Zobrazeno 1 - 10
of 79
pro vyhledávání: '"Lee, BoMee"'
Autor:
Crill, Brendan P., Werner, Michael, Akeson, Rachel, Ashby, Matthew, Bleem, Lindsey, Bock, James J., Bryan, Sean, Burnham, Jill, Byunh, Joyce, Chang, Tzu-Ching, Chiang, Yi-Kuan, Cook, Walter, Cooray, Asantha, Davis, Andrew, Doré, Olivier, Dowell, C. Darren, Dubois-Felsmann, Gregory, Eifler, Tim, Faisst, Andreas, Habib, Salman, Heinrich, Chen, Heitmann, Katrin, Heaton, Grigory, Hirata, Christopher, Hristov, Viktor, Hui, Howard, Jeong, Woong-Seob, Kang, Jae Hwan, Kecman, Branislav, Kirkpatrick, J. Davy, Korngut, Phillip M., Krause, Elisabeth, Lee, Bomee, Lisse, Carey, Masters, Daniel, Mauskopf, Philip, Melnick, Gary, Miyasaka, Hiromasa, Nayyeri, Hooshang, Nguyen, Hien, Öberg, Karin, Padin, Steve, Paladini, Roberta, Pourrahmani, Milad, Pyo, Jeonghyun, Smith, Roger, Song, Yong-Seong, Symons, Teresa, Teplitz, Harry, Tolls, Volker, Unwin, Steve, Windhorst, Rogier, Yang, Yujin, Zemcov, Michael
Publikováno v:
Proceedings Volume 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave; 114430I (2020)
SPHEREx, the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and ices Explorer, is a NASA MIDEX mission planned for launch in 2024. SPHEREx will carry out the first all-sky spectral survey at wavelengths between 0.75 micron
Externí odkaz:
http://arxiv.org/abs/2404.11017
Autor:
Feder, Richard M., Masters, Daniel C., Lee, Bomee, Bock, James J., Chiang, Yi-Kuan, Choi, Ami, Dore, Olivier, Hemmati, Shoubaneh, Ilbert, Olivier
We simulate galaxy properties and redshift estimation for SPHEREx, the next NASA Medium Class Explorer. To make robust models of the galaxy population and test spectro-photometric redshift performance for SPHEREx, we develop a set of synthetic spectr
Externí odkaz:
http://arxiv.org/abs/2312.04636
Autor:
Lee, Bomee, Giavalisco, Mauro, Whitaker, Katherine, Williams, Christina C., Ferguson, Henry C., Acquaviva, Viviana, Koekemoer, Anton M., Straughn, Amber N., Guo, Yicheng, Kartaltepe, Jeyhan S., Lotz, Jennifer, Pacifici, Camilla, Croton, Darren J., Somerville, Rachel S., Lu, Yu
We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass (M-*), star formation rate (SFR) and morphology, and to introduce a fourth dimension, the mass-weighted stellar age, in galaxies
Externí odkaz:
http://hdl.handle.net/10150/627039
http://arizona.openrepository.com/arizona/handle/10150/627039
http://arizona.openrepository.com/arizona/handle/10150/627039
Autor:
Williams, Christina C., Giavalisco, Mauro, Bezanson, Rachel, Cappelluti, Nico, Cassata, Paolo, Liu, Teng, Lee, Bomee, Tundo, Elena, Vanzella, Eros
We report the detection of morphology-dependent stellar age in massive quenched galaxies (QGs) at z similar to 1.2. The sense of the dependence is that compact QGs are 0.5-2 Gyr older than normal-sized ones. The evidence comes from three different ag
Externí odkaz:
http://hdl.handle.net/10150/623820
http://arizona.openrepository.com/arizona/handle/10150/623820
http://arizona.openrepository.com/arizona/handle/10150/623820
Autor:
Finner, Kyle, Lee, Bomee, Chary, Ranga-Ram, Jee, M. James, Hirata, Christopher, Congedo, Giuseppe, Taylor, Peter, Hyeonghan, Kim
We have undertaken a Near-IR Weak Lensing (NIRWL) analysis of the wide-field CANDELS HST/WFC3-IR F160W observations. With the Gaia proper-motion-corrected catalog as an astrometric reference, we updated the astrometry of the five CANDELS mosaics and
Externí odkaz:
http://arxiv.org/abs/2301.07725
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:
Lee, Bomee, Chary, Ranga-Ram
We use archival WISE and Spitzer photometry to derive optical line fluxes for a sample of distant quasars at z ~6. We find evidence for exceptionally high equivalent width [OIII] emission (rest-frame EW ~400 {\AA}) similar to that inferred for star-f
Externí odkaz:
http://arxiv.org/abs/2207.07290
Autor:
Makhathini, Sphesihle, Mooley, Kunal P., Brightman, Murray, Hotokezaka, Kenta, Nayana, AJ, Intema, Huib T., Dobie, Dougal, Lenc, E., Perley, Daniel A., Fremling, Christoffer, Moldon, Javier, Lazzati, Davide, Kaplan, David L., Balasubramanian, Arvind, Brown, Ian, Carbone, Dario, Chandra, Poonam, Corsi, Alessandra, Camilo, Fernando, Deller, Adam T., Frail, Dale A., Murphy, Tara, Murphy, Eric J., Nakar, Ehud, Smirnov, Oleg, Beswick, Robert, Fender, Rob, Hallinan, Gregg, Heywood, Ian, Kasliwal, Mansi M., Lee, Bomee, Lu, Wenbin, Rana, Javed, Perkins, S. J., White, Sarah V., Jozsa, Gyula I., Hugo, Benjamin, Kamphuis, Peter
We present the full panchromatic afterglow light curve data of GW170817, including new radio data as well as archival optical and X-ray data, between 0.5 and 940 days post-merger. By compiling all archival data, and reprocessing a subset of it, we ha
Externí odkaz:
http://arxiv.org/abs/2006.02382
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Akademický článek
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