Abstracts
I develop and explain a new method for interpolating detailed fertility schedules from agegroup data. The method allows estimation of fertility rates over any fine grid of ages, from either standard or nonstandard age groups. The new method, called the calibrated spline (CS) estimator, expands an abridged fertility schedule by finding the smooth curve that minimizes a squared error penalty. The penalty is based both on fit to the available agegroup data, and on similarity to patterns of 1f x schedules observed in the Human Fertility Database (HFD) and in the US Census International Database (IDB). I compare the CS estimator to a very good alternative method that requires more computation: Beers interpolation. The results show that CS replicates known 1f x schedules from 5f x data better, and its interpolated schedules are also smoother. The conclusion is that the CS method is an easily computed, flexible, and accurate method for interpolating detailed fertility schedules from agegroup data. Users can calculate detailed schedules directly from the input data, using only elementary arithmetic.
Fertility; Interpolation; Splines; Penalized least squares
Se desarrolla y explica un nuevo método para la interpolación de estructuras etarias detalladas de fecundidad a partir de datos agrupados por edad. El método permite la estimación de las tasas específicas de fecundidad para cualquier edad detallada, desde los diferentes segmentos etarios estándar hasta cualquier agrupamiento no utilizado usualmente. El nuevo método, llamado estimador spline calibrado (CS), expande las tasas de fecundidad agrupadas por edad encontrando una curva suavizada mediante la minimización de los errores cuadrados penalizados. La penalización se basa tanto en el ajuste de los datos de los grupos etarios disponibles como en la semejanza de los patrones de las estructuras de edad 1f x observados en la Human Fertility Database (HFD) y la US Census International Database (IDB). El estimador CS se comparó con un buen método alternativo que requiere más procesamiento: la interpolación de Beers. Los resultados muestran que el CS replica las conocidas estructuras etarias de fecundidad 1f x, a partir de las 5f x mejoradas, donde las estructuras etarias de la fecundidad interpoladas también se presentan más suavizadas. La conclusión a la que se arriba es que el CS constituye un método fácil de calcular, flexible y preciso para la interpolación de estructuras de fecundidad detalladas a partir de datos agrupados. Los usuarios pueden calcular estructuras específicas de fecundidad detalladas directamente por medio de los datos observados, solo utilizando la aritmética elemental.
Fecundidad; Interpolación; Splines; Mínimos cuadrados penalizados
É desenvolvido e explicado um novo método para a interpolação de estruturas etárias detalhadas de fecundidade, a partir de dados agrupados por idade. O método permite a estimativa das taxas específicas de fecundidade para qualquer idade detalhada, desde as diferentes faixas etárias padrão até qualquer agrupamento não usualmente utilizado. O novo método, chamado de estimador spline calibrado (CS), expande as taxas de fecundidade agrupadas por idade encontrando uma curva suavizada, por minimização dos erros quadrados penalizados. A penalidade é baseada tanto no ajuste aos dados dos grupos etários disponíveis, quanto na semelhança dos padrões das estruturas etárias 1f x observadas no Banco Human Fertility Database (HFD) e no US Census International Database (IDB). O estimador CS foi comparado a um bom método alternativo que requer mais computação: interpolação de Beers. Os resultados mostram que o CS replica as conhecidas estruturas etárias de fecundidade, 1f x, a partir das 5f x melhoradas, sendo que as estruturas etárias da fecundidade interpoladas apresentamse também mais suavizadas. A conclusão é que o CS constitui um método facilmente calculado, flexível e preciso para a interpolação de estruturas de fecundidade detalhadas a partir de dados agrupados. Os usuários podem calcular estruturas específicas de fecundidade detalhadas diretamente por meio dos dados observados, usando apenas aritmética elementar.
Fecundidade; Interpolação; Splines; Mínimos quadrados penalizados
ARTIGOS
Calibrated spline estimation of detailed fertility schedules from abridged data^{1} 1 Data and R programs for replicating this paper's results are available online at < http://calibratedspline.schmert.net/REBEP>.
Estimadores splines calibrados: estimativas de taxas detalhadas de fecundidade a partir de dados agrupados por idade
Estimadores spline calibrados para tasas detalladas de fecundidad a partir de datos agrupados por edad
Carl P. Schmertmann
Center for Demography and Population Health, Florida State University, Tallahassee, USA (schmertmann@fsu.edu)
Address
ABSTRACT
I develop and explain a new method for interpolating detailed fertility schedules from agegroup data. The method allows estimation of fertility rates over any fine grid of ages, from either standard or nonstandard age groups. The new method, called the calibrated spline (CS) estimator, expands an abridged fertility schedule by finding the smooth curve that minimizes a squared error penalty. The penalty is based both on fit to the available agegroup data, and on similarity to patterns of _{1}f_{x} schedules observed in the Human Fertility Database (HFD) and in the US Census International Database (IDB). I compare the CS estimator to a very good alternative method that requires more computation: Beers interpolation. The results show that CS replicates known _{1}f_{x} schedules from _{5}f_{x} data better, and its interpolated schedules are also smoother. The conclusion is that the CS method is an easily computed, flexible, and accurate method for interpolating detailed fertility schedules from agegroup data. Users can calculate detailed schedules directly from the input data, using only elementary arithmetic.
Keywords: Fertility. Interpolation. Splines. Penalized least squares
RESUMO
É desenvolvido e explicado um novo método para a interpolação de estruturas etárias detalhadas de fecundidade, a partir de dados agrupados por idade. O método permite a estimativa das taxas específicas de fecundidade para qualquer idade detalhada, desde as diferentes faixas etárias padrão até qualquer agrupamento não usualmente utilizado. O novo método, chamado de estimador spline calibrado (CS), expande as taxas de fecundidade agrupadas por idade encontrando uma curva suavizada, por minimização dos erros quadrados penalizados. A penalidade é baseada tanto no ajuste aos dados dos grupos etários disponíveis, quanto na semelhança dos padrões das estruturas etárias _{1}f_{x} observadas no Banco Human Fertility Database (HFD) e no US Census International Database (IDB). O estimador CS foi comparado a um bom método alternativo que requer mais computação: interpolação de Beers. Os resultados mostram que o CS replica as conhecidas estruturas etárias de fecundidade, _{1}f_{x}, a partir das _{5}f_{x} melhoradas, sendo que as estruturas etárias da fecundidade interpoladas apresentamse também mais suavizadas. A conclusão é que o CS constitui um método facilmente calculado, flexível e preciso para a interpolação de estruturas de fecundidade detalhadas a partir de dados agrupados. Os usuários podem calcular estruturas específicas de fecundidade detalhadas diretamente por meio dos dados observados, usando apenas aritmética elementar.
Palavraschave: Fecundidade. Interpolação. Splines. Mínimos quadrados penalizados
RESUMEN
Se desarrolla y explica un nuevo método para la interpolación de estructuras etarias detalladas de fecundidad a partir de datos agrupados por edad. El método permite la estimación de las tasas específicas de fecundidad para cualquier edad detallada, desde los diferentes segmentos etarios estándar hasta cualquier agrupamiento no utilizado usualmente. El nuevo método, llamado estimador spline calibrado (CS), expande las tasas de fecundidad agrupadas por edad encontrando una curva suavizada mediante la minimización de los errores cuadrados penalizados. La penalización se basa tanto en el ajuste de los datos de los grupos etarios disponibles como en la semejanza de los patrones de las estructuras de edad _{1}f_{x} observados en la Human Fertility Database (HFD) y la US Census International Database (IDB). El estimador CS se comparó con un buen método alternativo que requiere más procesamiento: la interpolación de Beers. Los resultados muestran que el CS replica las conocidas estructuras etarias de fecundidad _{1}f_{x}, a partir de las _{5}f_{x} mejoradas, donde las estructuras etarias de la fecundidad interpoladas también se presentan más suavizadas. La conclusión a la que se arriba es que el CS constituye un método fácil de calcular, flexible y preciso para la interpolación de estructuras de fecundidad detalladas a partir de datos agrupados. Los usuarios pueden calcular estructuras específicas de fecundidad detalladas directamente por medio de los datos observados, solo utilizando la aritmética elemental.
Palabras clave: Fecundidad. Interpolación. Splines. Mínimos cuadrados penalizados
Introduction
Demographers like precise data for exact ages, but unfortunately we often get the opposite noisy sample estimates aggregated into wide age groups. Worse, sometimes the age groups do not cover the entire range of interest for the behavior under study. With abridged, partial, or noisy data, demographic calculations often require interpolation and extrapolation of agespecific rates.
In this paper I introduce a method for fitting detailed fertility schedules to coarse, possibly noisy data. The method exploits a large new dataset, the Human Fertility Database (HFD), to identify empirical regularities in fertility schedules by single years of age 1254. It then uses these regularities in a penalized least squares framework to produce simple rules for expanding grouped data (usually _{5}f_{x} estimates) into detailed rates over an arbitrarily fine grid of ages that may extend outside the range of the original data (for example, below age 15 or above age 50).
The new method uses spline functions as building blocks, and identifies smooth fertility schedules that match grouplevel data closely while also conforming to patterns observed in the HFD. I call the result of the procedure a calibrated spline (CS) schedule. Its derivation uses some rather dense matrix algebra, but the end result is exceedingly simple: basic arithmetic with the grouped data and a set of predetermined constants.
Notation and derivation of the calibrated spline estimator
In the next two sections I explain and derive the CS estimator. Readers uninterested in the mathematical details may, without difficulty, skip ahead to the penultimate paragraph of the next section, beginning with The key point is....
Suppose that the fertility schedule can be well approximated by a weighted sum of K continuous basis functions:
over the reproductive age range [α,β]. In many applications demographers use a fine grid of ages {a_{1}...a_{N}} and assume that fertility is constant at some level f_{i} within each small interval . In such applications the discrete version of φ is an Nx1 vector:
where b_{i}΄is a 1xK vector containing the value of each basis function at a=a_{i}, and B is thus an NxK matrix of known constants.
In general, the {a_{1}} grid can be arbitrarily fine, over any age range of interest, and there are many possible choices for the number and form of basis functions {b_{k}}. In the calculations in this paper, α=12, β=55, N=86, Δ=.50, there are separate fertility rates for intervals centered at 12.25, 12.75,...54.75. I use quadratic Bspline basis functions (BOOR, 1978; EILERS; MARX, 1996) over uniform knots at twoyear intervals.^{2} 2 Specifically, basis functions come from the bs( ) function in R (R CORE DEVELOPMENT TEAM, 2011), with arguments x=seq(12.25, 54.75, .50), knots=seq(12,54,2), and degree=2. I retain the third through twentyfirst columns of the resulting matrix as an 86x19matrix B.
When fertility data is reported as averages for age groups (call the groups A_{1}...A_{g}), we need multipliers for aggregating f. The Nx1 vector f is related to the gx1 vector of group averages (called y from here on) by:
where G is gxN with and I[.] is a 0/1 indicator function. The fine grid f is similarly related to singleyear rates by:
where S_{ij} = Δ ⋅ I [(α + i)  1 < a_{j} < (α + i)].
Objective and estimation strategy
Suppose that we observe y, a g x 1 vector of sample estimates for age group averages. We want to estimate the K spline weights θ (and ultimately, the N elements of the discretized schedule f) from the g estimates in y. When K>g (i.e., when there are more than g basis functions) fitting and estimation requires additional identifying information of some kind.
I propose two criteria for a good schedule f: it should (1) closely fit the observed data y, (2) have an age pattern similar to known singleyear schedules specifically, to schedules downloaded from the Human Fertility Database (HFD, 2012) and in the US Census International Database (SCHMERTMANN, 2003, file III). For these criteria, which I call fit and shape respectively, one can construct vectors of residuals that should be near zero for good schedules. These vectors are:
The M matrix for shape residuals has a complicated construction, but a simple interpretation. Construction is as follows. I first assemble a 43x530 matrix F, comprising 304 singleyear ASFR schedules from the HFD over ages 12...54,^{3} 3 The HFD version that I used has 1480 singleyear schedules, many of which are from the same country in consecutive calendar years. In order to limit the overcounting of highly correlated schedules, I used every fifth year from each population e.g., Austria 1953, 1958, ..., 2008, Bulgaria 1949, 1954, ..., 2009, and so on. plus an additional 226 estimated singleyear schedules from the US Census International Database (IDB) using the quadratic spline model and coefficients from Schmertmann (2003,file III).^{4} 4 It is slightly clumsy to split the fiveyear IDB schedules into approximate singleyear schedules in order to include them in the analysis, but adding these schedules is important. The HFD does not yet include countries from Africa and Asia that have very distinct age patterns in particular African schedules often have relatively high fertility at ages 35+, and some East Asian schedules have extremely low fertility at ages below 25. Estimation of SVD principal components from a matrix that includes the wider variety of patterns in the IDB produces a much more representative set of "typical" age schedules. Singular value decomposition F=UDV' yields orthonormal principal component vectors in U's columns. The first three of these columns (call this 43x3 matrix X) account for approximately 95% of the variation in F, in the sense that projections of any singleyear schedule s onto the column space of X have small errors:
where P= X(X'X)^{1}X' is the projection matrix for the column space of X.
Defining M=(I_{43}P), shape residuals in Equation (5) represent the portion of a singleyear schedule that is unexplained by linear combinations of principal components. In other words, shape residuals ε_{s} in Equation (5) are large for singleyear schedules that have age patterns unlike those observed in the HFD and IDB.^{5} 5 More precisely, a schedule f has large shape residuals when S f lies far from the column space of X. It is possible for f to have low shape residuals even if it is unlike any observed schedule, if f is well approximated by a combination of principal components that has no counterpart in the database.
Each criterion can be converted into a scalar index of a schedule's "badness" by calculating an appropriately weighted sum of squares. These scalar penalty terms have generic form:
where V_{c} = E[ε_{c}ε_{c}'] is the covariance of ε_{c}.
The covariance matrix of fitting errors ε_{f} can be approximated logically. Supposing that the estimates in the vector y represent ratios of births to an average of W women sampled in each age group, and that a typical agespecific rate is approximately 0.10, then with independent sampling errors across groups the covariance of ε_{f} is:^{6} 6 The calculation assumes that B, the number of births to W women with true rate f, is a Poisson random variable with mean and variance Wf. A sample estimate yk= B/W therefore has variance f/W.
and its inverse is:
These assumptions are crude, but results are not very sensitive to them. The main point is that with large sample sizes, schedules that fit age group averages poorly get extremely heavy penalties.
For the covariance of shape residuals, we refer to the singleyear schedules in the HFD. For each of the 1480 schedules (s) in the HFD singleyear data, one can calculate e_{s}=M _{s}. The average outer product of these HFD shape residuals serves as a covariance estimate:
V_{s} provides information about which ages are likely to have large or small residuals, and about the age patterns among those residuals.^{7} 7 Adding a small constant to each diagonal element of V s before inverting stabilizes results considerably. I add 0.1 times the median value of the diagonal elements from Equation (10).
Summing the penalties produces a single index that is appropriately calibrated to the available information about errors:^{8} 8 There is also a natural Bayesian interpretation for this index: the fitting penalty comes from the log likelihood of a multivariate normal distribution, and the shape penalty terms come from an improper multivariate normal prior.
where
and
Because Q_{W} is positive definite, expression in Equation (11) has a unique minimum when weights are θ^{*} = R_{W}y. Thus, for estimated fertility rates y that come from samples of approximately W women per age group, the combination of basis function that minimizes the joint criterion in Equation (11) is a vector that I call the calibrated spline (CS) fit:
The key point is that this complex derivation leads to a simple result: the optimal schedule f is a linear function of the observed data y. Given a sample size, the N x g matrix K _{W} contains predetermined constants, so that we can write the CS vector f* as a weighted sum of g columns:
In principle, this framework allows a demographer to create customized, simple arithmetical rules for transforming fertility estimates from any set of g age groups into a schedule over an arbitrarily fine grid of N rates over any age span of interest. The method is particularly straightforward because the "parameters" for the empirical model are the estimated agegroup fertility rates themselves, so that fitting the model requires only multiplication and addition.
In practice, researchers can simplify further by using one of the precalculated K _{W} matrices, for W = 100, 1000, 10000, or 100000 and common age groups, available online at <http://calibratedspline.schmert.net/REBEP>. For larger sample sizes, multipliers vary little from the W=100,000 case; I recommend using the W=100,000 constants for samples with W > 100,000. If the sample size is unknown, I recommend using W=1000. After selecting the right order of magnitude W for sample sizes a demographer can produce a schedule for ages 12.25, ... 54.75 directly from age group averages y by multiplying f* = K _{W} y as in Equation (15).
Example fits with HFD, IDB, and Brazilian data
The CS method outlined above works for any set of age groups, but I deal with two specific examples in the rest of this paper cases in which (a) data are available for g=7 age groups 1519 through 4549, as in the US Census International Database (IDB) and many other datasets, or (b) data are available for g=9 fiveyear age groups 1014 through 5054, as in the HFD.^{9} 9 For both of these cases, supplemental files at < http://calibratedspline.schmert.net/REBEP> contain the calculated K W matrices for sample sizes W = 100, 1000, 10000, or 100,000. For the g=7 case, the 86x7 matrices of constants K W appear in commadelimited supplemental files K7100.csv ... K7100000.csv. For g=9 the corresponding 86x9 matrices appear in K9100.csv... K9100000.csv. Readers can adapt the supplemental programs to construct constants for other combinations of age grids, age groups, and average sample sizes.
Graph 1 illustrates K_{10000} for the g=7 and g=9 cases, by plotting each column as a function of age. For example, a unit increase in estimated _{5}f_{15} changes f* values at various ages by the height of the line labeled "15". A unit increase in estimated _{5}f_{20} changes f* according to the line labeled "20", and so on. Note that the range of estimated fertility f* may extend beyond that spanned by the input data: in the g=7 case the procedure produces estimated ASFRs below age 15 and above age 50, based on known regularities in the age pattern of rates.
Using Equation (14) or (15), basis functions in Graph 1 are multiplied by the observed y values and then summed to produce complete CS schedules over [α,β]. The top panel of Graph 2 illustrates the expansion of a set of g=7 fiveyear estimates into halfyear intervals, using IDB data from Uruguay. The input data for Uruguay, based on national data, are:
y_{URU} = 10^{3} x (49 116 135 99 54 16 2)'
United Nations data (UNSD, 2014) indicate that in 2002 there were approximately W=100,000 Uruguayan women in each fiveyear age group, so K_{100000} based on g=7 is the appropriate matrix to use.
Multiplying the y values by the columns of K and summing, as in Equation (15), produces an 86x1 vector f*=K _{y} for rates at halfyear intervals over 1255, shown in the top panel.
The agegroup averages for the CS model do not exactly replicate the input data. For example, the average of the CS schedule over ages 3539 in Uruguay is .0536, slightly lower than the original _{5}f_{35} value of .0540. This occurs because minimizing the penalty index in Equation (11) requires tradeoffs between model fit and the shape of schedule. The tradeoff for Uruguay was typical, in the sense that over all 226 IDB schedules, Uruguay's mean squared fitting error was closest to the median: half of IDB schedules have better CS fits to the _{5}f_{x} data, and half have worse.
The bottom panel of Graph 1 illustrates the CS schedule for Austria's 1952 period fertility, calculated from g=9 fiveyear rates for age groups 1014 through 5054. There were approximately 250,000 women in each fiveyear age group in 1952 (HMD, 2014), so the calculation in the lower panel of Graph 2 also uses the K_{100000} multipliers. Austrian fertility rates for the nine fiveyear age groups were:
Y_{AUT1952} = 10^{3} x (.14 34 118 116 82 46 16 1 .02)'
In this case one can check the accuracy of the CS fit, because Austria 1952 is one of 586 HFD schedules with _{1}f_{x} values over x=12...54 that come directly from original data (rather than being interpolated from _{5}f_{x} or other group averages). These original _{1}f_{x} values appear as black dots in the lower panel of Graph 1, and it is clear that for this schedule the CS fit to the histogram matches the single year data well: the root mean squared error (RMSE) across all 43 ages is 0.0019. This is close to the seventyfifth percentile of RMSE over the 586 complete singleyear schedules in the HFD. Thus the Austria 1952 fit to the singleyear data in Graph 2 is actually worse than average: threefourths of CS fits from fiveyear data match the original singleyear schedule more accurately, while approximately one quarter of fits to HFD data are more accurate.^{10} 10 99.7% of fitted singleyear rates with the CS model are within .01 of the equivalent HFD data. The largest CS fitting error over the 586 complete singleyear schedules is for 19yearolds in the Czech Republic in 1991: true and fitted rates were .140 and .120, respectively. This error arises because Czech 1991 rates had an unusually steep rise over ages 1620, which the CS model does not replicate precisely.
Graph 3 shows example fits to subnational data, for rural and urban residents of the Brazilian state of Rio de Janeiro. The plots use 2010 Demographic Census data (IBGE, 2010), downloaded as a five percent microdata sample from the IPUMSInternational website (MPC, 2014). Solid dots in the graph represent singleyear fertility rates _{1}f_{x}, calculated from reported births in the previous year. These rates are quite noisy for rural residents, because unweighted sample sizes are modest. Over ages 1054, the IPUMS sample for women in rural Rio de Janeiro contains a median of 202 records at a single year of age, and a median of 1024 records in a fiveyear age group. In contrast, urban _{1}f_{x} estimates are much less affected by sampling variability (median urban sample size is 4007 for single years, and 20,231 for the fiveyear groups).
Graph 3 illustrates the need for smoothing _{1}f_{x} estimates, especially in the rural case. The high volatility of _{1}f_{x} over small age ranges is implausible, and clearly due more to sampling variability than to any real patterns in Brazilian fertility.
However, Graph 3 also illustrates how the standard smoothing method (i.e., aggregating into fiveyear groups and treating the _{5}f_{x} rates as constant within groups) obscures important details of the true age pattern. In particular, aggregating into _{5}f_{x} hides a very steep rise in rates over ages 1519, and steep declines over ages 3034 and 3539.
The CS fit, which expands _{5}f_{x} values into a historically plausible schedule over a fine grid of ages, represents a better compromise. The CS model smooths away much of the sampling noise, without loss of age detail. In this case, as in the Austrian data shown earlier, the CS model (calculated only from the heights of the histograms in each panel) does in fact represent the underlying singleyear rates well.
Comparative accuracy of CS vs. Beers interpolation
Researchers from Columbia University and the UN Population Division (LIU et al., 2011) recently used HFD data to compare the accuracy of several interpolation methods for fertility schedules. They concluded that the best overall method for recovering singleyear agespecific rates from fiveyear averages was a variant^{11} 11 The Beers method often generates negative rate estimates at ages <20 and 40+. In the Liu et al. (2011) variant, negative rates are replaced with exponential curves, which are then rescaled so that the fiveyear age group totals match the input data. of Beers's ordinary osculatory interpolation method (SHRYOCK; SIEGEL, 1975, Table C3).
Because the Beers interpolation approach was selected in an earlier "competition", it is valuable to compare it to the CS approach over a wide range of schedules. Graph 4 offers an initial example for a single schedule, showing the interpolated fits from the two methods for Scotland in 2004, and a summary of the fitting errors. Scotland had more than 100,000 women in each of the fiveyear age groups (NRS, 2014), so the CS fit in Graph 4 uses the K_{100000} multipliers.
Several features of Graph 4 deserve mention. Both methods produce interpolated schedules that fit the singleyear rates well. For the Scotland 2004 schedule the CS method is generally more accurate at ages below 30, and unlike the Beers approach it captures the subtle inflection in rates for the early 20s. The Beers model fits the singleyear data better at ages 40+ (in part because extra adjustment that Liu et al. make for negative predicted rates at ages 4852 with these input data). Overall, the CS errors are smaller.
Moving from a single example to a global summary, Graph 5 summarizes the errors for the two methods over all 586 HFD schedules with known singleyear rates, disaggregated by age. Notice:

the vertical scale shows that average errors are very small for both methods;

the sawtooth pattern of errors at ages below 35 shows that both interpolation methods fit singleyear data better in the middle of fiveyear intervals than they do at the edges. This is an arithmetical property of interpolation when the underlying curve is approximately linear over fiveyear intervals: both the fitted and true schedules are likely to be close to the agegroup average at the center of the age range;

the pattern of comparative errors by age seen for Scotland 2004 in Graph 4 holds up across all schedules: calibrated spline fits are much better at ages below 40, while Beers fits (after fixing negative values) are slightly better at ages above 40;

most importantly, the total of average errors (all ages combined) is lower for the CS approach.
It is also useful to summarize errors over different dimensions. Graph 6 offers a second global comparison of the methods, this time aggregating over ages and showing the average RMSE by country. Average interpolation errors are lower for the CS method in all 20 populations. Once again, both methods perform very well, but the CS method fits better than Beers.
Table 1 provides a final comparison of the methods, with slightly more quantitative detail about some of the potential problems that may occur when interpolating rates from abridged data. Section A of the table contain fitting errors (104) by age group and interpolation method, for (age, period, country) cells where the HFD's _{1}f_{x} values come from original data sources rather than from a splitting algorithm. The CS method performs better overall, but at high maternal ages its fits are slightly worse than those of the adjusted Beers algorithm.
Section B reports measures of the roughness or wiggliness of interpolated schedules, summarizing second differences by age (_{1}f_{x+2}  _{1}f_{x+1})  (_{1}f_{x+1}  _{1}f_{x}) with root mean squared values (.10^{4}) across models fit to all 1480 HFD schedules (interpolation from g=9 age groups) and all 226 IDB schedules (g=7). Lower index values in Section B correspond to sets of interpolated schedules with fewer upanddown wiggles and fewer local maxima in the interpolated singleyear rates. Again the CS method performs better, producing smoother schedules.
Section C of Table 1 includes information on a performance criterion for which the CS method is inferior to the (adjusted) Beers approach: negative rate estimates. With the test data at hand, each method produces 1706x43=73358 singleyear rate estimates. In the original Beers approach (not shown in the table) approximately 12% of the estimates are negative and 3% are below .005. However, the Liu et al. variant used here eliminates all negative values through a postprocessing algorithm.
In contrast, without adjustment 2.7% of the CSestimated fertility rates are negative. Although this is of course logically impossible, the vast majority of these negative CS rate estimates are negligibly different from zero. As seen in Section C, only 0.4% of CS rates are below .0005 (i.e., negative after rounding to three decimal places). In practice, CS estimates are sufficiently close to zero that their direct use in calculations such as TFR, mean age of childbearing, etc. would cause no meaningful problems.
Small negative estimates are a minor problem for the CS method, small enough that I have not applied any postprocessing to the CS rates in any of this paper's tables or graphs. However, it is possible to use a very simple postprocessing procedure on CS rates namely, after calculating f*=K _{W} y, replace any negative values with zeroes. This is computationally much simpler than the Liu et al. (2011) postprocessing algorithm for Beers rates, and it would not alter any of the values in Sections A or B of Table 1.^{12} 12 With truncation at zero, the Calibrated Spline column of Table 1 would remain unchanged, except that the percentages in Section C would all be zero.
In sum, both methods are very good, but the CS method performs slightly better over all HFD countries, and over the ages at which fertility rates are highest. Interpolated CS schedules are smoother and fit known data better. CS calculation is also much simpler than the Beers variant used by Liu et al. (2011), because it does not require complex adjustments for edge effects and negative values.
Discussion
I have presented applications of the calibrated spline model for only two specific cases, but the general framework is extremely flexible. In principle one can construct expansion constants K that map input data from any set of age groups onto any fine grid of ages. The input age groups may be incomplete (e.g., {2529,3539,4044,4554}), irregularly spaced ({1214,1519,2024,2534,...}), or even overlapping ({1517,1524,...}).^{13} 13 In these cases, it would be necessary to modify the matrix G that computes group averages from the detailed schedule, so that y = G f for the new set of age groups.
The CS model fits observed schedules well, outperforming an alternative method that has done well in earlier research. It is also much simpler to estimate. Given the K constants (which in most cases are the ones already provided in this paper and the accompanying data files), fitting a detailed ASFR schedule requires only basic arithmetic. Unlike the Beers method and other generic polynomial fitting methods that are not designed specifically for fertility estimation, postestimation tweaks for negative fitted rates at the highest and lowest maternal ages are rarely necessary.
Although not explicitly Bayesian, the CS estimation approach makes heavy use of a priori information. The penalized least squares criterion gives priority to fertility schedules that not only fit input data well, but that also match historical or contemporary patterns seen in large databases. The technique of identifying such patterns through singular value decomposition of a large data array is not new in demography (for example, it is the basis of the LeeCarter [1992] mortality model), but to my knowledge researchers have not previously used such patterns in a simple, leastsquares method like that presented here.
Author
Carl P. Schmertmann is Doctor in Economics from the University of California Berkeley, researcher in Demography and Professor of Economics at Florida State University.
Recebido para publicação em 14/05/2014
Aceito para publicação em 08/09/2014
Appendix: Moment calculations from age group data
One possible use of the empirical model is estimation of moments of the continuous fertility schedule from grouped data. This type of approximation might be especially useful with indirect methods.
Begin by defining the function:
FRM A1
which can be approximated as
FRM A2
Where Q_{W} and R_{W} are defined as in equations (12) and (13), and c_{n}(x) is therefore a g x 1 vector of known constants.
With different (x,n) combinations, Equation (A2) produces different moments of the fertility function. Table A1 shows some of the calculated constants for the g=7 case; a more complete set of constants, calculated using the suggested default of W=1000, is available in supplemental file Cdata.csv.
By definition Q_{0}(∞) is a schedule's total fertility (TFR), and Q_{1}(∞)/Q_{0}(∞) is its mean age of childbearing µ. In the case of the Uruguay 2002 data shown earlier, for example, we can approximate these quantities as:
TFR = Q_{0}(∞) ≈ 3.44(.049) + ... + 0.66(.002) = 2.328
µ = Q_{1}(∞) / Q_{0}(∞) ≈ [60.78(.049) + ... + 27.15(.002)] / 2.328 = 28.23
Similarly, one can approximate conditional moments such as average parity of women 3034 [Q_{0}(32.5)] and the average age at which they had their previous births [Q_{1}(32.5)/ [Q_{0}(32.5)]. With the Uruguay data these moments would be:
P_{3034}≈ Q_{0}(32.5) ≈ 3.51(.049) + ... 0.03 (.002) = 1.753
µ_{3034}≈ Q_{1}(32.5) / Q_{0}(32.5) ≈ [63.46(.049) + ... 1.53(.002)] / 1.753 = 25.37
Calculations like this can be important for time allocation with indirect methods. For example, from the fiveyear rate schedule for Uruguay, moment approximations imply that with a cohort fertility schedule with this shape, women 3034 interviewed in a survey would have had their births an average of 32.5025.36 = 7.14 years earlier.
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Publication Dates

Publication in this collection
23 Jan 2015 
Date of issue
Dec 2014
History

Accepted
08 Sept 2014 
Received
14 May 2014