1,210 research outputs found
Predicting Customer Lifetime Value in Multi-Service Industries
Customer lifetime value (CLV) is a key-metric within CRM. Although, a large number of marketing scientists and practitioners argue in favor of this metric, there are only a few studies that consider the predictive modeling of CLV. In this study we focus on the prediction of CLV in multi-service industries. In these industries customer behavior is rather complex, because customers can purchase more than one service, and these purchases are often not independent from each other. We compare the predictive performance of different models, which vary in complexity and realism. Our results show that for our application simple models assuming constant profits over time have the best predictive performance at the individual customer level. At the customer base level more complicated models have the best performance. At the aggregate level, forecasting errors are rather small, which emphasizes the usability of CLV predictions for customer base valuation purposes. This might especially be interesting for accountants and financial analysts.forecasting;value;customer relationship management;customer lifetime value;customer segmentation;database marketing;interactive marketing
Evaluatie in de keel-, neus- en oorheelkunde
Rede uitgesproken bij de aanvaarding van het ambt van gewoon lector in de Keel-, Neus- en Oorheelkunde aan de Erasmus Universiteit te Rotterdam op woensdag 8 mei 197
Naamlijst van houtige gewassen = List of names of woody plants = Namenliste Gehoelze = Liste de noms des plantes ligneuses
A comparison of faecal analysis with backtracking to determine the diet composition and species preference of the black rhinoceros (Diceros bicornis minor)
The diet of black rhinoceros (Diceros bicornis minor) was studied using backtracking and faecal analysis in South Africa. Both methods yielded different results, with a large bias for dominant species. Results of backtracking showed that the rhinos browsed on 80 plant species. Grasses comprised 4.5% of the diet in the faecal analysis, but were not recorded during the backtracking. The backtracking method, along with a measure of forage availability, was used to identify two groups of plant species, those species taken in a higher proportion than available in the field and those taken in a lower proportion. Chemical analyses showed that these two species groups were similar in in vitro digestibility, macro-elements and fibre constituents. Mean bite size and species contribution to the diet were not correlated with any of the forage quality parameters, indicating that rhinos were not maximising nutrient intake or minimising fibre intake of these consumed plant species
Predicting Customer Lifetime Value in Multi-Service Industries
Customer lifetime value (CLV) is a key-metric within CRM. Although, a large number of marketing scientists and practitioners argue in favor of this metric, there are only a few studies that consider the predictive modeling of CLV. In this study we focus on the prediction of CLV in multi-service industries. In these industries customer behavior is rather complex, because customers can purchase more than one service, and these purchases are often not independent from each other. We compare the predictive performance of different models, which vary in complexity and realism. Our results show that for our application simple models assuming constant profits over time have the best predictive performance at the individual customer level. At the customer base level more c
Structure, mass and stability of galactic disks
In this review I concentrate on three areas related to structure of disks in
spiral galaxies. First I will review the work on structure, kinematics and
dynamics of stellar disks. Next I will review the progress in the area of
flaring of HI layers. These subjects are relevant for the presence of dark
matter and lead to the conclusion that disk are in general not `maximal', have
lower M/L ratios than previously suspected and are locally stable w.r.t.
Toomre's Q criterion for local stability. I will end with a few words on
`truncations' in stellar disks.Comment: Invited review at "Galaxies and their Masks" for Ken Freeman's 70-th
birthday, Sossusvlei, Namibia, April 2010. A version with high-res. figures
is available at
http://www.astro.rug.nl/~vdkruit/jea3/homepage/Namibiachapter.pd
Flowering and sex expression in Acer L. : a biosystematic study
A review and an analysis is given of flowering and sex expression in Acer. The process of sex differentiation was studied in physiological experiments and could be influenced by accelerated flowering and by removal of female.gif flower buds just after bud break. The paper further includes notes on the morphology, mainly of the reproductive organs, and a study of floral morphogenesis. A taxonomic study led to the division of Acer into 15 sections, partly subdivided into 2-3 series. Of these series, two, Ukurunduensia and Wardiana, are described for the first time. A key to the sections and series is added. The evolution of Acer, especially of its flowering and sex expression, and of its morphological characters, is discussed. Notes on sex expression in related genera are included
De chirurgische behandeling van het larynxcarcinoom in Nederland : resultaten bij 708 geopereerde patiënten, gevolgd door een kritische beschouwing over de klinische indeling van het larynxcarcinoom
In dit proefschrift worden de resultaten beschreven van een retrospectief onderzoek, verricht bij 708 patiënten, die een larynxexstirpatie ondergingen wegens een plaveiselcelcarcinoom. Het bestaat uit twee delen. Het eerste deel bevat, naast een aantal inleidende hoofdstukken, een drietal hoofdstukken, waarin klinische probleemstellingen behandeld worden. Het tweede deel bestaat uit
twee hoofdstukken met een meer theoretisch karakter, waarin de classificatie van het larynxcarcinoom besproken wordt
van der Kruit to Spitzer: A New Look at the FIR-Radio Correlation
We present an initial look at the far infrared-radio correlation within the
star-forming disks of four nearby, nearly face-on galaxies (NGC~2403, NGC~3031,
NGC~5194, and NGC~6946). Using {\it Spitzer} MIPS imaging and WSRT radio
continuum data, we are able to probe variations in the logarithmic
70~m/22~cm () flux density ratios across each disk at sub-kpc
scales. We find general trends of decreasing with declining surface
brightness and with increasing radius. We also find that the dispersion in
within galaxies is comparable to what is measured {\it globally} among
galaxies at around 0.2 dex. We have also performed preliminary phenomenological
modeling of cosmic ray electron (CR) diffusion using an image-smearing
technique, and find that smoothing the infrared maps improves their correlation
with the radio maps. The best fit smoothing kernels for the two less active
star-forming galaxies (NGC~2403 and NGC~3031) have much larger scale-lengths
than that of the more active star-forming galaxies (NGC~5194 and NGC~6946).
This difference may be due to the relative deficit of recent CR
injection into the interstellar medium (ISM) for the galaxies having largely
quiescent disks.Comment: 6 pages, 3 figures, To appear in the proceedings of the "Island
Universes: Structure and Evolution of Disk Galaxies" conference held in
Terschelling, Netherlands, July 2005, ed. R. de Jong (Springer: Dordrecht
Galaxy Disks
The formation and evolution of galactic disks is particularly important for
understanding how galaxies form and evolve, and the cause of the variety in
which they appear to us. Ongoing large surveys, made possible by new
instrumentation at wavelengths from the ultraviolet (GALEX), via optical (HST
and large groundbased telescopes) and infrared (Spitzer) to the radio are
providing much new information about disk galaxies over a wide range of
redshift. Although progress has been made, the dynamics and structure of
stellar disks, including their truncations, are still not well understood. We
do now have plausible estimates of disk mass-to-light ratios, and estimates of
Toomre's parameter show that they are just locally stable. Disks are mostly
very flat and sometimes very thin, and have a range in surface brightness from
canonical disks with a central surface brightness of about 21.5 -mag
arcsec down to very low surface brightnesses. It appears that galaxy
disks are not maximal, except possibly in the largest systems. Their HI layers
display warps whenever HI can be detected beyond the stellar disk, with
low-level star formation going on out to large radii. Stellar disks display
abundance gradients which flatten at larger radii and sometimes even reverse.
The existence of a well-defined baryonic Tully-Fisher relation hints at an
approximately uniform baryonic to dark matter ratio. Thick disks are common in
disk galaxies and their existence appears unrelated to the presence of a bulge
component; they are old, but their formation is not yet understood. Disk
formation was already advanced at redshifts of , but at that epoch
disks were not yet quiescent and in full rotational equilibrium. Downsizing is
now well-established. The formation and history of star formation in S0s is
still not fully understood.Comment: This review has been submitted for Annual Reviews of Astronomy &
Astrophysics, vol. 49 (2011); the final printed version will have fewer
figures and a somewhat shortened text. A pdf-version of this preprint with
high-resolution figures is available from
http://www.astro.rug.nl/~vdkruit/jea3/homepage/disks-ph.pdf. (table of
contents added; 71 pages, 24 figures, 529 references
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