2012
DOI: 10.1016/j.jnc.2012.07.004
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An assessment of the use of telemetry for primate reintroductions

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Cited by 19 publications
(14 citation statements)
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“…The images are produced with the radiative transfer code skirt [66]. This code generates images of the galaxy in the u, g, and r SDSS filters within a 30 kpc aperture of the galaxy centre; the dust distribution is inferred from the gas metal distribution in the interstellar medium [67,68]. From those images one can see that the majority of the selected objects shows clearly a disc component.…”
Section: Morphology Of Simulated Galaxies: Disc and Spheroidmentioning
confidence: 99%
See 1 more Smart Citation
“…The images are produced with the radiative transfer code skirt [66]. This code generates images of the galaxy in the u, g, and r SDSS filters within a 30 kpc aperture of the galaxy centre; the dust distribution is inferred from the gas metal distribution in the interstellar medium [67,68]. From those images one can see that the majority of the selected objects shows clearly a disc component.…”
Section: Morphology Of Simulated Galaxies: Disc and Spheroidmentioning
confidence: 99%
“…The so-called "Power radius" is R P03 = Figure 4. Pairs of mock three-colour composite grid observations for the 10 simulated galaxies in the EAGLE IR run with edge-on (left) and face-on (right) projections, within a 30 kpc aperture of the galaxy centre obtained using the skirt [66] radiative transfer code as described by [67,68] 3.6 kpc, 1.8 kpc and 1.8 kpc 4 for the EAGLE IR, EAGLE HR and APOSTLE IR runs. The very concept of convergence -that ever increasing resolution will cause the measured quantity to asymptotically tend towards some finite value -is much less clear in simulations that feature baryon physics, and so the innermost radius at which the profiles may be considered converged is ill-defined.…”
Section: The Galactic Dark Matter Density Profilementioning
confidence: 99%
“…The few primate‐focused studies in which GPS collars have been deployed thus far have largely presented various kinds of data on collar performance (e.g., Markham & Altmann, ; Pebsworth, Morgon, & Huffman, ; Sprague, Kahaya, & Hargihara, ). Although documenting GPS‐collar performance is important at this relatively early stage to test their value in primate‐typical habitats, improve the effectiveness of collars, and determine the best type of collar for a given study, we concur with many that it is also important to discuss the extent to which the process of GPS‐collar placement affects the animals themselves, with the goal of minimizing negative effects on individuals in the future (Ancrenaz, Setchell, & Curtis, ; Brett, Turner, Jolly, & Cauble, ; Honess & MacDonald ; Jolly, Phillips‐Conroy, & Müller, ; Juarez, Rotundo, Berg, & Fernández‐Duque, ; Jung & O'Donovan, ; Jung, Thompson, Hickey, & Titman, ; Trayford & Farmer, ). However, data are rarely presented on the collaring procedure itself or on the health, survival, or reproduction of collared individuals (Fehlmann et al, ; Markham & Altmann, ; Markham et al, ; Pebsworth et al, ; Pyritz, Kappeler, & Fichtel, ; Ren, Li, Long, Grüter, & Wei, ; Sprague et al, ).…”
Section: Introductionmentioning
confidence: 64%
“…Animals currently housed in rescue centres around the world, many of which are globally threatened, could, potentially, offer the last chance to save species through captive breeding and translocation (Trayford & Farmer 2012). We now discuss alternatives to the question raised earlier: What is the most viable option regarding compassionate conservation (Bekoff 2013a) for animals that cannot be released?…”
Section: Discussionmentioning
confidence: 99%