-300-1 to explore the halo occupation distribution (HOD) and environmental dependence of luminous…”
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The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations by Rodriguez-Gomez, Vicente, Snyder, Gregory F, Lotz, Jennifer M, Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Genel, Shy, Weinberger, Rainer, Tacchella, Sandro, Pakmor, Rüdiger, Torrey, Paul, Marinacci, Federico, Vogelsberger, Mark, Hernquist, Lars, Thilker, David A

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Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies by Mosleh, Moein, Hosseinnejad, Shiva, Hosseini-ShahiSavandi, S. Zahra, Tacchella, Sandro

“…How stellar mass assembles within galaxies is still an open question. We present measurements of the stellar mass distribution on kiloparsec-scales for ∼5500…”
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High-redshift predictions from IllustrisTNG – III. Infrared luminosity functions, obscured star formation, and dust temperature of high-redshift galaxies by Shen, Xuejian, Vogelsberger, Mark, Nelson, Dylan, Tacchella, Sandro, Hernquist, Lars, Springel, Volker, Marinacci, Federico, Torrey, Paul

“…ABSTRACT We post-process galaxies in the IllustrisTNG simulations with skirt radiative transfer calculations to make predictions for the rest-frame…”
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Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWST by 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

“…Abstract The first few 100 Myr at z > 10 mark the last major uncharted epoch in the history of the universe, where only a single galaxy (GN-z11 at z ≈ 11) is…”
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On the Stellar Populations of Galaxies at z = 9–11: The Growth of Metals and Stellar Mass at Early Times by Tacchella, Sandro, Finkelstein, Steven L., Bagley, Micaela, Dickinson, Mark, Ferguson, Henry C., Giavalisco, Mauro, Graziani, Luca, Grogin, Norman A., Hathi, Nimish, Hutchison, Taylor A., Jung, Intae, Koekemoer, Anton M., Larson, Rebecca L., Papovich, Casey, Pirzkal, Norbert, Rojas-Ruiz, Sofía, Song, Mimi, Schneider, Raffaella, Somerville, Rachel S., Wilkins, Stephen M., Yung, L. Y. Aaron

“…We present a detailed stellar population analysis of 11 bright (H < 26.6) galaxies at z=9−11 (three spectroscopically confirmed) to constrain the chemical…”
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Atomic and molecular gas in IllustrisTNG galaxies at low redshift by Diemer, Benedikt, Stevens, Adam R H, Lagos, Claudia del P, Calette, A R, Tacchella, Sandro, Hernquist, Lars, Marinacci, Federico, Nelson, Dylan, Pillepich, Annalisa, Rodriguez-Gomez, Vicente, Villaescusa-Navarro, Francisco, Vogelsberger, Mark

“…ABSTRACT We have recently developed a post-processing framework to estimate the abundance of atomic and molecular hydrogen (H i and H2, respectively) in…”
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The diversity and variability of star formation histories in models of galaxy evolution by Iyer, Kartheik G, Tacchella, Sandro, Genel, Shy, Hayward, Christopher C, Hernquist, Lars, Brooks, Alyson M, Caplar, Neven, Davé, Romeel, Diemer, Benedikt, Forbes, John C, Gawiser, Eric, Somerville, Rachel S, Starkenburg, Tjitske K

“…ABSTRACT Understanding the variability of galaxy star formation histories (SFHs) across a range of time-scales provides insight into the underlying physical…”
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Active Galactic Nuclei Feedback in SDSS-IV MaNGA: AGNs Have Suppressed Central Star Formation Rates by Lammers, Caleb, Iyer, Kartheik G., Ibarra-Medel, Hector, Pacifici, Camilla, Sánchez, Sebastián F., Tacchella, Sandro, Woo, Joanna

“…Abstract Despite the importance of feedback from active galactic nuclei (AGNs) in models of galaxy evolution, observational constraints on the influence of AGN…”
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The MUSE Atlas of Disks (MAD): resolving star formation rates and gas metallicities on <100 pc scales by Erroz-Ferrer, Santiago, Carollo, C Marcella, den Brok, Mark, Onodera, Masato, Brinchmann, Jarle, Marino, Raffaella A, Monreal-Ibero, Ana, Schaye, Joop, Woo, Joanna, Cibinel, Anna, Debattista, Victor P, Inami, Hanae, Maseda, Michael, Richard, Johan, Tacchella, Sandro, Wisotzki, Lutz

“…Abstract We study the physical properties of the ionized gas in local discs using the sample of 38 nearby ∼108.5–11.2 M⊙ Star-Forming Main-Sequence (SFMS)…”
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Self-similar Buildup and Inside-out Growth: Tracing the Evolution of Intermediate-to-high-mass Star-forming Galaxies since z = 2 by Hasheminia, Maryam, Mosleh, Moein, Hosseini-ShahiSavandi, S. Zahra, Tacchella, Sandro

“…Abstract We aim to discern scenarios of structural evolution of intermediate-to-high-mass star-forming galaxies (SFGs) since cosmic noon by comparing their…”
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Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations by Nelson, Erica J, Tacchella, Sandro, Diemer, Benedikt, Leja, Joel, Hernquist, Lars, Whitaker, Katherine E, Weinberger, Rainer, Pillepich, Annalisa, Nelson, Dylan, Terrazas, Bryan A, Nevin, Rebecca, Brammer, Gabriel B, Burkhart, Blakesley, Cochrane, Rachel K, van Dokkum, Pieter, Johnson, Benjamin D, Marinacci, Federico, Mowla, Lamiya, Pakmor, Rüdiger, Skelton, Rosalind E, Speagle, Joshua, Springel, Volker, Torrey, Paul, Vogelsberger, Mark, Wuyts, Stijn

“…ABSTRACT We compare the star-forming main sequence (SFMS) of galaxies – both integrated and resolved on 1 kpc scales – between the high-resolution TNG50…”
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Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2 by Mosleh, Moein, Tacchella, Sandro, Renzini, Alvio, Carollo, C. Marcella, Molaeinezhad, Alireza, Onodera, Masato, Khosroshahi, Habib G., Lilly, Simon

“…We study the history from to of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose, we use…”
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Rapid Quenching of Galaxies at Cosmic Noon by Park, Minjung, Belli, Sirio, Conroy, Charlie, Tacchella, Sandro, Leja, Joel, Cutler, Sam E., Johnson, Benjamin D., Nelson, Erica J., Emami, Razieh

“…Abstract The existence of massive quiescent galaxies at high redshift seems to require rapid quenching, but it is unclear whether all quiescent galaxies have…”
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First Sample of Hα+[O iii]λ5007 Line Emitters at z > 6 Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line-luminosity Functions by Sun, Fengwu, Egami, Eiichi, Pirzkal, Nor, Rieke, Marcia, Baum, Stefi, Boyer, Martha, Boyett, Kristan, Bunker, Andrew J., Cameron, Alex J., Curti, Mirko, Eisenstein, Daniel J., Gennaro, Mario, Greene, Thomas P., Jaffe, Daniel, Kelly, Doug, Koekemoer, Anton M., Kumari, Nimisha, Maiolino, Roberto, Maseda, Michael, Perna, Michele, Rest, Armin, Robertson, Brant E., Schlawin, Everett, Smit, Renske, Stansberry, John, Sunnquist, Ben, Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A.

“…Abstract We present a sample of four emission-line galaxies at z = 6.11–6.35 that were serendipitously discovered using the commissioning data for the James…”
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ΣSFR–M ∗ Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR–M ∗ Diagrams by Salim, Samir, Tacchella, Sandro, Osborne, Chandler, Faber, S. M., Lee, Janice C., Ellison, Sara L.

“…Abstract The specific star formation rate (sSFR) is commonly used to describe the level of galaxy star formation (SF) and to select quenched galaxies. However,…”
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Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View by Costantin, Luca, Pérez-González, Pablo G., Vega-Ferrero, Jesús, Huertas-Company, Marc, Bisigello, Laura, Buitrago, Fernando, Bagley, Micaela B., Cleri, Nikko J., Cooper, Michael C., Finkelstein, Steven L., Holwerda, Benne W., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Nelson, Dylan, Papovich, Casey, Pillepich, Annalisa, Pirzkal, Nor, Tacchella, Sandro, Yung, L. Y. Aaron

“…Abstract We present a catalog of about 25,000 images of massive ( M ⋆ ≥ 10 9 M ⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation,…”
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Building the First Galaxies—Chapter 2. Starbursts Dominate the Star Formation Histories of 6 < z < 12 Galaxies by Dressler, Alan, Rieke, Marcia, Eisenstein, Daniel, Stark, Daniel P., Burns, Chris, Bhatawdekar, Rachana, Bonaventura, Nina, Boyett, Kristan, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Hausen, Ryan, Misselt, Karl, Tacchella, Sandro, Willmer, Christopher

“…Abstract We use SEDz* —a code designed to chart the star formation histories (SFHs) of 6 < z < 12 galaxies—to analyze the spectral energy distributions (SEDs)…”
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