Zobrazeno 1 - 10
of 1 684
pro vyhledávání: '"Capak, P"'
Autor:
Taamoli, Sina, Nezhad, Negin, Mobasher, Bahram, Manesh, Faezeh, Chartab, Nima, Weaver, John R., Capak, Peter L., Casey, Caitlin M., Gozaliasl, Ghassem, Heintz, Kasper E., Ilbert, Olivier, Kartaltepe, Jeyhan S., McCracken, Henry J., Sanders, David B., Scoville, Nicholas, Toft, Sune, Watson, Darach
The role of internal and environmental factors in the star formation activity of galaxies is still a matter of debate, particularly at higher redshifts. Leveraging the most recent release of the COSMOS catalog, COSMOS2020, and density measurements fr
Externí odkaz:
http://arxiv.org/abs/2411.09522
Autor:
Taamoli, Sina, Mobasher, Bahram, Chartab, Nima, Darvish, Behnam, Weaver, John R., Hemmati, Shoubaneh, Casey, Caitlin M., Sattari, Zahra, Brammer, Gabriel B., Capak, Peter L., Ilbert, Olivier, Kartaltepe, Jeyhan S., McCracken, Henry J., Moneti, Andrea, Sanders, David B., Scoville, Nick Z., Steinhardt, Charles L., Toft, Sune
To study the role of environment in galaxy evolution, we reconstruct the underlying density field of galaxies based on COSMOS2020 (The Farmer catalog) and provide the density catalog for a magnitude limited ($K_{s}<24.5$) sample of $\sim 210 \, k$ ga
Externí odkaz:
http://arxiv.org/abs/2312.10222
Autor:
Weaver, J. R., Zalesky, L., Kokorev, V., McPartland, C. J. R., Chartab, N., Gould, K. M. L., Shuntov, M., Davidzon, I., Faisst, A., Stickley, N., Capak, P. L., Toft, S., Masters, D., Mobasher, B., Sanders, D. B., Kauffmann, O. B., McCracken, H. J., Ilbert, O., Brammer, G., Moneti, A.
While space-borne optical and near-infrared facilities have succeeded in delivering a precise and spatially resolved picture of our Universe, their small survey area is known to under-represent the true diversity of galaxy populations. Ground-based s
Externí odkaz:
http://arxiv.org/abs/2310.07757
Autor:
Ortiz, Oscar A. Chavez, Finkelstein, Steven L., Davis, Dustin, Leung, Gene, Cooper, Erin Mentuch, Bagley, Micaela, Larson, Rebecca, Casey, Caitlin M., McCarron, Adam P., Gebhardt, Karl, Guo, Yuchen, Liu, Chenxu, Laseter, Isaac, Rhodes, Jason, Bender, Ralf, Fabricius, Max, Sanchez, Ariel G., Scarlata, Claudia, Capak, Peter, Sanders, David, Szapudi, Istvan, Baxter, Eric, McPartland, Conor, Weaver, John R., Toft, Sune, Suzuki, Nao, Chartab, Nima
We present the Texas Euclid Survey for Lyman-Alpha (TESLA), a spectroscopic survey in the 10 square degree of the Euclid North Ecliptic Pole (NEP) field. Using TESLA, we study how the physical properties of Lyman-alpha emitters (LAEs) correlate with
Externí odkaz:
http://arxiv.org/abs/2304.03258
Autor:
Weaver, J. R., Davidzon, I., Toft, S., Ilbert, O., McCracken, H. J., Gould, K. M. L., Jespersen, C. K., Steinhardt, C., Lagos, C. D. P., Capak, P. L., Casey, C. M., Chartab, N., Faisst, A. L., Hayward, C. C., Kartaltepe, J. S., Kauffmann, O. B., Koekemoer, A. M., Kokorev, V., Laigle, C., Liu, D., Long, A., Magdis, G. E., McPartland, C. J. R., Milvang-Jensen, B., Mobasher, B., Moneti, A., Peng, Y., Sanders, D. B., Shuntov, M., Sneppen, A., Valentino, F., Zalesky, L., Zamorani, G.
Publikováno v:
A&A 677, A184 (2023)
How galaxies form, assemble, and cease their star-formation is a central question within the modern landscape of galaxy evolution studies. These processes are indelibly imprinted on the galaxy stellar mass function (SMF). We present constraints on th
Externí odkaz:
http://arxiv.org/abs/2212.02512
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:
Kwon, Hyoukjun, Nair, Krishnakumar, Seo, Jamin, Yik, Jason, Mohapatra, Debabrata, Zhan, Dongyuan, Song, Jinook, Capak, Peter, Zhang, Peizhao, Vajda, Peter, Banbury, Colby, Mazumder, Mark, Lai, Liangzhen, Sirasao, Ashish, Krishna, Tushar, Khaitan, Harshit, Chandra, Vikas, Reddi, Vijay Janapa
Real-time multi-task multi-model (MTMM) workloads, a new form of deep learning inference workloads, are emerging for applications areas like extended reality (XR) to support metaverse use cases. These workloads combine user interactivity with computa
Externí odkaz:
http://arxiv.org/abs/2211.08675
Autor:
Casey, Caitlin M., Kartaltepe, Jeyhan S., Drakos, Nicole E., Franco, Maximilien, Harish, Santosh, Paquereau, Louise, Ilbert, Olivier, Rose, Caitlin, Cox, Isabella G., Nightingale, James W., Robertson, Brant E., Silverman, John D., Koekemoer, Anton M., Massey, Richard, McCracken, Henry Joy, Rhodes, Jason, Akins, Hollis B., Amvrosiadis, Aristeidis, Arango-Toro, Rafael C., Bagley, Micaela B., Bongiorno, Angela, Capak, Peter L., Champagne, Jaclyn B., Chartab, Nima, Ortiz, Oscar A. Chavez, Chworowsky, Katherine, Cooke, Kevin C., Cooper, Olivia R., Darvish, Behnam, Ding, Xuheng, Faisst, Andreas L., Finkelstein, Steven L., Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gould, Katriona M. L., Gozaliasl, Ghassem, Hayward, Christopher C., He, Qiuhan, Hemmati, Shoubaneh, Hirschmann, Michaela, Jahnke, Knud, Jin, Shuowen, Khostovan, Ali Ahmad, Kokorev, Vasily, Lambrides, Erini, Laigle, Clotilde, Larson, Rebecca L., Leung, Gene C. K., Liu, Daizhong, Liaudat, Tobias, Long, Arianna S., Magdis, Georgios, Mahler, Guillaume, Mainieri, Vincenzo, Manning, Sinclaire M., Maraston, Claudia, Martin, Crystal L., McCleary, Jacqueline E., McKinney, Jed, McPartland, Conor J. R., Mobasher, Bahram, Pattnaik, Rohan, Renzini, Alvio, Rich, R. Michael, Sanders, David B., Sattari, Zahra, Scognamiglio, Diana, Scoville, Nick, Sheth, Kartik, Shuntov, Marko, Sparre, Martin, Suzuki, Tomoko L., Talia, Margherita, Toft, Sune, Trakhtenbrot, Benny, Urry, C. Megan, Valentino, Francesco, Vanderhoof, Brittany N., Vardoulaki, Eleni, Weaver, John R., Whitaker, Katherine E., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging survey in fou
Externí odkaz:
http://arxiv.org/abs/2211.07865
Autor:
Scoville, Nick, Faisst, Andreas, Weaver, John, Toft, Sune, McCracken, Henry, Ilbert, Olivier, Diaz-Santos, Tanio, Staguhn, Johannes, Koda, Jin, Casey, Caitlin, Sanders, David, Mobasher, Bahram, Chartab, Nima, Sattari, Zahra, Capak, Peter, Bout, Paul Vanden, Bongiorno, Angela, Vlahakis, Catherine, Sheth, Kartik, Yun, Min, Aussel, Herve, Laigle, Clotilde, Masters, Dan
ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the dependence of gas masses and star formation efficiencies (SFE=SFR per unit g
Externí odkaz:
http://arxiv.org/abs/2211.07836
Autor:
Chartab, Nima, Mobasher, Bahram, Cooray, Asantha, Hemmati, Shoubaneh, Sattari, Zahra, Ferguson, Henry C., Sanders, David B., Weaver, John R., Stern, Daniel, McCracken, Henry J., Masters, Daniel C., Toft, Sune, Capak, Peter L., Davidzon, Iary, Dickinson, Mark, Rhodes, Jason, Moneti, Andrea, Ilbert, Olivier, Zalesky, Lukas, McPartland, Conor, Szapudi, Istvan, Koekemoer, Anton M., Teplitz, Harry I., Giavalisco, Mauro
We present a new method based on information theory to find the optimal number of bands required to measure the physical properties of galaxies with a desired accuracy. As a proof of concept, using the recently updated COSMOS catalog (COSMOS2020), we
Externí odkaz:
http://arxiv.org/abs/2208.14781