Zobrazeno 1 - 10
of 2 130
pro vyhledávání: '"Brickhouse"'
Autor:
Chakraborty, Priyanka, Sarkar, Arnab, Wolk, Scott, Schneider, Benjamin, Brickhouse, Nancy, Lanzetta, Kenneth, Foster, Adam, Smith, Randall
We report the detection of seven new galaxy candidates with redshift $z$ $>$ 11 within the JWST Advanced Deep Extragalactic Survey (JADES) GOODS-S and GOODS-N fields. These new candidates are detected through meticulous analysis of NIRCam photometry
Externí odkaz:
http://arxiv.org/abs/2406.05306
Autor:
Brickhouse, Anna
Publikováno v:
Earthquake and the Invention of America: The Making of Elsewhere Catastrophe.
Externí odkaz:
https://doi.org/10.1093/9780198914174.003.0012
Autor:
Brickhouse, Anna
Publikováno v:
Earthquake and the Invention of America: The Making of Elsewhere Catastrophe.
Externí odkaz:
https://doi.org/10.1093/9780198914174.003.0010
Autor:
Brickhouse, Anna
Publikováno v:
Earthquake and the Invention of America: The Making of Elsewhere Catastrophe.
Externí odkaz:
https://doi.org/10.1093/9780198914174.003.0005
The detailed design and operation of the Smithsonian Astrophysical Observatory's EBIT are described for the first time, including recent design upgrades that have led to improved system stability and greater user control, increasing the scope of poss
Externí odkaz:
http://arxiv.org/abs/2401.13088
Autor:
Chakraborty, Priyanka, Hemmer, Rachel, Foster, Adam R., Raymond, John, Sarkar, Arnab, Smith, Randall, Brickhouse, Nancy
Accurate atomic data and plasma models are essential for interpreting the upcoming high-quality spectra from missions like XRISM and Athena. Estimating physical quantities, like temperature, abundance, turbulence, and resonance scattering factor, is
Externí odkaz:
http://arxiv.org/abs/2312.12712
In this paper, we present a simple, one-step, self-consistent, and fast resonance scattering model rsapec based on the AtomDB database. This model can be used as an alternative to the commonly used APEC model for fitting such X-ray spectra with optic
Externí odkaz:
http://arxiv.org/abs/2310.03892
Autor:
Herczeg, Gregory J., Chen, Yuguang, Donati, Jean-Francois, Dupree, Andrea K., Walter, Frederick M., Hillenbrand, Lynne A., Johns-Krull, Christopher M., Manara, Carlo F., Guenther, Hans Moritz, Fang, Min, Schneider, P. Christian, Valenti, Jeff A., Alencar, Silvia H. P., Venuti, Laura, Alcala, Juan Manuel, Frasca, Antonio, Arulanantham, Nicole, Linsky, Jeffrey L., Bouvier, Jerome, Brickhouse, Nancy S., Calvet, Nuria, Espaillat, Catherine C., Campbell-White, Justyn, Carpenter, John M., Chang, Seok-Jun, Cruz, Kelle L., Dahm, S. E., Eisloeffel, Jochen, Edwards, Suzan, Fischer, William J., Guo, Zhen, Henning, Thomas, Ji, Tao, Jose, Jesse, Kastner, Joel H., Launhardt, Ralf, Principe, David A., Robinson, Conner E., Serna, Javier, Siwak, Michal, Sterzik, Michael F., Takasao, Shinsuke
Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time of the mass accretion rate onto TW Hya, the nearest accreting solar-m
Externí odkaz:
http://arxiv.org/abs/2308.14590