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pro vyhledávání: '"Macdonald R"'
Autor:
Sarkar A, Fanous KI, Marei I, Ding H, Ladjimi M, MacDonald R, Hollenberg MD, Anderson TJ, Hill MA, Triggle CR
Publikováno v:
Vascular Health and Risk Management, Vol Volume 20, Pp 255-288 (2024)
Aparajita Sarkar,1 Kareem Imad Fanous,1 Isra Marei,2 Hong Ding,2 Moncef Ladjimi,3 Ross MacDonald,4 Morley D Hollenberg,5 Todd J Anderson,6 Michael A Hill,7 Chris R Triggle2 1Department of Medical Education, Weill Cornell Medicine-Qatar, Doha, Qatar;
Externí odkaz:
https://doaj.org/article/e52b7193180a41baa359557bb9e2701f
Autor:
Boehm, V. A., Lewis, N. K., Fairman, C. E., Moran, S. E., Gascón, C., Wakeford, H. R., Alam, M. K., Alderson, L., Barstow, J., Batalha, N. E., Grant, D., López-Morales, M., MacDonald, R. J., Marley, M. S., Ohno, K.
Ultraviolet wavelengths offer unique insights into aerosols in exoplanetary atmospheres. However, only a handful of exoplanets have been observed in the ultraviolet to date. Here, we present the ultraviolet-visible transmission spectrum of the inflat
Externí odkaz:
http://arxiv.org/abs/2410.17368
Autor:
Libralato, M., Bellini, A., van der Marel, R. P., Anderson, J., Sohn, S. T., Watkins, L. L., Alderson, L., Allen, N., Clampin, M., Glidden, A., Goyal, J., Hoch, K., Huang, J., Kammerer, J., Lewis, N. K., Lin, Z., Long, D., Louie, D., MacDonald, R. J., Mountain, M., Peña-Guerrero, M., Perrin, M. D., Pueyo, L., Rebollido, I., Rickman, E., Seager, S., Stevenson, K. B., Valenti, J. A., Valentine, D., Wakeford, H. R.
We develop and disseminate effective point-spread functions and geometric-distortion solutions for high-precision astrometry and photometry with the JWST NIRISS instrument. We correct field dependencies and detector effects, and assess the quality an
Externí odkaz:
http://arxiv.org/abs/2303.00009
Autor:
Lustig-Yaeger, J., Fu, G., May, E. M., Ceballos, K. N. Ortiz, Moran, S. E., Peacock, S., Stevenson, K. B., López-Morales, M., MacDonald, R. J., Mayorga, L. C., Sing, D. K., Sotzen, K. S., Valenti, J. A., Adams, J., Alam, M. K., Batalha, N. E., Bennett, K. A., Gonzalez-Quiles, J., Kirk, J., Kruse, E., Lothringer, J. D., Rustamkulov, Z., Wakeford, H. R.
The critical first step in the search for life on exoplanets over the next decade is to determine whether rocky planets transiting small M-dwarf stars possess atmospheres and, if so, what processes sculpt them over time. Because of its broad waveleng
Externí odkaz:
http://arxiv.org/abs/2301.04191
Autor:
Rustamkulov, Z., Sing, D. K., Mukherjee, S., May, E. M., Kirk, J., Schlawin, E., Line, M. R., Piaulet, C., Carter, A. L., Batalha, N. E., Goyal, J. M., López-Morales, M., Lothringer, J. D., MacDonald, R. J., Moran, S. E., Stevenson, K. B., Wakeford, H. R., Espinoza, N., Bean, J. L., Batalha, N. M., Benneke, B., Berta-Thompson, Z. K., Crossfield, I. J. M., Gao, P., Kreidberg, L., Powell, D. K., Cubillos, P. E., Gibson, N. P., Leconte, J., Molaverdikhani, K., Nikolov, N. K., Parmentier, V., Roy, P., Taylor, J., Turner, J. D., Wheatley, P. J., Aggarwal, K., Ahrer, E., Alam, M. K., Alderson, L., Allen, N. H., Banerjee, A., Barat, S., Barrado, D., Barstow, J. K., Bell, T. J., Blecic, J., Brande, J., Casewell, S., Changeat, Q., Chubb, K. L., Crouzet, N., Daylan, T., Decin, L., Désert, J., Mikal-Evans, T., Feinstein, A. D., Flagg, L., Fortney, J. J., Harrington, J., Heng, K., Hong, Y., Hu, R., Iro, N., Kataria, T., Kempton, E. M. -R., Krick, J., Lendl, M., Lillo-Box, J., Louca, A., Lustig-Yaeger, J., Mancini, L., Mansfield, M., Mayne, N. J., Miguel, Y., Morello, G., Ohno, K., Palle, E., de la Roche, D. J. M. Petit dit, Rackham, B. V., Radica, M., Ramos-Rosado, L., Redfield, S., Rogers, L. K., Shkolnik, E. L., Southworth, J., Teske, J., Tremblin, P., Tucker, G. S., Venot, O., Waalkes, W. C., Welbanks, L., Zhang, X., Zieba, S.
Transmission spectroscopy of exoplanets has revealed signatures of water vapor, aerosols, and alkali metals in a few dozen exoplanet atmospheres. However, these previous inferences with the Hubble and Spitzer Space Telescopes were hindered by the obs
Externí odkaz:
http://arxiv.org/abs/2211.10487
Autor:
Alderson, L., Wakeford, H. R., MacDonald, R. J., Lewis, N. K., May, E. M., Grant, D., Sing, D. K., Stevenson, K. B., Fowler, J., Goyal, J., Batalha, N. E., Kataria, T.
Due to its 1770 K equilibrium temperature, WASP-17b, a 1.99 $R_\mathrm{Jup}$, 0.486 $M_\mathrm{Jup}$ exoplanet, sits at the critical juncture between hot and ultra-hot Jupiters. We present its 0.3-5 $\mu m$ transmission spectrum, with newly obtained
Externí odkaz:
http://arxiv.org/abs/2203.02434