TY  - JOUR
A1  - Teriaca, Luca
A1  - Andretta, Vincenzo
A1  - Auchere, Frederic
A1  - Brown, Charles M.
A1  - Buchlin, Eric
A1  - Cauzzi, Gianna
A1  - Culhane, J. Len
A1  - Curdt, Werner
A1  - Davila, Joseph M.
A1  - Del Zanna, Giulio
A1  - Doschek, George A.
A1  - Fineschi, Silvano
A1  - Fludra, Andrzej
A1  - Gallagher, Peter T.
A1  - Green, Lucie
A1  - Harra, Louise K.
A1  - Imada, Shinsuke
A1  - Innes, Davina
A1  - Kliem, Bernhard
A1  - Korendyke, Clarence
A1  - Mariska, John T.
A1  - Martinez-Pillet, Valentin
A1  - Parenti, Susanna
A1  - Patsourakos, Spiros
A1  - Peter, Hardi
A1  - Poletto, Luca
A1  - Rutten, Robert J.
A1  - Schuehle, Udo
A1  - Siemer, Martin
A1  - Shimizu, Toshifumi
A1  - Socas-Navarro, Hector
A1  - Solanki, Sami K.
A1  - Spadaro, Daniele
A1  - Trujillo-Bueno, Javier
A1  - Tsuneta, Saku
A1  - Dominguez, Santiago Vargas
A1  - Vial, Jean-Claude
A1  - Walsh, Robert
A1  - Warren, Harry P.
A1  - Wiegelmann, Thomas
A1  - Winter, Berend
A1  - Young, Peter
T1  - LEMUR large european module for solar ultraviolet research
JF  - Experimental astronomy : an international journal on astronomical instrumentation and data analysis
N2  - The solar outer atmosphere is an extremely dynamic environment characterized by the continuous interplay between the plasma and the magnetic field that generates and permeates it. Such interactions play a fundamental role in hugely diverse astrophysical systems, but occur at scales that cannot be studied outside the solar system. Understanding this complex system requires concerted, simultaneous solar observations from the visible to the vacuum ultraviolet (VUV) and soft X-rays, at high spatial resolution (between 0.1'' and 0.3''), at high temporal resolution (on the order of 10 s, i.e., the time scale of chromospheric dynamics), with a wide temperature coverage (0.01 MK to 20 MK, from the chromosphere to the flaring corona), and the capability of measuring magnetic fields through spectropolarimetry at visible and near-infrared wavelengths. Simultaneous spectroscopic measurements sampling the entire temperature range are particularly important. These requirements are fulfilled by the Japanese Solar-C mission (Plan B), composed of a spacecraft in a geosynchronous orbit with a payload providing a significant improvement of imaging and spectropolarimetric capabilities in the UV, visible, and near-infrared with respect to what is available today and foreseen in the near future. The Large European Module for solar Ultraviolet Research (LEMUR), described in this paper, is a large VUV telescope feeding a scientific payload of high-resolution imaging spectrographs and cameras. LEMUR consists of two major components: a VUV solar telescope with a 30 cm diameter mirror and a focal length of 3.6 m, and a focal-plane package composed of VUV spectrometers covering six carefully chosen wavelength ranges between 170 and 1270 . The LEMUR slit covers 280'' on the Sun with 0.14'' per pixel sampling. In addition, LEMUR is capable of measuring mass flows velocities (line shifts) down to 2 km s (-aEuro parts per thousand 1) or better. LEMUR has been proposed to ESA as the European contribution to the Solar C mission.
KW  - Sun: atmosphere
KW  - Space vehicles: instruments
KW  - Techniques: spectroscopy
KW  - ESA cosmic vision
Y1  - 2012
U6  - https://doi.org/10.1007/s10686-011-9274-x
SN  - 0922-6435
VL  - 34
IS  - 2
SP  - 273
EP  - 309
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - JOUR
A1  - Mayans, Olga
A1  - VanDerVen, Peter F. M
A1  - Wilmanns, Matthias
A1  - Mues, Alexander
A1  - Young, Paul
A1  - Fürst, Dieter Oswald
A1  - Wilmanns, Matthias
A1  - Gautel, Mathias
T1  - The structural basis of the activation of the serine kinase domain of the giant muscle protein titin during myofibrillogenesis
Y1  - 1998
ER  - 
TY  - JOUR
A1  - Mues, Alexander
A1  - VanDerVen, Peter F. M
A1  - Young, Paul
A1  - Fürst, Dieter Oswald
A1  - Gautel, Mathias
T1  - Two immunoglobulin-like domains of the Z-disk portion of titin interact in a conformation-dependent way with telethonin
Y1  - 1998
ER  - 
TY  - JOUR
A1  - Read, Betsy A.
A1  - Kegel, Jessica
A1  - Klute, Mary J.
A1  - Kuo, Alan
A1  - Lefebvre, Stephane C.
A1  - Maumus, Florian
A1  - Mayer, Christoph
A1  - Miller, John
A1  - Monier, Adam
A1  - Salamov, Asaf
A1  - Young, Jeremy
A1  - Aguilar, Maria
A1  - Claverie, Jean-Michel
A1  - Frickenhaus, Stephan
A1  - Gonzalez, Karina
A1  - Herman, Emily K.
A1  - Lin, Yao-Cheng
A1  - Napier, Johnathan
A1  - Ogata, Hiroyuki
A1  - Sarno, Analissa F.
A1  - Shmutz, Jeremy
A1  - Schroeder, Declan
A1  - de Vargas, Colomban
A1  - Verret, Frederic
A1  - von Dassow, Peter
A1  - Valentin, Klaus
A1  - Van de Peer, Yves
A1  - Wheeler, Glen
A1  - Dacks, Joel B.
A1  - Delwiche, Charles F.
A1  - Dyhrman, Sonya T.
A1  - Glöckner, Gernot
A1  - John, Uwe
A1  - Richards, Thomas
A1  - Worden, Alexandra Z.
A1  - Zhang, Xiaoyu
A1  - Grigoriev, Igor V.
A1  - Allen, Andrew E.
A1  - Bidle, Kay
A1  - Borodovsky, M.
A1  - Bowler, C.
A1  - Brownlee, Colin
A1  - Cock, J. Mark
A1  - Elias, Marek
A1  - Gladyshev, Vadim N.
A1  - Groth, Marco
A1  - Guda, Chittibabu
A1  - Hadaegh, Ahmad
A1  - Iglesias-Rodriguez, Maria Debora
A1  - Jenkins, J.
A1  - Jones, Bethan M.
A1  - Lawson, Tracy
A1  - Leese, Florian
A1  - Lindquist, Erika
A1  - Lobanov, Alexei
A1  - Lomsadze, Alexandre
A1  - Malik, Shehre-Banoo
A1  - Marsh, Mary E.
A1  - Mackinder, Luke
A1  - Mock, Thomas
A1  - Müller-Röber, Bernd
A1  - Pagarete, Antonio
A1  - Parker, Micaela
A1  - Probert, Ian
A1  - Quesneville, Hadi
A1  - Raines, Christine
A1  - Rensing, Stefan A.
A1  - Riano-Pachon, Diego Mauricio
A1  - Richier, Sophie
A1  - Rokitta, Sebastian
A1  - Shiraiwa, Yoshihiro
A1  - Soanes, Darren M.
A1  - van der Giezen, Mark
A1  - Wahlund, Thomas M.
A1  - Williams, Bryony
A1  - Wilson, Willie
A1  - Wolfe, Gordon
A1  - Wurch, Louie L.
T1  - Pan genome of the phytoplankton Emiliania underpins its global distribution
JF  - Nature : the international weekly journal of science
N2  - Coccolithophores have influenced the global climate for over 200 million years(1). These marine phytoplankton can account for 20 per cent of total carbon fixation in some systems(2). They form blooms that can occupy hundreds of thousands of square kilometres and are distinguished by their elegantly sculpted calcium carbonate exoskeletons (coccoliths), rendering them visible from space(3). Although coccolithophores export carbon in the form of organic matter and calcite to the sea floor, they also release CO2 in the calcification process. Hence, they have a complex influence on the carbon cycle, driving either CO2 production or uptake, sequestration and export to the deep ocean(4). Here we report the first haptophyte reference genome, from the coccolithophore Emiliania huxleyi strain CCMP1516, and sequences from 13 additional isolates. Our analyses reveal a pan genome (core genes plus genes distributed variably between strains) probably supported by an atypical complement of repetitive sequence in the genome. Comparisons across strains demonstrate that E. huxleyi, which has long been considered a single species, harbours extensive genome variability reflected in different metabolic repertoires. Genome variability within this species complex seems to underpin its capacity both to thrive in habitats ranging from the equator to the subarctic and to form large-scale episodic blooms under a wide variety of environmental conditions.
Y1  - 2013
U6  - https://doi.org/10.1038/nature12221
SN  - 0028-0836
SN  - 1476-4687
VL  - 499
IS  - 7457
SP  - 209
EP  - 213
PB  - Nature Publ. Group
CY  - London
ER  -