Making better estimates with scarce information

TL;DR

I explore the pros and cons of different approaches to estimation. In general I find that:

  • interval estimates are stronger than point estimates

  • the lognormal distribution is better for modelling unknowns than the normal distribution

  • the “lognormal” mean is better than the arithmetic mean for building aggregate estimates

These differences are only significant in situations of high uncertainty, characterised by a high ratio between confidence interval bounds. Otherwise, simpler approaches like point estimates & the arithmetic mean are fine.

Summary

I am chiefly interested in how we can make better estimates from very limited evidence. Estimation strategies are key to sanity-checks, cost-effectiveness analyses and forecasting.

Speed and accuracy are important considerations when estimating, but so is legibility; we want our work to be easy to understand. This post explores which approaches are more accurate and when the increase in accuracy justifies the increase in complexity.

My key findings are:

  • Interval (or distribution) estimates are more accurate than point estimates because they capture more information. When dividing by an unknown of high variability (high ratio between confidence interval bounds) point estimates are significantly worse.

  • It is typically better to model distributions as lognormal rather than normal. Both are similar in situations with low variability, but lognormal appears to better describe situations of high variability.

  • The “lognormal” mean is good for building aggregate estimates. By calculating the mean of a lognormal distribution for which our inputs form a confidence interval, we capture the positive skew typical of more variable distributions.

  • In general, simple methods are fine while you are estimating quantities with low variability. The increased complexity of modelling distributions and using geometric means is worthwhile when the unknown values are highly variable.

Interval vs point estimates

In this section we will find that for calculations involving division, interval estimates are more accurate than point estimates. The difference is most stark in situations of high uncertainty.

Interval estimates, for which we give an interval within which we estimate the unknown value lies, capture more information than a point estimate (which is simply what we estimate the value to be). Interval estimates often include the probability that the value lies within our interval (confidence intervals) and sometimes specify the shape of the underlying distribution. In this post I treat interval estimates as distribution estimates as the same thing.

Here I attempt to answer the following question: how much more accurate are interval estimates and when is the increased complexity worthwhile?

Core examples

I will explore this through two examples which I will return to later in the post.

Fuel Cost: The amount I will spend on fuel on my road trip in Florida next month. The abundance of information I have about fuel prices, the efficiency of my car and the length of my trip means I can use narrow confidence intervals to build an estimate.

Inhabitable Planets: The number of planets in our galaxy with conditions that could harbour intelligent life. The lack of available information means I will use very wide confidence intervals.

Point estimates are fine for multiplication, lossy for division

Let’s start with Fuel Cost. Using Squiggle (which uses lognormal distributions by default: see the next section for more on why), I enter 90% confidence intervals to build distributions for fuel cost per mile (USD per mile) and distance of my trip (miles). This gives me an expected fuel cost of 49.18USD

What if I had used point estimates? I can check this by performing the same calculation using the expected values of each of the distributions formed by my interval estimates.

I get the same answer. In fact, this applies in all cases: if X and Y are normally or lognormally distributed,

In other words, the mean of the product of two normal/​lognormal distributions is the product of their means. The only drawback of using point-estimates for multiplication is that you only get a numerical answer—you lose the shape of the distribution.

What about division? Put simply,

so

Division will be lossy when you use point estimates. But how bad is it?

Using the Fuel Cost example we find that the point estimate result (0.099048) is within 1% of the interval estimate result (0.099809).

Now let’s turn to the inhabitable planets example. I use interval estimates for the number of stars in the galaxy and the number of stars per inhabitable planet. Because of the uncertainty the bounds of my intervals differ by 2-3 orders of magnitude.

I find that the interval-estimate approach gives an expected number of inhabitable planets of 3.5 billion, while my point-estimate approximation is just 100 million! Clearly when there are very high levels of uncertainty, dividing by a point estimate is inaccurate. Not only that, but the point estimate answer provides no information on the shape of the possible outcomes. The interval estimate approach shows us that although the expected number of planets is 3.5 billion, the median is just 220 million.

This heavy-tailed behaviour helps explain where the Drake Equation (which relies upon point-estimates of highly uncertain values and suggests that we should have heard from aliens by now) goes wrong: using interval estimates we can show that although the expected number of interstellar alien neighbours is high, the median is much lower. My very rough attempt finds a mean of 4700 alien neighbours, with a a 25-50% chance of none at all (although I may be pushing Squiggle past its limits).

Should we always use interval estimates?

Using interval estimates as inputs

As we have seen, interval estimates are better for modelling uncertainty. They do not introduce mathematical error and they can store more information about what we know.

In a sense a point estimate is a distribution estimate: one that assigns probability 1 to the point estimate and 0 to everything else. This means it isn’t hard to improve upon. However, if we don’t have strong objective evidence for the shape of the distribution, we have to use personal judgement to estimate it. If transparency and impartiality are important, this can be a problem.

Suppose I do a quick google search and determine that the fuel efficiency of my car is supposed to be 47mpg. If I’m estimating the fuel cost for an expense form, using this value makes sense: the person reading the form can verify that this is an objective estimate of my car’s efficiency. If I am doing he calculation for myself, on the other hand, it might make sense to use an interval estimate using my personal judgement (something like a 90% C.I. of 40 to 47mpg, on the basis that my car is no longer new and that cars don’t achieve their theoretical efficiency in real-world conditions).

Using interval estimates as outputs

When constructing an estimate from multiple sub-estimates, as I would in the Fuel Cost and Inhabited Planets examples, a key challenge is communicating the level of uncertainty in the final result.

On their own, point-estimates do not communicate any nuance. They should be paired with a statement on the uncertainty of the result, like “this value is highly uncertain and could be off by an order of magnitude”.

The trouble is that it’s difficult to know just how uncertain the final result is. Even when we calculate using interval estimates, the reliability of the final distribution is highly uncertain. Look back at the Inhabited Planets example in the previous section: we find a 90% confidence interval of 4.7 million to 11 billion inhabitable planets in our galaxy. But this only gives a flavour of the likely distribution of inhabited planets. The 90% confidence interval, calculated from two rough sub-estimates, just isn’t trustworthy.

So even though interval outputs communicate that the value is uncertain, readers may still overestimate the reliability of the estimate.

Toby Ord gives a good example of how to convey uncertainty in the Precipice. He accompanies table 6.1, which provides point-estimates for the magnitudes of various existential risks over the next 100 years, with the qualifier:

There is significant uncertainty remaining in these estimates and they should be treated as representing the right order of magnitude—each could easily be a factor of 3 higher or lower.

It’s nice because the description of the uncertainty is itself imprecise, which dissuades us from being over-confident in it.

[Thanks to Vasco Grilo for highlighting this example]

General findings: interval vs point estimates

I did some more experimentation on Squiggle to generalise the findings slightly.

  • It’s OK to multiply point-estimates. They will give the same mean as the mean of the product of two distributions.

  • Dividing by a point-estimate is accurate when the ratio between the interval bounds is low, and performs poorly when the ratio is more than 2. For example:

    • When dividing by a (lognormal, 90% C.I.) distribution where the upper bounds are 1.2 times the lower bounds, the point-estimate approach underestimates by 0.3%

    • When dividing by a (lognormal, 90% C.I.) distribution where the upper bounds are 2 times the lower bounds, the point-estimate approach underestimates by 4.3%

    • When dividing by a (lognormal, 90% C.I.) distribution where the upper bounds are 10 times the lower bounds, the point-estimate approach underestimates by 39%

  • Interval estimates are stronger, but prone to personal bias when evidence is scarce. Deciding between interval and point-estimates is a trade-off between accuracy and accountability.

Normal vs Lognormal modelling

Squiggle uses lognormal distributions by default. Why?

In this section we will find that lognormal distributions are very similar to normal distributions when they share the same, narrow confidence intervals. As the intervals widen the distributions diverge, and the lognormal distribution usually becomes superior. Hence I suggest that using the lognormal distribution by default is the best strategy. I don’t consider other distributions (like the power-law distribution) that may be an ever better fit in some cases.

Turning to the Fuel Price example, we see that the normal/​lognormal choice makes little difference when the ratio between interval bounds is small:

In this case lognormal and normal look very similar, and the distributions give means of 43.885 and 44 respectively.

With the Inhabited Planets example, however, there is a different story. Using 0.5 and 50 as the 5th and 95th percentiles, I get very different-looking distributions:

The means are 13.32 and 25.25 for the lognormal and normal models respectively, and the shapes are very different.

Which is a better match for our understanding of the situation? In my opinion, the lognormal distribution is better. If we expect the number of planets per star to be between 0.5 and 50, the “expected” number of planets should be closer to 13 than to 25. Furthermore, the normal distribution assigns a nontrivial probability to (impossible) negative outcomes.

I think it’s clear that in this case the lognormal distribution is superior. But that’s just a gut feeling. Let’s explore this.

A high ratio between interval bounds implies positive skew

Consider datasets with a high ratio between the 5th and 95th percentiles:

  • The lengths of rivers (often used to exemplify Benford’s law)

  • The populations of cities/​countries

  • Property prices

These all have positively-skewed distributions that could be approximated by the lognormal distribution.

Now consider broadly symmetric datasets:

  • The heights of adult males

  • The durations of pop singles

  • The price of gas in Florida gas stations today

These could probably be modelled with the normal distribution. Notice that in all of these cases, the ratio between the 5th and 95th percentiles will be low. A tall man is perhaps only 20% taller than a short man.

So in general a high ratio between 90% C.I. bounds implies positive skew and is hence better modelled by a lognormal distribution.

This isn’t a rigorous argument, but I suspect that you will struggle to think of examples that buck the trend. I can think of one. It’s possible that a normally-distributed variable could happen to have a small, positive 5th percentile. This would lead to a high ratio between 5th and 95th percentiles: suppose the temperature in my hometown has 5th and 95th percentiles of 0.1°C and 30.0°C respectively. The ratio between the bounds is 300, but the underlying distribution is probably symmetric and best modelled by a normal distribution. Note that the rule of thumb would apply if we measured temperature in Kelvin instead.

General findings: normal vs lognormal

  • The lognormal and normal distributions are similar when the ratio between interval bounds is low. The difference in means is just 3.6% when one bound is 2x the other.

  • The lognormal distribution is usually superior when the ratio between interval bounds is high. These circumstances usually imply negative skew, which make the lognormal distribution a better fit.

  • Although the lognormal is usually better, there are important considerations:

    • The lognormal distribution can only model positive values.

    • If you have reliable estimates of the mean and/​or standard deviation of a distribution, the normal can be easier to model with.

    • Quantities with strict upper bounds (such as probabilities) may not be suitable for the lognormal distribution, although the normal distribution is usually not suitable either in these instances.

    • Not everything is positively-skewed or symmetric. The number of teeth in the next dental patient’s mouth, for example, would likely be positively skewed. But you could model “32 - number of teeth” as lognormal instead.

Creating aggregate estimates

In this section we will find that the “lognormal mean” can outperform the arithmetic mean, but may only be worthwhile in situations of high variability.

All else equal, modelling with distributions is better than using point-estimates. However we often don’t have reliable evidence for the shape of a distribution. This section explores the question: how can we use multiple point-estimates to create reliable aggregate estimates?

In this section I will consider three means:

  • The arithmetic mean

  • The geometric mean

  • The “lognormal mean”: the mean of the lognormal distribution for which x₁, x₂ form an n% confidence interval. The lognormal mean will depend upon the size of this confidence interval.

Choice of mean should depend on the expected underlying distribution

Earlier we saw that estimating underlying distributions (rather than simply working with point-estimates) introduces personal bias. Our choice of mean is linked to our estimate for the shape of the underlying distribution, and unfortunately there is no way around it: each choice of mean makes an implicit assumption about the underlying distribution.

For simplicity, assume we have two sub-estimates which we wish to weight equally.

  • The arithmetic mean finds the mean of a symmetric distribution (such as the normal distribution) with symmetric confidence interval (x₁, x₂)

  • The geometric mean finds the median of any lognormal distribution with symmetric confidence interval (this is always lower th).

  • The lognormal mean finds the mean of a lognormal distribution with symmetric n% confidence interval (x₁, x₂)

The geometric mean is usually better than the arithmetic mean

Interestingly, it hardly matters which mean we use when the ratio between inputs is low.

Suppose, for example, that I have two estimates for the fuel-efficiency of my car.

  • The carmaker’s website claims 50mpg

  • My mechanic, who has experience with older models of my car, claims 40mpg

Type of mean usedResult
Arithmetic45
Geometric44.72
Lognormal, 68% C.I45.004
Lognormal, 90% C.I44.824


The four means differ by less than 1%.

The lognormal mean calculated from a 68% confidence interval is higher than the one calculated from a 90% interval. This is because the former distribution has higher standard deviation and therefore a bigger right tail.

What about when the sub-estimates are further apart? Let’s take two estimates for the number of planets per star in the galaxy: 1 and 10.

Type of mean usedResult
Arithmetic5.5
Geometric3.16
Lognormal, 68% C.I6.18
Lognormal, 90% C.I4.04


The arithmetic mean is now 74% greater than the geometric mean, and the lognormal mean calculated from a 68% confidence interval is nearly double the geometric mean. Once again, it’s the ratio between inputs that matters here. When the ratio is low, the means are close. When the ratio is high, the means diverge.

I built a tool to explore this further. x represents the ratio between the two sub estimates (x₂/​x₁) and p represents the size of the confidence interval used to generate the lognormal mean.

Try moving p towards 1: you will see that the lognormal mean tends to the geometric mean.

So which mean is better when the ratio between inputs is high? In the last section we saw that a high ratio between C.I. bounds implies a positive skew. It follows that a high ratio between sub-estimates also implies a positive skew in the underlying distribution.

  • Clearly the arithmetic mean (which assumes an symmetric underlying distribution) is no good in this scenario.

  • The geometric mean is essentially the lognormal mean formed by a 100% confidence interval. If we have reason to believe x₁, x₂ are extreme outliers (worst- and best-case estimates, say) then this could be a good choice.

  • The lognormal means are viable candidates, but they vary considerably based on the assumed size of the confidence interval used. If we have no objective evidence for the size of the confidence interval, we have to use subjective judgement to decide the size.

  • Of course, the underlying distribution may be neither normal nor lognormal. As uncertainty increases the distribution of the long tails become increasingly influential on the mean. But I won’t explore other tail types here.

In short, it makes sense to assume a lognormal distribution when the ratio between sub-estimates is high, and hence a lognormal mean is a good choice. However this requires a judgement call on the size of the confidence interval represented by x₁, x₂.

If you want a rule of thumb, it may make sense to generate lognormal means from a 90% confidence interval by default. As long as the ratio between sub estimates is under 1000, the lognormal mean will lie roughly midway between the geometric and arithmetic means: a good compromise. The main worry should be that you are ignoring the effects of an undetected fat tail.

Here’s how I would apply the above to my two key examples.

Fuel Cost example:

I have two estimates for the fuel-efficiency of my car.

  • The carmaker’s website claims 50mpg

  • My mechanic, who has experience with older models of my car, claims 40mph

It seems reasonable that these estimates represent best- and worst-case estimates for the true fuel efficiency of my car, so I suspect the geometric mean (or, similarly, lognormal mean using 99% C.I of (40,50)) will be most accurate. However, since the ratio between estimates is low, I opt for the simpler arithmetic mean, 45.

Inhabitable Planets example:

An astronomy paper claims that “stars in our galaxy probably have on average 1 to 10 planets each”.

The source gives no confidence intervals, but I choose to interpret “probably” as 90% confidence, and hence use a 90% confidence interval to generate a lognormal mean of 4.04 planets per star.

Weighted means

Sometimes we have multiple point-estimates and varying levels of confidence in each one. So we use a weighted mean to build an aggregate estimate.

The thought of weighted lognormal means is exploding my brain at the moment, so I will stick to weighted arithmetic and geometric means, which are very straightforward.

We apply weights to our sub-estimates to build an arithmetic weighted mean:

where ,

The equivalent for the geometric mean is

where ,

As with the unweighted means, the weighted arithmetic and geometric means are close when the ratios between estimates are low. The graph shows the two-estimate example, where the x-value is the ratio between the sub-estimates:

Again, I would argue that the geometric mean is generally superior. When the sub-estimates are close it hardly matters, and when they are far apart the geometric mean better captures the positive skew in the underlying distribution.

General findings: aggregate estimates

  • When the ratio between the inputs is <3, the arithmetic, geometric and lognormal means are similar. Since the arithmetic mean is more widely understood, it may be a better choice when the ratio between inputs is low.

  • As the ratio between inputs grows, the means diverge. The high ratio suggests underlying positive skew, which makes the arithmetic mean unreliable. A judgement call is needed to estimate the size of the confidence interval represented by our inputs, which introduces subjectivity. One way to avoid this is to state in advance that you will use 90% lognormal means in place of unweighted arithmetic means of two values.

  • The geometric mean can be thought of as the mean of a lognormal distribution for which the inputs form extreme outer limits

  • We have not explored how to apply the lognormal mean in situations with three or more inputs, or with weighting

Conclusion: complexity vs legibility

We have seen a common theme throughout: simple methods show high fidelity in situations of low variability (as measured by the ratio between confidence interval bounds or of sub-estimates).

So I would make the following suggestion: If your work is for public scrutiny, needs to avoid subjectivity or is time-sensitive, only use the more complex methods when it makes a significant difference.

  • Point estimates are fine if your final calculation is not too long and the ratio between 90% confidence interval bounds is less than 2 (or if you don’t need to divide by an unknown and you don’t care about the “shape” of your answer).

  • The normal distribution is easier to understand than lognormal, so favour it when the ratio between confidence interval bounds is low

  • The arithmetic mean is widely understood, so use it as long as most of the inputs vary by less than a factor of 2

On the other hand, simple methods can lead to spurious results in situations of super-high variability. For example, estimates for the incidence of intelligent life in the galaxy (a high variability, multi-stage calculation) vary wildly depending on the complexity of the methods used.

Thanks to the makers of Squiggle, which has made working with more complex models much faster.

Changes

  • [23 Mar] Amended point-estimate section to reflect that multiplication is fine with point estimates, while division introduces error. Changed summaries accordingly. Thanks to @Thomas Sepulchre (LessWrong) for the comment.

  • [27 Mar] Corrected errors on Squiggle graphs that compare similar lognormal/​normal distributions—I had been using the wrong standard deviations for the normal distributions before.

  • [1 Apr] Brought work on the lognormal mean into the post and ceased to interpret its sensitivity to heavy right-tails as a sign of unreliability. Added more on the pros and cons of using interval estimates as inputs and outputs. Thanks to @Vasco Grilo for feedback.

  • [3 Apr] Re-wrote the section “Should we always use interval estimates?” to separate the question of using interval estimates for inputs vs outputs, and to add examples.