Influence of timing of sea ice retreat on phytoplankton size during marginal ice zone bloom period on the Chukchi and Bering shelves

Autor: A. Fujiwara, T. Hirawake, K. Suzuki, L. Eisner, I. Imai, S. Nishino, T. Kikuchi, S.-I. Saitoh

Publikováno v: Biogeosciences, Vol 13, Iss 1, Pp 115-131 (2016)

The size structure and biomass of a phytoplankton community during the spring bloom period can affect the energy use of higher-trophic-level organisms through the predator–prey body size relationships. The timing of the sea ice retreat (TSR) also p

Externí odkaz: https://doaj.org/article/553f7d9411f04693b8eafff6000b5fdf

Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data

Autor: Sean M. O’Brien, Megan E. Schwamb, Samuel Gill, Christopher A. Watson, Matthew R. Burleigh, Alicia Kendall, Sarah L. Casewell, David R. Anderson, José I. Vines, James S. Jenkins, Douglas R. Alves, Laura Trouille, Solène Ulmer-Moll, Edward M. Bryant, Ioannis Apergis, Matthew Battley, Daniel Bayliss, Nora L. Eisner, Edward Gillen, Michael R. Goad, Maximilian N. Günther, Beth A. Henderson, Jeong-Eun Heo, David G. Jackson, Chris Lintott, James McCormac, Maximiliano Moyano, Louise D. Nielsen, Ares Osborn, Suman Saha, Ramotholo R. Sefako, Andrew W. Stephens, Rosanna H. Tilbrook, Stéphane Udry, Richard G. West, Peter J. Wheatley, Tafadzwa Zivave, See Min Lim, Arttu Sainio

Publikováno v: The Astronomical Journal, Vol 167, Iss 5, p 238 (2024)

We present the results from the first two years of the Planet Hunters Next Generation Transit Survey (NGTS) citizen science project, which searches for transiting planet candidates in data from the NGTS by enlisting the help of members of the general

Externí odkaz: https://doaj.org/article/4f569bb3bc7c49b9b2f4b7f90f82d918

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Evaluating monitoring array performance using upper limit magnitude prediction

Autor: L. Eisner, N. Cao, J. Verdon, Z. Jechumtalová, U. Bin Waheed, F. Stanek

Publikováno v: 84th EAGE Annual Conference & Exhibition.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::ca1ae63c59870b80629157cc324834f8
https://doi.org/10.3997/2214-4609.202310365

Surface Properties of Near-Sun Asteroids

Autor: Carrie E. Holt, Matthew M. Knight, Michael S. P. Kelley, Quanzhi Ye, Henry H. Hsieh, Colin Snodgrass, Alan Fitzsimmons, Derek C. Richardson, Jessica M. Sunshine, Nora L. Eisner, Annika Gustaffson

Publikováno v: Holt, C E, Knight, M M, Kelley, M S P, Ye, Q, Hsieh, H H, Snodgrass, C, Fitzsimmons, A, Richardson, D C, Sunshine, J M, Eisner, N L & Gustaffson, A 2022, ' Surface Properties of Near-Sun Asteroids ', The Planetary Science Journal, vol. 3, no. 8, 187, pp. 1-17 . https://doi.org/10.3847/PSJ/ac77f6
Holt, C E, Knight, M M, Kelley, M S P, Ye, Q, Hsieh, H H, Snodgrass, C, Fitzsimmons, A, Richardson, D C, Sunshine, J M, Eisner, N L & Gustaffson, A 2022, ' Surface properties of near-sun asteroids ', The Planetary Science Journal, vol. 3, no. 8, 187 . https://doi.org/10.3847/psj/ac77f6

Near-Earth Asteroids (NEAs) with small perihelion distances reach sub-solar temperatures of > 1000 K. They are hypothesized to undergo "super-catastrophic" disruption, potentially caused by near-Sun processes such as thermal cracking, spin-up, meteor

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1400c0de0e660398cc7b385be313a1a2
https://hdl.handle.net/20.500.11820/0e006298-9e9e-45ab-b7d1-7b54c5d1157c