Search Results - "Galaxy formation and evolution"

Semi-analytic model predictions of the galaxy population in protoclusters by Contini, E., De Lucia, G., Hatch, Nina A., Borgani, Stefano, Kang, X.

Subjects: “…Galaxy: formation; galaxies: evolution…”
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Structural evolution of massive galaxies in the last 11 Gyr by Buitrago Alonso, Fernando

Subjects: “…galaxy formation and evolution; galaxies: high redshift; galaxies: massive; galaxies…”
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How to build a cluster: the formation and evolution of galaxies in high-redshift clusters and protoclusters by Cooke, Elizabeth A.

Subjects: “…Astronomy Extragalactic Galaxies Clusters Protoclusters Galaxy formation Galaxy evolution…”
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Radio-quiet quasars in the VIDEO survey: evidence for AGN-powered radio emission at S1.4 GHz < 1 mJy by White, Sarah, Jarvis, M., Häußler, B., Maddox, N.

“…Understanding the interplay between black-hole accretion and star formation, and how to disentangle the two, is crucial to our understanding of galaxy formation and evolution. To investigate, we use a combination of optical and near-infrared photometry to select a sample of 74 quasars from the VISTA Deep Extragalactic Observations (VIDEO) survey, over 1 deg2. …”
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The formation and evolution of massive galaxies and their supermassive black holes over the past 12 billion years by Bluck, Asa Frederick Leon

“…We conclude in Chapter 5 by summarising these findings and commenting upon the powerful role of both internal and external influences on galaxy formation and evolution over the past 12 billion years.…”
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Ultra-fine dark matter structure in the solar neighbourhood by Fantin, Daniele S.M.

“…Thus every attempt to model galaxy formation and evolution has to take into consideration the presence of dark halos. …”
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Sussing merger trees: the impact of halo merger trees on galaxy properties in a semi-analytic model by Lee, Jaehyun, Yi, Sukyoung K., Elahi, Pascal J., Thomas, Peter A., Pearce, Frazer R., Behroozi, Peter, Han, Jiaxin, Helly, John, Jung, Intae, Knebe, Alexander, Mao, Yao-Yuan, Onions, Julian, Rodriguez-Gomez, Vincente, Schneider, Aurel, Srisawat, Chaichalit, Tweed, Dylan

“…A halo merger tree forms the essential backbone of a semi-analytic model for galaxy formation and evolution. Recent studies have pointed out that extracting merger trees from numerical simulations of structure formation is non-trivial; different tree building algorithms can give differing merger histories. …”
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Chromodynamical analysis of lenticular galaxies using globular clusters and planetary nebulae by Zanatta, Emilio J.B., Cortesi, Arianna, Chies-Santos, Ana L., Forbes, Duncan A., Romanowsky, Aaron J., Alabi, Adebusola B., Coccato, Lodovico, Mendes de Oliveira, Claudia, Brodie, Jean P., Merrifield, Michael

“…Recovering the origins of lenticular galaxies can shed light on the understanding of galaxy formation and evolution, since they present properties that can be found in both elliptical and spiral galaxies. …”
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MIGHTEE-H i: the H i size-mass relation over the last billion years by Rajohnson, S.H.A., Frank, B.S., Ponomare, A.A., Maddox, N., Kraan-Korteweg, R.C., Jarvis, M.J., Adams, E.A.K., Oosterloo, T., Baes, M., Spekkens, K., Adams, N.J., Glowacki, Marcin, Kurapati, S., Prandoni, I., Heywood, I., Collier, J.D., Sekhar, S., Taylor, R.

“…For the first time, we quantify the intrinsic scatter of 0.054 ± 0.003 dex (∼10 percent), which provides a constraint for cosmological simulations of galaxy formation and evolution. We derive the relation as a function of galaxy type and find that their intrinsic scatters and slopes are consistent within the errors. …”
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The HerMES SPIRE submillimeter local luminosity function by Vaccari, M., Marchetti, L., Franceschini, A., Altieri, B., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Fox, M., Gear, W., Glenn, J., González Solares, E., Griffin, M., Halpern, M., Hatziminaoglou, E., Huang, J., Ibar, E., Isaak, K., Ivison, R., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Mortier, A., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rigopoulou, D., Rizzo, D., Rodighiero, G., Roseboom, I., Rowan-Robinson, M., Sánchez Portal, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Valiante, E., Valtchanov, I., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C., Zemcov, M.

“…Local luminosity functions are fundamental benchmarks for high-redshift galaxy formation and evolution studies as well as for models describing these processes. …”
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The Herschel Multi-tiered Extragalactic Survey: HerMES by Oliver, S., Bock, J., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Beelen, A., Bethermin, M., Blain, A., Boselli, A., Bridge, C., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chania, P., Cirasuolo, M., Clements, D., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dubois, E., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Feltre, A., Ferrero, P., Fiolet, N., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Gong, Y., Solares, E., Griffin, M., Halpern, M., Harwit, M., Hatziminaoglou, E., Heinis, S., Hurley, P., Hwang, H., Hyde, A., Ibar, E., Ilbert, O., Isaak, K., Ivison, R., Lagache, G., Le Floc'h, E., Levenson, L., Lo Faro, B., Lu, N., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Marchetti, L., Marsden, G., Marshall, J., Mortier, A., Nguyen, H., O'Halloran, B., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Patel, H., Pearson, C., Perez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I., Rowan-Robinson, M., Portal, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Vigroux, L., Wang, L., Ward, R., Wardlow, J., Wright, G., Xu, C., Zemcov, M.

“…These bands cover the peak of the redshifted thermal spectral energy distribution from interstellar dust and thus capture the reprocessed optical and ultraviolet radiation from star formation that has been absorbed by dust, and are critical for forming a complete multiwavelength understanding of galaxy formation and evolution. The survey will detect of the order of 100000 galaxies at 5s in some of the best-studied fields in the sky. …”
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Physical properties of z > 4 submillimeter galaxies in the COSMOS field by Smolcic, V., Karim, A., Miettinen, O., Novak, M., Magnelli, B., Riechers, D., Schinnerer, E., Capak, P., Bondi, M., Ciliegi, P., Aravena, M., Bertoldi, F., Bourke, S., Banfield, J., Carilli, C., Civano, F., Ilbert, O., Intema, Hubertus, Le Fèvre, O., Finoguenov, A., Hallinan, G., Klöckner, H., Koekemoer, A., Laigle, C., Masters, D., McCracken, H., Mooley, K., Murphy, E., Navarette, F., Salvato, M., Sargent, M., Sheth, K., Toft, S., Zamorani, G.

“…Thus, additional in-depth analyses of large, statistical samples of high-redshift SMGs are needed to fully understand their role in galaxy formation and evolution.…”
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Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3 by Guo, Yicheng, Rafelski, Marc, Bell, Eric F., Conselice, Christopher J., Dekel, Avishai, Faber, S. M., Giavalisco, Mauro, Koekemoer, Anton M., Koo, David C., Lu, Yu, Mandelker, Nir, Primack, Joel R., Ceverino, Daniel, de Mello, Duilia F., Ferguson, Henry C., Hathi, Nimish, Kocevski, Dale, Lucas, Ray A., Pérez-González, Pablo G., Ravindranath, Swara, Soto, Emmaris, Straughn, Amber, Wang, Weichen

“…Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists have not reached a consensus on whether the observed "clumps" in distant galaxies are the same phenomenon that is seen in simulations. …”
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The history of stellar mass in the most massive galaxies at z < 3.5 by Mundy, Carl J.

“…This is achieved through the analyses of several publicly a available semi-analytic models of galaxy formation and evolution, combined with a large sample of approximately 350,000 galaxies at 0.005< z <3.5. …”
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The formation and evolution of galaxies as a function of environment by Jaffe, Yara Lorena

“…This thesis investigates the role of environment on galaxy formation and evolution, giving particular focus to the transformation of star forming spirals into passive S0s. …”
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The Cosmic Evolution of Galaxy Structure and Morphology at 0.5 < z < 8 by Ferreira, Leonardo

“…We briefly discuss the implica- tions of this result and how it fits in the galaxy formation and evolution evolution Over Chapter 5 we expand the framework of Chapter 4 to the early CEERS JWST observations that have overlap with the EGS observations from the CAN- DELS fields with HST. …”
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