Zobrazeno 1 - 10
of 8 262
pro vyhledávání: '"Champagne P"'
Autor:
Lin, Xiaojing, Wang, Feige, Fan, Xiaohui, Cai, Zheng, Champagne, Jaclyn B., Sun, Fengwu, Volonteri, Marta, Yang, Jinyi, Hennawi, Joseph F., Bañados, Eduardo, Barth, Aaron, Eilers, Anna-Christina, Farina, Emanuele Paolo, Liu, Weizhe, Jin, Xiangyu, Jun, Hyunsung D., Lupi, Alessandro, Kakiichi, Koki, Mazzucchelli, Chiara, Onoue, Masafusa, Pan, Zhiwei, Pizzati, Elia, Rojas-Ruiz, Sofía, Schindler, Jan-Torge, Trakhtenbrot, Benny, Shen, Yue, Trebitsch, Maxime, Zhuang, Ming-Yang, Endsley, Ryan, Meyer, Romain A., Li, Zihao, Li, Mingyu, Pudoka, Maria, Tee, Wei Leong, Wu, Yunjing, Zhang, Haowen
Low-luminosity AGNs with low-mass black holes (BHs) in the early universe are fundamental to understanding the BH growth and their co-evolution with the host galaxies. Utilizing JWST NIRCam Wide Field Slitless Spectroscopy (WFSS), we perform a system
Externí odkaz:
http://arxiv.org/abs/2407.17570
Publikováno v:
Phys. Rev. E 110, 014301 (2024)
Diffusion plays an important role in a wide variety of phenomena, from bacterial quorum sensing to the dynamics of traffic flow. While it generally tends to level out gradients and inhomogeneities, diffusion has nonetheless been shown to promote patt
Externí odkaz:
http://arxiv.org/abs/2407.02385
Let $(p_n)$ denote the sequence of prime numbers, with $2=p_1 Comment: 4 pages
Externí odkaz:
http://arxiv.org/abs/2406.19491
Autor:
Akins, Hollis B., Casey, Caitlin M., Lambrides, Erini, Allen, Natalie, Andika, Irham T., Brinch, Malte, Champagne, Jaclyn B., Cooper, Olivia, Ding, Xuheng, Drakos, Nicole E., Faisst, Andreas, Finkelstein, Steven L., Franco, Maximilien, Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gozaliasl, Ghassem, Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Ilbert, Olivier, Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Long, Arianna S., McCracken, Henry Joy, McKinney, Jed, Onoue, Masafusa, Paquereau, Louise, Renzini, Alvio, Rhodes, Jason, Robertson, Brant E., Shuntov, Marko, Silverman, John D., Tanaka, Takumi S., Toft, Sune, Trakhtenbrot, Benny, Valentino, Francesco, Zavala, Jorge
JWST has revealed a population of compact and extremely red galaxies at $z>4$, which likely host active galactic nuclei (AGN). We present a sample of 434 ``little red dots'' (LRDs), selected from the 0.54 deg$^2$ COSMOS-Web survey. We fit galaxy and
Externí odkaz:
http://arxiv.org/abs/2406.10341
Autor:
Pudoka, Maria, Wang, Feige, Fan, Xiaohui, Yang, Jinyi, Champagne, Jaclyn, Jones, Victoria, Bian, Fuyan, Cai, Zheng, Jiang, Linhua, Liu, Dezi, Wu, Xue-Bing
We study the environment of the z=6.33 ultraluminous quasar SDSS J010013.02+280225.8 (J0100) to understand its association with large-scale structure. Theoretical models propose high-redshift quasars as markers of galaxy overdensities residing in the
Externí odkaz:
http://arxiv.org/abs/2405.03781
Autor:
Susobhanan, Abhimanyu, Kaplan, David, Archibald, Anne, Luo, Jing, Ray, Paul, Pennucci, Timothy, Ransom, Scott, Agazie, Gabriella, Fiore, William, Larsen, Bjorn, O'Neill, Patrick, van Haasteren, Rutger, Anumarlapudi, Akash, Bachetti, Matteo, Bhakta, Deven, Champagne, Chloe, Cromartie, H. Thankful, Demorest, Paul, Jennings, Ross, Kerr, Matthew, Levina, Sasha, McEwen, Alexander, Shapiro-Albert, Brent, Swiggum, Joseph
PINT is a pure-Python framework for high-precision pulsar timing developed on top of widely used and well-tested Python libraries, supporting both interactive and programmatic data analysis workflows. We present a new frequentist framework within PIN
Externí odkaz:
http://arxiv.org/abs/2405.01977
Autor:
Wang, Feige, Yang, Jinyi, Hennawi, Joseph F., Fan, Xiaohui, Yue, Minghao, Bañados, Eduardo, Bechtel, Shane, Bian, Fuyan, Bosman, Sarah, Champagne, Jaclyn B., Davies, Frederick B., Decarli, Roberto, Farina, Emanuele Paolo, Mazzucchelli, Chiara, Venemans, Bram, Walter, Fabian
Protoclusters, the progenitors of galaxy clusters, trace large scale structures in the early Universe and are important to our understanding of structure formation and galaxy evolution. To date, only a handful of protoclusters have been identified in
Externí odkaz:
http://arxiv.org/abs/2402.01844
Autor:
Zou, Siwei, Cai, Zheng, Wang, Feige, Fan, Xiaohui, Champagne, Jaclyn B., Hennawi, Joseph F., Schindler, Jan-Torge, Farina, Emanuele P., Yang, Jinyi, Inayoshi, Kohei, Banados, Eduardo, Bosman, Sarah E. I., Li, Zihao, Lin, Xiaojing, Wu, Yunjing, Sun, Fengwu, Guo, Zi-Yi, Kulkarni, Girish, Habouzit, Melanie, Charlot, Stephane, Chevallard, Jacopo, Connor, Thomas, Eilers, Anna-Christina, Jiang, Linhua, Jin, Xiangyu, Kakiichi, Koki, Li, Mingyu, Meyer, Romain A., Walter, Fabian, Zhang, Huanian
We characterize the multiphase circumgalactic medium and galaxy properties at z = 6.0-6.5 in four quasar fields from the James Webb Space Telescope A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE) program. We use the Very Large
Externí odkaz:
http://arxiv.org/abs/2402.00113
Autor:
Shamsesalehi, Mohammad, Attari, Mahmoud Ahmadian, Sadr, Mohammad Amin Maleki, Champagne, Benoit, Qaraqe, Marwa
This paper explores a novel Neural Network (NN) architecture suitable for Beamformed Fingerprint (BFF) localization in a millimeter-wave (mmWave) multiple-input multiple-output (MIMO) outdoor system. The mmWave frequency bands have attracted signific
Externí odkaz:
http://arxiv.org/abs/2401.13059
Publikováno v:
Adv. Mater.2024, 2313629
Two-dimensional materials (2DMs) are fundamentally electro-mechanical systems. Their environment unavoidably strains them and modifies their quantum transport properties. For instance, a simple uniaxial strain could completely turn off the conductivi
Externí odkaz:
http://arxiv.org/abs/2312.00177