228 research outputs found
Effects of dietary cottonseed meal protein levels on growth and feed utilization of Nile tilapia, Oreochromis niloticus L
The nutritional suitability and cost effectiveness of cottonseed meal (CSM) as protein source in the diet of Nile tilapia (Oreochromis niloticus L.) with mean initial weight 4.24±0.20 g, was evaluated over a 56-day growth period. Four isonitrogenous (320 g kg-1), isolipidic (100 g kg-1) and isoenergetic (18 KJ g-1) test diets were formulated in which CSM protein replaced fish meal (FM) protein at levels of 0% (control), 25%, 50% and 75%. The control diet had FM as the sole protein source. The growth experiment was conducted in plastic tanks in a recirculation system each dietary treatment was in triplicate. After 56 days of feeding fish at 6% - 4% body weight per day, CSM protein replacements of 25% and 50% did not significantly (
Mixtures of oilseed meals as dietary protein sources in diets of juvenile Nile tilapia (Oreochromis niloticus l.)
The suitability of different mixtures of soybean meal (SBM), cottonseed meal (CSM) and groundnut cake (GNC) as ingredients to replace fish meal in the diets of Nile tilapia (Oreochromis niloticus L.), was evaluated over a 56-day growth period. Nine isonitrogenous (320g.kg-1), isolipidic (100 g.kg-1) and isoenergetic (18 KJ.g-1) test diets were formulated in which different mixture combinations of SBM, CSM and GNC proteins replaced fish meal (FM) protein at levels of 50% and 75%. The control diet had FM as the sole protein source. Fish were fed at 6 - 4% body weight per day. The growth experiment was conducted in plastic tanks in a recirculation system. Each dietary treatment was in triplicate. Growth performance and feed utilization of fish fed with the oilseed meal mixtures indicated that up to 50% replacement could be more effective than a single source for the substitution of fish meal in tilapia diets. This was particularly evident with the diet containing equal proportions of all oilseed meals (EQ50). Combination of oilseed meals in different proportions was more effective than the single individual sources. This could be due to a compensatory effect which led to some reduction of antinutritional factors coupled with improved essential amino acid profile in the diet as a result of mixing.Keywords: Oilseed meals, Nile tilapia, protein sources, mixtures, growth performanc
Observations of Intrahour Variable Quasars: Scattering in our Galactic Neighbourhood
Interstellar scintillation (ISS) has been established as the cause of the
random variations seen at centimetre wavelengths in many compact radio sources
on timescales of a day or less. Observations of ISS can be used to probe
structure both in the ionized insterstellar medium of the Galaxy, and in the
extragalactic sources themselves, down to microarcsecond scales. A few quasars
have been found to show large amplitude scintillations on unusually rapid,
intrahour timescales. This has been shown to be due to weak scattering in very
local Galactic ``screens'', within a few tens of parsec of the Sun. The short
variability timescales allow detailed study of the scintillation properties in
relatively short observing periods with compact interferometric arrays. The
three best-studied ``intrahour variable'' quasars, PKS 0405-385, J1819+3845 and
PKS 1257-326, have been instrumental in establishing ISS as the principal cause
of intraday variability at centimetre wavelengths. Here we review the relevant
results from observations of these three sources.Comment: 10 pages, 4 figures, to appear in Astronomical and Astrophysical
Transaction
Rapid interstellar scintillation of PKS B1257-326: two-station pattern time delays and constraints on scattering and microarcsecond source structure
We report measurements of time delays of up to 8 minutes in the centimeter
wavelength variability patterns of the intra-hour scintillating quasar PKS
1257-326 as observed between the VLA and the ATCA on three separate epochs.
These time delays confirm interstellar scintillation as the mechanism
responsible for the rapid variability, at the same time effectively ruling out
the coexistence of intrinsic intra-hour variability in this source. The time
delays are combined with measurements of the annual variation in variability
timescale exhibited by this source to determine the characteristic length scale
and anisotropy of the quasar's intensity scintillation pattern, as well as
attempting to fit for the bulk velocity of the scattering plasma responsible
for the scintillation. We find evidence for anisotropic scattering and highly
elongated scintillation patterns at both 4.9 and 8.5 GHz, with an axial ratio >
10:1, extended in a northwest direction on the sky. The characteristic scale of
the scintillation pattern along its minor axis is well determined, but the high
anisotropy leads to degenerate solutions for the scintillation velocity. The
decorrelation of the pattern over the baseline gives an estimate of the major
axis length scale of the scintillation pattern. We derive an upper limit on the
distance to the scattering plasma of no more than 10 pc.Comment: 27 pages, 6 figures, accepted for publication in Ap
Effects of dietary cottonseed meal protein levels on growth and feed utilization of Nile tilapia, Oreochromis niloticus L
The nutritional suitability and cost effectiveness of cottonseed meal
(CSM) as protein source in the diet of Nile tilapia ( Oreochromis
niloticus L.) with mean initial weight 4.24\ub10.20 g, was
evaluated over a 56-day growth period. Four isonitrogenous (320 g
kg-1), isolipidic (100 g kg-1) and isoenergetic (18 KJ g-1) test diets
were formulated in which CSM protein replaced fish meal (FM) protein at
levels of 0% (control), 25%, 50% and 75%. The control diet had FM as
the sole protein source. The growth experiment was conducted in plastic
tanks in a recirculation system each dietary treatment was in
triplicate. After 56 days of feeding fish at 6% - 4% body weight per
day, CSM protein replacements of 25% and 50% did not significantly
(P<0.05) affect growth (Specific Growth Rate, Weight Gain) and feed
utilization (Feed Intake, Feed Conversion Ratio, Protein Efficiency
Ratio, Apparent Net Protein Utilization and Energy Retention). However,
the highest replacement level (75%) significantly reduced these
parameters compared to the control diet and this was attributed to low
levels of lysine, methionine and threonine and also to high levels of
gossypol, trypsin inhibitors saponin and phytic acid in the diet. In
terms of cost effectiveness, all the CSM based diets were more
profitable than the control. The study indicated that CSM could replace
at least 50% of fish meal protein in the diet of O. niloticus without
adversely affecting growth and feed utilization and the most cost
effective diet was also the diet with 50% inclusion level of CSM
The IDV source J1128+5925, a new candidate for annual modulation?
Short time-scale radio variations of compact extragalactic radio sources,
known as IntraDay Variability, can be explained in at least some sources by a
source-extrinsic effect, in which the variations are interpreted as
scintillation of radio waves caused by the turbulent ISM of the Milky Way. One
of the most convincing observational arguments in favour of propagation-induced
variability is the so called annual modulation of the characteristic
variability time-scale, which is due to the orbital motion of the Earth. Data
for the recently discovered and highly variable IDV source J1128+5925 are
presented. We study the frequency and time dependence of the IDV in this
compact quasar. We measure the characteristic variability time-scale of the IDV
throughout the year, and analyze whether the observed changes in the
variability time-scale are consistent with annual modulation. We monitored the
flux density variability of J1128+5925 with dense time sampling between 2.7 and
10.45GHz with the 100m Effelsberg radio telescope of the MPIfR and with the 25m
Urumqi radio telescope. From ten observing sessions, we determine the
variability characteristics and time-scales. The observed pronounced changes of
the variability time-scale of J1128+5925 are modelled with an anisotropic
annual modulation model. The observed frequency dependence of the variation is
in good agreement with the prediction from interstellar scintillation. Adopting
a simple model for the annual modulation model and using also the frequency
dependence of the IDV, we derive a lower limit to the distance of the
scattering screen and an upper limit to the scintillating source size. The
latter is found to be consistent with the measured core size from VLBI.Comment: 15 pages, 9 figures Accepted for publication in Astronomy and
Astrophysic
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