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5. The Potential of Exozodiacal Disks Observations with the WFIRST Coronagraph Instrument

Author

Mennesson, B., Bailey, V., Kasdin, J., Trauger, J., Absil, O., Akeson, R., Armus, L., Baudino, J. L., Baudoz, P., Bellini, A., Bennett, D., Berriman, B., Boccaletti, A., Calchi-Novati, S., Carpenter, K., Chen, C., Danchi, W., Debes, J., Defrere, D., Ertel, S., Frerking, M., Gelino, C., Girard, J., Groff, T., Kane, S., Helou, G., Kalirai, J., Kral, Q., Krist, J., Kruk, J., Hasegawa, Y., Lagrange, A. M., Laine, S., Langlois, M., Lowrance, P., Maire, A. L., Malhotra, S., Mandell, A., Marshall, P., McElwain, M., Meshkat, T., Millan-Gabet, R., Moustakas, L., Nemati, B., Paladini, R., Postman, M., Pueyo, L., Quintana, E., Ramirez, S., Rhodes, J., Riggs, A. J. E., Rizzo, M., Rouan, D., Soummer, R., Stapelfeldt, K., Stark, C., Turnbull, M., van der Marel, R., Vigan, A., Ygouf, M., Wyatt, M., Zhao, F., and Zimmerman, N.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

The Wide Field Infrared Survey Telescope (WFIRST) Coronagraph Instrument (CGI) will be the first high-performance stellar coronagraph using active wavefront control for deep starlight suppression in space, providing unprecedented levels of contrast, spatial resolution, and sensitivity for astronomical observations in the optical. One science case enabled by the CGI will be taking images and(R~50)spectra of faint interplanetary dust structures present in the habitable zone of nearby sunlike stars (~10 pc) and within the snow-line of more distant ones(~20pc), down to dust density levels commensurate with that of the solar system zodiacal cloud. Reaching contrast levels below~10-7 for the first time, CGI will cross an important threshold in debris disks physics, accessing disks with low enough optical depths that their structure is dominated by transport phenomena than collisions. Hence, CGI results will be crucial for determining how exozodiacal dust grains are produced and transported in low-density disks around mature stars. Additionally, CGI will be able to measure the brightness level and constrain the degree of asymmetry of exozodiacal clouds around individual nearby sunlike stars in the optical, at the ~10x solar zodiacal emission level. This information will be extremely valuable for optimizing the observational strategy of possible future exo-Earth direct imaging missions, especially those planning to operate at optical wavelengths, such as Habitable Exoplanet Observatory (HabEx) and the Large Ultraviolet/Optical/Infrared Surveyor (LUVOIR)., Comment: 6 pages, 2 figures

Published
2019

6. EELS: Autonomous snake-like robot with task and motion planning capabilities for ice world exploration

Author

Vaquero, T. S., primary, Daddi, G., additional, Thakker, R., additional, Paton, M., additional, Jasour, A., additional, Strub, M. P., additional, Swan, R. M., additional, Royce, R., additional, Gildner, M., additional, Tosi, P., additional, Veismann, M., additional, Gavrilov, P., additional, Marteau, E., additional, Bowkett, J., additional, de Mola Lemus, D. Loret, additional, Nakka, Y., additional, Hockman, B., additional, Orekhov, A., additional, Hasseler, T. D., additional, Leake, C., additional, Nuernberger, B., additional, Proença, P., additional, Reid, W., additional, Talbot, W., additional, Georgiev, N., additional, Pailevanian, T., additional, Archanian, A., additional, Ambrose, E., additional, Jasper, J., additional, Etheredge, R., additional, Roman, C., additional, Levine, D., additional, Otsu, K., additional, Yearicks, S., additional, Melikyan, H., additional, Rieber, R. R., additional, Carpenter, K., additional, Nash, J., additional, Jain, A., additional, Shiraishi, L., additional, Robinson, M., additional, Travers, M., additional, Choset, H., additional, Burdick, J., additional, Gardner, A., additional, Cable, M., additional, Ingham, M., additional, and Ono, M., additional

Published
2024
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9. Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

Author

Spergel, D., Gehrels, N., Baltay, C., Bennett, D., Breckinridge, J., Donahue, M., Dressler, A., Gaudi, B. S., Greene, T., Guyon, O., Hirata, C., Kalirai, J., Kasdin, N. J., Macintosh, B., Moos, W., Perlmutter, S., Postman, M., Rauscher, B., Rhodes, J., Wang, Y., Weinberg, D., Benford, D., Hudson, M., Jeong, W. -S., Mellier, Y., Traub, W., Yamada, T., Capak, P., Colbert, J., Masters, D., Penny, M., Savransky, D., Stern, D., Zimmerman, N., Barry, R., Bartusek, L., Carpenter, K., Cheng, E., Content, D., Dekens, F., Demers, R., Grady, K., Jackson, C., Kuan, G., Kruk, J., Melton, M., Nemati, B., Parvin, B., Poberezhskiy, I., Peddie, C., Ruffa, J., Wallace, J. K., Whipple, A., Wollack, E., and Zhao, F.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

This report describes the 2014 study by the Science Definition Team (SDT) of the Wide-Field Infrared Survey Telescope (WFIRST) mission. It is a space observatory that will address the most compelling scientific problems in dark energy, exoplanets and general astrophysics using a 2.4-m telescope with a wide-field infrared instrument and an optical coronagraph. The Astro2010 Decadal Survey recommended a Wide Field Infrared Survey Telescope as its top priority for a new large space mission. As conceived by the decadal survey, WFIRST would carry out a dark energy science program, a microlensing program to determine the demographics of exoplanets, and a general observing program utilizing its ultra wide field. In October 2012, NASA chartered a Science Definition Team (SDT) to produce, in collaboration with the WFIRST Study Office at GSFC and the Program Office at JPL, a Design Reference Mission (DRM) for an implementation of WFIRST using one of the 2.4-m, Hubble-quality telescope assemblies recently made available to NASA. This DRM builds on the work of the earlier WFIRST SDT, reported by Green et al. (2012) and the previous WFIRST-2.4 DRM, reported by Spergel et. (2013). The 2.4-m primary mirror enables a mission with greater sensitivity and higher angular resolution than the 1.3-m and 1.1-m designs considered previously, increasing both the science return of the primary surveys and the capabilities of WFIRST as a Guest Observer facility. The addition of an on-axis coronagraphic instrument to the baseline design enables imaging and spectroscopic studies of planets around nearby stars., Comment: This report describes the 2014 study by the Science Definition Team of the Wide-Field Infrared Survey Telescope mission. 319 pages; corrected a misspelled name in the authors list and a typo in the abstract

Published
2015

10. Toward A Self Consistent MHD Model of Chromospheres and Winds From Late Type Evolved Stars

Author

Airapetian, V. S., Leake, J. E., and Carpenter, K. G.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present the first magnetohydrodynamic model of the stellar chromospheric heating and acceleration of the outer atmospheres of cool evolved stars, using alpha Tau as a case study. We used a 1.5D MHD code with a generalized Ohm's law that accounts for the effects of partial ionization in the stellar atmosphere to study Alfven wave dissipation and wave reflection. We have demonstrated that due to inclusion of the effects of ion-neutral collisions in magnetized weakly ionized chromospheric plasma on resistivity and the appropriate grid resolution, the numerical resistivity becomes 1-2 orders of magnitude smaller than the physical resistivity. The motions introduced by non-linear transverse Alfven waves can explain non-thermally broadened and non-Gaussian profiles of optically thin UV lines forming in the stellar chromosphere of alpha Tau and other late-type giant and supergiant stars. The calculated heating rates in the stellar chromosphere due to resistive (Joule) dissipation of electric currents, induced by upward propagating non-linear Alfven waves, are consistent with observational constraints on the net radiative losses in UV lines and the continuum from alpha Tau. At the top of the chromosphere, Alfven waves experience significant reflection, producing downward propagating transverse waves that interact with upward propagating waves and produce velocity shear in the chromosphere. Our simulations also suggest that momentum deposition by non-linear Alfven waves becomes significant in the outer chromosphere at 1 stellar radius from the photosphere. The calculated terminal velocity and the mass loss rate are consistent with the observationally derived wind properties in alpha Tau., Comment: To be appeared in 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun Proceedings of Lowell Observatory (9-13 June 2014) Edited by G. van Belle & H. Harris

Published
2014

12. Exoplanet Characterization and the Search for Life

Author

Kasting, J., Traub, W., Roberge, A., Leger, A., Schwartz, A., Wooten, A., Vosteen, A., Lo, A., Brack, A., Tanner, A., Coustenis, A., Lane, B., Oppenheimer, B., Mennesson, B., Lopez, B., Grillmair, C., Beichman, C., Cockell, C., Hanot, C., McCarthy, C., Stark, C., Marois, C., Aime, C., Angerhausen, D., Montes, D., Wilner, D., Defrere, D., Mourard, D., Lin, D., Kite, E., Chassefiere, E., Malbet, F., Tian, F., Westall, F., Illingworth, G., Vasisht, G., Serabyn, G., Marcy, G., Bryden, G., White, G., Laughlin, G., Torres, G., Hammel, H., Ferguson, H., Shibai, H., Rottgering, H., Surdej, J., Wiseman, J., Ge, J., Bally, J., Krist, J., Monnier, J., Trauger, J., Horner, J., Catanzarite, J., Harrington, J., Nishikawa, J., Stapelfeldt, K., von Braun, K., Biazzo, K., Carpenter, K., Balasubramanian, K., Kaltenegger, L., Postman, M., Spaans, M., Turnbull, M., Levine, M., Burchell, M., Ealey, M., Kuchner, M., Marley, M., Dominik, M., Mountain, M., Kenworthy, M., Muterspaugh, M., Shao, M., Zhao, M., Tamura, M., Kasdin, N., Haghighipour, N., Kiang, N., Elias, N., Woolf, N., Mason, N., Absil, O., Guyon, O., Lay, O., Borde, P., Fouque, P., Kalas, P., Lowrance, P., Plavchan, P., Hinz, P., Kervella, P., Chen, P., Akeson, R., Soummer, R., Waters, R., Barry, R., Kendrick, R., Brown, R., Vanderbei, R., Woodruff, R., Danner, R., Allen, R., Polidan, R., Seager, S., MacPhee, S., Hosseini, S., Metchev, S., Kafka, S., Ridgway, S., Rinehart, S., Unwin, S., Shaklan, S., Brummelaar, T. ten, Mazeh, T., Meadows, V., Weiss, W., Danchi, W., Ip, W., and Rabbia, Y.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmospheres and surfaces with spectroscopy. Rocky planets within their star's habitable zones have the highest priority, as these have the potential to harbor life. Our science goal is to find and characterize all nearby exoplanets; this requires that we measure the mass, orbit, and spectroscopic signature of each one at visible and infrared wavelengths. The techniques for doing this are at hand today. Within the decade we could answer long-standing questions about the evolution and nature of other planetary systems, and we could search for clues as to whether life exists elsewhere in our galactic neighborhood., Comment: 7 pages, 2 figures, submitted to Astro2010 Decadal Review

Published
2009

13. Towards a Small Prototype Planet Finding Interferometer: The next step in planet finding and characterization in the infrared

Author

Danchi, W. C., Deming, D., Carpenter, K. G., Barry, R. K., Hinz, P., Johnston, K. J., Lawson, P., Lay, O., Monnier, J. D., Richardson, L. J., Rinehart, S., and Traub, W.

Subjects
Astrophysics
Abstract

During the last few years, considerable effort has been directed towards large-scale (>> $1 Billion US) missions to detect and characterize earth-like planets around nearby stars, such as the Terrestrial Planet Finder Interferometer (TPF-I) and Darwin missions. However, technological and budgetary issues as well as shifting science priorities will likely prevent these missions from entering Phase A until the next decade. The secondary eclipse technique using the Spitzer Space Telescope has been used to directly measure the temperature and emission spectrum of extrasolar planets. However, only a small fraction of known extrasolar planets are in transiting orbits. Thus, a simplified nulling interferometer, which produces an artificial eclipse or occultation, and operates in the near- to mid-infrared (e.g. ~ 3 to 8 or 10 microns), can characterize the atmospheres of this much larger sample of the known but non-transiting exoplanets. Many other scientific problems can be addressed with a system like this, including imaging debris disks, active galactic nuclei, and low mass companions around nearby stars. We discuss the rationale for a probe-scale mission in the $600-800 Million range, which we name here as the Small Prototype Planet Finding Interferometer (SPPFI)., Comment: 8 pages, 4 figures, white paper for Exoplanet Task Force, March 2007

Published
2008

16. High Mass Triple Systems: The Classical Cepheid Y Car

Author

Evans, N. R., Carpenter, K. G., Robinson, R., Kienzle, F., and Dekas, A. E.

Subjects
Astrophysics
Abstract

We have obtained an HST STIS ultraviolet high dispersion Echelle mode spectrum the binary companion of the double mode classical Cepheid Y Car. The velocity measured for the hot companion from this spectrum is very different from reasonable predictions for binary motion, implying that the companion is itself a short period binary. The measured velocity changed by 7 km/ s during the 4 days between two segments of the observation confirming this interpretation. We summarize "binary" Cepheids which are in fact members of triple system and find at least 44% are triples. The summary of information on Cepheids with orbits makes it likely that the fraction is under-estimated., Comment: accepted by AJ

Published
2005
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20. AB Dor in '94: I. HST/GHRS Observations of the Quiescent Chromosphere of an Active Star

Author

Brandt, J. C., Heap, S. R., Walter, F. M., Beaver, E. A., Boggess, A., Carpenter, K. G., Ebbets, D. C., Hutchings, J. B., Jura, M., Leckrone, D. S., Linsky, J. L., Maran, S. P., Savage, B. D., Smith, A. M., Trafton, L. M., Weymann, R. J., Norman, D., and Redfield, S.

Subjects
Astrophysics
Abstract

We analyze HST/GHRS spectra of AB Doradus, the prototypical ultra-rapidly rotating K dwarf. We observed chromospheric (Mg II) and transition region (C II, Si IV, C IV, and N V) lines periodically throughout the stellar rotation period, and provide a low dispersion stellar atlas of 78 emission lines. The quiescent line profiles of the chromospheric and transition region lines show narrow cores superposed on very broad wings. The broad wings of the Mg II k & h lines and of the transition region lines can be explained by emission from gas co-rotating with the star and extending out to near the Keplerian co-rotation radius (2.8 stellar radii). While this is not a unique solution, it is consistent with previous studies of H-alpha emission that are naturally explained by large co-rotating prominences. We find no evidence for rotational modulation of the emission line fluxes. The density diagnostics suggest that the transition region is formed at constant pressure, with an electron density 2-3 E12 /cm^3 at a temperature of 30,000 K. The electron pressure is about 100 times larger than that for the quiet Sun. The emission measure distribution shows a minimum between log(T) = 5 and 5.5. The Mg II line exhibits three interstellar absorption components along the 15 pc line of sight. We identify the lowest velocity component with the G cloud, but the other components are not identified with any interstellar clouds previously detected from other lines of sight., Comment: to appear in The Astronomical Journal, April 2001

Published
2000

28. Specimen collection: An essential tool

Author

Rocha, L. A., Aleixo, A., Allen, G., Almeda, F., Baldwin, C. C., Barclay, M. V. L., Bates, J. M., Bauer, A. M., Benzoni, F., Berns, C. M., Berumen, M. L., Blackburn, D. C., Blum, S., Bolaños, F., Bowie, R. C. K., Britz, R., Brown, R. M., Cadena, C. D., Carpenter, K., Ceríaco, L. M., Chakrabarty, P., Chaves, G., Choat, J. H., Clements, K. D., Collette, B. B., Collins, A., Coyne, J., Cracraft, J., Daniel, T., de Carvalho, M. R., de Queiroz, K., Di Dario, F., Drewes, R., Dumbacher, J. P., Engilis, A., Erdmann, M. V., Eschmeyer, W., Feldman, C. R., Fisher, B. L., Fjeldså, J., Fritsch, P. W., Fuchs, J., Getahun, A., Gill, A., Gomon, M., Gosliner, T., Graves, G. R., Griswold, C. E., Guralnick, R., Hartel, K., Helgen, K. M., Ho, H., Iskandar, D. T., Iwamoto, T., Jaafar, Z., James, H. F., Johnson, D., Kavanaugh, D., Knowlton, N., Lacey, E., Larson, H. K., Last, P., Leis, J. M., Lessios, H., Liebherr, J., Lowman, M., Mahler, D. L., Mamonekene, V., Matsuura, K., Mayer, G. C., Mays, H., McCosker, J., McDiarmid, R. W., McGuire, J., Miller, M. J., Mooi, R., Mooi, R. D., Moritz, C., Myers, P., Nachman, M. W., Nussbaum, R. A., Foighil, D. Ó, Parenti, L. R., Parham, J. F., Paul, E., Paulay, G., Pérez-Emán, J., Pérez-Matus, A., Poe, S., Pogonoski, J., Rabosky, D. L., Randall, J. E., Reimer, J. D., Robertson, D. R., Rödel, M.-O., Rodrigues, M. T., Roopnarine, P., Rüber, L., Ryan, M. J., Sheldon, F., Shinohara, G., Short, A., Simison, W. B., Smith-Vaniz, W. F., Springer, V. G., Stiassny, M., Tello, J. G., Thompson, C. W., Trnski, T., Tucker, P., Valqui, T., Vecchione, M., Verheyen, E., Wainwright, P. C., Wheeler, T. A., White, W. T., Will, K., Williams, J. T., Williams, G., Wilson, E. O., Winker, K., Winterbottom, R., and Witt, C. C.

Published
2014

35. High Value and Long Life—Double Jeopardy for Tunas and Billfishes

Author

Collette, B. B., Carpenter, K. E., Polidoro, B. A., Juan-Jordá, M. J., Boustany, A., Die, D. J., Elfes, C., Fox, W., Graves, J., Harrison, L. R., McManus, R., Minte-Vera, C. V., Nelson, R., Restrepo, V., Schratwieser, J., Sun, C.-L., Amorim, A., Peres, M. Brick, Canales, C., Cardenas, G., Chang, S.-K., Chiang, W.-C., Leite, N. de Oliveira, Harwell, H., Lessa, R., Fredou, F. L., Oxenford, H. A., Serra, R., Shao, K.-T., Sumaila, R., Wang, S.-P., Watson, R., and Yáñez, E.

Published
2011
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40. Applicability of linear elastic fracture mechanics to compressive damage in carbon fiber reinforced epoxy matrix composites.

Author

Carpenter, K., Lei, Y., Asadi, A., Parmigiani, J., and Tabei, A.

Subjects
*LINEAR elastic fracture mechanics, *FIBROUS composites, *CARBON fibers, *COMPRESSION loads, *EPOXY resins, *FINITE element method
Abstract

The failure of carbon fiber reinforced epoxy matrix composites has been attributed to different mechanisms involving tensile, compressive and shear failure of the fibers or the matrix. This research serves to understand whether linear elastic fracture mechanics can explain the matrix behavior under compressive loading. Experiments and finite element analysis (FEA) are used to confirm that the matrix under compressive loads follows the relationships established by linear elastic fracture mechanics. The failure load is related to the corresponding notch length, and the observed relationship is compared to the relationship defined by linear elastic fracture mechanics. [ABSTRACT FROM AUTHOR]

Published
2022
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44. Correction to: Variation in neurosurgical management of traumatic brain injury: a survey in 68 centers participating in the CENTER-TBI study (Acta Neurochirurgica, (2019), 161, 3, (435-449), 10.1007/s00701-018-3761-z)

Author

van Essen T. A., van Essen, T, den Boogert, H, Cnossen, M, de Ruiter, G, Haitsma, I, Polinder, S, Steyerberg, E, Menon, D, Maas, A, Lingsma, H, Peul, W, Ackerlund, C, Adams, H, Agnoletti, V, Allanson, J, Amrein, K, Andaluz, N, Andelic, N, Andreassen, L, Antun, A, Anke, A, Antoni, A, Ardon, H, Audibert, G, Auslands, K, Azouvi, P, Azzolini, M, Baciu, C, Badenes, R, Bartels, R, Larizza, D, Barzo, P, Bauerfeind, U, Beauvais, R, Beer, R, Belda, F, Bellander, B, Belli, A, Bellier, R, Benali, H, Benard, T, Berardino, M, Beretta, L, Beynon, C, Bilotta, F, Binder, H, Biqiri, E, Blaabjerg, M, Bouzat, P, Bragge, P, Brazinova, A, Brinck, V, Brooker, J, Brorsson, C, Buki, A, Bullinger, M, Calappi, E, Calvi, M, Cameron, P, Carbayo, L, Carbonara, M, Carise, E, Carpenter, K, Castano-Leon, A, Causin, F, Chevallard, G, Chieregato, A, Citerio, G, Coburn, M, Coles, J, Coles-Kemp, L, Collett, J, Cooper, J, Correia, M, Covic, A, Curry, N, Czeiter, E, Czosnyka, M, Dahyot-Fizelier, C, Damas, F, Damas, P, Dawes, H, De Keyser, V, Della, C, Depreitere, B, Dilvesi, D, Ding, S, Dippel, D, Dixit, A, Donoghue, E, Dreier, J, Duliere, G, Eapen, G, Engemann, H, Ercole, A, Esser, P, Ezer, E, Fabricius, M, Feigin, V, Feng, J, Foks, K, Fossi, F, Francony, G, Freo, U, Frisvold, S, Furmanov, A, Gagliardo, P, Galanaud, D, Gantner, D, Gao, G, Geleijns, K, George, P, Ghuysen, A, Giga, L, Giraud, B, Glocker, B, Golubovic, J, Gomez, P, Grossi, F, Gruen, R, Gupta, D, Haagsma, J, Hartings, J, Helbok, R, Helseth, E, Hertle, D, Hoedemaekers, A, Hoefer, S, Horton, L, Huijben, J, Hutchinson, P, Haberg, A, Jacobs, B, Jankowski, S, Jarrett, M, Jelaca, B, Jiang, J, Jones, K, Kamnitsas, K, Karan, M, Katila, A, Kaukonen, M, Kerforne, T, Kivisaari, R, Kolias, A, Kolumban, B, Kompanje, E, Kolundzija, K, Kondziella, D, Koskinen, L, Kovacs, N, Lagares, A, Lanyon, L, Laureys, S, Lecky, F, Ledig, C, Lefering, R, Legrand, V, Lei, J, Levi, L, Lightfoot, R, Loeckx, D, Lozano, A, Macdonald, S, Maegele, M, Majdan, M, Major, S, Manara, A, Manley, G, Martin, D, Martin, L, Martino, C, Maruenda, A, Marechal, H, Masala, A, Mattern, J, Mcfadyen, C, Mcmahon, C, Melegh, B, Menovsky, T, Morganti-Kossmann, C, Mulazzi, D, Muraleedharan, V, Murray, L, Muhlan, H, Nair, N, Negru, A, Nelson, D, Newcombe, V, Nieboer, D, Noirhomme, Q, Nyiradi, J, Oddo, M, Oldenbeuving, A, Oresic, M, Ortolano, F, Palotie, A, Parizel, P, Patruno, A, Payen, J, Perera, N, Perlbarg, V, Persona, P, Piippo-Karjalainen, A, Pili, F, Pirinen, M, Ples, H, Poca, M, Pomposo, I, Posti, J, Puybasset, L, Radoi, A, Ragauskas, A, Raj, R, Rambadagalla, M, Real, R, Rehorcikova, V, Rhodes, J, Ripatti, S, Rocka, S, Roe, C, Roise, O, Roks, G, Rosand, J, Rosenfeld, J, Rosenlund, C, Rosenthal, G, Rossaint, R, Rossi, S, Rueckert, D, Rusnak, M, Sacchi, M, Sahakian, B, Sahuquillo, J, Sakowitz, O, Sala, F, Sanchez-Porras, R, Sandor, J, Santos, E, Sasu, L, Savo, D, Schaffer, N, Schipper, I, Schlosser, B, Schmidt, S, Schoechl, H, Schoonman, G, Schou, R, Schwendenwein, E, Scholl, M, Sir, O, Skandsen, T, Smakman, L, Smeets, D, Smielewski, P, Sorinola, A, Stamatakis, E, Stanworth, S, Steinbuchel, N, Stevanovic, A, Stevens, R, Stewart, W, Stocchetti, N, Sundstrom, N, Synnot, A, Taccone, F, Takala, R, Tamas, V, Tanskanen, P, Taylor, M, Te Ao, B, Tenovuo, O, Telgmann, R, Teodorani, G, Theadom, A, Thomas, M, Tibboel, D, Tolias, C, Tshibanda, J, Trapani, T, Tudora, C, Vajkoczy, P, Vallance, S, Valeinis, E, Van der Steen, G, van der Jagt, M, van der Naalt, J, van Dijck, J, Van Hecke, W, van Heugten, C, Van Praag, D, Vande Vyvere, T, Van Waesberghe, J, Vanhaudenhuyse, A, Vargiolu, A, Vega, E, Velt, K, Verheyden, J, Vespa, P, Vik, A, Vilcinis, R, Vizzino, G, Vleggeert-Lankamp, C, Volovici, V, Voormolen, D, Vulekovic, P, Vamos, Z, Wade, D, Wang, K, Wang, L, Wessels, L, Wildschut, E, Williams, G, Wilson, L, Winkler, M, Wolf, S, Ylen, P, Younsi, A, Zaaroor, M, Zhihui, Y, Ziverte, A, Zumbo, F, van Essen T. A., den Boogert H. F., Cnossen M. C., de Ruiter G. C. W., Haitsma I., Polinder S., Steyerberg E. W., Menon D., Maas A. I. R., Lingsma H. F., Peul W. C., Ackerlund C., Adams H., Agnoletti V., Allanson J., Amrein K., Andaluz N., Andelic N., Andreassen L., Antun A., Anke A., Antoni A., Ardon H., Audibert G., Auslands K., Azouvi P., Azzolini M. L., Baciu C., Badenes R., Bartels R., Larizza D., Barzo P., Bauerfeind U., Beauvais R., Beer R., Belda F. J., Bellander B. -M., Belli A., Bellier R., Benali H., Benard T., Berardino M., Beretta L., Beynon C., Bilotta F., Binder H., Biqiri E., Blaabjerg M., den Boogert H., Bouzat P., Bragge P., Brazinova A., Brinck V., Brooker J., Brorsson C., Buki A., Bullinger M., Calappi E., Calvi M. R., Cameron P., Carbayo L. G., Carbonara M., Carise E., Carpenter K., Castano-Leon A. M., Causin F., Chevallard G., Chieregato A., Citerio G., Cnossen M., Coburn M., Coles J., Coles-Kemp L., Collett J., Cooper J. D., Correia M., Covic A., Curry N., Czeiter E., Czosnyka M., Dahyot-Fizelier C., Damas F., Damas P., Dawes H., De Keyser V., Della C. F., Depreitere B., Dilvesi D., Ding S., Dippel D., Dixit A., Donoghue E., Dreier J., Duliere G. -L., Eapen G., Engemann H., Ercole A., Esser P., Ezer E., Fabricius M., Feigin V. L., Feng J., Foks K., Fossi F., Francony G., Freo U., Frisvold S., Furmanov A., Gagliardo P., Galanaud D., Gantner D., Gao G., Geleijns K., George P., Ghuysen A., Giga L., Giraud B., Glocker B., Golubovic J., Gomez P. A., Grossi F., Gruen R. L., Gupta D., Haagsma J. A., Hartings J. A., Helbok R., Helseth E., Hertle D., Hoedemaekers A., Hoefer S., Horton L., Huijben J., Hutchinson P. J., Haberg A. K., Jacobs B., Jankowski S., Jarrett M., Jelaca B., Jiang J. -Y., Jones K., Kamnitsas K., Karan M., Katila A., Kaukonen M., Kerforne T., Kivisaari R., Kolias A. G., Kolumban B., Kompanje E., Kolundzija K., Kondziella D., Koskinen L. -O., Kovacs N., Lagares A., Lanyon L., Laureys S., Lecky F., Ledig C., Lefering R., Legrand V., Lei J., Levi L., Lightfoot R., Lingsma H., Loeckx D., Lozano A., MacDonald S., Maegele M., Majdan M., Major S., Manara A., Manley G., Martin D., Martin L. F., Martino C., Maruenda A., Marechal H., Masala A., Mattern J., McFadyen C., McMahon C., Melegh B., Menovsky T., Morganti-Kossmann C., Mulazzi D., Muraleedharan V., Murray L., Muhlan H., Nair N., Negru A., Nelson D., Newcombe V., Nieboer D., Noirhomme Q., Nyiradi J., Oddo M., Oldenbeuving A., Oresic M., Ortolano F., Palotie A., Parizel P. M., Patruno A., Payen J. -F., Perera N., Perlbarg V., Persona P., Peul W., Piippo-Karjalainen A., Pili F. S., Pirinen M., Ples H., Poca M. A., Pomposo I., Posti J., Puybasset L., Radoi A., Ragauskas A., Raj R., Rambadagalla M., Real R., Rehorcikova V., Rhodes J., Ripatti S., Rocka S., Roe C., Roise O., Roks G., Rosand J., Rosenfeld J., Rosenlund C., Rosenthal G., Rossaint R., Rossi S., Rueckert D., Rusnak M., Sacchi M., Sahakian B., Sahuquillo J., Sakowitz O., Sala F., Sanchez-Porras R., Sandor J., Santos E., Sasu L., Savo D., Schaffer N., Schipper I., Schlosser B., Schmidt S., Schoechl H., Schoonman G., Schou R. F., Schwendenwein E., Scholl M., Sir O., Skandsen T., Smakman L., Smeets D., Smielewski P., Sorinola A., Stamatakis E., Stanworth S., Steinbuchel N., Stevanovic A., Stevens R., Stewart W., Stocchetti N., Sundstrom N., Synnot A., Taccone F. S., Takala R., Tamas V., Tanskanen P., Taylor M. S., Te Ao B., Tenovuo O., Telgmann R., Teodorani G., Theadom A., Thomas M., Tibboel D., Tolias C., Tshibanda J. -F. L., Trapani T., Tudora C. M., Vajkoczy P., Vallance S., Valeinis E., Van der Steen G., van der Jagt M., van der Naalt J., van Dijck J. T. J. M., Van Hecke W., van Heugten C., Van Praag D., Vande Vyvere T., Van Waesberghe J., Vanhaudenhuyse A., Vargiolu A., Vega E., Velt K., Verheyden J., Vespa P. M., Vik A., Vilcinis R., Vizzino G., Vleggeert-Lankamp C., Volovici V., Voormolen D., Vulekovic P., Vamos Z., Wade D., Wang K. K. W., Wang L., Wessels L., Wildschut E., Williams G., Wilson L., Winkler M. K. L., Wolf S., Ylen P., Younsi A., Zaaroor M., Zhihui Y., Ziverte A., Zumbo F., van Essen T. A., van Essen, T, den Boogert, H, Cnossen, M, de Ruiter, G, Haitsma, I, Polinder, S, Steyerberg, E, Menon, D, Maas, A, Lingsma, H, Peul, W, Ackerlund, C, Adams, H, Agnoletti, V, Allanson, J, Amrein, K, Andaluz, N, Andelic, N, Andreassen, L, Antun, A, Anke, A, Antoni, A, Ardon, H, Audibert, G, Auslands, K, Azouvi, P, Azzolini, M, Baciu, C, Badenes, R, Bartels, R, Larizza, D, Barzo, P, Bauerfeind, U, Beauvais, R, Beer, R, Belda, F, Bellander, B, Belli, A, Bellier, R, Benali, H, Benard, T, Berardino, M, Beretta, L, Beynon, C, Bilotta, F, Binder, H, Biqiri, E, Blaabjerg, M, Bouzat, P, Bragge, P, Brazinova, A, Brinck, V, Brooker, J, Brorsson, C, Buki, A, Bullinger, M, Calappi, E, Calvi, M, Cameron, P, Carbayo, L, Carbonara, M, Carise, E, Carpenter, K, Castano-Leon, A, Causin, F, Chevallard, G, Chieregato, A, Citerio, G, Coburn, M, Coles, J, Coles-Kemp, L, Collett, J, Cooper, J, Correia, M, Covic, A, Curry, N, Czeiter, E, Czosnyka, M, Dahyot-Fizelier, C, Damas, F, Damas, P, Dawes, H, De Keyser, V, Della, C, Depreitere, B, Dilvesi, D, Ding, S, Dippel, D, Dixit, A, Donoghue, E, Dreier, J, Duliere, G, Eapen, G, Engemann, H, Ercole, A, Esser, P, Ezer, E, Fabricius, M, Feigin, V, Feng, J, Foks, K, Fossi, F, Francony, G, Freo, U, Frisvold, S, Furmanov, A, Gagliardo, P, Galanaud, D, Gantner, D, Gao, G, Geleijns, K, George, P, Ghuysen, A, Giga, L, Giraud, B, Glocker, B, Golubovic, J, Gomez, P, Grossi, F, Gruen, R, Gupta, D, Haagsma, J, Hartings, J, Helbok, R, Helseth, E, Hertle, D, Hoedemaekers, A, Hoefer, S, Horton, L, Huijben, J, Hutchinson, P, Haberg, A, Jacobs, B, Jankowski, S, Jarrett, M, Jelaca, B, Jiang, J, Jones, K, Kamnitsas, K, Karan, M, Katila, A, Kaukonen, M, Kerforne, T, Kivisaari, R, Kolias, A, Kolumban, B, Kompanje, E, Kolundzija, K, Kondziella, D, Koskinen, L, Kovacs, N, Lagares, A, Lanyon, L, Laureys, S, Lecky, F, Ledig, C, Lefering, R, Legrand, V, Lei, J, Levi, L, Lightfoot, R, Loeckx, D, Lozano, A, Macdonald, S, Maegele, M, Majdan, M, Major, S, Manara, A, Manley, G, Martin, D, Martin, L, Martino, C, Maruenda, A, Marechal, H, Masala, A, Mattern, J, Mcfadyen, C, Mcmahon, C, Melegh, B, Menovsky, T, Morganti-Kossmann, C, Mulazzi, D, Muraleedharan, V, Murray, L, Muhlan, H, Nair, N, Negru, A, Nelson, D, Newcombe, V, Nieboer, D, Noirhomme, Q, Nyiradi, J, Oddo, M, Oldenbeuving, A, Oresic, M, Ortolano, F, Palotie, A, Parizel, P, Patruno, A, Payen, J, Perera, N, Perlbarg, V, Persona, P, Piippo-Karjalainen, A, Pili, F, Pirinen, M, Ples, H, Poca, M, Pomposo, I, Posti, J, Puybasset, L, Radoi, A, Ragauskas, A, Raj, R, Rambadagalla, M, Real, R, Rehorcikova, V, Rhodes, J, Ripatti, S, Rocka, S, Roe, C, Roise, O, Roks, G, Rosand, J, Rosenfeld, J, Rosenlund, C, Rosenthal, G, Rossaint, R, Rossi, S, Rueckert, D, Rusnak, M, Sacchi, M, Sahakian, B, Sahuquillo, J, Sakowitz, O, Sala, F, Sanchez-Porras, R, Sandor, J, Santos, E, Sasu, L, Savo, D, Schaffer, N, Schipper, I, Schlosser, B, Schmidt, S, Schoechl, H, Schoonman, G, Schou, R, Schwendenwein, E, Scholl, M, Sir, O, Skandsen, T, Smakman, L, Smeets, D, Smielewski, P, Sorinola, A, Stamatakis, E, Stanworth, S, Steinbuchel, N, Stevanovic, A, Stevens, R, Stewart, W, Stocchetti, N, Sundstrom, N, Synnot, A, Taccone, F, Takala, R, Tamas, V, Tanskanen, P, Taylor, M, Te Ao, B, Tenovuo, O, Telgmann, R, Teodorani, G, Theadom, A, Thomas, M, Tibboel, D, Tolias, C, Tshibanda, J, Trapani, T, Tudora, C, Vajkoczy, P, Vallance, S, Valeinis, E, Van der Steen, G, van der Jagt, M, van der Naalt, J, van Dijck, J, Van Hecke, W, van Heugten, C, Van Praag, D, Vande Vyvere, T, Van Waesberghe, J, Vanhaudenhuyse, A, Vargiolu, A, Vega, E, Velt, K, Verheyden, J, Vespa, P, Vik, A, Vilcinis, R, Vizzino, G, Vleggeert-Lankamp, C, Volovici, V, Voormolen, D, Vulekovic, P, Vamos, Z, Wade, D, Wang, K, Wang, L, Wessels, L, Wildschut, E, Williams, G, Wilson, L, Winkler, M, Wolf, S, Ylen, P, Younsi, A, Zaaroor, M, Zhihui, Y, Ziverte, A, Zumbo, F, van Essen T. A., den Boogert H. F., Cnossen M. C., de Ruiter G. C. W., Haitsma I., Polinder S., Steyerberg E. W., Menon D., Maas A. I. R., Lingsma H. F., Peul W. C., Ackerlund C., Adams H., Agnoletti V., Allanson J., Amrein K., Andaluz N., Andelic N., Andreassen L., Antun A., Anke A., Antoni A., Ardon H., Audibert G., Auslands K., Azouvi P., Azzolini M. L., Baciu C., Badenes R., Bartels R., Larizza D., Barzo P., Bauerfeind U., Beauvais R., Beer R., Belda F. J., Bellander B. -M., Belli A., Bellier R., Benali H., Benard T., Berardino M., Beretta L., Beynon C., Bilotta F., Binder H., Biqiri E., Blaabjerg M., den Boogert H., Bouzat P., Bragge P., Brazinova A., Brinck V., Brooker J., Brorsson C., Buki A., Bullinger M., Calappi E., Calvi M. R., Cameron P., Carbayo L. G., Carbonara M., Carise E., Carpenter K., Castano-Leon A. M., Causin F., Chevallard G., Chieregato A., Citerio G., Cnossen M., Coburn M., Coles J., Coles-Kemp L., Collett J., Cooper J. D., Correia M., Covic A., Curry N., Czeiter E., Czosnyka M., Dahyot-Fizelier C., Damas F., Damas P., Dawes H., De Keyser V., Della C. F., Depreitere B., Dilvesi D., Ding S., Dippel D., Dixit A., Donoghue E., Dreier J., Duliere G. -L., Eapen G., Engemann H., Ercole A., Esser P., Ezer E., Fabricius M., Feigin V. L., Feng J., Foks K., Fossi F., Francony G., Freo U., Frisvold S., Furmanov A., Gagliardo P., Galanaud D., Gantner D., Gao G., Geleijns K., George P., Ghuysen A., Giga L., Giraud B., Glocker B., Golubovic J., Gomez P. A., Grossi F., Gruen R. L., Gupta D., Haagsma J. A., Hartings J. A., Helbok R., Helseth E., Hertle D., Hoedemaekers A., Hoefer S., Horton L., Huijben J., Hutchinson P. J., Haberg A. K., Jacobs B., Jankowski S., Jarrett M., Jelaca B., Jiang J. -Y., Jones K., Kamnitsas K., Karan M., Katila A., Kaukonen M., Kerforne T., Kivisaari R., Kolias A. G., Kolumban B., Kompanje E., Kolundzija K., Kondziella D., Koskinen L. -O., Kovacs N., Lagares A., Lanyon L., Laureys S., Lecky F., Ledig C., Lefering R., Legrand V., Lei J., Levi L., Lightfoot R., Lingsma H., Loeckx D., Lozano A., MacDonald S., Maegele M., Majdan M., Major S., Manara A., Manley G., Martin D., Martin L. F., Martino C., Maruenda A., Marechal H., Masala A., Mattern J., McFadyen C., McMahon C., Melegh B., Menovsky T., Morganti-Kossmann C., Mulazzi D., Muraleedharan V., Murray L., Muhlan H., Nair N., Negru A., Nelson D., Newcombe V., Nieboer D., Noirhomme Q., Nyiradi J., Oddo M., Oldenbeuving A., Oresic M., Ortolano F., Palotie A., Parizel P. M., Patruno A., Payen J. -F., Perera N., Perlbarg V., Persona P., Peul W., Piippo-Karjalainen A., Pili F. S., Pirinen M., Ples H., Poca M. A., Pomposo I., Posti J., Puybasset L., Radoi A., Ragauskas A., Raj R., Rambadagalla M., Real R., Rehorcikova V., Rhodes J., Ripatti S., Rocka S., Roe C., Roise O., Roks G., Rosand J., Rosenfeld J., Rosenlund C., Rosenthal G., Rossaint R., Rossi S., Rueckert D., Rusnak M., Sacchi M., Sahakian B., Sahuquillo J., Sakowitz O., Sala F., Sanchez-Porras R., Sandor J., Santos E., Sasu L., Savo D., Schaffer N., Schipper I., Schlosser B., Schmidt S., Schoechl H., Schoonman G., Schou R. F., Schwendenwein E., Scholl M., Sir O., Skandsen T., Smakman L., Smeets D., Smielewski P., Sorinola A., Stamatakis E., Stanworth S., Steinbuchel N., Stevanovic A., Stevens R., Stewart W., Stocchetti N., Sundstrom N., Synnot A., Taccone F. S., Takala R., Tamas V., Tanskanen P., Taylor M. S., Te Ao B., Tenovuo O., Telgmann R., Teodorani G., Theadom A., Thomas M., Tibboel D., Tolias C., Tshibanda J. -F. L., Trapani T., Tudora C. M., Vajkoczy P., Vallance S., Valeinis E., Van der Steen G., van der Jagt M., van der Naalt J., van Dijck J. T. J. M., Van Hecke W., van Heugten C., Van Praag D., Vande Vyvere T., Van Waesberghe J., Vanhaudenhuyse A., Vargiolu A., Vega E., Velt K., Verheyden J., Vespa P. M., Vik A., Vilcinis R., Vizzino G., Vleggeert-Lankamp C., Volovici V., Voormolen D., Vulekovic P., Vamos Z., Wade D., Wang K. K. W., Wang L., Wessels L., Wildschut E., Williams G., Wilson L., Winkler M. K. L., Wolf S., Ylen P., Younsi A., Zaaroor M., Zhihui Y., Ziverte A., and Zumbo F.

Abstract

The names of themembers of the IOPSMS study Group was inverted in the original paper and is now corrected in this article.

Published
2019

45. Biomarkers for Traumatic Brain Injury: Data Standards and Statistical Considerations

Author

Huie, J. Russell, primary, Mondello, Stefania, additional, Lindsell, Christopher J., additional, Antiga, Luca, additional, Yuh, Esther L., additional, Zanier, Elisa R., additional, Masson, Serge, additional, Rosario, Bedda L., additional, Ferguson, Adam R., additional, Adeoye, Opeolu, additional, Badjatia, Neeraj, additional, Boase, Kim, additional, Bodien, Yelena, additional, Bullock, M. Ross, additional, Chesnut, Randall, additional, Corrigan, John D., additional, Crawford, Karen, additional, Diaz-Arrastia, Ramon, additional, Dikmen, Sureyya, additional, Duhaime, Ann-Christine, additional, Ellenbogen, Richard, additional, Feeser, V. Ramana, additional, Foreman, Brandon, additional, Gardner, Raquel, additional, Gaudette, Etienne, additional, Giacino, Joseph, additional, Goldman, Dana, additional, Gonzalez, Luis, additional, Gopinath, Shankar, additional, Gullapalli, Rao, additional, Hemphill, J. Claude, additional, Hotz, Gillian, additional, Jain, Sonia, additional, Korley, Frederick, additional, Kramer, Joel, additional, Kreitzer, Natalie, additional, Levin, Harvey, additional, Machamer, Joan, additional, Madden, Christopher, additional, Manley, Geoffrey T., additional, Martin, Alastair, additional, McAllister, Thomas, additional, McCrea, Michael, additional, Merchant, Randall, additional, Mukherjee, Pratik, additional, Nelson, Lindsay, additional, Ngwenya, Laura B., additional, Noel, Florence, additional, Okonkwo, David, additional, Perl, Daniel, additional, Puccio, Ava, additional, Rabinowitz, Miri, additional, Robertson, Claudia, additional, Rosand, Jonathan, additional, Sander, Angelle, additional, Schnyer, David, additional, Seabury, Seth, additional, Stein, Murray, additional, Taylor, Sabrina, additional, Temkin, Nancy, additional, Toga, Arthur, additional, Valadka, Alex, additional, Vassar, Mary, additional, Vespa, Paul, additional, Wang, Kevin, additional, Yue, John K., additional, Zafonte, Ross, additional, Ackerlund, Cecilia, additional, Adams, Hadie, additional, Agnoletti, Vanni, additional, Allanson, Judith, additional, Amrein, Krisztina, additional, Andaluz, Norberto, additional, Andelic, Nada, additional, Andreassen, Lasse, additional, Anke, Audny, additional, Antun, Azasevac, additional, Antoni, Anna, additional, Ardon, Hilko, additional, Auslands, Kaspars, additional, Azouvi, Philippe, additional, Luisa Azzolini, Maria, additional, Baciu, Camelia, additional, Badenes, Rafael, additional, Bartels, Ronald, additional, Barzó, Pál, additional, Bauerfeind, Ursula, additional, Beauvais, Romuald, additional, Beer, Ronny, additional, Belda, Francisco Javier, additional, Bellander, Bo Michael, additional, Belli, Antonio, additional, Bellier, Rémy, additional, Benali, Habib, additional, Benard, Thierry, additional, Berardino, Maurizio, additional, Beretta, Luigi, additional, Beynon, Christopher, additional, Bilotta, Federico, additional, Binder, Harald, additional, Biqiri, Erta, additional, Blaabjerg, Morten, additional, Boogert, Hugo den, additional, Bragge, Peter, additional, Brazinova, Alexandra, additional, Brinck, Vibeke, additional, Brooker, Joanne, additional, Brorsson, Camilla, additional, Buki, Andras, additional, Bullinger, Monika, additional, Cabeleira, Manuel, additional, Calappi, Emiliana, additional, Calvi, Maria Rosa, additional, Cameron, Peter, additional, Carbayo, Lozano Guillermo, additional, Carbonara, Marco, additional, Carise, Elsa, additional, Carpenter, K., additional, Castaño León, Ana M., additional, Causin, Francesco, additional, Chevallard, Giorgio, additional, Chieregato, Arturo, additional, Citerio, Giuseppe, additional, Cnossen, Maryse, additional, Coburn, Mark, additional, Coles, Jonathan, additional, Coles-Kemp, Lizzie, additional, Collett, Johnny, additional, Cooper, Jamie D., additional, Correia, Marta, additional, Covic, Amra, additional, Curry, Nicola, additional, Czeiter, Endre, additional, 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George, Pradeep, additional, Ghuysen, Alexandre, additional, Giga, Lelde, additional, Giraud, Benoit, additional, Glocker, Ben, additional, Golubovic, Jagos, additional, Gomez, Pedro A., additional, Gravesteijn, Benjamin, additional, Grossi, Francesca, additional, Gruen, Russell L., additional, Gupta, Deepak, additional, Haagsma, Juanita A., additional, Håberg, Asta Kristine, additional, Jacobs, Bram, additional, Haitsma, Iain, additional, Hartings, Jed A., additional, Helbok, Raimund, additional, Helseth, Eirik, additional, Hertle, Daniel, additional, Hoedemaekers, Astrid, additional, Hoefer, Stefan, additional, Horton, Lindsay, additional, Huijben, Jilske, additional, Hutchinson, Peter J., additional, Jankowski, Stefan, additional, Jarrett, Mike, additional, Jelaca, Bojan, additional, Jiang, Ji yao, additional, Jones, Kelly, additional, Kamnitsas, Konstantinos, additional, Karan, Mladen, additional, Katila, Ari, additional, Kaukonen, Maija, additional, Kerforne, Thomas, additional, 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Published
2021
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47. Cover profile: How comparable are microbial electrochemical systems around the globe? An electrochemical and microbiological cross‐laboratory study

Author

Santoro, C., Babanova, S., Cristiani, P., Artyushkova, K., Atanassov, P., Bergel, A., Bretschger, O., Brown, R.K., Carpenter, K., Colombo, A., Cortese, R., Erable, B., Harnisch, Falk, Kodali, M., Phadke, S., Riedl, S., Rosa, Luis Filipe Morgado, Schröder, U., Santoro, C., Babanova, S., Cristiani, P., Artyushkova, K., Atanassov, P., Bergel, A., Bretschger, O., Brown, R.K., Carpenter, K., Colombo, A., Cortese, R., Erable, B., Harnisch, Falk, Kodali, M., Phadke, S., Riedl, S., Rosa, Luis Filipe Morgado, and Schröder, U.

Abstract

no abstract

Published
2021

48. EzRAD detail protocol v1

Author

not provided Vu, Bird, C., Truong, T. O., Tran, Q.S., Tran, T. L., Biesack, E. E., Ackiss, A. S., Carpenter, K. E., and Dang, B. T.

Abstract

This protocol describes the methodologies used for DNA extraction, quantification, restriction digestion, and make libraries from non-model organisms following Toonen el al. (2013). Toonen, R. J., Puritz, J. B., Forsman, Z. H., Whitney, J. L., Fernandez-Silva, I., Andrews, K. R., et al. (2013). ezRAD: a simplified method for genomic genotyping in non-model organisms. PeerJ 1, e203. doi:10.7717/peerj.203.

Published
2021

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