Team Scoring Shots and Conversion Rates

In response to my earlier post on the explained and unexplained portions of game margins, Friend of MatterOfStats, Michael, e-mailed me to suggest that variability in teams' points-scoring per scoring shot - or, equivalently, teams' conversion rates - might usefully be explored as a source of unexplained variability. 

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Explaining Variability in Game Margins

Some seasons are notable for the large number of blowout victories they force us to endure - a few recent seasons come immediately to mind - while others are more memorable because of their highly competitive nature. To what extent, I've often wondered, could we attribute a season full of sizable victory margins to the fact that strong teams were more often facing weak teams, making the magnitude of the defeats predictable if still lamentable, versus instead attributing them to on-the-day or random events that were genuinely unforeseeable pre-game?

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Home Team and Away Team Scores Across VFL/AFL History

About 18 months ago I investigated the statistical properties of home teams' and away teams' scoring behaviour over the period from the start of the 2006 season to the middle of the 2012 season taken as a whole. In that blog, using the VGAM package, I found that the Normal distribution provided a reasonable fit to the scores of Home teams and a much better fit to the scores of Away teams over that entire period.

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A Comparison of SOGR & VSRS Ratings

Earlier posts on the Very Simple Rating System (VSRS) and Set of Games Ratings (SOGR) included a range of attractive graphs depicting team performance within and across seasons.

But, I wondered: how do the two Systems compare in terms of the team ratings they provide and the accuracy with which game outcomes can be modelled using them, and what do any differences suggest about changes in team performance within and across seasons?

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Set of Games Ratings: All Teams' Charts

The Set of Games Ratings post from late December introduced a twist on Tony’s VSRS concept. For any given set of games, the SOGR approach produces a rating for each team indicating its relative scoring ability within those games. Each SOGR model is optimised for the set of games on which it was fitted (in the least squares sense).

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The Dynamics of ChiPS Ratings: 2000 to 2013

Visitors to the MatterOfStats site in 2014 will be reading about ChiPS team Ratings and the new Margin Predictor and Probability Predictor that are based on them, which I introduced in this previous blog. I'll not be abandoning my other team Ratings System, MARS, since its Ratings have proven to be so statistically valuable over the years as inputs to Fund algorithms and various Predictors, but I will be comparing and contrasting the MARS and the ChiPS Ratings at various times during the season.

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Introducing ChiPS

In years past, the MAFL Fund, Tipping and Prediction algorithms have undergone significant revision during the off-season, partly in reaction to their poor performances but partly also because of my fascination - some might call it obsession - with the empirical testing of new-to-me analytic and modelling techniques. Whilst that's been enjoyable for me, I imagine that it's made MAFL frustrating and difficult to follow at times.

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Set of Games Ratings: A Comparison With VSRS

A few weeks back, Tony introduced the Very Simple Rating System (VSRS). It’s an ELO-style rating system applied to the teams in the AFL, designed so that the difference in the ratings between any pair of teams plus some home ground advantage (HGA) can be interpreted as the expected difference in scores for a game involving those two teams played at a neutral venue. Tony's explored a number of variants of the basic VSRS approach across a number of blogs, but I'll be focussing here on the version he created in that first blog.

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Is That a Good Probability Score - the Brier Score Edition

In recent blogs about the Very Simple Ratings System (VSRS) I've been using as my Probability Score metric the Brier Score, which assigns scores to probability estimates on the following basis:

Brier Score = (Actual Result - Probability Assigned to Actual Result)^2

For the purposes of calculating this score the Actual Result is treated as (0,1) variable, taking on a value of 1 if the team in question wins, and a value of zero if that team, instead, loses. Lower values of the Brier Score, which can be achieved by attaching large probabilities to teams that win or, equivalently, small probabilities to teams that lose, reflect better probability estimates.

Elsewhere in MAFL I've most commonly used, rather than the Brier Score, a variant of the Log Probability Score (LPS) in which a probability assessment is scored using the following equation:

Log Probability Score = 1 + logbase2(Probability Associated with Winning team)

In contrast with the Brier Score, higher log probabilities are associated with better probability estimates.

Both the Brier Score and the Log Probability Score metrics are what are called Proper Scoring Rules, and my preference for the LPS has been largely a matter of taste rather than of empirical evidence of superior efficacy.

Because the LPS has been MAFL's probability score of choice for so long, however, I have previously written a blog about empirically assessing the relative merits of a predictor's season-average LPS result in the context of the profile of pre-game probabilities that prevailed in the season under review. Such context is important because the average LPS that a well-calibrated predictor can be expected to achieve depends on the proportion of evenly-matched and highly-mismatched games in that season. (For the maths on this please refer to that earlier blog.)

WHAT'S A GOOD BRIER SCORE?

What I've not done previously is provide similar, normative data about the Brier Score. That's what this blog will address.

Adopting a methodology similar to that used in the earlier blog establishing the LPS norms, for this blog I've: 

  • Calculated the implicit bookmaker probabilities (using the Risk-Equalising approach) for all games in the 2006 to 2013 period
  • Assumed that the predictor to be simulated assigns probabilities to games as if making a random selection from a Normal distribution with mean equal to the true probability - as assessed in the step above - plus some bias between -10% and +10% points, and with some standard deviation (sigma) in the range 1% to 10% points. Probability assessments that fall outside the (0.01, 0.99) range are clipped. Better tipsters are those with smaller (in absolute terms) bias and smaller sigma.
  • For each of the simulated (bias, sigma) pairs, simulated 1,000 seasons with the true probabilities for every game drawn from the empirical implicit bookmaker probabilities for a specific season.

Before I reveal the results for the first set of simulations let me first report on the season-by-season profile of implicit bookmaker probabilities, based on my TAB Sportsbet data.

The black bars reflect the number of games for which the home team's implicit home team probability fell into the bin-range recorded in the x-axis, and the blue lines map out the smoothed probability density of that same data. These blue lines highlight the similarity in terms of the profile of home team probabilities of the last three seasons. In these three years we've seen quite high numbers of short-priced (ie high probability) home team favourites and few - though not as few as in some other years - long-shot home teams. 

Seasons 2008, 2009 and 2010 saw a more even spread of home team probabilities and fewer extremes of probability at either end, though home team favourites still comfortably outnumbered home team underdogs. Seasons 2006 and 2007 were different again, with 2006 exhibiting some similarities to the 2008 to 2010 period, but with 2007 standing alone as a season with a much larger proportion of contests pitting relatively evenly-matched tips. That characteristic makes prediction more difficult, which we'd expect to be reflected in expected probability scores.

So, with a view to assessing the typical range of Brier Scores under the most diverse sets of conditions, I ran the simulation steps described above once using the home team probability distribution from 2013, and once using the distribution from 2007.

THE BRIER SCORE RESULTS

Here, firstly, are the results for all (bias, sigma) pairs, each simulated for 1,000 seasons that look like 2013.

As we'd expect, the best average Brier Scores are achieved by a tipster with zero bias and the minimum, 1% standard deviation. Such a tipster could expect to achieve an average Brier Score of about 0.167 in seasons like 2013.

For a given standard deviation, the further is the bias from zero the poorer (higher) the expected Brier Score and, for a given bias, the larger the standard deviation the poorer the expected Brier Score as well. So, for example, we can see from the graph that an unbiased tipster with a 5% point standard deviation should expect to record an average Brier Score of about 0.175.

Using Eureqa to fit an equation to the Brier Score data for all 210 simulated (bias, sigma) pairs produces the following approximation:

Expected Brier Score = 0.168 + 0.89 x Bias^2 + 0.87 x Sigma^2

This equation, which explains 98% of the variability in the average Brier Scores across the 210 combinations, suggests that the Brier Score of a tipster is about equally harmed by equivalent changes in percentage point terms in bias and variance (ie sigma squared). Every 1% point change in squared bias or in variance adds about 0.09 to the expected Brier Score.

Next, we simulate Brier Score outcomes for seasons that look like 2007 and obtain the following picture:

The general shape of the relationships shown here are virtually identical to those we saw when using the 2013 data, but the expected Brier Score values are significantly higher.

Now, an unbiased tipster with a 1% point standard deviation can expect to register a Brier Score of about 0.210 per game (up from 0.167), while one with a 5% point standard deviation can expect to return a Brier Score of about 0.212 (up from 0.175).

Eureqa now offers the following equation to explain the results for the 210 (bias, sigma) pairs:

Expected Brier Score = 0.210 + 0.98 x Bias^2 + 0.94 x Sigma^2

This equation explains 99% of the variability in average Brier Scores across the 210 combinations and, when compared with the earlier equation, suggests that: 

  • A perfect tipster - that is one with zero bias and zero variance - would achieve a Brier Score of about 0.210 in seasons like 2007 and of 0.168 in seasons like 2013
  • Additional bias and variability in a tipster's predictions are punished more in absolute terms in seasons like 2007 than in seasons like 2013. This is evidenced by the larger coefficients on the bias and variance terms in the equation for 2007 compared to those for 2013.

In seasons in which probability estimation is harder - that is, in seasons full of contests pitting evenly-matched teams against one another - Brier Scores will tend to do a better job of differentiating weak from strong predictors. 

THE LPS RESULTS

Though I have performed simulations to determine empirical norms for the LPS metric before, I included this metric in the current round of simulations as well. Electrons are cheap.

Here are the curves for simulations of LPS for the 2013-like seasons.

Eureqa suggests that the relationship between expected LPS, bias and variance is, like that between Brier Score, bias and variance, quadratic in nature, though here the curves are concave rather than convex. We get:

Expected LPS = 0.271 - 4.68 x Bias^2 - 4.71 x Sigma^2

This equation explains 99% of the variability in average LPSs observed across the 210 combinations of bias and sigma.

Finally, simulating using 2007-like seasons gives us this picture.

Again we find that the shape when using the 2007 data is the same as that when using the 2013 data, but the absolute scores are poorer (which here means lower).

Eureqa now offers up this equation:

Expected LPS = 0.127 - 4.17 x Bias^2 - 4.35 x Sigma^2

This equation accounts for 97% of the total variability in average LPS across the 210 simulated pairs of bias and sigma and suggests that expected LPSs in seasons like 2007 are less sensitive to changes in bias and variance than are expected LPSs in seasons like 2013. This is contrary to the result we found for expected Brier Scores, which were more sensitive to changes in bias and variance in seasons like 2007 than in seasons like 2013.

In more challenging predictive environments, therefore, differences in predictive ability as measured by different biases and variances, are likely to result in larger absolute differences in Brier Scores than differences in LPSs.

SUMMARY AND CONCLUSION

We now have some bases on which to make normative judgements about Brier Scores and Log Probability Scores, though these judgements require some knowledge about the underlying distribution of true home team probabilities.

If 2014 is similar to the three seasons that have preceded it then a "good" probability predictor should produce an average Brier Score of about 0.170 to 0.175, and an average LPS of about 0.230 to 0.260. In 2013, the three bookmaker-derived Probability Predictors all finished the season with average LPS' of about 0.260.

[EDIT : It's actually not difficult to derive the following relationship theoretically for a forecaster whose predictions are 0 or 1 with fixed probability and independent of the actual outcome

Expected Brier Score = True Home Probability x (1 - True Home Probability) + Bias^2 + Sigma^2

The proof appears in the image at left.

(Click on the image for a larger version.)

Now the fitted equations for Expected Brier Scores above have coefficients on Bias and Sigma that are less than 1 mostly due, I think, to the effects of probability truncation, which tend to improve (ie lower) Brier Scores for extreme probabilities. There might also be some contribution from the fact that I've modelled the forecasts using a Normal rather than a Binomial distribution.

Deriving a similar equation theoretically rather than empirically for the Expected LPS of a contest is a far more complicated endeavour ...]

Estimating Team-and-Venue Specific Home Ground Advantage Using the VSRS

In the Very Simple Rating System as I've described it so far, a single parameter, HGA, is used to adjust the expected game margin to account for the well-documented advantages of playing at home. We found that, depending on the timeframe we consider and the performance metric that we chose to optimise, the estimated size of this advantage varied generally in the 6 to 8-point range.
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Optimising the Very Simple Rating System (VSRS)

In the previous blog, introducing the VSRS, I provided optimal values for the tuning parameters of that System, optimal in the sense that they minimised either the mean absolute or the mean squared error across the period 1999 to 2013
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A Very Simple Team Ratings System

Just this week, 23 year-old chess phenom Magnus Carlsen wrested the title of World Champion from Vishwathan Anand, in so doing lifting his Rating to a stratospheric 2,870. Chess, like MAFL, uses an an ELO-style Rating System to assess and update the strength of its players.
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Estimating Home Ground Advantage by Venue

In the previous blog I fitted models to the game margins of each team separately, seeking to explain the margin in any game in terms of the Venue at which the game was played and three "Excess" variables summarising from the designated home team's perspective its relative Venue Experience, MARS Rating and recent form.
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What's More Important: Who You Play or Where You Play Them?

The benefits of playing at home have been extensively investigated both here on MAFL for Australian Rules football and more generally within the sports prediction community for this and other sports. Put simply, teams that play at home win more often and score more points than you'd otherwise expect them to after adjusting for the quality of the opponents they face.
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Revisiting Home Ground Advantage

This week I've been part of a Twitter conversation about Home Ground Advantage in the AFL, a trending topic because of the shift from Football Park to Adelaide Oval for the home games of Adelaide and Port Adelaide in the 2014 season.
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MARS Rating Changes and Scoring Percentages: 1897-2013

The idea for this blog sprang from some correspondence with Friend of MAFL, Michael, so let me start by thanking him for being the inspiration. Michael was interested in exploring the relationship between team performances and the resulting change in their MARS Ratings across a season, which I'll explore here by charting, for each team and every season, the for-and-against percentage they achieved in all games including Finals, and the change in their MARS Rating per game during that same season.
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Another View of All-Time AFL Team MARS Ratings Post the 2013 Season

Recently I'd been noticing some traffic to the site from the Big Footy website where the Forum members had been discussing the relative strengths of Bulldogs teams across VFL/AFL history. That, coupled with my continuing desire to become more proficient in the ggplot2 R package of Hadley Wickham, dragged me out of my off-season blog malaise to perform the analyses underpinning this current posting.
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Building Your Own Team Rating System

Just before the 2nd Round of 2008 I created MAFL's Team Ratings System, MARS, never suspecting that I'd still be writing about it 5 years later. At the time, I described MARS in the newsletter for that week in a document still available from the Newsletters 2005-2008 section section of this website (it's linked under the "MAFL The Early Years" menu item in the navigation bar on the right of screen). Since then, MARS, as much to my surprise as I think to anyone's, has been a key input to the Line Funds that have operated in each of the ensuing years.
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How Good Are Hawthorn, How Poor GWS?

Without the benefit of emotional and chronological distance it's often difficult to rate the historical merit of recent sporting performances. MAFL's MARS Ratings, whilst by no means the definitive measure of a team's worth, provides one, objective basis on which to assess the teams that ran around in 2013.
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