Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Haeussler, Boris"'
Autor:
Singh, Akriti, Guaita, Lucia, Hibon, Pascale, Häussler, Boris, Lee, Kyoung-Soo, Ramakrishnan, Vandana, Kumar, Ankit, Padilla, Nelson, Firestone, Nicole M., Song, Hyunmi, Artale, Maria Celeste, Hwang, Ho Seong, Iribarren, Paulina Troncoso, Gronwall, Caryl, Gawiser, Eric, Nantais, Julie, Valdes, Francisco, Park, Changbom, Yang, Yujin
The aim of this study is to identify quiescent galaxies in the 2-deg$^2$ COSMOS field at $z \sim 3.1$ and analyze their environment. Using data from the ODIN survey and COSMOS2020 catalog, we identify 24 massive quiescent galaxies (MQGs) with stellar
Externí odkaz:
http://arxiv.org/abs/2411.12722
Autor:
Nedkova, Kalina V., Häußler, Boris, Marchesini, Danilo, Brammer, Gabriel B., Feinstein, Adina D., Johnston, Evelyn J., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Martis, Nicholas S., Muzzin, Adam, Rafelski, Marc, Shipley, Heath V., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E.
Using deep imaging from the CANDELS and HFF surveys, we present bulge+disc decompositions with GalfitM for $\sim$17,000 galaxies over $0.2 \leq z\leq 1.5$. We use various model parameters to select reliable samples of discs and bulges, and derive the
Externí odkaz:
http://arxiv.org/abs/2406.14613
Autor:
Nedkova, Kalina V., Rafelski, Marc, Teplitz, Harry I., Mehta, Vihang, DeGroot, Laura, Ravindranath, Swara, Alavi, Anahita, Beckett, Alexander, Grogin, Norman A., Häußler, Boris, Koekemoer, Anton M., Oyarzún, Grecco A., Prichard, Laura, Revalski, Mitchell, Snyder, Gregory F., Sunnquist, Ben, Wang, Xin, Windhorst, Rogier A., Chartab, Nima, Conselice, Christopher J., Guo, Yicheng, Hathi, Nimish, Hayes, Matthew J., Ji, Zhiyuan, Kim, Keunho J., Lucas, Ray A., Mobasher, Bahram, O'Connell, Robert W., Sattari, Zahra, Smith, Brent M., Taamoli, Sina, Yung, L. Y. Aaron, Team, the UVCANDELS
We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for $\sim$16,000 disk-like galaxies over $0.5\leq z \leq 3$. We compare these
Externí odkaz:
http://arxiv.org/abs/2405.10908
The many unique properties of galaxies are shaped by physical processes that affect different components of the galaxy - like the bulges and discs - in different ways, and leave characteristic imprints on the light and spectra of these components. Di
Externí odkaz:
http://arxiv.org/abs/2402.00959
Autor:
Pacifici, Camilla, Iyer, Kartheik G., Mobasher, Bahram, da Cunha, Elisabete, Acquaviva, Viviana, Burgarella, Denis, Rivera, Gabriela Calistro, Carnall, Adam C., Chang, Yu-Yen, Chartab, Nima, Cooke, Kevin C., Fairhurst, Ciaran, Kartaltepe, Jeyhan, Leja, Joel, Malek, Katarzyna, Salmon, Brett, Torelli, Marianna, Vidal-Garcia, Alba, Boquien, Mederic, Brammer, Gabriel G., Brown, Michael J. I., Capak, Peter L., Chevallard, Jacopo, Circosta, Chiara, Croton, Darren, Davidzon, Iary, Dickinson, Mark, Duncan, Kenneth J., Faber, Sandra M., Ferguson, Harry C., Fontana, Adriano, Guo, Yicheng, Haeussler, Boris, Hemmati, Shoubaneh, Jafariyazani, Marziye, Kassin, Susan A., Larson, Rebecca L., Lee, Bomee, Mantha, Kameswara Bharadwaj, Marchi, Francesca, Nayyeri, Hooshang, Newman, Jeffrey A., Pandya, Viraj, Pforr, Janine, Reddy, Naveen, Sanders, Ryan, Shah, Ekta, Shahidi, Abtin, Stevans, Matthew L., Triani, Dian Puspita, Tyler, Krystal D., Vanderhoof, Brittany N., de la Vega, Alexander, Wang, Weichen, Weston, Madalyn E.
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models which allow us to infer physical parameters
Externí odkaz:
http://arxiv.org/abs/2212.01915
Autor:
Cooke, Kevin C., Kartaltepe, Jeyhan S., Rose, Caitlin, Tyler, K. D., Darvish, Behnam, Leslie, Sarah K., Peng, Ying-jie, Häußler, Boris, Koekemoer, Anton M.
We investigate the relationship between environment, morphology, and the star formation rate -- stellar mass relation derived from a sample of star-forming galaxies (commonly referred to as the `star formation main sequence') in the COSMOS field from
Externí odkaz:
http://arxiv.org/abs/2211.16527
Autor:
Rose, Caitlin, Kartaltepe, Jeyhan S., Snyder, Gregory F., Rodriguez-Gomez, Vicente, Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Calabrò, Antonello, Cleri, Nikko J., Cooper, M. C., Costantin, Luca, Croton, Darren, Dickinson, Mark, Finkelstein, Steven L., Häußler, Boris, Holwerda, Benne W., Koekemoer, Anton M., Kurczynski, Peter, Lucas, Ray A., Mantha, Kameswara Bharadwaj, Papovich, Casey, Pérez-González, Pablo G., Pirzkal, Nor, Somerville, Rachel S., Straughn, Amber N., Tacchella, Sandro
Identifying merging galaxies is an important - but difficult - step in galaxy evolution studies. We present random forest classifications of galaxy mergers from simulated JWST images based on various standard morphological parameters. We describe (a)
Externí odkaz:
http://arxiv.org/abs/2208.11164
Autor:
Casura, Sarah, Liske, Jochen, Robotham, Aaron S. G., Brough, Sarah, Driver, Simon P., Graham, Alister W., Häußler, Boris, Holwerda, Benne W., Hopkins, Andrew M., Kelvin, Lee S., Moffett, Amanda J., Taranu, Dan S., Taylor, Edward N.
We derive single S\'ersic fits and bulge-disk decompositions for 13096 galaxies at redshifts z < 0.08 in the GAMA II equatorial survey regions in the Kilo-Degree Survey (KiDS) g, r and i bands. The surface brightness fitting is performed using the Ba
Externí odkaz:
http://arxiv.org/abs/2208.07608
Many galaxies display clear bulges and discs, and understanding how these components form is a vital step towards understanding how the galaxy has evolved into what we see today. The BUDDI-MaNGA project aims to study galaxy evolution and morphologica
Externí odkaz:
http://arxiv.org/abs/2206.08877
Autor:
Johnston, Evelyn J., Häußler, Boris, Jegatheesan, Keerthana, Fraser-McKelvie, Amelia, Coccato, Lodovico, Cortesi, Ariana, Jaffé, Yara, Galaz, Gaspar, Mora, Marcelo, Ordenes-Briceño, Yasna
Many processes have been proposed to explain the quenching of star formation in spiral galaxies and their transformation into S0s. These processes affect the bulge and disc in different ways, and so by isolating the bulge and disc spectra, we can loo
Externí odkaz:
http://arxiv.org/abs/2206.08878