Zobrazeno 1 - 10
of 18 957
pro vyhledávání: '"Charles, J P"'
Autor:
Temmink, Milou, Booth, Alice S., Leemker, Margot, van der Marel, Nienke, van Dishoeck, Ewine F., Evans, Lucy, Keyte, Luke, Law, Charles J., Notsu, Shota, Öberg, Karin, Walsh, Catherine
The ongoing physical and chemical processes in planet-forming disks set the stage for planet formation. The asymmetric disk around the young star Oph-IRS 48 has one of the most well-characterised chemical inventories, showing molecular emission from
Externí odkaz:
http://arxiv.org/abs/2411.12418
Autor:
Gal, Ciprian, Ghosh, Chandan, Park, Sanghwa, Adhikari, Devi, Armstrong, David, Beminiwattha, Rakitha, Camsonne, Alexandre, Chandrasena, Shashini, Dalton, Mark, Deshpande, Abhay, Gaskell, Dave, Higinbotham, Douglas, Horowitz, Charles J., King, Paul, Kumar, Krishna, Kutz, Tyler, Mammei, Juliette, McNulty, Dustin, Michaels, Robert, Palatchi, Caryn, Panta, Anil, Paschke, Kent, Pitt, Mark, Sen, Arindam, Simicevic, Neven, Weliyanga, Lasitha, Wells, Steven P.
We propose to measure the beam normal single spin asymmetry in elastic scattering of transversely polarized electron from target nuclei with 12 $\leq Z \leq$ 90 at Q$^2$ = 0.0092 GeV$^2$ to study its nuclear dependence. While the theoretical calculat
Externí odkaz:
http://arxiv.org/abs/2411.10267
Learning causal effects of a binary exposure on time-to-event endpoints can be challenging because survival times may be partially observed due to censoring and systematically biased due to truncation. In this work, we present debiased machine learni
Externí odkaz:
http://arxiv.org/abs/2411.09017
Autor:
Law, Charles J., Zhang, Qizhou, Frommer, Arielle C., Öberg, Karin I., Galván-Madrid, Roberto, Keto, Eric, Liu, Hauyu Baobab, Ho, Paul T. P., Izquierdo, Andrés F., Cleeves, L. Ilsedore
Massive star-forming regions exhibit a rich chemistry with complex gas distributions, especially on small scales. While surveys have yielded constraints on typical gas conditions, they often have coarse spatial resolution and limited bandwidths. Thus
Externí odkaz:
http://arxiv.org/abs/2411.00941
Autor:
Woo, Jooyun, Mori, Kaya, Hailey, Charles J., Spira-Savett, Elizabeth, Bamba, Aya, Grefenstette, Brian W., Humensky, Thomas B., Mukherjee, Reshmi, Safi-Harb, Samar, Temim, Tea, Tsuji, Naomi
Young supernova remnants (SNRs) are believed to be the origin of energetic cosmic rays (CRs) below the "knee" of their spectrum at $\sim3$ petaelectronvolt (PeV, $10^{15}$ eV). Nevertheless, the precise location, duration, and operation of CR acceler
Externí odkaz:
http://arxiv.org/abs/2410.16522
Autor:
Getman, Konstantin V., Feigelson, Eric D., Waggoner, Abygail R., Cleeves, L. Ilsedore, Forbrich, Jan, Ninan, Joe P., Kochukhov, Oleg, Airapetian, Vladimir S., Dzib, Sergio A., Law, Charles J., Rab, Christian
The most powerful stellar flares driven by magnetic energy occur during the early pre-main sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single poi
Externí odkaz:
http://arxiv.org/abs/2410.05126
The composition of a planet's atmosphere is intricately linked to the chemical makeup of the protoplanetary disk in which it formed. Determining the elemental abundances from key volatiles within disks is therefore essential for establishing connecti
Externí odkaz:
http://arxiv.org/abs/2410.01418
Intracranial aneurysms (IAs) that rupture result in significant morbidity and mortality. While traditional risk models such as the PHASES score are useful in clinical decision making, machine learning (ML) models offer the potential to provide more a
Externí odkaz:
http://arxiv.org/abs/2410.00121
Autor:
Salcedo, Ciro, Mori, Kaya, Bridges, Gabriel, Hailey, Charles J., Buckley, David A. H., de Oliveira, Raimundo Lopes, Ramsay, Gavin, van Dyk, Anke
We report on XMM-Newton, NuSTAR, and NICER X-ray observations of CTCV J2056-3014, a cataclysmic variable (CV) with one of the fastest-spinning white dwarfs (WDs) at P = 29.6 s. While previously classified as an intermediate polar (IP), CJ2056 also ex
Externí odkaz:
http://arxiv.org/abs/2409.18247
Autor:
Canossa-Gosteinski, Marco A., Chies-Santos, Ana L., Furlanetto, Cristina, Bonatto, Charles J., Flores-Freitas, Rodrigo, Schoenell, William, Beasley, Michael A., Overzier, Roderik, Santiago, Basilio X., Pieres, Adriano, Zanatta, Emílio J. B., Alamo-Martinez, Karla A., Balbinot, Eduardo, Queiroz, Anna B. A., Alves-Brito, Alan
Understanding faint dwarf galaxies is fundamental to the development of a robust theory of galaxy formation on small scales. Since the discovery of a population of ultra diffuse galaxies (UDGs) rich in globular clusters (GCs) in Coma, an increasing n
Externí odkaz:
http://arxiv.org/abs/2409.10205