Search Results - "Thob, Adrien C. R."

The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE by Thob, Adrien C R, Crain, Robert A, McCarthy, Ian G, Schaller, Matthieu, Lagos, Claudia D P, Schaye, Joop, Talens, Geert Jan J, James, Philip A, Theuns, Tom, Bower, Richard G

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Generating synthetic star catalogs from simulated data for next-gen observatories with py-ananke by Thob, Adrien C. R, Sanderson, Robyn E, Eden, Andrew P, Nikakhtar, Farnik, Panithanpaisal, Nondh, Garavito-Camargo, Nicolás, Sharma, Sanjib

“…Journal of Open Source Software, October 2024, vol. 9, issue 102, id. 6234 We find ourselves on the brink of an exciting era in observational astrophysics,…”
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The relation between galaxy morphology and colour in the EAGLE simulation by Correa, Camila A., Schaye, Joop, Clauwens, Bart, Bower, Richard G., Crain, Robert A., Schaller, Matthieu, Theuns, Tom, Thob, Adrien C. R.

“…Abstract We investigate the relation between kinematic morphology, intrinsic colour and stellar mass of galaxies in the EAGLE cosmological hydrodynamical…”
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Generating synthetic star catalogs from simulated data for next-gen observatories with py-ananke by Thob, Adrien C. R., Sanderson, Robyn E., Eden, Andrew P., Nikakhtar, Farnik, Panithanpaisal, Nondh, Garavito-Camargo, Nicolás, Sharma, Sanjib

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The relation between galaxy morphology and colour in the EAGLE simulation by Correa, Camila A, Schaye, Joop, Clauwens, Bart, Bower, Richard G, Crain, Robert A, Schaller, Matthieu, Theuns, Tom, Thob, Adrien C. R

“…We investigate the relation between kinematic morphology, intrinsic colour and stellar mass of galaxies in the EAGLE cosmological hydrodynamical simulation. We…”
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The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE by Thob, Adrien C. R, Crain, Robert A, McCarthy, Ian G, Schaller, Matthieu, Lagos, Claudia D. P, Schaye, Joop, Talens, Geert Jan J, James, Philip A, Theuns, Tom, Bower, Richard G

“…We investigate the connection between the morphology and internal kinematics of the stellar component of central galaxies with mass $M_\star > {10}^{9.5} {\rm…”
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RomAndromeda: The Roman Survey of the Andromeda Halo by Dey, Arjun, Najita, Joan, Filion, Carrie, Han, Jiwon Jesse, Pearson, Sarah, Wyse, Rosemary, Thob, Adrien C. R, Anguiano, Borja, Apfel, Miranda, Arnaboldi, Magda, Bell, Eric F, Silva, Leandro Beraldo e, Besla, Gurtina, Bhattacharya, Aparajito, Bhattacharya, Souradeep, Chandra, Vedant, Choi, Yumi, Collins, Michelle L. M, Cunningham, Emily C, Dalcanton, Julianne J, Escala, Ivanna, Foote, Hayden R, Ferguson, Annette M. N, Gibson, Benjamin J, Gnedin, Oleg Y, Guhathakurta, Puragra, Hawkins, Keith, Horta, Danny, Ibata, Rodrigo, Kallivayalil, Nitya, Koch, Eric W, Koposov, Sergey, Lewis, Geraint F, Macri, Lucas, McKinnon, Kevin A, Nidever, David L, Olsen, Knut A. G, Patel, Ekta, Petersen, Michael S, Petric, Andreea, Price-Whelan, Adrian M, Rich, R. Michael, Riley, Alexander H, Saha, Abhijit, Sanderson, Robyn E, Sharma, Sanjib, Sohn, Sangmo Tony, Soraisam, Monika D, Steinmetz, Matthias, Valluri, Monica, Vivas, A. Katherina, Williams, Benjamin F, Wojno, J. Leigh

“…As our nearest large neighbor, the Andromeda Galaxy provides a unique laboratory for investigating galaxy formation and the distribution and substructure…”
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