@article{HofmanHaywardHeimetal.2019,
  author    = {Hofman, Maarten P. G. and Hayward, M. W. and Heim, M. and Marchand, P. and Rolandsen, C. M. and Mattisson, Jenny and Urbano, F. and Heurich, M. and Mysterud, A. and Melzheimer, J. and Morellet, N. and Voigt, Ulrich and Allen, B. L. and Gehr, Benedikt and Rouco Zufiaurre, Carlos and Ullmann, Wiebke and Holand, O. and Jorgensen, n H. and Steinheim, G. and Cagnacci, F. and Kroeschel, M. and Kaczensky, P. and Buuveibaatar, B. and Payne, J. C. and Palmegiani, I and Jerina, K. and Kjellander, P. and Johansson, O. and LaPoint, S. and Bayrakcismith, R. and Linnell, J. D. C. and Zaccaroni, M. and Jorge, M. L. S. and Oshima, J. E. F. and Songhurst, A. and Fischer, C. and Mc Bride, R. T. and Thompson, J. J. and Streif, S. and Sandfort, R. and Bonenfant, Christophe and Drouilly, M. and Klapproth, M. and Zinner, Dietmar and Yarnell, Richard and Stronza, A. and Wilmott, L. and Meisingset, E. and Thaker, Maria and Vanak, A. T. and Nicoloso, S. and Graeber, R. and Said, S. and Boudreau, M. R. and Devlin, A. and Hoogesteijn, R. and May-Junior, J. A. and Nifong, J. C. and Odden, J. and Quigley, H. B. and Tortato, F. and Parker, D. M. and Caso, A. and Perrine, J. and Tellaeche, C. and Zieba, F. and Zwijacz-Kozica, T. and Appel, C. L. and Axsom, I and Bean, W. T. and Cristescu, B. and Periquet, S. and Teichman, K. J. and Karpanty, S. and Licoppe, A. and Menges, V and Black, K. and Scheppers, Thomas L. and Schai-Braun, S. C. and Azevedo, F. C. and Lemos, F. G. and Payne, A. and Swanepoel, L. H. and Weckworth, B. and Berger, A. and Bertassoni, Alessandra and McCulloch, G. and Sustr, P. and Athreya, V and Bockmuhl, D. and Casaer, J. and Ekori, A. and Melovski, D. and Richard-Hansen, C. and van de Vyver, D. and Reyna-Hurtado, R. and Robardet, E. and Selva, N. and Sergiel, A. and Farhadinia, M. S. and Sunde, P. and Portas, R. and Ambarli, H{\"u}seyin and Berzins, R. and Kappeler, P. M. and Mann, G. K. and Pyritz, L. and Bissett, C. and Grant, T. and Steinmetz, R. and Swedell, Larissa and Welch, R. J. and Armenteras, D. and Bidder, O. R. and Gonzalez, T. M. and Rosenblatt, A. and Kachel, S. and Balkenhol, N.},
  title     = {Right on track?},
  series = {PLoS one},
  volume    = {14},
  journal   = {PLoS one},
  number    = {5},
  publisher = {PLoS},
  address   = {San Fransisco},
  issn      = {1932-6203},
  doi       = {10.1371/journal.pone.0216223},
  pages     = {26},
  year      = {2019},
  abstract  = {Satellite telemetry is an increasingly utilized technology in wildlife research, and current devices can track individual animal movements at unprecedented spatial and temporal resolutions. However, as we enter the golden age of satellite telemetry, we need an in-depth understanding of the main technological, species-specific and environmental factors that determine the success and failure of satellite tracking devices across species and habitats. Here, we assess the relative influence of such factors on the ability of satellite telemetry units to provide the expected amount and quality of data by analyzing data from over 3,000 devices deployed on 62 terrestrial species in 167 projects worldwide. We evaluate the success rate in obtaining GPS fixes as well as in transferring these fixes to the user and we evaluate failure rates. Average fix success and data transfer rates were high and were generally better predicted by species and unit characteristics, while environmental characteristics influenced the variability of performance. However, 48\% of the unit deployments ended prematurely, half of them due to technical failure. Nonetheless, this study shows that the performance of satellite telemetry applications has shown improvements over time, and based on our findings, we provide further recommendations for both users and manufacturers.},
  language  = {en}
}
@article{SramaKempfMoragasKlostermeyeretal.2006,
  author    = {Srama, Ralf and Kempf, S. and Moragas-Klostermeyer, Georg and Helfert, S. and Ahrens, T. J. and Altobelli, N. and Auer, S. and Beckmann, U. and Bradley, J. G. and Burton, M. and Dikarev, V. V. and Economou, T. and Fechtig, H. and Green, S. F. and Grande, M. and Havnes, O. and Hillierf, J.K. and Horanyii, M. and Igenbergsj, E. and Jessberger, E. K. and Johnson, T. V. and Kr{\"u}ger, H. and Matt, G. and McBride, N. and Mocker, A. and Lamy, P. and Linkert, D. and Linkert, G. and Lura, F. and McDonnell, J.A.M. and M{\"o}hlmann, D. and Morfill, G. E. and Postberg, F. and Roy, M. and Schwehm, G.H. and Spahn, Frank and Svestka, J. and Tschernjawski, V. and Tuzzolino, A. J. and W{\"a}sch, R. and Gr{\"u}n, E.},
  title     = {In situ dust measurements in the inner Saturnian system},
  series = {Planetary and space science},
  volume    = {54},
  journal   = {Planetary and space science},
  number    = {9-10},
  publisher = {Elsevier},
  address   = {Oxford},
  issn      = {0032-0633},
  doi       = {10.1016/j.pss.2006.05.021},
  pages     = {967 -- 987},
  year      = {2006},
  abstract  = {In July 2004 the Cassini-Huygens mission reached the Saturnian system and started its orbital tour. A total of 75 orbits will be carried out during the primary mission until August 2008. In these four years Cassini crosses the ring plane 150 times and spends approx. 400 h within Titan's orbit. The Cosmic Dust Analyser (CDA) onboard Cassini characterises the dust environment with its extended E ring and embedded moons. Here, we focus on the CDA results of the first year and we present the Dust Analyser (DA) data within Titan's orbit. This paper does investigate High Rate Detector data and dust composition measurements. The authors focus on the analysis of impact rates, which were strongly variable primarily due to changes of the spacecraft pointing. An overview is given about the ring plane crossings and the DA counter measurements. The DA dust impact rates are compared with the DA boresight configuration around all ring plane crossings between June 2004 and July 2005. Dust impacts were registered at altitudes as high as 100 000 km above the ring plane at distances from Saturn between 4 and 10 Saturn radii. In those regions the dust density of particles bigger than 0.5 can reach values of 0.001m-3.},
  language  = {en}
}