Zobrazeno 1 - 10
of 1 074
pro vyhledávání: '"P. Behroozi"'
Autor:
G. Yang, K. I. Caputi, C. Papovich, P. Arrabal Haro, M. B. Bagley, P. Behroozi, E. F. Bell, L. Bisigello, V. Buat, D. Burgarella, Y. Cheng, N. J. Cleri, R. Davé, M. Dickinson, D. Elbaz, H. C. Ferguson, S. L. Finkelstein, N. A. Grogin, N. P. Hathi, M. Hirschmann, B. W. Holwerda, M. Huertas-Company, T. A. Hutchison, E. Iani, J. S. Kartaltepe, A. Kirkpatrick, D. D. Kocevski, A. M. Koekemoer, V. Kokorev, R. L. Larson, R. A. Lucas, P. G. Pérez-González, P. Rinaldi, L. Shen, J. R. Trump, A. de la Vega, L. Y. A. Yung, J. A. Zavala
Publikováno v:
The Astrophysical Journal Letters, Vol 950, Iss 1, p L5 (2023)
Mid-infrared (mid-IR) observations are powerful in identifying heavily obscured active galactic nuclei (AGN) that have weak emission in other wavelengths. Data from the Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope provides a
Externí odkaz:
https://doaj.org/article/fa22cf636dc34cb18e85e7df786afc93
Autor:
Dehghani, Mahshid, Shafiee, Amirahmad, Shafiei, Ali, Fallah, Neda, Alizadeh, Farahmand, Gholinejad, Mohammad Mehdi, Behroozi, Hamid, Habibi, Jafar, Asgari, Ehsaneddin
Existing 3D facial emotion modeling have been constrained by limited emotion classes and insufficient datasets. This paper introduces "Emo3D", an extensive "Text-Image-Expression dataset" spanning a wide spectrum of human emotions, each paired with i
Externí odkaz:
http://arxiv.org/abs/2410.02049
Autor:
Zhang, Haowen, Behroozi, Peter, Volonteri, Marta, Silk, Joseph, Fan, Xiaohui, Aird, James, Yang, Jinyi, Wang, Feige, Hopkins, Philip F.
We infer supermassive black hole (SMBH) accretion rates and Eddington ratios as a function of SMBH/host galaxy mass and redshift with the empirical TRINITY model of dark matter halo--galaxy--SMBH connection. The galaxy--SMBH mass and growth rate conn
Externí odkaz:
http://arxiv.org/abs/2409.16347
Autor:
Behroozi, Ali, Edrisi, Ali
Public transportation systems play a crucial role in daily commutes, business operations, and leisure activities, emphasizing the need for effective management to meet public demands. One approach to achieve this goal is by predicting demand at the s
Externí odkaz:
http://arxiv.org/abs/2408.09317
Autor:
Khan, Aafaque R., Hamden, Erika, Chung, Haeun, Choi, Heejoo, Kim, Daewook, Melso, Nicole, Hoadley, Keri, Vargas, Carlos J., Truong, Daniel, Garcia, Elijah, Verts, Bill, Coronado, Fernando, Noenickx, Jamison, Corliss, Jason, Tanquary, Hannah, Mcmahon, Tom, Hamara, Dave, Agarwal, Simran, Augustin, Ramona, Behroozi, Peter, Bradley, Harrison, Brendel, Trenton, Burchett, Joe, Castillo, Jasmine Martinez, Chambers, Jacob, Corlies, Lauren, Davis, Greyson, Dettmar, Ralf-Jürgen, Douglas, Ewan, Ghidoli, Giulia, Goodwin, Alfred, Harris, Walter, Hergenrother, Carl, Howk, J. Christopher, Keppler, Miriam, Kerkeser, Nazende Ipek, Kidd Jr., John N., Li, Jessica S., Noriega, Gabe, Park, Sooseong, Pecha, Ryan, Sauve, Cork, Schiminovich, David, Selznick, Sanford, Siegmund, Oswald, Su, Rebecca, Uppnor, Sumedha, Vider, Jacob, Wolcott, Ellie, Yescas, Naomi, Zaritsky, Dennis
Aspera is a NASA Astrophysics Pioneers SmallSat mission designed to study diffuse OVI emission from the warm-hot phase gas in the halos of nearby galaxies. Its payload consists of two identical Rowland Circle-type long-slit spectrographs, sharing a s
Externí odkaz:
http://arxiv.org/abs/2407.15391
For the joint analysis of second-order weak lensing and galaxy clustering statistics, so-called $3{\times}2$ analyses, the selection and characterization of optimal galaxy samples is a major area of research. One promising choice is to use the same g
Externí odkaz:
http://arxiv.org/abs/2406.17985
Autor:
Wang, Yunchong, Nadler, Ethan O., Mao, Yao-Yuan, Wechsler, Risa H., Abel, Tom, Behroozi, Peter, Geha, Marla, Asali, Yasmeen, Reyes, Mithi A. C. de los, Kado-Fong, Erin, Kallivayalil, Nitya, Tollerud, Erik J., Weiner, Benjamin, Wu, John F.
Environment plays a critical role in shaping the assembly of low-mass galaxies. Here, we use the UniverseMachine (UM) galaxy-halo connection framework and the Data Release 3 of the Satellites Around Galactic Analogs (SAGA) Survey to place dwarf galax
Externí odkaz:
http://arxiv.org/abs/2404.14500
Autor:
Kakos, James, Rodriguez-Puebla, Aldo, Primack, Joel R., Faber, Sandra M., Koo, David C., Behroozi, Peter, Avila-Reese, Vladimir
We measure the clustering of low-redshift SDSS galaxies as a function of stellar mass ($10.0<\log(M_*/M_\odot)<11.5$) and specific star formation rate (sSFR) and compare the results to models of the galaxy--halo connection. We find that the auto-corr
Externí odkaz:
http://arxiv.org/abs/2403.01393
Autor:
Wang, Yirong, Yang, Xiaohu, Gu, Yizhou, Xu, Xiaoju, Xu, Haojie, Wang, Yuyu, Katsianis, Antonios, Han, Jiaxin, He, Min, Zheng, Yunliang, Li, Qingyang, Wang, Yaru, Hong, Wensheng, Wang, Jiaqi, Tan, Zhenlin, Zou, Hu, Lange, Johannes Ulf, Hahn, ChangHoon, Behroozi, Peter, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Claybaugh, Todd, Cole, Shaun, de la Macorra, Axel, Dey, Biprateep, Doel, Peter, Forero-Romero, Jaime E., Honscheid, Klaus, Kehoe, Robert, Kisner, Theodore, Lambert, Andrew, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Poppett, Claire, Rezaie, Mehdi, Rossi, Graziano, Sanchez, Eusebio, Schubnell, Michael, Tarlé, Gregory, Weaver, Benjamin Alan, Zhou, Zhimin
In this investigation, we leverage the combination of Dark Energy Spectroscopic Instrument Legacy imaging Surveys Data Release 9 (DESI LS DR9), Survey Validation 3 (SV3), and Year 1 (Y1) data sets to estimate the conditional luminosity and stellar ma
Externí odkaz:
http://arxiv.org/abs/2312.17459
Autor:
Wilkins, Stephen M., Turner, Jack C., Bagley, Micaela B., Finkelstein, Steven L., Amorín, Ricardo O., Hautefort, Adrien Aufan Stoffels D, Behroozi, Peter, Bhatawdekar, Rachana, Dekel, Avishai, Donnellan, James, Drakos, Nicole E., Fortuni, Flaminia, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Irodotou, Dimitrios, Koekemoer, Anton M., Lovell, Christopher C., Merlin, Emiliano, Roper, Will J., Seeyave, Louise T. C., Vijayan, Aswin P., Yung, L. Y. Aaron
The wavelength-coverage and sensitivity of JWST now enables us to probe the rest-frame UV - optical spectral energy distributions (SEDs) of galaxies at high-redshift ($z>4$). From these SEDs it is, in principle, through SED fitting possible to infer
Externí odkaz:
http://arxiv.org/abs/2311.08065