Zobrazeno 1 - 10
of 134
pro vyhledávání: '"Lagos, Claudia D P"'
Autor:
Weibel, Andrea, de Graaff, Anna, Setton, David J., Miller, Tim B., Oesch, Pascal A., Brammer, Gabriel, Lagos, Claudia D. P., Whitaker, Katherine E., Williams, Christina C., Baggen, Josephine F. W., Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Greene, Jenny E., Hirschmann, Michaela, Hviding, Raphael E., Kuruvanthodi, Adarsh, Labbé, Ivo, Leja, Joel, Maseda, Michael V., Matthee, Jorryt, McConachie, Ian, Naidu, Rohan P., Roberts-Borsani, Guido, Schaerer, Daniel, Suess, Katherine A., Valentino, Francesco, van Dokkum, Pieter, Wang, Bingjie
We report the spectroscopic discovery of a massive quiescent galaxy at $z_{\rm spec}=7.29\pm0.01$, just $\sim700\,$Myr after the Big Bang. RUBIES-UDS-QG-z7 was selected from public JWST/NIRCam and MIRI imaging from the PRIMER survey and observed with
Externí odkaz:
http://arxiv.org/abs/2409.03829
Autor:
Mai, Yifan, Croom, Scott M., Wisnioski, Emily, Vaughan, Sam P., Varidel, Mathew R., Battisti, Andrew J., Mendel, J. Trevor, Mun, Marcie, Tsukui, Takafumi, Foster, Caroline, Harborne, Katherine E., Lagos, Claudia D. P., Wang, Di, Bellstedt, Sabine, Bland-Hawthorn, Joss, Colless, Matthew, D'Eugenio, Francesco, Grasha, Kathryn, Peng, Yingjie, Santucci, Giulia, Sweet, Sarah M., Thater, Sabine, Valenzuela, Lucas M., Ziegler, Bodo
We measure the ionised gas velocity dispersions of star-forming galaxies in the MAGPI survey ($z\sim0.3$) and compare them with galaxies in the SAMI ($z\sim0.05$) and KROSS ($z\sim1$) surveys to investigate how the ionised gas velocity dispersion evo
Externí odkaz:
http://arxiv.org/abs/2408.12224
Autor:
Zhou, Dazhi, Greve, Thomas R., Gullberg, Bitten, Lee, Minju M., Di Mascolo, Luca, Dicker, Simon R., Romero, Charles E., Chapman, Scott C., Chen, Chian-Chou, Cornish, Thomas, Devlin, Mark J., Ho, Luis C., Kohno, Kotaro, Lagos, Claudia D. P., Mason, Brian S., Mroczkowski, Tony, Wagg, Jeff F. W., Wang, Q. Daniel, Wang, Ran, Brinch, Malte., Dannerbauer, Helmut, Jiang, Xue-Jian, Lauritsen, Lynge R. B., Vijayan, Aswin P., Vizgan, David, Wardlow, Julie L., Sarazin, Craig L., Sarmiento, Karen P., Serjeant, Stephen, Bhandarkar, Tanay A., Haridas, Saianeesh K., Moravec, Emily, Orlowski-Scherer, John, Sievers, Jonathan L. R., Tanaka, Ichi, Wang, Yu-Jan, Zeballos, Milagros, Laza-Ramos, Andres, Liu, Yuanqi, Hassan, Mohd Shaiful Rizal, Jwel, Abdul Kadir Md, Nazri, Affan Adly, Lim, Ming-Kang, Ibrahim, Ungku Ferwani Salwa Ungku
High-redshift radio(-loud) galaxies (H$z$RGs) are massive galaxies with powerful radio-loud active galactic nuclei (AGNs) and serve as beacons for protocluster identification. However, the interplay between H$z$RGs and the large-scale environment rem
Externí odkaz:
http://arxiv.org/abs/2408.02177
Autor:
Derkenne, Caro, McDermid, Richard M., D'Eugenio, Francesco, Foster, Caroline, Khalid, Aman, Harborne, Katherine E., van de Sande, Jesse, Croom, Scott M., Lagos, Claudia D. P., Bellstedt, Sabine, Mendel, J. Trevor, Mun, Marcie, Wisnioski, Emily, Bagge, Ryan S., Battisti, Andrew J., Bland-Hawthorn, Joss, Ferré-Mateu, Anna, Peng, Yingjie, Santucci, Giulia, Sweet, Sarah M., Thater, Sabine, Valenzuela, Lucas M., Ziegler, Bodo
We use the `Middle Ages Galaxy Properties with Integral field spectroscopy' (MAGPI) survey to investigate whether galaxies have evolved in the distribution of their stellar angular momentum in the past 3-4 Gyr, as probed by the observational proxy fo
Externí odkaz:
http://arxiv.org/abs/2406.02185
Autor:
Hansen, Samuel P., Lagos, Claudia D. P., Bonato, Matteo, Cook, Robin H. W., Davies, Luke J. M., Delvecchio, Ivan, Tompkins, Scott A.
We present a model of radio continuum emission associated with star formation (SF) and active galactic nuclei (AGN) implemented in the Shark semi-analytic model of galaxy formation. SF emission includes free-free and synchrotron emission, which depen
Externí odkaz:
http://arxiv.org/abs/2405.05586
Autor:
Mun, Marcie, Wisnioski, Emily, Battisti, Andrew J., Mendel, J. Trevor, Ellison, Sara L., Taylor, Edward N., Lagos, Claudia D. P., Harborne, Katherine E., Foster, Caroline, Croom, Scott M., Bellstedt, Sabine, Barsanti, Stefania, Gupta, Anshu, Valenzuela, Lucas M., Chen, Qian-Hui, Grasha, Kathryn, Mukherjee, Tamal, Park, Hye-Jin, Sharda, Piyush, Sweet, Sarah M., Remus, Rhea-Silvia, Zafar, Tayyaba
Using adaptive optics with the Multi-Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT), the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey allows us to study the spatially resolved Universe at a cruci
Externí odkaz:
http://arxiv.org/abs/2404.16319
Autor:
Chen, Qian-Hui, Grasha, Kathryn, Battisti, Andrew J., Wisnioski, Emily, Mendel, Trevor, Sharda, Piyush, Santucci, Giulia, Li, Zefeng, Foster, Caroline, Mun, Marcie, Park, Hye-Jin, Tsukui, Takafumi, Sharma, Gauri, Lagos, Claudia D. P., Barsanti, Stefania, Valenzuela, Lucas M., Gupta, Anshu, Thater, Sabine, Jin, Yifei, Kewley, Lisa
Spiral structures are important drivers of the secular evolution of disc galaxies, however, the origin of spiral arms and their effects on the development of galaxies remain mysterious. In this work, we present two three-armed spiral galaxies at z~0.
Externí odkaz:
http://arxiv.org/abs/2310.20073
Autor:
D'Silva, Jordan C. J., Driver, Simon P., Lagos, Claudia D. P., Robotham, Aaron S. G., Summers, Jake, Windhorst, Rogier A.
We consider the effect of including an active galactic nuclei (AGN) component when fitting spectral energy distributions of 109 spectroscopically confirmed $z\approx 3.5-12.5$ galaxies with JWST. Remarkably, we find that the resulting cosmic star for
Externí odkaz:
http://arxiv.org/abs/2310.03081
Autor:
Lagos, Claudia D. P., Bravo, Matias, Tobar, Rodrigo, Obreschkow, Danail, Power, Chris, Robotham, Aaron S. G., Proctor, Katy L., Hansen, Samuel, Chandro-Gomez, Angel, Carrivick, Julian
We introduce version 2.0 of the SHARK semi-analytic model of galaxy formation after many improvements to the physics included. The most significant being: (i) a model describing the exchange of angular momentum (AM) between the interstellar medium an
Externí odkaz:
http://arxiv.org/abs/2309.02310
Autor:
Brown, Toby, Roberts, Ian D., Thorp, Mallory, Ellison, Sara L., Zabel, Nikki, Wilson, Christine D., Bahé, Yannick M., Bisaria, Dhruv, Bolatto, Alberto D., Boselli, Alessandro, Chung, Aeree, Cortese, Luca, Catinella, Barbara, Davis, Timothy A., Jiménez-Donaire, María J., Lagos, Claudia D. P., Lee, Bumhyun, Parker, Laura C., Smith, Rory, Spekkens, Kristine, Stevens, Adam R. H., Villanueva, Vicente, Watts, Adam B.
We study how environment regulates the star formation cycle of 33 Virgo Cluster satellite galaxies on 720 parsec scales. We present the first resolved star-forming main sequence for cluster galaxies, dividing the sample based on their global HI prope
Externí odkaz:
http://arxiv.org/abs/2308.10943