Zobrazeno 1 - 10
of 387 150
pro vyhledávání: '"SMC"'
Autor:
Keita, Kaba Saran1 (AUTHOR) kabassan85@gmail.com, Camara, Bienvenu Salim2 (AUTHOR), Camara, Sadan1 (AUTHOR), Barry, Fanta1 (AUTHOR), Sidibe, Tiany1 (AUTHOR), Kourouma, Karifa2,3 (AUTHOR), Diallo, Ramata1 (AUTHOR), Toure, Madeleine1 (AUTHOR), Camara, Alioune4 (AUTHOR), Balde, Mamadou Dioulde1 (AUTHOR)
Publikováno v:
Malaria Journal. 8/8/2024, Vol. 23 Issue 1, p1-8. 8p.
Autor:
Ibinaiye, Taiwo1 (AUTHOR), Balogun, Ayodeji1 (AUTHOR), Salifu, Emmanuel1 (AUTHOR), Amao, Benjamin1 (AUTHOR), Musa, Emmanuel1 (AUTHOR), Emeto, Daniel1 (AUTHOR), Ayoola, Samuel1 (AUTHOR), Hussaini, Usman1 (AUTHOR), Oguoma, Chibuzo1 (AUTHOR), Abdulrazak, Abdullahi1 (AUTHOR), Maleeks, Zechariah1 (AUTHOR), Ogunmola, Olabisi1 (AUTHOR), Oresanya, Olusola1 (AUTHOR), Rotimi, Kunle1 (AUTHOR) rotimiolukunle@gmail.com
Publikováno v:
Malaria Journal. 10/7/2024, Vol. 23 Issue 1, p1-8. 8p.
Publikováno v:
Scientific Reports. 10/25/2024, Vol. 14 Issue 1, p1-27. 27p.
Autor:
Lindberg, Christina W., Murray, Claire E., Merica-Jones, Petia Yanchulova, Bot, Caroline, Burhenne, Clare, Choi, Yumi, Clark, Christopher J. R., Cohen, Roger E., Gilbert, Karoline M., Goldman, Steven R., Gordon, Karl D., Hirschauer, Alec S., McQuinn, Kristen B. W., Roman-Duval, Julia C., Sandstrom, Karin M., Tarantino, Elizabeth, Williams, Benjamin F.
By analyzing the spectral energy distributions (SEDs) of resolved stars in nearby galaxies, we can constrain their stellar properties and line-of-sight dust extinction. From the Scylla survey, we obtain ultraviolet to near-infrared photometry from Wi
Externí odkaz:
http://arxiv.org/abs/2410.19910
Autor:
Karam, Rawan, Dage, Kristen C., Tetarenko, Bailey E., Brumback, McKinley C., Haggard, Daryl, Bahramian, Arash, Hu, Chin-Ping, Neilsen, Joey, Altamirano, Diego, Athukoralalage, Wasundara, Charles, Philip A., Clarkson, William I., Hickox, Ryan C., Kennea, Jamie
The MOOSE (Monitoring Observations of SMC X-1 Excursions) program uses the Neutron Star Interior Composition Explorer Mission (NICER) to monitor the high mass X-ray binary SMC X-1 during its superorbital period excursions. Here we perform X-ray spect
Externí odkaz:
http://arxiv.org/abs/2410.17307
Massive main-sequence stars have convective cores and radiative envelopes, and sub-surface convection zones. However, their properties strongly depend on a star's opacity and metallicity. Non-rotating 1D evolution models of main-sequence stars betwee
Externí odkaz:
http://arxiv.org/abs/2410.12726
Autor:
Murray, Claire E., Lindberg, Christina W., Merica-Jones, Petia Yanchulova, Williams, Benjamin F., Cohen, Roger E., Gordon, Karl D., McQuinn, Kristen B. W., Choi, Yumi, Burhenne, Clare, Sandstrom, Karin M., Bot, Caroline, Johnson, L. Clifton, Goldman, Steven R., Clark, Christopher J. R., Roman-Duval, Julia C., Gilbert, Karoline M., Peek, J. E. G., Hirschauer, Alec S., Boyer, Martha L., Dolphin, Andrew E.
Scylla is a deep Hubble Space Telescope survey of the stellar populations, interstellar medium and star formation in the LMC and SMC. As a pure-parallel complement to the Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES) surv
Externí odkaz:
http://arxiv.org/abs/2410.11695
Autor:
Moon, Kyoung-Wook1 (AUTHOR), Kim, Do-Gyun1 (AUTHOR), Ryu, Je-Kyung1,2,3,4,5 (AUTHOR) prof.love@snu.ac.kr
Publikováno v:
Communications Biology. 7/19/2024, Vol. 7 Issue 1, p1-7. 7p.
Autor:
Hobbs, Jordan, Gibb, Calum J., Pociecha, Damian, Szydłowska, Jadwiga, Górecka, Ewa, Mandle, Richard. J.
The discovery of fluid states of matter with spontaneous bulk polar order is appreciated as a major discovery in the fields of soft matter and liquid crystals. Typically, this manifests as polar order superimposed atop conventional phase structures a
Externí odkaz:
http://arxiv.org/abs/2408.15859
Sequential Monte Carlo Squared (SMC$^2$) is a Bayesian method which can infer the states and parameters of non-linear, non-Gaussian state-space models. The standard random-walk proposal in SMC$^2$ faces challenges, particularly with high-dimensional
Externí odkaz:
http://arxiv.org/abs/2407.17296