Zobrazeno 1 - 10
of 108
pro vyhledávání: '"McPartland, Conor"'
Autor:
Killi, Meghana, Watson, Darach, Brammer, Gabriel, McPartland, Conor, Antwi-Danso, Jacqueline, Newshore, Rosa, Coe, Dan, Allen, Natalie, Fynbo, Johan P. U., Gould, Katriona, Heintz, Kasper E., Rusakov, Vadim, Vejlgaard, Simone
JWST has revealed a class of numerous, extremely compact sources, with rest-frame red optical/near-infrared (NIR) and blue ultraviolet (UV) colours, nicknamed "little red dots". We present one of the highest signal-to-noise ratio JWST NIRSpec/PRISM s
Externí odkaz:
http://arxiv.org/abs/2312.03065
Autor:
Brinch, Malte, Greve, Thomas R., Sanders, David B., McPartland, Conor J. R., Chartab, Nima, Gillman, Steven, Vijayan, Aswin P., Lee, Minju M., Brammer, Gabriel, Casey, Caitlin M., Ilbert, Olivier, Jin, Shuowen, Magdis, Georgios, McCracken, H. J., Sillassen, Nikolaj B., Toft, Sune, Zavala, Jorge A.
We present the results of our Keck/DEIMOS spectroscopic follow-up of candidate galaxies of i-band-dropout protocluster candidate galaxies at $z\sim6$ in the COSMOS field. We securely detect Lyman-$\alpha$ emission lines in 14 of the 30 objects target
Externí odkaz:
http://arxiv.org/abs/2311.00511
Autor:
Ito, Kei, Valentino, Francesco, Brammer, Gabriel, Faisst, Andreas L., Gillman, Steven, Gomez-Guijarro, Carlos, Gould, Katriona M. L., Heintz, Kasper E., Ilbert, Olivier, Jespersen, Christian Kragh, Kokorev, Vasily, Kubo, Mariko, Magdis, Georgios E., McPartland, Conor, Onodera, Masato, Rizzo, Francesca, Tanaka, Masayuki, Toft, Sune, Vijayan, Aswin P., Weaver, John R., Whitaker, Katherine E., Wright, Lillian
We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera (NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$ color, we focus on 26
Externí odkaz:
http://arxiv.org/abs/2307.06994
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:
Farrah, Duncan, Croker, Kevin S., Tarlé, Gregory, Faraoni, Valerio, Petty, Sara, Afonso, Jose, Fernandez, Nicolas, Nishimura, Kurtis A., Pearson, Chris, Wang, Lingyu, Zevin, Michael, Clements, David L, Efstathiou, Andreas, Hatziminaoglou, Evanthia, Lacy, Mark, McPartland, Conor, Pitchford, Lura K, Sakai, Nobuyuki, Weiner, Joel
Publikováno v:
ApJL 944 L31 (2023)
Observations have found black holes spanning ten orders of magnitude in mass across most of cosmic history. The Kerr black hole solution is however provisional as its behavior at infinity is incompatible with an expanding universe. Black hole models
Externí odkaz:
http://arxiv.org/abs/2302.07878
Autor:
Steinhardt, Charles L., Rusakov, Vadim, Clark, Thomas H., Diaconu, Andrei, McPartland, Conor, Forbes, John, Sneppen, Albert, Weaver, John
Using a recently-developed technique to estimate gas temperatures ($T_\textrm{SF}$) in star-forming regions from large photometric surveys, we propose a diagram, analogous to the Hertzsprung-Russell diagram for individual stars, to probe the evolutio
Externí odkaz:
http://arxiv.org/abs/2301.01774
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:
Brinch, Malte, Greve, Thomas R., Weaver, John R., Brammer, Gabriel, Ilbert, Olivier, Shuntov, Marko, Jin, Shuowen, Liu, Daizhong, Giménez-Arteaga, Clara, Casey, Caitlin M., Davidson, Iary, Fujimoto, Seiji, Koekemoer, Anton M., Kokorev, Vasily, Magdis, Georgios, McCracken, H. J., McPartland, Conor J. R., Mobasher, Bahram, Sanders, David B., Toft, Sune, Valentino, Francesco, Zamorani, Giovanni, Zavala, Jorge
We conduct a systematic search for protocluster candidates at $z \geq 6$ in the COSMOS field using the recently released COSMOS2020 source catalog. We select galaxies using a number of selection criteria to obtain a sample of galaxies that have a hig
Externí odkaz:
http://arxiv.org/abs/2210.17334
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
We perform an analysis of two-point galaxy clustering and galaxy bias using Subaru Hyper-Suprime Cam (HSC) data taken jointly by the Subaru Strategic Program and the University of Hawaii in the COSMOS field. The depth of the data is similar to the on
Externí odkaz:
http://arxiv.org/abs/1909.12854