Zobrazeno 1 - 10
of 350
pro vyhledávání: '"Schlawin, E"'
Autor:
Carter, A. L., May, E. M., Espinoza, N., Welbanks, L., Ahrer, E., Alderson, L., Brahm, R., Feinstein, A. D., Grant, D., Line, M., Morello, G., O'Steen, R., Radica, M., Rustamkulov, Z., Stevenson, K. B., Turner, J. D., Alam, M. K., Anderson, D. R., Batalha, N. M., Battley, M. P., Bayliss, D., Bean, J. L., Benneke, B., Berta-Thompson, Z. K., Brande, J., Bryant, E. M., Burleigh, M. R., Coulombe, L., Crossfield, I. J. M., Damiano, M., Désert, J. -M., Flagg, L., Gill, S., Inglis, J., Kirk, J., Knutson, H., Kreidberg, L., Morales, M. López, Mansfield, M., Moran, S. E., Murray, C. A., Nixon, M. C., de la Roche, D. J. M. Petit dit, Rackham, B. V., Schlawin, E., Sing, D. K., Wakeford, H. R., Wallack, N. L., Wheatley, P. J., Zieba, S., Aggarwal, K., Barstow, J. K., Bell, T. J., Blecic, J., Caceres, C., Crouzet, N., Cubillos, P. E., Daylan, T., de Val-Borro, M., Decin, L., Fortney, J. J., Gibson, N. P., Heng, K., Hu, R., Kempton, E M. -R., Lagage, P., Lothringer, J. D., Lustig-Yaeger, J., Mancini, L., Mayne, N. J., Mayorga, L. C., Molaverdikhani, K., Nasedkin, E., Ohno, K., Parmentier, V., Powell, D., Redfield, S., Roy, P., Taylor, J., Zhang, X.
Observing exoplanets through transmission spectroscopy supplies detailed information on their atmospheric composition, physics, and chemistry. Prior to JWST, these observations were limited to a narrow wavelength range across the near-ultraviolet to
Externí odkaz:
http://arxiv.org/abs/2407.13893
Autor:
Keles, E., Czesla, S., Poppenhaeger, K., Hauschildt, P., Carroll, T. A., Ilyin, I., Baratella, M., Steffen, M., Strassmeier, K. G., Bonomo, A. S., Gaudi, B. S., Henning, T., Johnson, M. C., Molaverdikhani, K., Nascimbeni, V., Patience, J., Reiners, A., Scandariato, G., Schlawin, E., Shkolnik, E., Sicilia, D., Sozzetti, A., Mallonn, M., Veillet, C., Wang, J., Yan, F.
Absorption lines from exoplanet atmospheres observed in transmission allow us to study atmospheric characteristics such as winds. We present a new high-resolution transit time-series of HD 189733b, acquired with the PEPSI instrument at the LBT and an
Externí odkaz:
http://arxiv.org/abs/2404.13586
Autor:
Scandariato, G., Borsa, F., Bonomo, A. S., Gaudi, B. S., Henning, Th., Ilyin, I., Johnson, M. C., Malavolta, L., Mallonn, M., Molaverdikhani, K., Nascimbeni, V., Patience, J., Pino, L., Poppenhaeger, K., Schlawin, E., Shkolnik, E. L., Sicilia, D., Sozzetti, A., Strassmeier, K. G., Veillet, C., Wang, J., Yan, F.
Publikováno v:
A&A 674, A58 (2023)
Hot giant planets like MASCARA-1 b are expected to have thermally inverted atmospheres, that makes them perfect laboratory for the atmospheric characterization through high-resolution spectroscopy. Nonetheless, previous attempts of detecting the atmo
Externí odkaz:
http://arxiv.org/abs/2304.03328
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
A challenge in absolute calibration is to relate very bright stars with physical flux measurements to faint ones within range of modern instruments, e.g. those on large groundbased telescopes or on the James Webb Space Telescope (JWST). We propose Si
Externí odkaz:
http://arxiv.org/abs/2111.10444
Autor:
Welbanks L; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. luis.welbanks@asu.edu., Bell TJ; Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA.; Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA., Beatty TG; Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA., Line MR; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA., Ohno K; Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA.; Division of Science, National Astronomical Observatory of Japan (NAOJ), Tokyo, Japan., Fortney JJ; Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA., Schlawin E; Steward Observatory, University of Arizona, Tucson, AZ, USA., Greene TP; Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA., Rauscher E; Department of Astronomy, University of Michigan, Ann Arbor, MI, USA., McGill P; Space Science Institute, Lawrence Livermore National Laboratory, Livermore, CA, USA., Murphy M; Steward Observatory, University of Arizona, Tucson, AZ, USA., Parmentier V; Laboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice, France., Tang Y; Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA., Edelman I; Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA., Mukherjee S; Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA., Wiser LS; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA., Lagage PO; Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France., Dyrek A; Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France., Arnold KE; Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA.
Publikováno v:
Nature [Nature] 2024 Jun; Vol. 630 (8018), pp. 836-840. Date of Electronic Publication: 2024 May 20.
Autor:
Fu G; Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA. guangweifu@gmail.com., Welbanks L; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA., Deming D; Department of Astronomy, University of Maryland, College Park, MD, USA., Inglis J; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA., Zhang M; Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA., Lothringer J; Department of Physics, Utah Valley University, Orem, UT, USA., Ih J; Department of Astronomy, University of Maryland, College Park, MD, USA., Moses JI; Space Science Institute, Boulder, CO, USA., Schlawin E; Steward Observatory, University of Arizona, Tucson, AZ, USA., Knutson HA; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA., Henry G; Center of Excellence in Information Systems, Tennessee State University, Nashville, TN, USA., Greene T; NASA Ames Research Center, Moffett Field, CA, USA., Sing DK; Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA., Savel AB; Department of Astronomy, University of Maryland, College Park, MD, USA., Kempton EM; Department of Astronomy, University of Maryland, College Park, MD, USA., Louie DR; NASA Goddard Space Flight Center, Greenbelt, MD, USA., Line M; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA., Nixon M; Department of Astronomy, University of Maryland, College Park, MD, USA.
Publikováno v:
Nature [Nature] 2024 Aug; Vol. 632 (8026), pp. 752-756. Date of Electronic Publication: 2024 Jul 08.
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Autor:
Santerne, A., Beaulieu, J. -P., Ayala, B. Rojas, Boisse, I., Schlawin, E., Almenara, J. -M., Batista, V., Bennett, D., Díaz, R. F., Figueira, P., James, D. J., Herter, T., Lillo-Box, J., Marquette, J. B., Ranc, C., Santos, N. C., Sousa, S. G.
Publikováno v:
A&A 595, L11 (2016)
The microlensing event OGLE-2011-BLG-0417 is an exceptionally bright lens binary that was predicted to present radial velocity variation at the level of several km/s. Pioneer radial velocity follow-up observations with the UVES spectrograph at the ES
Externí odkaz:
http://arxiv.org/abs/1610.04446
Autor:
Keles, E, Czesla, S, Poppenhaeger, K, Hauschildt, P, Carroll, T A, Ilyin, I, Baratella, M, Steffen, M, Strassmeier, K G, Bonomo, A S, Gaudi, B S, Henning, T, Johnson, M C, Molaverdikhani, K, Nascimbeni, V, Patience, J, Reiners, A, Scandariato, G, Schlawin, E, Shkolnik, E
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jun2024, Vol. 530 Issue 4, p4826-4838, 13p