Variation in the food intake of grass carp, Ctenopharyngodon idella (Val.), fed singly or in groups

Each animal may be assumed to possess a unique combination of physiological traits (Bennett, 1987). However, there is little information on thc effects of interindividual variation in fish (Cui and Liu, 1990). Individual differences in competitive ability, aggressiveness and or size can lead to the establishment of dominance hierarchies within groups of fish (Metcalfe, 1989; Metcalfe et al., 1989). The variation in growth rates in groups of fish are rclated to dominance hierarchies and preferential access to food resources by dominant individuals (Jenkins, 1969; Fausch, 1984; Koebele, 1985). Recently, radiography has been used to measure individual consumption rates for groups of salmonids and has demonstrated considerable inter-individual variation in food intake (Jobling et al., 1989; Carter et al., 1992a; McCarthy et al., 1992). Two aims of this study were to use radiography to examine the variation in the food consumption rate of grass carp, Ctenopharyngodon idellu (Val.), held together and to assess whcther variation in growth rates could bc explained by variation in consumption rates. A final aim of this study was to compare the day to day variation in consumption rates of grass carp held in a group to thosc held individually, in terms of the individual meal share, in order to examine the cffect of endogenous influences on appetite

GRB optical and IR rapid follow-up with the 2 m Liverpool Robotic Telescope

The Liverpool Telescope, owned and operated by Liverpool John Moores University and situated at Roque de los Muchachos, La Palma, is the first 2-m, fully instrumented robotic telescope. We plan to use the LT in conjunction with Gamma Ray Observatories (HETE-2, INTEGRAL, Swift) to study GRB physics. A special over-ride mode will enable observations commencing less than a minute after the GRB alert, including optical and near infrared imaging and spectroscopy. These observations, together with systematic monitoring of the burst through the afterglow, will help to unravel the nature of prompt optical flashes, short bursts, optically dark bursts, redshift distribution, GRB - supernova connection and other questions related to the GRB phenomenon. In particular, the combination of aperture, instrumentation and rapid automated response makes the Liverpool Telescope excellently suited to the investigation of optically dark bursts and currently optically unstudied short bursts