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Allen Cring Productions in association with Emergent Light Studio presents...

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The Illinois State Collegiate Compendium, academic lectures in Business and Economics.

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This is Business Finance FIL-194, spring semester 2024.

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Today, risk and return.

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Now, the complicated part of this is not that complicated,

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but it does call you to do some things,

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and I would certainly expect you to do this in Excel.

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I don't even care to do it myself by hand

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because it can be tedious sometimes.

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But it is, it's not terribly complicated in Excel,

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but there is a caution that I have to give you

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when I do it in Excel.

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But before we do that, let me do a quick look at the numbers

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here.

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Yahoo.

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And as you can see, that is about as lackluster

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as a market can get.

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It's just like sitting there looking stupid.

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The Dow is flat right now.

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And then the S&P 500 is pretty much the same.

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And then the NASDAQ, a little bit of bias to the downside,

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tiny, tiny bit.

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But they all came, started out,

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kind of dropped real fast right on the opening bell.

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And well, this one didn't.

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But then it's been struggling to come back up,

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but there is a lot of volatility right now.

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The volatility is quite noticeable, at least visually.

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Now, however, very quickly, let me look at the VIX

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to see what the vol is on the VIX real quick.

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That's not much.

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Yeah, see the volatility early this morning really spiked.

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And it's dropped off really a lot

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in just the last couple of minutes.

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And I don't know what that's all about.

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So we'll have to see how that goes from here.

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But anyway, let me get back to the main show here.

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And crude oil still in its band now.

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About 81, I'd say, up to 88, is where I'm seeing it right now.

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And it's staying in that band.

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And as I said, that's going to lead to higher gas prices.

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And you're seeing them at the gas pump right now, 379 locally,

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379, 369.

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But where it's going to go, you notice that it has been tailing

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off through the day.

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But that drop isn't all that noticeable.

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It did fall well.

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I shouldn't say that.

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Because since last night, now remember,

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oil commodities markets don't trade like stock markets do.

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They have different time frames.

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And it looks like it was up there rather noticeably

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last night.

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And it's been tailing downward ever since.

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And that is a lot to do with the,

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we know there's a lot of supply.

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The supply chain is full at the sources, on the high seas,

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at the refineries.

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So the cause of that higher price that's

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been there for the last week or so

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is mostly expectations of something

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that the market thought was going to happen.

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And now that expectation seems to be draining out

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a little bit.

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But again, you have to always remember that in our markets,

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expectations are everything.

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Gold, it's just all over the place.

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It's just really volatile right now.

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It's spiked up.

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But it still seems to, right now, it doesn't really

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want to find out much about $2,200 an ounce.

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It's keeping down a little bit more.

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Silver, quieter, of course.

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Now the 10-year bond, we do have at least a modest,

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a tiny 4 tenths of a basis point easing off.

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But it's really, for the most part,

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that's just really quiet, 0.09%.

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So the bond market is just sort of sitting there pretty much

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flat, like the equities are.

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So the market overall is just sitting back

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and waiting to see what's going to happen next.

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Running over here just very quickly, the Nikkei,

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it started down.

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And then it climbed up in the last half of the trading

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last night over in Tokyo.

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But it did manage to get kind of a respectable 2 thirds

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of a percent out of its day.

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And when we came over to London, they started out down

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and then groveled back.

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They're still trading.

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And now they're back in positive territory too.

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And if we look back over here at the equity side of it,

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well, there you go.

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We're just sitting there looking,

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not really knowing what to do next.

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It's a really quiet day.

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I don't see anything exciting coming along.

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Yeah, but it's just going to be one of those days

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where there's nothing going on.

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Very quickly, let me show you.

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And I'm just going to, well, that was brilliant.

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I'm just going to pull up a stock out of thin air

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for a little bit here.

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I don't know.

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General, let me look at General Mills, something quiet.

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And I have a specific purpose here.

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General Mills, General Motors, I'd rather look at something

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a little bit calmer.

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What in the heck?

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Come on.

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Why am I having difficulties here?

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Oh, I put it in the wrong place.

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General Mills.

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GM.

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General Mills.

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I didn't think that was as simple, but I guess there it is.

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OK.

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Really came off of, today, it really came out good.

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Strong, strong opening.

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And it's been sliding off since then.

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There's some profit taking going on since the opening bell.

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But man, it's really been a decent day on there.

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And I've gone through the numbers before,

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and I'm hopeful that you know how to look at those numbers

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now.

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The one I want to focus on right here, right now,

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is this guy right here, Beta.

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And as I've said before, in finance,

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this is our go-to measure of risk.

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Now, we do have other measures of risk.

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The standard deviation of returns is a measure.

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And everything is on returns.

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These are price metrics.

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These are returns metrics.

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So you're taking this Beta is a measure

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of the volatility of the returns.

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Now, we can talk about, pretend it's the volatility of the price,

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because the price is related to the returns.

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But technically speaking, where we have to be now in the course

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is volatility of returns.

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And this is our go-to.

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It is not just the standard deviation.

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And I'll get into that in just a few minutes here,

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what I mean by that.

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But for the time being, just understand

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that this is different.

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Now, we've got to understand that.

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This is different.

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Now, we do have some other ones.

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The standard deviation is a measure of risk.

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The Beta is a measure of risk, too.

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And there's another one here, too, the Sharpe ratio.

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And there are different books have different letters for that.

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I'll just write it as SR, the Sharpe ratio.

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It is a measure.

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And it's a very popular measure in mutual funds.

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I mean, I'm not sure where that came from.

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It's mostly historical, because mutual funds have a Beta.

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And I look at the Beta.

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But I swear, whenever you're looking at mutual funds,

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as you notice with GM here, Sharpe ratio is nowhere.

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But if you're looking at a mutual fund,

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all the Sharpe ratio is going to show.

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And I hope you'll see why it's not a really great measure.

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But it is popular in that niche market of mutual funds.

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Whatever.

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Now, there's one other one that I would bring up here, too,

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the coefficient of variation, the CV.

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Now, this is where I never can remember.

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Did you take the statistics course yet,

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the management course?

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I can't remember.

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I think it's 150 or something like that.

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Have you had that course yet?

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OK.

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It's OK, because I'm going to teach it a lot better

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than they would anyway, because I'm

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going to focus on what these things mean to us in our work.

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And I do use Excel like a boss.

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I do not use the formulas, because the formulas

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can get to be a lot like work.

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And it's not that they're hard, complex.

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But man, you just have to keep calculating over,

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adding and taking differences, then squaring them,

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then weighting it by the probability,

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and then going on to the next one,

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and then adding all of those up, then taking

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the square root of it.

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That's way too much like accounting work to me.

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So we take Excel very seriously.

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And all these we can calculate with Excel.

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One caution, and then I'll get off this subject,

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because it's so important that it's not something

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that I want to talk a whole lot about.

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A lot of times, we will calculate

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these with historical data.

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And that's not what we should be doing.

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We should be calculating it with future data,

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or future expected data.

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And that gets into the kind of obvious question,

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how the hell do you do that?

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If we haven't had the future yet, how do you get it?

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The typical way that we do that, we

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do an adjustment from history to the future.

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How far do I want to take this?

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OK.

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We do it actually the way we taught artificial intelligence

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systems to do a lot of things that they

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do in modeling and data analysis.

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What we'll do is we will take, let's say, a year of data.

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And we will get the expected, we'll get, say,

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the average of that.

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And then what we'll do is we'll go up, say, two months.

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And we'll take data that, let me do it this way.

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We've got a vector of data, a historical vector of data.

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We'll take this, OK?

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And we'll get the average of this data.

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This is just one of the metrics.

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Let's say the average of the returns.

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And we put an R bar.

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That's for an average.

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And then we will say, OK, let's take this last data.

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This is the simulated history.

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And then we will pretend that this was the future data,

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R capital F, I better put, because it

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looks like a risk-free rate.

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And then we'll look at how much the historical data deviated

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from this quote unquote future data.

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It was all historical, of course,

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but we're going to pretend that this was future data.

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And we'll see how much different this future

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was than what we thought it would

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be from the historical data.

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And then that will be our adjustment

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for all of the historical data.

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Ouch.

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That difference tells us how much different the history

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is from what happens next.

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And that's a simple way of doing it.

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We have much more complex ways, but honestly, they all

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kind of boil down to this.

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And that way, we can get an estimate

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of how much another data set.

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So in other words, we would now take a whole set of data

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and get its historical.

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And we say that up here, it would be R bar

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plus this adjustment figure.

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That's how we would get a future expected value.

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This is done all the time.

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So when I talk about these metrics over there,

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we are doing historical.

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We're not going to do that adjustment.

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But that's how you would do an adjustment

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so that you're looking at the expected future standard

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deviation.

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The expected future beta.

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It would be the historical with that adjustment factor

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added in or subtracted from.

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OK.

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Now let me get down to some brass tacks here on this.

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I'm going to pull up.

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And I'm actually just going to pull up some live data for us

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to use to actually do these calculations here.

264
00:15:32,020 --> 00:15:42,900
But before I do that, a little bit of notation here

265
00:15:42,900 --> 00:15:44,420
and terminology.

266
00:15:50,020 --> 00:15:54,460
The book is using a term that has come up

267
00:15:54,460 --> 00:15:57,380
as the way to describe it.

268
00:15:57,380 --> 00:16:00,260
But it hasn't been around for all that many years.

269
00:16:00,260 --> 00:16:02,660
But it seems to be pretty popular.

270
00:16:02,660 --> 00:16:09,100
Distinguishing between standalone risk and portfolio

271
00:16:09,100 --> 00:16:09,600
risk.

272
00:16:12,660 --> 00:16:14,300
And there's even another one too.

273
00:16:14,300 --> 00:16:22,580
But unfortunately, this edition of the book takes that out.

274
00:16:32,460 --> 00:16:34,660
But before we talk too much about these,

275
00:16:34,660 --> 00:16:39,500
we have to talk about standalone with an E.

276
00:16:39,500 --> 00:16:42,100
We have to talk about risk.

277
00:16:42,100 --> 00:16:47,540
Risk is the variability of possible outcomes.

278
00:16:47,540 --> 00:16:53,540
If there is only one possible outcome, there's no risk.

279
00:16:53,540 --> 00:16:57,460
If there is more than one possible outcome,

280
00:16:57,460 --> 00:17:00,540
then there is risk.

281
00:17:00,540 --> 00:17:03,540
Now it's not just how many outcomes.

282
00:17:03,540 --> 00:17:09,540
It's how much those outcomes can be different from one another.

283
00:17:09,540 --> 00:17:10,940
That's the next step.

284
00:17:10,940 --> 00:17:21,860
So in other words, there is the how many outcomes.

285
00:17:28,860 --> 00:17:30,220
That's the big one first.

286
00:17:35,620 --> 00:17:37,500
Oh, that didn't work.

287
00:17:37,500 --> 00:17:48,140
The next one would be how different

288
00:17:48,140 --> 00:17:49,900
are the possible outcomes.

289
00:17:49,900 --> 00:18:03,660
That's the next one.

290
00:18:03,660 --> 00:18:20,980
Then the next one is how, for lack of a better word,

291
00:18:20,980 --> 00:18:44,540
how clustered are the possible outcomes.

292
00:18:44,540 --> 00:18:51,420
So in other words, you have 100 different possible outcomes.

293
00:18:51,420 --> 00:18:52,820
Well, that's noticeable right there.

294
00:18:52,820 --> 00:18:53,540
That's important.

295
00:18:53,540 --> 00:18:58,700
But what if all of them are really close to each other,

296
00:18:58,700 --> 00:19:00,980
the outcomes are?

297
00:19:00,980 --> 00:19:04,620
Then that's not a very risky situation compared to one

298
00:19:04,620 --> 00:19:09,020
where the outcomes are quite different.

299
00:19:09,020 --> 00:19:12,940
And then one last one that I will somewhat explore,

300
00:19:12,940 --> 00:19:16,500
and I will show you something.

301
00:19:16,500 --> 00:19:18,900
You haven't had a management course,

302
00:19:18,900 --> 00:19:20,660
so I don't want to get into it too much.

303
00:19:20,660 --> 00:19:25,140
But I will show you in Excel how you can calculate it.

304
00:19:25,140 --> 00:19:26,460
There are a couple of other ones.

305
00:19:26,460 --> 00:19:28,540
One that's kind of important to me

306
00:19:28,540 --> 00:19:37,540
is how biased is the clustering.

307
00:19:37,540 --> 00:19:44,140
And by that I mean you might have 100 possible outcomes.

308
00:19:44,140 --> 00:19:46,420
95 of them are very close.

309
00:19:46,420 --> 00:19:51,380
But then you have a tail that is on one side,

310
00:19:51,380 --> 00:19:55,820
a tail of potential outcomes.

311
00:19:55,820 --> 00:19:59,940
That would be important too, because there

312
00:19:59,940 --> 00:20:02,460
is this typical assumption we make.

313
00:20:02,460 --> 00:20:05,020
And that is that the outcome is not

314
00:20:05,020 --> 00:20:07,700
as good as the outcome of the other.

315
00:20:07,700 --> 00:20:10,340
There is this typical assumption we make.

316
00:20:10,340 --> 00:20:12,700
And it's actually not as good.

317
00:20:12,700 --> 00:20:17,140
It's used all of the time that outcomes

318
00:20:17,140 --> 00:20:21,980
are distributed normally.

319
00:20:21,980 --> 00:20:27,740
They are the bell curve, the famous bell curve.

320
00:20:27,740 --> 00:20:32,620
Now there is a law of mathematics

321
00:20:32,620 --> 00:20:40,060
that says that if you make a bell curve with a single data,

322
00:20:40,060 --> 00:20:45,460
it will begin to behave like this bell curve,

323
00:20:45,460 --> 00:20:49,420
what we call the normal curve.

324
00:20:49,420 --> 00:20:51,660
That's great.

325
00:20:51,660 --> 00:20:54,580
However, the reality is that there

326
00:20:54,580 --> 00:21:00,180
is some data that just you cannot make that assumption.

327
00:21:00,180 --> 00:21:02,740
Is we always, well, it's a bell curve.

328
00:21:02,740 --> 00:21:04,500
Your average is 75%.

329
00:21:04,500 --> 00:21:06,260
And it's a bell curve and all that.

330
00:21:06,260 --> 00:21:09,660
Because there are all these mathematical simplifications

331
00:21:09,660 --> 00:21:13,100
we can make, very cool things you can do with a normal curve.

332
00:21:13,100 --> 00:21:14,980
So we hope that it is normal.

333
00:21:14,980 --> 00:21:17,020
And even if it's not, we pretend it's normal.

334
00:21:17,020 --> 00:21:21,220
But I can tell you right now, there's a problem with it.

335
00:21:21,220 --> 00:21:25,860
Well, in education, there's a great problem with it.

336
00:21:25,860 --> 00:21:34,740
You see, if the average of an exam is 75%,

337
00:21:34,740 --> 00:21:36,860
that's our ideal, perfect 75%.

338
00:21:36,860 --> 00:21:38,100
Of course, you screwed that up.

339
00:21:38,100 --> 00:21:39,740
You got an 80%.

340
00:21:39,740 --> 00:21:46,900
But the problem is that, OK, the highest score possible

341
00:21:46,900 --> 00:21:49,500
would be 100%.

342
00:21:49,500 --> 00:21:52,900
The lowest score possible would be a 0.

343
00:21:52,900 --> 00:21:56,820
So do you see that there would be a tail down here

344
00:21:56,820 --> 00:21:59,220
of scores that would not be matched

345
00:21:59,220 --> 00:22:02,820
by a tail of the same distance from the average

346
00:22:02,820 --> 00:22:04,940
on the outside?

347
00:22:04,940 --> 00:22:08,660
In other words, I could have an outcome on the outside no more

348
00:22:08,660 --> 00:22:12,940
than 25 points above the average.

349
00:22:12,940 --> 00:22:20,340
But I could have a test score that was 75% 75 points

350
00:22:20,340 --> 00:22:23,060
below the average.

351
00:22:23,060 --> 00:22:26,700
So we could get a 0 or a 5 or something like that.

352
00:22:26,700 --> 00:22:31,820
So in other words, the assumption of a bell curve

353
00:22:31,820 --> 00:22:34,460
is invalid.

354
00:22:34,460 --> 00:22:39,660
The same, unfortunately, is true of stock returns.

355
00:22:42,860 --> 00:22:46,540
And it's actually, OK.

356
00:22:46,540 --> 00:22:50,660
In other words, stock returns, we assume

357
00:22:50,660 --> 00:22:54,020
that there is an expected return to a stock.

358
00:22:54,020 --> 00:22:57,620
And we would assume that it could possibly deviate

359
00:22:57,620 --> 00:22:59,060
from that on either side.

360
00:23:02,660 --> 00:23:05,300
So it would be a normal distribution.

361
00:23:05,300 --> 00:23:08,500
And we use all of these cool little metric tricks

362
00:23:08,500 --> 00:23:12,220
for finding the mean, the standard deviation,

363
00:23:12,220 --> 00:23:13,700
all that kind of cool stuff.

364
00:23:13,700 --> 00:23:17,140
Unfortunately, we know for a fact

365
00:23:17,140 --> 00:23:21,140
that it is not a normal curve.

366
00:23:21,140 --> 00:23:27,860
In fact, it has a very, at first glance,

367
00:23:27,860 --> 00:23:31,500
stock returns do behave, look like a normal.

368
00:23:31,500 --> 00:23:35,580
But if you look a little more carefully

369
00:23:35,580 --> 00:23:43,660
over a long period of data, historical data,

370
00:23:43,660 --> 00:24:02,780
it looks actually like this.

371
00:24:02,780 --> 00:24:05,980
The first thing that it is biased upward.

372
00:24:05,980 --> 00:24:10,020
We know that stock markets, stocks in general,

373
00:24:10,020 --> 00:24:14,460
their returns are biased upward.

374
00:24:14,460 --> 00:24:17,260
In other words, over a long period of time,

375
00:24:17,260 --> 00:24:21,620
returns are positive.

376
00:24:21,620 --> 00:24:28,700
The second thing is these two little bastards right here.

377
00:24:28,700 --> 00:24:32,540
A normal distribution has very thin tails.

378
00:24:32,540 --> 00:24:35,900
After the clumping, in a normal distribution,

379
00:24:35,900 --> 00:24:40,900
67% of the returns are between one standard deviation above

380
00:24:40,900 --> 00:24:42,780
and one standard deviation below.

381
00:24:42,780 --> 00:24:44,540
95% are here.

382
00:24:44,540 --> 00:24:45,940
99% are here.

383
00:24:45,940 --> 00:24:47,380
That's normal.

384
00:24:47,380 --> 00:24:53,260
Unfortunately, we have what are called black swans

385
00:24:53,260 --> 00:24:54,020
and white swans.

386
00:24:57,140 --> 00:25:03,620
In certain periods of time, you can have too many black swans.

387
00:25:03,620 --> 00:25:09,100
In other times, we can have too many white swans.

388
00:25:09,100 --> 00:25:13,980
The normal distribution would say it's a very unusual event.

389
00:25:13,980 --> 00:25:17,060
To give you an idea, once in 100 years,

390
00:25:17,060 --> 00:25:20,140
you would have a black swan if returns are normally

391
00:25:20,140 --> 00:25:21,980
distributed.

392
00:25:21,980 --> 00:25:29,020
We have so far had seven black swans in the last century.

393
00:25:29,020 --> 00:25:32,540
We've had three white swans.

394
00:25:32,540 --> 00:25:34,220
There should be one of each on each side

395
00:25:34,220 --> 00:25:36,220
if it's normally distributed.

396
00:25:36,220 --> 00:25:39,420
So unfortunately, it's not normally distributed.

397
00:25:39,420 --> 00:25:42,540
In fact, we even know what that one is.

398
00:25:42,540 --> 00:25:46,260
The mathematics of probability theory is very old

399
00:25:46,260 --> 00:25:47,500
and it's very complete.

400
00:25:50,620 --> 00:25:59,700
This one down there, it was discovered over 200 years ago.

401
00:25:59,700 --> 00:26:01,780
It's called a Cauchy distribution.

402
00:26:01,780 --> 00:26:03,660
You don't need to know that.

403
00:26:03,660 --> 00:26:08,260
But Cauchy distributions are awful.

404
00:26:08,260 --> 00:26:11,020
I dealt with them in probability theory classes

405
00:26:11,020 --> 00:26:12,340
in graduate school.

406
00:26:12,340 --> 00:26:16,740
They don't have standard deviations, oddly enough.

407
00:26:16,740 --> 00:26:19,940
That's something that nice, quiet, pleasant distributions

408
00:26:19,940 --> 00:26:20,580
have.

409
00:26:20,580 --> 00:26:23,540
Cauchy is a monster.

410
00:26:23,540 --> 00:26:28,540
We pretend that stock returns are normally distributed,

411
00:26:28,540 --> 00:26:33,260
even though we know that by using those for forecasting,

412
00:26:33,260 --> 00:26:35,860
we're going to get our butts kicked every now and then

413
00:26:35,860 --> 00:26:40,460
by a black swan or happily by a white swan.

414
00:26:40,460 --> 00:26:43,140
I'm taking that just as in context here.

415
00:26:48,220 --> 00:26:52,420
Get that son of a bitch off the board.

416
00:26:52,420 --> 00:26:56,260
Fortunately, computers can do this now,

417
00:26:56,260 --> 00:26:57,940
work with Cauchy distributions.

418
00:26:57,940 --> 00:26:59,740
You have to work with them numerically.

419
00:26:59,740 --> 00:27:03,700
But they still carry an underlying little nastiness.

420
00:27:03,700 --> 00:27:08,140
OK, so let me get this off the board here for you

421
00:27:08,140 --> 00:27:09,020
for just a minute.

422
00:27:18,700 --> 00:27:19,900
OK, first thing first.

423
00:27:23,580 --> 00:27:25,980
That's the average.

424
00:27:25,980 --> 00:27:33,980
This is our measure of central tendency, the point where

425
00:27:33,980 --> 00:27:36,580
things want to be.

426
00:27:36,580 --> 00:27:38,700
They're up here, down here.

427
00:27:38,700 --> 00:27:43,620
The x bar is simply, and I'm going

428
00:27:43,620 --> 00:27:54,940
to write this in fancy mathematical notation,

429
00:27:54,940 --> 00:27:56,620
with a will.

430
00:27:56,620 --> 00:27:59,020
Well, actually, I should put this as an r bar.

431
00:27:59,020 --> 00:27:59,780
These are returns.

432
00:28:05,380 --> 00:28:12,900
Our expected return is the sum of each

433
00:28:12,900 --> 00:28:17,340
of the individual returns divided by n.

434
00:28:17,340 --> 00:28:19,460
Add them up, divide by the number of data points.

435
00:28:19,460 --> 00:28:23,460
However, we do have to appreciate that sometimes we

436
00:28:23,460 --> 00:28:24,140
don't have.

437
00:28:24,140 --> 00:28:29,940
This would be true if we had a lot of data.

438
00:28:29,940 --> 00:28:35,780
Each one would have 1 over n probability of occurrence.

439
00:28:35,780 --> 00:28:41,860
In general, if you are running into data

440
00:28:41,860 --> 00:28:44,420
that's a little more complicated,

441
00:28:44,420 --> 00:28:53,740
it would be the sum from i equals 1

442
00:28:53,740 --> 00:28:58,460
to n of each return times the probability

443
00:28:58,460 --> 00:29:01,940
of occurrence of that term.

444
00:29:01,940 --> 00:29:06,020
And let me do it in Excel so you see what I mean by this.

445
00:29:06,020 --> 00:29:06,500
Watch.

446
00:29:06,500 --> 00:29:08,700
Where the hell is my Excel?

447
00:29:08,700 --> 00:29:10,460
I'm just going to whip up a sheet here.

448
00:29:13,620 --> 00:29:14,100
Excel.

449
00:29:14,100 --> 00:29:14,580
Open.

450
00:29:21,700 --> 00:29:24,700
And you can pull up your own Excel for this.

451
00:29:24,700 --> 00:29:33,220
So I'm going to write this as a

452
00:29:33,220 --> 00:29:36,460
and you can pull up your own Excel for this.

453
00:29:36,460 --> 00:29:38,540
I would encourage you to.

454
00:29:45,020 --> 00:29:47,260
I'm sticking with returns.

455
00:29:47,260 --> 00:30:04,420
So return probability.

456
00:30:04,420 --> 00:30:05,780
And I'll go through a couple here.

457
00:30:05,780 --> 00:30:13,980
Let's say that a return of negative 12% on a stock

458
00:30:13,980 --> 00:30:20,860
has a probability of 0.10.

459
00:30:20,860 --> 00:30:32,260
A return of negative 3% has a probability of 0.15.

460
00:30:32,260 --> 00:30:42,140
A return of 5% has a probability of 0.30.

461
00:30:42,140 --> 00:30:57,060
A return of 10% has a probability of 0.25, let's say.

462
00:30:57,060 --> 00:31:18,620
And a return of 14% has a probability 0.2.

463
00:31:18,620 --> 00:31:33,060
So now, the expected return.

464
00:31:37,420 --> 00:31:38,580
Let me separate these.

465
00:31:41,500 --> 00:31:45,660
You would take this times this plus this times this plus this

466
00:31:45,660 --> 00:31:52,420
times this plus this times this.

467
00:31:52,420 --> 00:31:54,780
But we don't have to do it that way.

468
00:31:54,780 --> 00:31:57,100
We can do it by some product.

469
00:31:57,100 --> 00:31:58,700
Are you familiar with some product?

470
00:32:07,100 --> 00:32:09,220
Some product.

471
00:32:09,220 --> 00:32:12,980
This vector, what Excel calls array,

472
00:32:12,980 --> 00:32:15,780
by this vector or array.

473
00:32:20,740 --> 00:32:21,860
And that would be a percent.

474
00:32:21,860 --> 00:32:44,500
So the expected return to the portfolio would be 5.15%.

475
00:32:44,500 --> 00:32:51,740
And then the spread, the standard deviation,

476
00:32:51,740 --> 00:33:04,820
I would need to take each of these returns.

477
00:33:04,820 --> 00:33:06,460
Oops, I did that wrong.

478
00:33:06,460 --> 00:33:07,940
Not an equal sign.

479
00:33:07,940 --> 00:33:09,660
Equals.

480
00:33:09,660 --> 00:33:14,780
The next step is, and I'll put this one up on the web for you

481
00:33:14,780 --> 00:33:17,700
if you're getting behind a little bit.

482
00:33:17,700 --> 00:33:22,380
I would take each of the individual returns

483
00:33:22,380 --> 00:33:25,100
minus the expected return.

484
00:33:29,740 --> 00:33:31,620
And I would make that an absolute

485
00:33:31,620 --> 00:33:35,700
so I could just run it down the line.

486
00:33:35,700 --> 00:33:47,620
And then I would square the result times the probability.

487
00:33:47,620 --> 00:33:58,340
I don't even have to do that, but I will.

488
00:34:07,500 --> 00:34:09,380
And then I would add them up.

489
00:34:09,380 --> 00:34:12,860
I'd get that for every one of them.

490
00:34:12,860 --> 00:34:39,180
And then the standard deviation would be the square root

491
00:34:39,180 --> 00:34:45,500
of the sum of those.

492
00:34:51,500 --> 00:34:52,660
And that is a percent.

493
00:34:52,660 --> 00:35:03,900
It's a measure of the spread.

494
00:35:15,620 --> 00:35:20,460
And the last one that I would, another one.

495
00:35:20,460 --> 00:35:24,740
You see, the problem with the standard deviation

496
00:35:24,740 --> 00:35:29,860
is that it would depend upon the size of the data, what

497
00:35:29,860 --> 00:35:33,180
the numbers were in the original data.

498
00:35:33,180 --> 00:35:39,940
If I wanted to look at different stocks against each other

499
00:35:39,940 --> 00:35:44,500
to measure their standalone risk,

500
00:35:44,500 --> 00:35:49,700
I would need to scale those numbers.

501
00:35:49,700 --> 00:35:59,980
So the coefficient of variation, I have to expand this one more

502
00:35:59,980 --> 00:36:08,700
time, I would take the standard deviation divided

503
00:36:08,700 --> 00:36:12,740
by the expected return.

504
00:36:12,740 --> 00:36:15,660
This would make it so that I could look at different data

505
00:36:15,660 --> 00:36:21,180
sets where the returns had different possibilities

506
00:36:21,180 --> 00:36:23,180
and different probabilities.

507
00:36:23,180 --> 00:36:28,620
And they would all be in the same units.

508
00:36:28,620 --> 00:36:30,980
My ass.

509
00:36:30,980 --> 00:36:31,460
Really?

510
00:36:35,140 --> 00:36:35,940
Good grief.

511
00:36:40,100 --> 00:36:41,340
Did I do that right?

512
00:36:41,340 --> 00:36:48,140
Equals the standard deviation divided by the expected return.

513
00:36:48,140 --> 00:36:51,100
That should not be that, oh, it's doing it as a percent,

514
00:36:51,100 --> 00:36:53,620
and it's not a percent.

515
00:36:53,620 --> 00:36:54,500
It's just a number.

516
00:36:59,380 --> 00:37:00,380
Come figure out.

517
00:37:00,380 --> 00:37:03,180
So in other words, this is just a pure number.

518
00:37:03,180 --> 00:37:04,260
It's not a percent.

519
00:37:04,260 --> 00:37:07,100
It's just a factor.

520
00:37:07,100 --> 00:37:08,780
And that makes it so that I could

521
00:37:08,780 --> 00:37:13,220
see another set of data that had much different looking return,

522
00:37:13,220 --> 00:37:16,340
spreads, and probabilities.

523
00:37:16,340 --> 00:37:19,140
And I could compare the two because they would be unitless.

524
00:37:22,420 --> 00:37:25,140
So I can say, well, I had this other returns.

525
00:37:25,140 --> 00:37:29,500
I had eight returns and eight associated probabilities.

526
00:37:29,500 --> 00:37:36,420
And their standard deviation was like 12.7.

527
00:37:36,420 --> 00:37:40,620
Well, because the numbers were bigger, probably.

528
00:37:40,620 --> 00:37:43,460
And this, the coefficient of variation,

529
00:37:43,460 --> 00:37:48,420
scales the numbers so that they all are unitless.

530
00:37:48,420 --> 00:37:49,860
They're no longer percents.

531
00:37:58,460 --> 00:38:03,660
However, fortunately, we don't have to do this too much.

532
00:38:03,660 --> 00:38:08,140
Because if your data set is large enough,

533
00:38:08,140 --> 00:38:12,940
these probabilities don't mean anything.

534
00:38:12,940 --> 00:38:18,100
All of the probabilities will just be 1, in this case,

535
00:38:18,100 --> 00:38:21,860
1 fifth, 0.20.

536
00:38:21,860 --> 00:38:26,340
If you have enough data, the probabilities kind of wash out

537
00:38:26,340 --> 00:38:27,660
over a large period of time.

538
00:38:27,660 --> 00:38:29,740
And I'm going to show you that in just a minute here

539
00:38:29,740 --> 00:38:31,580
with the much larger data sets where

540
00:38:31,580 --> 00:38:33,740
we don't have to worry about this nonsense.

541
00:38:38,740 --> 00:38:58,220
So in Excel, in Excel, the x bar is,

542
00:38:58,220 --> 00:39:11,260
the way you write that is average of the data set,

543
00:39:11,260 --> 00:39:12,780
average of the data set.

544
00:39:16,180 --> 00:39:21,820
And the standard deviation, STDEV,

545
00:39:21,820 --> 00:39:28,860
is STDEV, open the parentheses.

546
00:39:28,860 --> 00:39:31,140
Now, you've got to be careful here.

547
00:39:31,140 --> 00:39:35,660
Because the formula for a sample is not the same

548
00:39:35,660 --> 00:39:39,980
as the formula for a population.

549
00:39:39,980 --> 00:39:44,580
You will almost never have a population.

550
00:39:44,580 --> 00:39:46,620
Let me show you what happens.

551
00:39:46,620 --> 00:39:47,940
And we'll get one here.

552
00:39:47,940 --> 00:39:49,900
I'll pull up some data, and we'll

553
00:39:49,900 --> 00:39:51,900
play with it here for a little bit.

554
00:39:58,860 --> 00:40:00,940
Is there anything else I want to do here?

555
00:40:00,940 --> 00:40:03,940
I could do, technically, I could do sharp.

556
00:40:03,940 --> 00:40:07,220
But it doesn't really have any meaning in this one

557
00:40:07,220 --> 00:40:09,660
because I didn't have a risk-free rate involved.

558
00:40:09,660 --> 00:40:11,900
But let me take some data here.

559
00:40:11,900 --> 00:40:14,380
OK.

560
00:40:14,380 --> 00:40:23,380
Now, in order to do this, I'm going to go to a place called,

561
00:40:23,380 --> 00:40:26,380
it's an old site.

562
00:40:26,380 --> 00:40:28,900
And everything, all the data sets,

563
00:40:28,900 --> 00:40:31,820
data is everything to us in finance.

564
00:40:31,820 --> 00:40:33,220
Data, data, data.

565
00:40:33,220 --> 00:40:35,380
Everything is data-driven.

566
00:40:35,380 --> 00:40:40,380
And unfortunately, we don't have a data set.

567
00:40:40,380 --> 00:40:46,100
Unfortunately, the data is almost always costly.

568
00:40:46,100 --> 00:40:48,740
You have to pay a subscription fee.

569
00:40:48,740 --> 00:40:52,980
And sometimes that subscription fee can be insane.

570
00:40:52,980 --> 00:40:57,580
And that's the kind of stuff that artificial intelligence

571
00:40:57,580 --> 00:41:00,340
needs to do its modeling.

572
00:41:00,340 --> 00:41:03,340
It has to have millions of data points

573
00:41:03,340 --> 00:41:05,660
for it to have reliability.

574
00:41:05,660 --> 00:41:08,500
So that means you have to have the ability

575
00:41:08,500 --> 00:41:14,220
to subscribe the AI into these expensive data sets.

576
00:41:14,220 --> 00:41:16,220
And they're all over the place.

577
00:41:16,220 --> 00:41:19,220
Now, the Federal Reserve has data.

578
00:41:19,220 --> 00:41:22,300
But it actually isn't that dense.

579
00:41:22,300 --> 00:41:26,380
In order for you to go and get real actual data that

580
00:41:26,380 --> 00:41:30,020
is like millions and millions of data points,

581
00:41:30,020 --> 00:41:32,860
you have to subscribe to some of these services.

582
00:41:32,860 --> 00:41:36,620
I mean, I just ran into one a couple of weeks ago

583
00:41:36,620 --> 00:41:38,620
called PIG.

584
00:41:38,620 --> 00:41:41,620
And PIG is just vast.

585
00:41:41,620 --> 00:41:43,620
But you subscribe to it.

586
00:41:43,620 --> 00:41:46,620
S&P has databases, too.

587
00:41:46,620 --> 00:41:48,620
They are vast.

588
00:41:48,620 --> 00:41:50,620
But you have to subscribe to those.

589
00:41:50,620 --> 00:41:53,620
And there are dozens of other services.

590
00:41:53,620 --> 00:41:56,620
This site that I'm going to try to find here for you,

591
00:41:56,620 --> 00:41:58,620
it's been around forever.

592
00:41:58,620 --> 00:42:00,620
Its data isn't that vast.

593
00:42:00,620 --> 00:42:02,620
But it's free.

594
00:42:02,620 --> 00:42:04,620
And it's very reliable.

595
00:42:04,620 --> 00:42:09,620
We know that the data doesn't have any mistakes in it.

596
00:42:09,620 --> 00:42:12,620
And every year, they update it.

597
00:42:12,620 --> 00:42:14,620
Let me see.

598
00:42:14,620 --> 00:42:24,620
Stock returns historical data.

599
00:42:24,620 --> 00:42:27,620
And the place that I'm going to look for is one stock one.

600
00:42:27,620 --> 00:42:34,620
One stock one.

601
00:42:34,620 --> 00:42:37,620
One stock one dot com.

602
00:42:37,620 --> 00:42:41,620
There it is.

603
00:42:41,620 --> 00:42:43,620
Now I want you to look at something.

604
00:42:43,620 --> 00:42:47,620
What's cool about this data set is that they have these indexes.

605
00:42:47,620 --> 00:42:53,620
The Dow, the return to the Dow since 1975, the return to S&P.

606
00:42:53,620 --> 00:42:55,620
But it has ETFs.

607
00:42:55,620 --> 00:43:01,620
Any stock you could think of that is publicly traded, you can find here.

608
00:43:01,620 --> 00:43:08,620
You can also find data for other countries, for their markets in here as well.

609
00:43:08,620 --> 00:43:13,620
So if you're not trying to solve the problems of the world,

610
00:43:13,620 --> 00:43:18,620
you just want to get data and do some modeling or testing

611
00:43:18,620 --> 00:43:24,620
or just try out your mad Excel skills, you can't beat this.

612
00:43:24,620 --> 00:43:28,620
So watch, what I'll do here, there are a couple of ways in Excel

613
00:43:28,620 --> 00:43:31,620
that you can capture data from a website.

614
00:43:31,620 --> 00:43:37,620
And I'm almost reticent to do this here, but what the hell.

615
00:43:37,620 --> 00:43:39,620
I'll try it and see.

616
00:43:39,620 --> 00:43:45,620
First things first, in order to use Excel to capture a data table,

617
00:43:45,620 --> 00:43:46,620
I'll go to this.

618
00:43:46,620 --> 00:43:51,620
Oh, will you stop it with that?

619
00:43:51,620 --> 00:43:54,620
Okay, here is the Dow Jones.

620
00:43:54,620 --> 00:44:02,620
Now what I'm going to need to do to accomplish this is I'm going to actually

621
00:44:02,620 --> 00:44:08,620
copy, control C, the URL, the web address.

622
00:44:08,620 --> 00:44:20,620
Now I'm going to go over here to Excel and I'm going to say data,

623
00:44:20,620 --> 00:44:25,620
get a data set.

624
00:44:25,620 --> 00:44:28,620
Oh, come on.

625
00:44:28,620 --> 00:44:32,620
There's one for get it from the web.

626
00:44:32,620 --> 00:44:38,620
Oh, yeah, this new one actually can get a picture, the data from a picture.

627
00:44:38,620 --> 00:44:41,620
No, is that maybe what I want?

628
00:44:41,620 --> 00:44:43,620
Okay, close.

629
00:44:43,620 --> 00:44:47,620
If I can find, this is, oh, quit it, cancel.

630
00:44:47,620 --> 00:44:50,620
I want to get data from the web.

631
00:44:50,620 --> 00:44:53,620
And I'm not familiar with this 365.

632
00:44:53,620 --> 00:44:58,620
I've got the professional version.

633
00:44:58,620 --> 00:45:04,620
From, yeah, it's got some of the major ones, from a file, no,

634
00:45:04,620 --> 00:45:14,620
from a power platform, online, from other sources, from the web.

635
00:45:14,620 --> 00:45:15,620
There we go.

636
00:45:15,620 --> 00:45:17,620
There's the one I want from the web.

637
00:45:17,620 --> 00:45:18,620
Apologies for that.

638
00:45:18,620 --> 00:45:21,620
And it will say, all right, where is this data?

639
00:45:21,620 --> 00:45:27,620
Control V, that's when I'll paste in the URL.

640
00:45:27,620 --> 00:45:29,620
And I'll say, okay.

641
00:45:29,620 --> 00:45:35,620
Now it's going to run over there and it's going to say, okay, I see it right there.

642
00:45:35,620 --> 00:45:36,620
I think.

643
00:45:36,620 --> 00:45:43,620
Now, connect.

644
00:45:43,620 --> 00:45:47,620
And it's going to say, I see a bunch of tables there.

645
00:45:47,620 --> 00:45:54,620
Now, one of the problems with websites, and this is, this wasn't how we did it in the old days,

646
00:45:54,620 --> 00:45:59,620
but that top thing you see in websites, the menus, and the clickdowns and all that,

647
00:45:59,620 --> 00:46:02,620
that's actually set up as a table.

648
00:46:02,620 --> 00:46:05,620
And that's not what you probably want.

649
00:46:05,620 --> 00:46:07,620
So I'll bet it's the second table.

650
00:46:07,620 --> 00:46:08,620
And it'll give me a preview.

651
00:46:08,620 --> 00:46:09,620
Ah, it is.

652
00:46:09,620 --> 00:46:10,620
Well, spank me, Jesus.

653
00:46:10,620 --> 00:46:11,620
Look at that.

654
00:46:11,620 --> 00:46:13,620
Do you see it?

655
00:46:13,620 --> 00:46:15,620
Okay, that's the one I want.

656
00:46:15,620 --> 00:46:19,620
Okay, so load that mother.

657
00:46:19,620 --> 00:46:22,620
Oh, that data set.

658
00:46:22,620 --> 00:46:24,620
You know what I mean, for God's sake.

659
00:46:24,620 --> 00:46:28,620
Look, it's right there.

660
00:46:28,620 --> 00:46:33,620
Well, isn't that a very convenient thing?

661
00:46:33,620 --> 00:46:39,620
Okay, so I will now call, give that a meaningful name.

662
00:46:39,620 --> 00:46:41,620
I will call it George.

663
00:46:41,620 --> 00:46:42,620
No, I won't.

664
00:46:42,620 --> 00:46:49,620
I'll call it Dow 30.

665
00:46:49,620 --> 00:46:51,620
And I've got it.

666
00:46:51,620 --> 00:46:55,620
So now let me do sheet two.

667
00:46:55,620 --> 00:46:56,620
Go over here.

668
00:46:56,620 --> 00:47:05,620
And I'm going to go back to, back up one, the S&P 500.

669
00:47:05,620 --> 00:47:08,620
And I'm going to get its URL.

670
00:47:08,620 --> 00:47:14,620
And I'm going to do the same stupid pet trick, now that I remember.

671
00:47:14,620 --> 00:47:22,620
Data from the web.

672
00:47:22,620 --> 00:47:28,620
Give it that webpage and say Okie Dokie.

673
00:47:28,620 --> 00:47:30,620
And I'll also say, let's have a look at table.

674
00:47:30,620 --> 00:47:32,620
Yes, that's table one there.

675
00:47:32,620 --> 00:47:35,620
So load that mother, or that thing.

676
00:47:35,620 --> 00:47:39,620
See it?

677
00:47:39,620 --> 00:47:41,620
And I got that one.

678
00:47:41,620 --> 00:47:53,620
And I'll call that S&P 500.

679
00:47:53,620 --> 00:47:58,620
And now I'm going to do the trick one more time.

680
00:47:58,620 --> 00:48:01,620
I'm going to go to the site and I'm going to get the NASDAQ,

681
00:48:01,620 --> 00:48:05,620
historical data, or the health.

682
00:48:05,620 --> 00:48:07,620
There it is.

683
00:48:07,620 --> 00:48:12,620
And I will capture its web address.

684
00:48:12,620 --> 00:48:24,620
And I'll go back to Excel and I'll say data, get data from the web.

685
00:48:24,620 --> 00:48:27,620
Ok.

686
00:48:27,620 --> 00:48:28,620
And it's table one.

687
00:48:28,620 --> 00:48:29,620
It is every time.

688
00:48:29,620 --> 00:48:33,620
So load that data.

689
00:48:33,620 --> 00:48:37,620
Now if you do this right, it saves you a lot of pain.

690
00:48:37,620 --> 00:48:46,620
Because a long time ago, we actually had to type in each data entry on our own,

691
00:48:46,620 --> 00:48:52,620
or do a copy and paste and have Excel misunderstand how it worked.

692
00:48:52,620 --> 00:48:53,620
This way is a lot more powerful.

693
00:48:53,620 --> 00:48:56,620
And you can just draw down masses.

694
00:48:56,620 --> 00:49:02,620
If you can find a place like, well, FRED, the Federal Reserve's database,

695
00:49:02,620 --> 00:49:06,620
that data is kind of, they do it by day sometimes.

696
00:49:06,620 --> 00:49:08,620
You might want ten years.

697
00:49:08,620 --> 00:49:13,620
Well you just do this trick I did here and it will slam that data right,

698
00:49:13,620 --> 00:49:16,620
all of it, into Excel.

699
00:49:16,620 --> 00:49:18,620
As a matter of fact, FRED is even better than that.

700
00:49:18,620 --> 00:49:22,620
You can actually tell it to download the data as an Excel sheet.

701
00:49:22,620 --> 00:49:24,620
So they're cheating these days.

702
00:49:24,620 --> 00:49:26,620
Ok.

703
00:49:26,620 --> 00:49:28,620
There we go.

704
00:49:28,620 --> 00:49:33,620
Now let's go back here and do some stupid pet tricks.

705
00:49:33,620 --> 00:49:37,620
Remember that what I want are returns.

706
00:49:37,620 --> 00:49:38,620
Ok.

707
00:49:38,620 --> 00:49:39,620
I want returns.

708
00:49:39,620 --> 00:49:43,620
So these other ones really, the year obviously matters,

709
00:49:43,620 --> 00:49:49,620
but what I really want are the returns for each of these.

710
00:49:49,620 --> 00:49:51,620
So, whoops.

711
00:49:51,620 --> 00:49:59,620
Oh, I should have, I forgot to label that NASDAQ.

712
00:49:59,620 --> 00:50:01,620
So here we are.

713
00:50:01,620 --> 00:50:02,620
We got all our returns.

714
00:50:02,620 --> 00:50:05,620
So here's what we're going to do.

715
00:50:05,620 --> 00:50:09,620
And this is another stupid pet trick.

716
00:50:09,620 --> 00:50:17,620
I'm going to highlight all of these numbers.

717
00:50:17,620 --> 00:50:18,620
All of these.

718
00:50:18,620 --> 00:50:22,620
I hold down the control key and I click on the ones that I want.

719
00:50:22,620 --> 00:50:32,620
Now I'm going to go down here and I'm going to put in the average.

720
00:50:32,620 --> 00:50:36,620
And I'm going to put in one more here too that I haven't talked about.

721
00:50:36,620 --> 00:50:38,620
The median.

722
00:50:38,620 --> 00:50:41,620
The median is the halfway point in the data.

723
00:50:41,620 --> 00:50:43,620
That's not the average.

724
00:50:43,620 --> 00:50:47,620
And in fact, the difference between them is kind of important.

725
00:50:47,620 --> 00:50:57,620
But then I'm also going to do the standard deviation.

726
00:50:57,620 --> 00:51:10,620
And I'm going to do also the coefficient of variation.

727
00:51:10,620 --> 00:51:14,620
Now remember, I've got all three sheets highlighted.

728
00:51:14,620 --> 00:51:20,620
So what I do to one will be done to all of them.

729
00:51:20,620 --> 00:51:29,620
So the first thing I'm going to do is I'm going to say equals average of all the date, of the returns.

730
00:51:29,620 --> 00:51:33,620
The average of the returns.

731
00:51:33,620 --> 00:51:44,620
Now I'll turn these into percents eventually here.

732
00:51:44,620 --> 00:51:48,620
And then I'm going to do the median.

733
00:51:48,620 --> 00:52:00,620
The central point of all the data.

734
00:52:00,620 --> 00:52:04,620
Now this next one I caution. Watch out for what you do.

735
00:52:04,620 --> 00:52:09,620
I'm going to write the standard deviation equals STDEV.

736
00:52:09,620 --> 00:52:12,620
Now notice that it gives you a whole menu.

737
00:52:12,620 --> 00:52:16,620
The second one,.S, is the one we want.

738
00:52:16,620 --> 00:52:22,620
But if you don't put anything there, it will do.S.

739
00:52:22,620 --> 00:52:24,620
You don't have to. It defaults to.S.

740
00:52:24,620 --> 00:52:27,620
Thank heaven. I never remembered to do that.

741
00:52:27,620 --> 00:52:40,620
Okay, STDEV.

742
00:52:40,620 --> 00:52:44,620
Close the parentheses.

743
00:52:44,620 --> 00:52:51,620
And finally, the coefficient of variation equals,

744
00:52:51,620 --> 00:53:02,620
and this one you just do by, you just do the standard deviation divided by the average.

745
00:53:02,620 --> 00:53:06,620
Now let me turn all these, these first three are percentages.

746
00:53:06,620 --> 00:53:13,620
So I'll turn those into percentages to two decimal places.

747
00:53:13,620 --> 00:53:15,620
Okay, so there's my Uncle Bob.

748
00:53:15,620 --> 00:53:20,620
Now let's go back through and look at what we found.

749
00:53:20,620 --> 00:53:24,620
The average.

750
00:53:24,620 --> 00:53:32,620
For the Dow, the average over the last, now this data was from 1975 to 2023.

751
00:53:32,620 --> 00:53:37,620
So that would make it, what, 25, 48 years.

752
00:53:37,620 --> 00:53:40,620
This is 48 years of data.

753
00:53:40,620 --> 00:53:45,620
The average return to the Dow was 9.79%.

754
00:53:45,620 --> 00:54:05,620
The average return to the, whoops, it didn't work, equals average, I went too far.

755
00:54:15,620 --> 00:54:19,620
Median.

756
00:54:19,620 --> 00:54:23,620
I have to do median of this data.

757
00:54:23,620 --> 00:54:28,620
I took that too far with that, all sheets.

758
00:54:28,620 --> 00:54:40,620
It took the first set of data for all of the sheets.

759
00:54:40,620 --> 00:55:02,620
Again, equals median, median of the second tape, that table of data.

760
00:55:02,620 --> 00:55:17,620
Standard deviation of all that data.

761
00:55:17,620 --> 00:55:18,620
There we go.

762
00:55:18,620 --> 00:55:38,620
Now let me do this S&P 500 again, average of that data.

763
00:55:38,620 --> 00:55:43,620
Equals median of that data.

764
00:55:43,620 --> 00:55:52,620
Yeah, I was taking the first table for all of them.

765
00:55:52,620 --> 00:56:03,620
And for that one, equals STDEV of this data.

766
00:56:03,620 --> 00:56:06,620
Wow.

767
00:56:06,620 --> 00:56:09,620
My cool pet trick didn't work there.

768
00:56:09,620 --> 00:56:11,620
Okay, so now let's go back.

769
00:56:11,620 --> 00:56:17,620
The Dow, for the last 48 years, the average return.

770
00:56:17,620 --> 00:56:28,620
If you had just put money in and left it there, your average annual return would have been 9.79%.

771
00:56:28,620 --> 00:56:38,620
For the S&P 500, a somewhat riskier portfolio, it would have been 10.32%.

772
00:56:38,620 --> 00:56:49,620
For the NASDAQ, if you had just stuck the money in there and left it, the average return would have been 14.84%.

773
00:56:49,620 --> 00:56:53,620
There is the risk-return relationship.

774
00:56:53,620 --> 00:56:57,620
The greater the risk, the greater the return.

775
00:56:57,620 --> 00:57:03,620
Now let's go back here and look at some things.

776
00:57:03,620 --> 00:57:14,620
The median tells us half of the numbers are below that number and half are above that number.

777
00:57:14,620 --> 00:57:23,620
When the average and the median are different, that tells us about the skewedness.

778
00:57:23,620 --> 00:57:29,620
Here's what it means.

779
00:57:29,620 --> 00:57:36,620
To a certain extent, it tells us about how much different from a perfect bell curve the data is.

780
00:57:36,620 --> 00:57:38,620
Look at this one.

781
00:57:38,620 --> 00:57:46,620
Suppose that you had this long tail of data like that.

782
00:57:46,620 --> 00:57:58,620
These low numbers would actually pull down the average from what it should be.

783
00:57:58,620 --> 00:58:04,620
So you have, on this case, the average would be higher than the median.

784
00:58:04,620 --> 00:58:07,620
The median doesn't care the size of the numbers.

785
00:58:07,620 --> 00:58:09,620
See all these big numbers up here?

786
00:58:09,620 --> 00:58:13,620
They are being counterbalanced by this long tail down here.

787
00:58:13,620 --> 00:58:16,620
The same would go the other way.

788
00:58:16,620 --> 00:58:23,620
So I could have some high returns that would pull the average upward.

789
00:58:23,620 --> 00:58:29,620
That's a problem on tests where a lot of people are not doing all that great.

790
00:58:29,620 --> 00:58:35,620
But you have just a small cluster, maybe five, eight students who ace the test.

791
00:58:35,620 --> 00:58:41,620
They make the average look higher than the data is really telling you it is.

792
00:58:41,620 --> 00:58:48,620
So in this case, the average is being drawn down by heavy losses in a few years.

793
00:58:48,620 --> 00:58:51,620
That's the black swans.

794
00:58:51,620 --> 00:59:01,620
The median, half the numbers are below it, half of them are above it, is telling us a different story.

795
00:59:01,620 --> 00:59:09,620
So in a case like this, I would say that the average is being affected by heavy losses that make the average,

796
00:59:09,620 --> 00:59:14,620
those really low numbers, those negative numbers, are affecting the average,

797
00:59:14,620 --> 00:59:17,620
but they don't do anything to the median.

798
00:59:17,620 --> 00:59:22,620
Look at the S&P 500, the same problem is occurring there.

799
00:59:22,620 --> 00:59:27,620
The black swans are pulling the average downward.

800
00:59:27,620 --> 00:59:32,620
But look at the NASDAQ.

801
00:59:32,620 --> 00:59:38,620
The black swans don't affect the distribution as much.

802
00:59:38,620 --> 00:59:51,620
In other words, small cap companies are not as sensitive to black swans as the big 500 or the massive Dow are.

803
00:59:51,620 --> 00:59:54,620
Now look at the coefficients of variation.

804
00:59:54,620 --> 01:00:05,620
For the Dow, the CV, well, let me put this to about 2%.

805
01:00:05,620 --> 01:00:12,620
For the Dow, the coefficient of variation is 1.5.

806
01:00:12,620 --> 01:00:19,620
For the S&P 500, it's 1.56.

807
01:00:19,620 --> 01:00:23,620
In other words, there's a little more absolute spread.

808
01:00:23,620 --> 01:00:35,620
And for the NASDAQ, there's more spread, absolutely.

809
01:00:35,620 --> 01:00:45,620
So that's why the CV, see if I just look at the numbers, you get that.

810
01:00:45,620 --> 01:00:55,620
For the Dow, you get 14.67. For the S&P 500, you get 16.8.

811
01:00:55,620 --> 01:00:59,620
But that's because the Dow's numbers are bigger.

812
01:00:59,620 --> 01:01:05,620
Once I get that bigness, that difference in size of the numbers out of there,

813
01:01:05,620 --> 01:01:10,620
we can see the true risk-return relationship coming through.

814
01:01:10,620 --> 01:01:20,620
So look at this. 9.79 on an absolute risk metric of 1.5.

815
01:01:20,620 --> 01:01:34,620
10.32, 1.56. 14.84, 1.68, the risk-return relationship.

816
01:01:34,620 --> 01:01:42,620
Now I'll put this up for you to play around with, but this gives you visually what we constantly are talking about,

817
01:01:42,620 --> 01:01:46,620
that risk-return relationship, the greater the risk, the greater the return.

818
01:01:46,620 --> 01:01:54,620
And here, over a very large amount of data, we see it shining through.

819
01:01:54,620 --> 01:01:57,620
We also see some hints, too.

820
01:01:57,620 --> 01:02:09,620
We see some hints that, for example, like I said, black swans pulled down the average for the Dow

821
01:02:09,620 --> 01:02:19,620
and for the S&P 500 far more than they do for the small cap stocks.

822
01:02:19,620 --> 01:02:23,620
And we also see that risk-return relationship coming through again.

823
01:02:23,620 --> 01:02:29,620
And you can do this with tons of different companies, tons of different indexes.

824
01:02:29,620 --> 01:02:33,620
It always shows up. It always does.

825
01:02:33,620 --> 01:02:43,620
The same phenomenon, lower risk portfolios, lower expected returns, more skew in the data.

826
01:02:43,620 --> 01:02:54,620
And as you get higher and higher risk of the portfolio, you get less skew and you get higher spread, absolutely speaking,

827
01:02:54,620 --> 01:02:57,620
which is what the CV does.

828
01:02:57,620 --> 01:03:01,620
That's good to know for all of us in our business.

829
01:03:01,620 --> 01:03:04,620
And we can play with this on Monday.

830
01:03:04,620 --> 01:03:07,620
I'm going to, if you don't have it, I'll try to do it real quick here.

831
01:03:07,620 --> 01:03:10,620
Let me show you something.

832
01:03:10,620 --> 01:03:21,620
In files, options, I think it's options, go to add-ins.

833
01:03:21,620 --> 01:03:27,620
See this right here, this analysis tool pack?

834
01:03:27,620 --> 01:03:31,620
You click on that one and say go.

835
01:03:31,620 --> 01:03:35,620
And you want the analysis tool pack, okay.

836
01:03:35,620 --> 01:03:44,620
Now what that will do is it will give you the access to a pile of data analytics.

837
01:03:44,620 --> 01:03:51,620
You can do all kinds of things like this and all kinds of other things with that data analysis pack.

838
01:03:51,620 --> 01:03:55,620
And all you have to do is say here's the data, use the data analysis pack,

839
01:03:55,620 --> 01:04:01,620
and it will make an extra spreadsheet with all of these statistics on it for you.

840
01:04:01,620 --> 01:04:10,620
So again, in order to do that, you do files, options, and you go down to the add-ins,

841
01:04:10,620 --> 01:04:15,620
and you choose the data analysis pack and you say go.

842
01:04:15,620 --> 01:04:18,620
And it will put it in there for you.

843
01:04:18,620 --> 01:04:22,620
Now for some of you, you'll have to do it every time you,

844
01:04:22,620 --> 01:04:29,620
if you want to do a new data analysis, some Office 365s,

845
01:04:29,620 --> 01:04:33,620
you have to do this little thing every time to get the pack loaded.

846
01:04:33,620 --> 01:04:37,620
Others, it will be in there permanently.

847
01:04:37,620 --> 01:04:39,620
But anyway, you have a quiz to take.

848
01:04:39,620 --> 01:04:44,620
Please take that quiz, and once you're finished with it, that's all I have for you today.

849
01:04:44,620 --> 01:04:59,620
Thank you.

