Zobrazeno 1 - 10
of 579
pro vyhledávání: '"Deshmukh, S. P."'
Autor:
Sicardy, B., Tej, A., Gomes-Junior, A. R., Romanov, F. D., Bertrand, T., Ashok, N. M., Lellouch, E., Morgado, B. E., Assafin, M., Desmars, J., Camargo, J. I. B., Kilic, Y., Ortiz, J. L., Vieira-Martins, R., Braga-Ribas, F., Ninan, J. P., Bhatt, B. C., Kumar, S. Pramod, Swain, V., Sharma, S., Saha, A., Ojha, D. K., Pawar, G., Deshmukh, S., Deshpande, A., Ganesh, S., Jain, J. K., Mathew, S. K., Kumar, H., Bhalerao, V., Anupama, G. C., Barway, S., Brandeker, A., Floren, H. G., Olofsson, G., Bruno, G., Mao, Y. M., Ye, R. H., Zou, Q. Y., Sun, Y. K., Shen, Y. Y., Zhao, J. Y., Grishin, D. N., Romanova, L. V., Marchis, F., Fukui, K., Kukita, R., Benedetti-Rossi, G., Santos-Sanz, P., Dhyani, N., Gokhale, A., Kate, A.
Context - Around the year 2000, Triton's south pole experienced an extreme summer solstice that occurs every about 650 years, when the subsolar latitude reached about 50{\deg}. Bracketing this epoch, a few occultations probed Triton's atmosphere in 1
Externí odkaz:
http://arxiv.org/abs/2402.02476
Autor:
Deshmukh, S. A., Ludwig, H. -G.
Publikováno v:
A&A 675, A146 (2023)
Binary molecules such as CO, OH, CH, CN, and C$_2$ are often used as abundance indicators in stars. These species are usually assumed to be formed in chemical equilibrium. The time-dependent effects of hydrodynamics can affect the formation and disso
Externí odkaz:
http://arxiv.org/abs/2305.18854
Autor:
Deshmukh, S. A., Ludwig, H. -G., Kučinskas, A., Steffen, M., Barklem, P. S., Caffau, E., Dobrovolskas, V., Bonifacio, P.
Publikováno v:
A&A 668, A48 (2022)
In this work, we present a photospheric solar silicon abundance derived using CO5BOLD model atmospheres and the LINFOR3D spectral synthesis code. Previous works have differed in their choice of a spectral line sample and model atmosphere as well as t
Externí odkaz:
http://arxiv.org/abs/2212.07485
Autor:
Caputi, K. I., Caminha, G. B., Fujimoto, S., Kohno, K., Sun, F., Egami, E., Deshmukh, S., Tang, F., Ao, Y., Bradley, L., Coe, D., Espada, D., Grillo, C., Hatsukade, B., Knudsen, K. K., Lee, M. M., Magdis, G. E., Morokuma-Matsui, K., Oesch, P., Ouchi, M., Rosati, P., Umehata, H., Valentino, F., Vanzella, E., Wang, W. -H., Wu, J. F., Zitrin, A.
We report the discovery of a Multi Unit Spectroscopic Explorer (MUSE) galaxy group at z=4.32 lensed by the massive galaxy cluster ACT-CL J0102-4915 (aka El Gordo) at z=0.87, associated with a 1.2 mm source which is at a 2.07+/-0.88 kpc projected dist
Externí odkaz:
http://arxiv.org/abs/2009.04838
Akademický článek
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Publikováno v:
A&A 633, A159 (2020)
We search for bright Ly$\rm \alpha$ emitters among Spitzer SMUVS galaxies at z > 2.9 with homogeneous MUSE data. Although it only covers a small region of COSMOS, MUSE has the unique advantage of providing spectral information over the entire field,
Externí odkaz:
http://arxiv.org/abs/1910.04771
Autor:
Lee, Hao, Deshmukh, S., Wen, Jing, Costa, V. Z., Schuder, J. S., Sanchez, M., Ichimura, A. S., Pop, Eric, Wang, Bin, Newaz, A. K. M.
Publikováno v:
ACS Applied Materials and Interfaces (2019)
Transition metal dichalcogenides (TMDs) are layered semiconducting van der Waal crystals and promising materials for a wide range of electronic and optoelectronic devices. Realizing practical electrical and optoelectronic device applications requires
Externí odkaz:
http://arxiv.org/abs/1908.00609
Autor:
Yadav, Manojkumar1 manojkpyadav91@gmail.com, Deshmukh, S. P.1
Publikováno v:
Journal of Composite & Advanced Materials / Revue des Composites et des Matériaux Avancés. Feb2024, Vol. 34 Issue 1, p19-25. 7p.
Autor:
Deshmukh, S., Caputi, K. I., Ashby, M. L. N., Cowley, W. I., McCracken, H. J., Fynbo, J. P. U., Fèvre, O. Le, Milvang-Jensen, B., Ilbert, O.
The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS) has obtained the largest ultra-deep Spitzer maps to date in a single field of the sky. We considered the sample of about 66,000 SMUVS sources at $z=2-6$ to investigate the evolu
Externí odkaz:
http://arxiv.org/abs/1712.03905
Autor:
Caputi, K. I., Deshmukh, S., Ashby, M. L. N., Cowley, W. I., Bisigello, L., Fazio, G. G., Fynbo, J. P. U., Fevre, O. Le, Milvang-Jensen, B., Ilbert, O.
We study a large galaxy sample from the Spitzer Matching Survey of the UltraVISTA ultra-deep Stripes (SMUVS) to search for sources with enhanced 3.6 micron fluxes indicative of strong Halpha emission at z=3.9-4.9. We find that the percentage of "Halp
Externí odkaz:
http://arxiv.org/abs/1705.06179