Zobrazeno 1 - 10
of 44 333
pro vyhledávání: '"Vivian P To"'
Autor:
Tan, Vivian Yun Yan, Muzzin, Adam, Sarrouh, Ghassan T. E., Antwi-Danso, Jacqueline, Sok, Visal, Jagga, Naadiyah, Abraham, Roberto, Asada, Yoshihisa, Desprez, Guillaume, Iyer, Kartheik, Martis, Nicholas S., Mérida, Rosa M., Mowla, Lamiya A., Noirot, Gaël, Omori, Kiyoaki Christopher, Sawicki, Marcin, Tripodi, Roberta, Willott, Chris J.
We present a resolved study of $>900$ progenitors of Milky Way Analogs (MWAs) at $0.3
Externí odkaz:
http://arxiv.org/abs/2412.07829
Autor:
Dage, Kristen C., Tremou, Evangelia, Otahola, Bolivia Cuevas, Koch, Eric W., Oh, Kwangmin, Plotkin, Richard M., Tang, Vivian L., Aldhalemi, Muhammad Ridha, Bustani, Zainab, Fawaz, Mariam Ismail, Harff, Hans J., Khalyleh, Amna, McBride, Timothy, Mason, Jesse, Preston, Anthony, Rinehart, Cortney, Vinson, Ethan, Anderson, Gemma, Cackett, Edward M., Fu, Shih Ching, Kamann, Sebastian, Panurach, Teresa, Pechetti, Renuka, Saikia, Payaswini, Sett, Susmita, Urquhart, Ryan, Usher, Christopher
Intermediate mass black holes (10^2 < M_BH< 10^5 Msun) are an open question in our understanding of black hole evolution and growth. They have long been linked to dense star cluster environments thanks to cluster dynamics, but there are a limited num
Externí odkaz:
http://arxiv.org/abs/2412.07284
Autor:
Saravia, Alejandro, Rodas-Quito, Eduardo, Barcos-Muñoz, Loreto, Evans, Aaron S., Kunneriath, Devaky, Privon, George, Song, Yiqing, Yoon, Ilsang, Emig, Kimberly, Sánchez-García, María, Linden, Sean, Green, Kara, Johnstone, Makoto, Nagarajan-Swenson, Jaya, Meza, Gabriela, Momjian, Emmanuel, Armus, Lee, Charmandaris, Vassilis, Diaz-Santos, Tanio, Eibensteiner, Cosima, Howell, Justin, Inami, Hanae, Kader, Justin, Ricci, Claudio, Treister, Ezequiel, U, Vivian, Bohn, Thomas, Sanders, David B.
The molecular Kennicutt-Schmidt (mK-S) Law has been key for understanding star formation (SF) in galaxies across all redshifts. However, recent sub-kpc observations of nearby galaxies reveal deviations from the nearly unity slope (N) obtained with di
Externí odkaz:
http://arxiv.org/abs/2412.07985
This manuscript signals a new era in the integration of artificial intelligence with software engineering, placing machines at the pinnacle of coding capability. We present a formalized, iterative methodology proving that AI can fully replace human p
Externí odkaz:
http://arxiv.org/abs/2412.05098
Autor:
Tang, Xianzhe TZ, Brout, Dillon, Karwal, Tanvi, Chang, Chihway, Miranda, Vivian, Vincenzi, Maria
Recent results from Type Ia Supernovae (SNe), baryon acoustic oscillations (BAO), and the cosmic microwave background (CMB) indicate 1) potentially discrepant measurements of the matter density $\Omega_m$ and Hubble constant $ H_0 $ in a $\Lambda$CDM
Externí odkaz:
http://arxiv.org/abs/2412.04430
Building on work of Doyle and Hyde on polynomial maps in one variable, we produce for each odd integer $d \geq 2$ a H\'enon map of degree $d$ defined over $\mathbb{Q}$ with at least $(d-4)^2$ integral periodic points. This provides a quadratic lower
Externí odkaz:
http://arxiv.org/abs/2412.01668
While recent advancements in machine learning, such as LLMs, are revolutionizing software development and creative industries, they have had minimal impact on engineers designing mechanical parts, which remains largely a manual process. Existing appr
Externí odkaz:
http://arxiv.org/abs/2411.15279
Autor:
Eifler, Tim, Fang, Xiao, Krause, Elisabeth, Hirata, Christopher M., Xu, Jiachuan, Benabed, Karim, Ferraro, Simone, Miranda, Vivian, S., Pranjal R., Ayçoberry, Emma, Dubois, Yohan
We explore synergies between the Nancy Grace Roman Space Telescope High Latitude Wide Area Survey (HLWAS) and CMB experiments, specifically Simons Observatory (SO) and CMB-Stage4 (S4). Our simulated analyses include weak lensing, photometric galaxy c
Externí odkaz:
http://arxiv.org/abs/2411.04088
Autor:
Winkel, Nico, Bennert, Vardha N., Remigio, Raymond P., Treu, Tommaso, Jahnke, Knud, U, Vivian, Barth, Aaron J., Malkan, Matthew, Husemann, Bernd, Ding, Xuheng, Birrer, Simon
The origin of the tight scaling relation between the mass of supermassive black holes (SMBHs; $M_{\rm BH}$) and their host-galaxy properties remains unclear. Active galactic nuclei (AGNs) probe phases of ongoing SMBH growth and offer the only opportu
Externí odkaz:
http://arxiv.org/abs/2411.02488
Early dark energy, an additional component of dark energy active in the decade of redshift before recombination, has emerged as one of the most effective models at reducing the $H_0$ tension between direct measurement of the Hubble parameter $H_0$ in
Externí odkaz:
http://arxiv.org/abs/2410.21459