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What I want to do now is let's
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go through some photographs that we photographed of
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Lisa and Dylan, and these are the shots.
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They're straight out of the camera.
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They're all raw.
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Nothing's been done to these photographs whatsoever.
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But what actually is a histogram, and what
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does it represent?
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Because as far as we're concerned, it's just
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peaks and valleys, and it's all confusing.
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So what do we, what do we need
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to know?
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Well, let's go a little bit closer, and
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let's have a look.
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So, what is a histogram?
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Well, it's a graphic representation of the number
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of pixels at each luminance value in an
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image.
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Now, here we've got different values.
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As you can see, we've got the value
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from all the way from black, which is
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0, and then 255 is white.
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So even though we've got 0 to 255,
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there's not 255 levels of brightness.
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It's actually 256, because we have to count
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0 as black, 255 as white, and that's
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how we go.
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Now, here we see the actual histogram.
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Of course, as you can see, the left
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side indicates shadow clipping.
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All right, so in other words, clipping basically
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means that we have no detail in blacks.
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On the right-hand side, we have the
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actual, it indicates highlight clipping, or it's, this
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is the highlights.
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The way I like to remember it is
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SH, shadow highlights.
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Remember, shh, remember, remember that.
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That'll actually really help you understand it.
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And of course, now the height of the
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peaks, what does that represent?
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Well, that's actually how many pixels you have
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in a particular range.
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So, a common suggestion is to spread the
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pixel values evenly across the, the way here,
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and I'm thinking, well, you know what, that's
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not always the case.
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It's nice to have a nice little peak
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of a little mountain, and then coming all
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the way down, but your histogram will never
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be perfect.
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So, we have to understand that.
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Now, what about this red, green, blue?
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What does that basically mean?
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Well, it's made up of three colors, and
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red, green, and blue are the color channels.
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Now, where red and green actually overlap, you
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get yellow.
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Where red and blue overlap, you get magenta.
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And of course, blue and green is cyan.
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And white appears when all three channels overlap.
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So, as you can see, all of these
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sections over here.
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So, what we'll do at times is actually
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remove the RGB histogram to reveal just the
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exposure part of it, and that'll actually help
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us even further.
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So, what we have to do, guys, it
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depends on how you've actually photographed.
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As far as I'm concerned, I prefer to
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look at the back of the camera, or
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in my case, because I'm shooting mirrorless, I'm
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looking in the viewfinder, and I am seeing
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detail in the highlights and detail in the
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skin tones.
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Of course, the brightest part of an image
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of a person usually should be of that
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person's face.
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Then, that is where the detail should be,
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and everything will take care of itself.
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See, in the film days, you would expose
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for shadows, develop for the highlights, and with
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digital and transparency, for that matter, it's a
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very different scenario.
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So, what we're trying to do here, guys,
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is get detail in the brightest highlight in
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the face.
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And once you do that, or the dress,
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they both take care of each other.
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Does that make sense?
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So, here we've got out-of-camera exposure.
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Yes, she's a little bit shiny.
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That doesn't mean that this is a bad
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exposure, nor does it mean it's a bad
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exposure if we have a deep shadow on
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her face.
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Of course, if you remember, this is actually
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photographing in full sun.
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So, what I want to do now is
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let's flick this.
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You can see we can actually go to
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black and white, and if you look at
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these points here, the levels of brightness will
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be revealed.
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But I'm going to click my picker here.
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Now, do you see where my mouse is
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going, the little picker?
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And as we're doing that, you've got those
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levels of brightness.
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It's giving us like that 25.
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Do you see how that's very, very dark?
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It's not exactly black.
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It's not zero.
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Zero is black.
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No detail.
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It's pure black.
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If we go to the highlights, you'll start
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to see where it's getting closer to that
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255 back.
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So, let's see if I've actually blown out
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anything.
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I'm just trying to see.
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As soon as we get the 255, let's
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look at that area.
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No, let me put my glasses on, actually.
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I can see this a lot better.
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So, it looks like we have pretty much
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detail everywhere.
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Now, you might say, Jerry, well, why don't
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I just shoot aperture priority in and then
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hope for the best, and then I can
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just get detail in my shadows and highlights
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and things like that.
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Well, of course you can.
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You can get more details in shadows only.
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You can lift up the mid-tones and
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all that kind of stuff.
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But can you see how we're starting to
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lose a bit of detail and we get
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a lot of grain?
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So, nothing beats an in-camera good exposure
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rather than just trying to do it after
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the fact.
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Excuse my dog barking in the background there.
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He's probably missing daddy there.
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But again, this is a good exposure.
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We have detail in skin tones.
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We have detail in highlights.
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Life is good.
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Let's go down a little bit further.
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This one here of Lisa and Dylan, I
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love the way the light is skimming off
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Dylan there.
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We've got beautiful highlights over there as well,
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deep shadows, but you can see quite clearly
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the detail in them.
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But again, if you want to increase the
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exposure, you can, but of course you're going
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to blow out the highlights.
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So, if you expose well, that exposure slider
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will hardly be touched.
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You might just want to put some detail
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in those shadows.
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Personally, I love deep, dark shadows.
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It gives us beautiful depth and dimension and
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drama.
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It's one of the signatures to my work,
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which I really love.
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Let's just keep on going down and find
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some different shots here as well.
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So again, I love the fact that we're
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playing with shadows.
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Those half shadows underneath a guy's eyes, very
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masculine, looks good.
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I wouldn't do that for a girl, so
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I make sure her eye sock is completely
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lit.
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Love the shadow on her lips.
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It makes her lips look fuller, as well
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as the shadow underneath her top lip, which
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is amazing.
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Now, let's go to this.
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This is going to be almost impossible to
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get a perfect exposure, short of actually using
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off-camera flash, balancing that light that's hitting
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behind her veil and so on.
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Now, let's put our little picker here.
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So again, let's look at the RGB there.
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So again, although I'm going to flick it
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to black and white, it still gives us
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the luminance values from 0 to 255.
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So if you can sort of see there,
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well, there's some mid-tones, right?
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Mid-tones, it's going a bit darker.
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As you can see, it's going darker and
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darker.
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Now, let's put it on the veil.
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All right.
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Do you see how it's 255?
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We actually got some clipping.
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What that basically means, clipping means that if
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you go to the end here, like you
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want to contain usually your histogram within this
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way.
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You do not want this particular part of
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the mountain, so to speak, to clip and
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to hit that side of the histogram.
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Remember, shadows, highlights.
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Remember, like you're shushing someone.
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That makes you remember that the shadows are
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on the left and the highlights on the
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right.
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Now, does this make this a disposable photograph?
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This is a bad photograph.
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Do I just get rid of it?
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Well, as far as I'm concerned, I eliminated
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distraction by cropping closer.
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Yes, these are white and bright.
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If I exposed for the highlight here, in
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other words, I want detail in that veil.
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Well, of course, that light is going to
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be nowhere near as beautiful because we actually
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use light, the sun bouncing off a wall,
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hitting her face.
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Now, yes, if you entered into this competition,
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photographers would say, well, there's no detail on
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the highlights.
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That's terrible.
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Well, don't forget that most of the time,
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guys, well, most of the time we should
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be photographing for our clients.
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We're not there to actually photograph for other
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photographers.
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So just know what you're shooting for.
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And yes, if you want to be more
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critical and actually make sure that the judges
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in a competition say, well, this is a
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perfect exposure.
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Well, is there such a thing as a
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perfect exposure?
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I believe a perfect exposure is pretty much
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the execution of your desired result.
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In this case, I'm picking the lesser of
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the evils.
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I don't care about the detail here.
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All I care about is her face looking
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amazing and having a beautiful direction of light.
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Now, can I get detail in shadows?
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You see how I'm going over here now
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that looks a little bit fake.
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You can sort of see what's happening on
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the on the fringe of that highlight there.
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I would probably say you can certainly do
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that.
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That actually looks pretty good.
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But then I would massage this in Photoshop
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later on so I don't get that unrealistic
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sort of glow that's on the outside.
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So you can see, of course, that the
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the latitude that we have when it comes
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to digital processing after the fact is just
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it makes our life so much easier.
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But I'm saying don't rely on it because
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the quality will never be as good and
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compared to a good exposure in camera under
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the circumstances and what you're photographing.
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So, like I said, we've got no no
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detail on those whites, but we can bring
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it back.
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And that's quite amazing that we can do
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that.
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Let's keep on going here.
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00:08:52,080 --> 00:08:55,000
So and these are just, you know, beautiful
274
00:08:55,000 --> 00:08:55,440
images.
275
00:08:55,660 --> 00:08:57,080
Let's see if we've got detail here, what
276
00:08:57,080 --> 00:08:58,760
we're looking, what we don't want to see
277
00:08:58,760 --> 00:09:00,980
in this particular part of the histogram.
278
00:09:01,460 --> 00:09:03,220
We don't want to see a luminance value
279
00:09:03,220 --> 00:09:04,720
of two hundred and fifty five.
280
00:09:05,280 --> 00:09:06,640
Now, yes, we are shooting white.
281
00:09:07,280 --> 00:09:09,220
See, we're sort of getting there, but we
282
00:09:09,220 --> 00:09:10,020
still see detail.
283
00:09:10,320 --> 00:09:12,180
But if you look at her face and
284
00:09:12,180 --> 00:09:14,680
look at those mid tones, then we've also
285
00:09:14,680 --> 00:09:15,920
got detail over here as well.
286
00:09:16,120 --> 00:09:18,620
Now here, if it was completely dark and
287
00:09:18,620 --> 00:09:20,800
no detail, this would be zero.
288
00:09:20,800 --> 00:09:23,600
So you can see this histogram and this
289
00:09:23,600 --> 00:09:26,660
beautiful peaks and there's beautiful valleys and it
290
00:09:26,660 --> 00:09:27,240
crosses over.
291
00:09:28,200 --> 00:09:29,560
And again, let's go to black and white
292
00:09:29,560 --> 00:09:31,140
so we can just see the actual exposure
293
00:09:31,140 --> 00:09:33,300
histogram, ignoring the color into it.
294
00:09:33,980 --> 00:09:37,020
Now, so your histogram should not always go
295
00:09:37,020 --> 00:09:38,160
up and always go down.
296
00:09:38,560 --> 00:09:40,860
This is basically just little peaks and valleys
297
00:09:40,860 --> 00:09:43,040
of different tones in the image.
298
00:09:43,460 --> 00:09:45,600
And you can see how it tapers off
299
00:09:45,600 --> 00:09:46,780
over here.
300
00:09:46,780 --> 00:09:49,040
And it tapers off over here, which basically
301
00:09:49,040 --> 00:09:50,740
technically means we got a good exposure.
302
00:09:50,920 --> 00:09:53,300
But ignoring the histogram, we do have a
303
00:09:53,300 --> 00:09:55,220
good exposure because it's exactly what we want.
304
00:09:55,740 --> 00:09:58,040
Now, let me give you a more polarizing
305
00:09:58,040 --> 00:10:03,340
shot that arguably you would say is bordering
306
00:10:03,340 --> 00:10:04,200
on no detail.
307
00:10:04,580 --> 00:10:06,940
OK, so here we have Dylan.
308
00:10:07,080 --> 00:10:08,260
He's just sort of squatting down.
309
00:10:08,560 --> 00:10:09,860
We've got a deep, dark shadow.
310
00:10:10,100 --> 00:10:11,380
Let's have a look and see if we
311
00:10:11,380 --> 00:10:14,280
have any kind of detail there.
312
00:10:14,280 --> 00:10:17,160
And again, if we don't, this would be
313
00:10:17,160 --> 00:10:17,500
zero.
314
00:10:17,800 --> 00:10:20,100
So I'm moving the color picker all around.
315
00:10:21,000 --> 00:10:24,300
But you can see how those values are
316
00:10:24,300 --> 00:10:25,440
not actually clipping.
317
00:10:25,620 --> 00:10:26,520
They're not getting to the zero.
318
00:10:26,660 --> 00:10:27,980
Now, if you look at the histogram there,
319
00:10:28,020 --> 00:10:30,060
you can see how it falls short just
320
00:10:30,060 --> 00:10:33,300
of extending out on the left hand side.
321
00:10:33,400 --> 00:10:34,860
And of course, it comes back over here
322
00:10:34,860 --> 00:10:35,300
as well.
323
00:10:35,740 --> 00:10:38,080
Now, yes, you can move this up and
324
00:10:38,080 --> 00:10:40,320
down so you can see the blacks.
325
00:10:40,980 --> 00:10:42,500
I'm getting the blacks and moving them.
326
00:10:42,620 --> 00:10:44,520
And you see that slider moving this way.
327
00:10:45,060 --> 00:10:46,980
Now, if I do it this way, you'll
328
00:10:46,980 --> 00:10:49,780
see that the whites are getting we're changing
329
00:10:49,780 --> 00:10:51,280
the value of those whites as well.
330
00:10:51,780 --> 00:10:53,540
And then, of course, we've got the mid
331
00:10:53,540 --> 00:10:55,240
tones that we can that we can use.
332
00:10:55,280 --> 00:10:58,000
So you can see how there's five sections
333
00:10:58,000 --> 00:11:00,780
that we can play with five parts of
334
00:11:00,780 --> 00:11:01,220
that image.
335
00:11:01,280 --> 00:11:04,060
You've got the shadows, the highlights, and then
336
00:11:04,060 --> 00:11:05,760
you've got the mid tones representing in those
337
00:11:05,760 --> 00:11:06,300
three panels.
338
00:11:06,760 --> 00:11:09,020
Now, let's go a little bit further here
339
00:11:09,020 --> 00:11:11,360
because I want to show you this shot.
340
00:11:11,560 --> 00:11:14,020
OK, so this one, if you look at
341
00:11:14,020 --> 00:11:16,180
that histogram, let's take out that RGB.
342
00:11:16,460 --> 00:11:18,200
That looks like a terrible histogram.
343
00:11:18,520 --> 00:11:20,540
If you did not look at that photograph
344
00:11:20,540 --> 00:11:22,920
and all you saw was that histogram on
345
00:11:22,920 --> 00:11:24,240
the back of the camera, someone would say
346
00:11:24,240 --> 00:11:25,260
that's a terrible exposure.
347
00:11:25,400 --> 00:11:26,620
You've underexposed it.
348
00:11:27,500 --> 00:11:30,460
It's terrible because we said shadows, highlights.
349
00:11:30,460 --> 00:11:32,860
We've got highlights and not even going to
350
00:11:32,860 --> 00:11:35,240
the end, which means there's nothing white in
351
00:11:35,240 --> 00:11:36,800
this image or nothing close to it.
352
00:11:36,920 --> 00:11:38,320
So we don't have that full range.
353
00:11:38,580 --> 00:11:41,240
And then we've got those shadows clipping, which
354
00:11:41,240 --> 00:11:43,580
basically means that there's going to be points
355
00:11:43,580 --> 00:11:46,400
to this image where we will get zero.
356
00:11:46,520 --> 00:11:47,400
So there we've got one.
357
00:11:48,420 --> 00:11:49,120
There we go.
358
00:11:49,240 --> 00:11:50,500
We've got zero just there.
359
00:11:50,560 --> 00:11:50,920
There we go.
360
00:11:51,180 --> 00:11:52,320
It's completely black.
361
00:11:52,420 --> 00:11:53,140
There's no detail.
362
00:11:53,840 --> 00:11:55,600
Guys, what I'm saying to you is this
363
00:11:55,600 --> 00:11:59,160
is a good exposure because that's the desired
364
00:11:59,160 --> 00:12:00,160
effect that I wanted.
365
00:12:01,580 --> 00:12:03,540
So, yes, you can be like me.
366
00:12:03,820 --> 00:12:05,120
And I look at the back of the
367
00:12:05,120 --> 00:12:06,680
camera or in my case, because I shoot
368
00:12:06,680 --> 00:12:09,000
mirrorless, I'm looking in the viewfinder and I've
369
00:12:09,000 --> 00:12:11,160
learned to see what a good exposure looks
370
00:12:11,160 --> 00:12:12,040
like in my camera.
371
00:12:12,280 --> 00:12:13,400
I rely on that.
372
00:12:13,480 --> 00:12:15,280
And as you can see, all my exposures
373
00:12:15,280 --> 00:12:17,240
are good for my desired result.
374
00:12:17,940 --> 00:12:20,640
And there's nothing there's no there's no shot
375
00:12:20,640 --> 00:12:22,340
here, for example, where I'm like, you know
376
00:12:22,340 --> 00:12:24,520
what, I didn't nail it in camera.
377
00:12:24,680 --> 00:12:25,980
Now, look at this shot, for example.
378
00:12:26,320 --> 00:12:28,140
We turn the body away from the light
379
00:12:28,140 --> 00:12:29,420
source, turn the face back in.
380
00:12:29,420 --> 00:12:31,580
We've got detail in those highlights.
381
00:12:32,400 --> 00:12:33,840
You know, obviously, we've got shadow highlights, shadow
382
00:12:33,840 --> 00:12:34,260
highlights.
383
00:12:34,520 --> 00:12:36,480
We've got detail basically here.
384
00:12:37,280 --> 00:12:39,280
We've got detail in those dark tones.
385
00:12:39,640 --> 00:12:40,820
And life is pretty good there.
386
00:12:41,320 --> 00:12:43,740
Now, I can increase the mid tones.
387
00:12:43,920 --> 00:12:47,440
I can give us more detail and highlights.
388
00:12:47,580 --> 00:12:48,800
That just depends on your style.
389
00:12:49,460 --> 00:12:51,720
It depends on what you like.
390
00:12:52,360 --> 00:12:55,500
There is no perfect histogram.
391
00:12:55,800 --> 00:12:56,900
We have to say that again.
392
00:12:57,300 --> 00:12:58,820
Now, let's just talk about this for a
393
00:12:58,820 --> 00:12:59,000
moment.
394
00:13:01,460 --> 00:13:04,920
If you look into the camera, let's say
395
00:13:04,920 --> 00:13:05,740
you don't have mirrorless.
396
00:13:05,880 --> 00:13:06,900
Let's say you have to look at the
397
00:13:06,900 --> 00:13:08,440
back of the camera and determine a good
398
00:13:08,440 --> 00:13:09,780
exposure from what you're seeing.
399
00:13:11,020 --> 00:13:12,820
Well, it's like watching TV.
400
00:13:13,160 --> 00:13:15,480
If you watch TV indoors, if we're watching
401
00:13:15,480 --> 00:13:17,540
a TV indoors, there's going to be a
402
00:13:17,540 --> 00:13:19,480
certain kind of saturation and contrast that we
403
00:13:19,480 --> 00:13:22,480
see because we're looking at TV indoor with
404
00:13:22,480 --> 00:13:23,540
no sun hitting the TV.
405
00:13:23,800 --> 00:13:25,820
Therefore, it's contrasty and it looks good.
406
00:13:26,520 --> 00:13:28,860
But what happens when you watch TV outdoors
407
00:13:28,860 --> 00:13:29,980
in full sun?
408
00:13:29,980 --> 00:13:31,900
Well, that's no different than actually getting a
409
00:13:31,900 --> 00:13:33,720
flurry day as sun's flaring.
410
00:13:34,240 --> 00:13:36,040
You know, you may be like me where
411
00:13:36,040 --> 00:13:37,460
you have to wear glasses to see up
412
00:13:37,460 --> 00:13:37,880
close.
413
00:13:38,100 --> 00:13:39,620
And it's like, well, I don't know.
414
00:13:39,700 --> 00:13:41,100
I can't I can't even see the detail.
415
00:13:41,260 --> 00:13:42,280
I don't know what it is.
416
00:13:42,580 --> 00:13:43,420
I don't have mirrorless.
417
00:13:43,960 --> 00:13:44,960
I don't know what's going on.
418
00:13:45,040 --> 00:13:46,280
Well, you might want to rely on the
419
00:13:46,280 --> 00:13:46,640
histogram.
420
00:13:46,860 --> 00:13:49,380
But again, I've proven to you that a
421
00:13:49,380 --> 00:13:51,640
histogram based upon your desired result like this
422
00:13:51,640 --> 00:13:54,800
one is actually going to look the histograms
423
00:13:54,800 --> 00:13:55,400
going to look terrible.
424
00:13:56,140 --> 00:13:58,740
Now, can I resurrect some detail if I
425
00:13:58,740 --> 00:13:59,360
wanted to?
426
00:13:59,360 --> 00:14:00,500
Well, let's see.
427
00:14:00,860 --> 00:14:01,800
Let's go back to color.
428
00:14:03,000 --> 00:14:04,920
And it'll freak you out that this can
429
00:14:04,920 --> 00:14:07,900
happen, but you can actually resurrect the detail.
430
00:14:08,060 --> 00:14:09,320
That was a silhouette.
431
00:14:10,720 --> 00:14:13,620
Look at that five stops difference of exposure.
432
00:14:14,380 --> 00:14:16,520
Now, yes, what happens is that if you
433
00:14:16,520 --> 00:14:18,980
don't know the exposure in camera, you are
434
00:14:18,980 --> 00:14:21,500
going to get terrible quality, bad.
435
00:14:21,860 --> 00:14:24,360
You're going to get this grain effect.
436
00:14:24,460 --> 00:14:26,860
You're going to get this this this weird
437
00:14:26,860 --> 00:14:28,560
tones in the in the photograph.
438
00:14:28,560 --> 00:14:31,020
So I'm saying to you, don't just shoot
439
00:14:31,020 --> 00:14:33,440
aperture priority and hope for the best, because
440
00:14:33,440 --> 00:14:34,760
that is not going to work a lot
441
00:14:34,760 --> 00:14:36,440
of the time, because the minute you have
442
00:14:36,440 --> 00:14:38,080
a bride and a groom.
443
00:14:38,260 --> 00:14:40,780
So you got black suit, white dress, and
444
00:14:40,780 --> 00:14:42,100
then all of a sudden we've got this
445
00:14:42,100 --> 00:14:42,840
white wall.
446
00:14:43,180 --> 00:14:46,320
The camera is going to basically see a
447
00:14:46,320 --> 00:14:48,240
lot of white, a bit more white here
448
00:14:48,240 --> 00:14:48,940
and a bit of black.
449
00:14:49,340 --> 00:14:50,940
It'll pretend like it's a paint bucket.
450
00:14:51,500 --> 00:14:53,620
It'll mix that paint in if you're actually
451
00:14:53,620 --> 00:14:55,980
photographing with matrix or evaluative metering where you're
452
00:14:55,980 --> 00:14:59,380
evaluating the whole scene, and then it's going
453
00:14:59,380 --> 00:15:01,040
to actually make that like a light gray.
454
00:15:01,660 --> 00:15:04,500
If the camera sees light gray, it wants
455
00:15:04,500 --> 00:15:07,800
mid gray, therefore underexposing the photograph.
456
00:15:08,240 --> 00:15:09,900
What you have to know is when you
457
00:15:09,900 --> 00:15:11,580
look at an image like that, you have
458
00:15:11,580 --> 00:15:14,080
to know that you have to technically well,
459
00:15:14,480 --> 00:15:16,240
you have to overexpose.
460
00:15:16,340 --> 00:15:18,300
And I say that inverted commas because you
461
00:15:18,300 --> 00:15:19,160
are exposing correctly.
462
00:15:19,800 --> 00:15:22,720
But not by what the camera is saying,
463
00:15:22,900 --> 00:15:24,440
which means that you have to either with
464
00:15:24,440 --> 00:15:26,760
your ISO, your aperture or your shutter speed,
465
00:15:27,120 --> 00:15:29,420
you have to move the dial, your exposure
466
00:15:29,420 --> 00:15:30,120
compensation.
467
00:15:30,540 --> 00:15:32,480
However you want to get there, you have
468
00:15:32,480 --> 00:15:34,480
to lean towards the plus sign, because in
469
00:15:34,480 --> 00:15:36,820
the camera we have minus, we have plus,
470
00:15:36,980 --> 00:15:37,560
we have zero.
471
00:15:37,800 --> 00:15:42,880
Plus represents overexposing, minus represents underexposing, zero represents
472
00:15:42,880 --> 00:15:43,940
a good exposure.
473
00:15:44,480 --> 00:15:46,260
So like I said, the good way of
474
00:15:46,260 --> 00:15:48,820
remembering it is if your subject matter is
475
00:15:48,820 --> 00:15:50,980
bright, you go bright, lean towards the plus.
476
00:15:51,340 --> 00:15:54,100
If your subject matter is dark, lean towards
477
00:15:54,100 --> 00:15:56,340
a dark, as in with one of your
478
00:15:56,340 --> 00:16:02,080
either your ISO, your shutter speed or your
479
00:16:02,080 --> 00:16:02,620
aperture.
480
00:16:03,600 --> 00:16:06,700
So again, guys, that you can read the
481
00:16:06,700 --> 00:16:07,760
histogram if you wish.
482
00:16:07,920 --> 00:16:09,880
It really depends on what you prefer.
483
00:16:09,880 --> 00:16:11,800
But if you read the back of the
484
00:16:11,800 --> 00:16:14,980
camera, it's very, very important that you have
485
00:16:14,980 --> 00:16:20,100
to determine what that exposure looks like indoors,
486
00:16:20,560 --> 00:16:21,040
outdoors.
487
00:16:21,500 --> 00:16:23,480
And also you might find, well, Jerry, I'm
488
00:16:23,480 --> 00:16:25,140
looking at the back of the screen and
489
00:16:25,140 --> 00:16:26,460
the exposure looked perfect.
490
00:16:26,940 --> 00:16:29,820
And I don't know why when I look
491
00:16:29,820 --> 00:16:32,680
at my photographs on a calibrated monitor, I
492
00:16:32,680 --> 00:16:34,200
wonder why my exposure is different.
493
00:16:34,320 --> 00:16:35,580
Well, your screen in the back of the
494
00:16:35,580 --> 00:16:37,180
camera could be too dark or too light.
495
00:16:37,180 --> 00:16:40,340
Not all cameras and LCD screens are created
496
00:16:40,340 --> 00:16:40,700
equal.
497
00:16:41,080 --> 00:16:42,800
So what you want to do when you
498
00:16:42,800 --> 00:16:46,540
first get a camera is photograph some different
499
00:16:46,540 --> 00:16:48,220
subject matter, what you believe to be a
500
00:16:48,220 --> 00:16:48,740
good exposure.
501
00:16:48,900 --> 00:16:51,020
In my case, I don't really I don't
502
00:16:51,020 --> 00:16:52,840
really worry about the histogram, although I know
503
00:16:52,840 --> 00:16:54,360
what it means and I know what it
504
00:16:54,360 --> 00:16:54,860
reads.
505
00:16:55,260 --> 00:16:57,060
But the way I shoot, I shoot very
506
00:16:57,060 --> 00:16:59,760
dramatic highlights and deep shadows and things like
507
00:16:59,760 --> 00:16:59,940
that.
508
00:16:59,960 --> 00:17:01,340
So my histograms are not going to always
509
00:17:01,340 --> 00:17:02,000
look that great.
510
00:17:02,460 --> 00:17:04,240
So what I suggest you do is when
511
00:17:04,240 --> 00:17:06,720
you first get a camera, learn what a
512
00:17:06,720 --> 00:17:08,160
good exposure looks like in the back of
513
00:17:08,160 --> 00:17:08,520
the camera.
514
00:17:08,980 --> 00:17:10,579
And that'll be just do a couple of
515
00:17:10,579 --> 00:17:12,280
shots, shoot a friend, shoot, shoot a partner,
516
00:17:12,380 --> 00:17:12,579
whatever.
517
00:17:13,319 --> 00:17:15,819
Then now you know what a good exposure
518
00:17:15,819 --> 00:17:17,079
looks like on the back of the camera,
519
00:17:17,079 --> 00:17:19,119
on the back of the camera, outdoors, indoors,
520
00:17:19,359 --> 00:17:20,000
you name it.
521
00:17:20,339 --> 00:17:22,500
Then you load it on your computer.
522
00:17:23,040 --> 00:17:25,000
Make sure you have a calibrated monitor.
523
00:17:25,200 --> 00:17:26,819
In other words, what you see here in
524
00:17:26,819 --> 00:17:28,360
this monitor is what you get in print.
525
00:17:29,220 --> 00:17:32,140
Then bring up a photograph and then put
526
00:17:32,140 --> 00:17:33,660
that same photograph, put the card back in
527
00:17:33,660 --> 00:17:35,860
the camera and compare your screen with a
528
00:17:35,860 --> 00:17:36,620
calibrated screen.
529
00:17:36,960 --> 00:17:39,560
You might find your screen is too dark.
530
00:17:40,000 --> 00:17:41,700
Go into your camera manual on your settings,
531
00:17:42,200 --> 00:17:43,040
increase the brightness.
532
00:17:43,340 --> 00:17:45,220
And now what you see on the back
533
00:17:45,220 --> 00:17:46,500
of the screen is what you get.
534
00:17:46,740 --> 00:17:48,480
That's why mirrorless is so good, because you've
535
00:17:48,480 --> 00:17:50,660
got a built in loop where you can
536
00:17:50,660 --> 00:17:53,580
shield away all the sunlight coming through all
537
00:17:53,580 --> 00:17:55,720
that crap and just look at that exposure.
538
00:17:55,720 --> 00:17:58,740
What I'm looking for, I'm looking for detail
539
00:17:58,740 --> 00:18:01,060
in the whites.
540
00:18:01,360 --> 00:18:03,100
I'm looking for detail on the skin.
541
00:18:03,400 --> 00:18:04,860
The skin is my first guide.
542
00:18:05,200 --> 00:18:07,080
Then I glance down and I make sure
543
00:18:07,080 --> 00:18:07,820
I see detail.
544
00:18:08,740 --> 00:18:10,540
Now, you might be saying, well, Jerry, what
545
00:18:10,540 --> 00:18:12,720
do I do with, say, African-American skin
546
00:18:12,720 --> 00:18:15,880
or I've got an African-American groom, maybe,
547
00:18:16,040 --> 00:18:17,900
and then maybe a Caucasian bride?
548
00:18:18,600 --> 00:18:20,820
The biggest problem is that most of the
549
00:18:20,820 --> 00:18:23,620
time most photographers who get that exposure wrong
550
00:18:23,620 --> 00:18:26,200
is you're trying to make the African-American
551
00:18:26,200 --> 00:18:29,240
skin look Caucasian and get all this detail
552
00:18:29,240 --> 00:18:30,920
in those in the dark skin.
553
00:18:31,080 --> 00:18:32,960
I'm saying you can get detail.
554
00:18:33,160 --> 00:18:35,440
What I do is I let the Caucasian
555
00:18:35,440 --> 00:18:37,940
person be my guide for my exposure.
556
00:18:38,300 --> 00:18:40,100
And I'm telling you, the rest will take
557
00:18:40,100 --> 00:18:40,740
care of itself.
558
00:18:40,840 --> 00:18:41,840
You're overthinking it.
559
00:18:41,840 --> 00:18:44,900
And, of course, after the fact, whether it's
560
00:18:44,900 --> 00:18:47,800
in camera raw, whether it's in Lightroom, whether
561
00:18:47,800 --> 00:18:50,040
it's in Capture One, of course, you can
562
00:18:50,040 --> 00:18:52,380
increase that detail in those shadow areas and
563
00:18:52,380 --> 00:18:53,160
all that kind of stuff.
564
00:18:53,260 --> 00:18:55,340
But you can sort of see how, again,
565
00:18:56,040 --> 00:18:57,740
you know, we've got detail there.
566
00:18:57,940 --> 00:19:00,920
You can see how this exposure is just
567
00:19:00,920 --> 00:19:02,440
going to go to black and white here.
568
00:19:02,520 --> 00:19:04,300
You can see how it's just going short
569
00:19:04,300 --> 00:19:04,680
of clipping.
570
00:19:04,940 --> 00:19:06,900
And then you can sort of see how
571
00:19:06,900 --> 00:19:08,920
those highlights are there as well.
572
00:19:08,920 --> 00:19:12,520
So this is a good histogram by the
573
00:19:12,520 --> 00:19:13,880
nature of what I'm actually doing.
574
00:19:15,960 --> 00:19:17,960
I just enjoy the ride, guys, like now
575
00:19:17,960 --> 00:19:20,340
here, 100 percent, we are going to get
576
00:19:20,340 --> 00:19:21,120
clipping.
577
00:19:21,620 --> 00:19:23,560
So we're going to basically see, let's go
578
00:19:23,560 --> 00:19:25,220
look right in the candles at 255.
579
00:19:25,280 --> 00:19:25,980
We've got no detail.
580
00:19:26,240 --> 00:19:27,300
It's a light source.
581
00:19:27,380 --> 00:19:29,120
You are not going to get detail there.
582
00:19:29,380 --> 00:19:31,700
It's pure white, because if we are exposing
583
00:19:31,700 --> 00:19:34,420
for the result of that light, how would
584
00:19:34,420 --> 00:19:36,680
we expect detail in that candlelight?
585
00:19:36,680 --> 00:19:38,940
I mean, it's glorified fire, right?
586
00:19:39,580 --> 00:19:42,200
Now, if we look over here, we are
587
00:19:42,200 --> 00:19:43,380
going to get values of zero.
588
00:19:43,480 --> 00:19:43,840
There we go.
589
00:19:43,920 --> 00:19:45,840
We've got ones, ones, ones.
590
00:19:48,560 --> 00:19:50,340
Can we find the zero somewhere?
591
00:19:51,320 --> 00:19:51,720
No.
592
00:19:52,500 --> 00:19:53,860
Surely it'd be somewhere here.
593
00:19:54,060 --> 00:19:54,180
No.
594
00:19:54,400 --> 00:19:55,420
OK, there we go.
595
00:19:58,620 --> 00:19:59,800
But there you have it, guys.
596
00:20:00,660 --> 00:20:02,340
First of all, that is the way you
597
00:20:02,340 --> 00:20:03,060
read a histogram.
598
00:20:03,780 --> 00:20:06,100
You can go, you can get all geeky
599
00:20:06,100 --> 00:20:07,380
about it and all that kind of stuff.
600
00:20:07,520 --> 00:20:08,900
And if you want it as a guide,
601
00:20:09,000 --> 00:20:11,360
you can certainly look at your camera, your
602
00:20:11,360 --> 00:20:13,460
camera settings and press the display where your
603
00:20:13,460 --> 00:20:14,320
histogram is there.
604
00:20:14,520 --> 00:20:16,760
But just know there is no perfect histogram.
605
00:20:16,940 --> 00:20:19,240
The histogram will be based upon what you're
606
00:20:19,240 --> 00:20:19,780
photographing.
607
00:20:20,180 --> 00:20:22,220
Like I said, with me, I prefer deep,
608
00:20:22,380 --> 00:20:23,000
dark shadows.
609
00:20:23,040 --> 00:20:25,060
I'm not I don't really care about perfect
610
00:20:25,060 --> 00:20:27,860
detail in shadows on every single photograph.
611
00:20:28,420 --> 00:20:30,800
I expose for the highlights, as in I
612
00:20:30,800 --> 00:20:32,760
want detail in the highlights on the face
613
00:20:32,760 --> 00:20:33,720
and the dress.
614
00:20:33,760 --> 00:20:35,100
In this case, we're talking about a wedding
615
00:20:35,100 --> 00:20:37,660
and the rest will take care of itself.
616
00:20:38,040 --> 00:20:39,140
So don't overthink it.
617
00:20:39,380 --> 00:20:41,720
But just remember, the camera can't think like
618
00:20:41,720 --> 00:20:42,160
a human.
619
00:20:42,680 --> 00:20:45,560
Always remember to think of the complete opposites.
620
00:20:45,700 --> 00:20:46,840
And it makes you understand.
621
00:20:46,940 --> 00:20:48,380
So let's go over those one more time.
622
00:20:48,780 --> 00:20:50,960
If you photograph four African-American men wearing
623
00:20:50,960 --> 00:20:52,640
a black suit leaning on a black wall
624
00:20:52,640 --> 00:20:54,880
and you were to photograph aperture priority, the
625
00:20:54,880 --> 00:20:56,620
camera sees black and says, I don't like
626
00:20:56,620 --> 00:20:56,940
black.
627
00:20:57,400 --> 00:21:00,260
It'll make it me great, therefore overexpose.
628
00:21:00,760 --> 00:21:02,980
And we showed you in our demonstration that
629
00:21:02,980 --> 00:21:04,800
if you've got something black, a black suit,
630
00:21:05,220 --> 00:21:07,560
then we said that you have to actually
631
00:21:07,560 --> 00:21:09,240
underexpose.
632
00:21:09,480 --> 00:21:10,860
And I say that again, inverted commas, because
633
00:21:10,860 --> 00:21:13,440
we are not underexposing or exposing correctly, but
634
00:21:13,440 --> 00:21:15,540
we are underexposing by what the camera is
635
00:21:15,540 --> 00:21:18,240
saying up to five to six clicks.
636
00:21:18,440 --> 00:21:20,520
And I say clicks as in third stop
637
00:21:20,520 --> 00:21:23,620
increments, which means that we are one one
638
00:21:23,620 --> 00:21:26,420
and two thirds up to two stops under.
639
00:21:26,940 --> 00:21:29,560
So let's remember we said if something is
640
00:21:29,560 --> 00:21:31,980
dark, you go dark, lean towards the minus.
641
00:21:32,160 --> 00:21:35,040
So you either use your aperture, your shutter
642
00:21:35,040 --> 00:21:36,900
speed or your ISO or a combination.
643
00:21:37,320 --> 00:21:39,600
So you lean towards the minus with your
644
00:21:39,600 --> 00:21:42,040
compensation or you just use exposure compensation like
645
00:21:42,040 --> 00:21:43,560
plus and minus, depending on how you like
646
00:21:43,560 --> 00:21:43,860
to shoot.
647
00:21:44,260 --> 00:21:46,720
So you can shoot aperture priority and use
648
00:21:46,720 --> 00:21:47,420
your compensation.
649
00:21:47,420 --> 00:21:50,180
But just know you shoot a black subject.
650
00:21:50,480 --> 00:21:52,860
You are going to have to underexpose because
651
00:21:52,860 --> 00:21:55,020
the camera is seeing black and it's not
652
00:21:55,020 --> 00:21:55,380
racist.
653
00:21:55,380 --> 00:21:57,000
It doesn't care about black or white.
654
00:21:57,120 --> 00:21:58,060
It just wants mid gray.
655
00:21:58,380 --> 00:22:00,420
It has to it has to have a
656
00:22:00,420 --> 00:22:00,780
standard.
657
00:22:01,220 --> 00:22:04,020
If you're photographing a pale skinned bride wearing
658
00:22:04,020 --> 00:22:05,820
a white dress, leaning on a white wall,
659
00:22:06,160 --> 00:22:07,140
the camera sees white.
660
00:22:07,320 --> 00:22:08,380
It doesn't like white.
661
00:22:08,680 --> 00:22:10,240
It again, if you rely on the on
662
00:22:10,240 --> 00:22:12,500
the exposure mode, whether you're shooting on manual
663
00:22:12,500 --> 00:22:14,940
or aperture priority and you move one of
664
00:22:14,940 --> 00:22:17,280
those dials that you determine your exposure, you
665
00:22:17,280 --> 00:22:18,220
move it to zero.
666
00:22:18,480 --> 00:22:20,240
You are going to make what was once
667
00:22:20,240 --> 00:22:22,980
white into gray, mid gray.
668
00:22:23,320 --> 00:22:24,120
So what did we say?
669
00:22:24,120 --> 00:22:25,800
How do we go from mid gray to
670
00:22:25,800 --> 00:22:27,600
white and detail in those whites?
671
00:22:28,040 --> 00:22:29,180
Well, we said it's going to be about
672
00:22:29,180 --> 00:22:30,700
one to two stops.
673
00:22:30,860 --> 00:22:32,680
I find it's one to two third stops
674
00:22:32,680 --> 00:22:33,080
difference.
675
00:22:34,180 --> 00:22:35,880
And now what's in between?
676
00:22:36,000 --> 00:22:38,820
If you're photographing a mountain range and it's
677
00:22:38,820 --> 00:22:40,100
a dark mountain, you've got to be a
678
00:22:40,100 --> 00:22:40,460
sunset.
679
00:22:40,540 --> 00:22:41,580
You get a bit of light coming through.
680
00:22:41,660 --> 00:22:44,000
You get some light hitting your subjects.
681
00:22:44,280 --> 00:22:45,340
You've got some clouds.
682
00:22:45,540 --> 00:22:48,060
So now you've got the blue sky, which
683
00:22:48,060 --> 00:22:49,560
is a dark gray sky.
684
00:22:49,800 --> 00:22:51,160
Now you've got the clouds.
685
00:22:51,200 --> 00:22:52,100
That's white.
686
00:22:52,520 --> 00:22:53,600
You've got the dark mountains.
687
00:22:53,600 --> 00:22:54,520
That's a dark gray.
688
00:22:54,680 --> 00:22:55,800
You've got the skin tones.
689
00:22:56,080 --> 00:22:56,840
That's a light gray.
690
00:22:57,080 --> 00:22:59,040
Now mix those tones in.
691
00:22:59,720 --> 00:23:01,820
It may not be polarizingly black or white.
692
00:23:02,020 --> 00:23:04,980
It might be, say, a dark gray.
693
00:23:05,520 --> 00:23:06,500
So here's what you do.
694
00:23:06,900 --> 00:23:08,320
The camera is going to make it mid
695
00:23:08,320 --> 00:23:08,620
gray.
696
00:23:08,720 --> 00:23:09,840
But you want to go back to where
697
00:23:09,840 --> 00:23:12,420
you started to basically get detail in those
698
00:23:12,420 --> 00:23:12,980
highlights.
699
00:23:13,360 --> 00:23:14,940
And again, the rest will take care of
700
00:23:14,940 --> 00:23:15,220
itself.
701
00:23:15,420 --> 00:23:17,460
So if we're thinking, you know what, if
702
00:23:17,460 --> 00:23:19,660
black is about one to two thirds to
703
00:23:19,660 --> 00:23:23,440
two stops difference from black to mid gray.
704
00:23:23,440 --> 00:23:25,180
And therefore we have to do that, then
705
00:23:25,180 --> 00:23:28,000
maybe a dark gray might be one stop.
706
00:23:28,580 --> 00:23:29,380
Does that make sense?
707
00:23:29,680 --> 00:23:32,160
So once you understand those extremes, the in
708
00:23:32,160 --> 00:23:33,240
-between becomes easy.
709
00:23:33,380 --> 00:23:35,400
So when you're in your environment and you
710
00:23:35,400 --> 00:23:36,700
take a shot and have a look at
711
00:23:36,700 --> 00:23:38,460
the back of the camera and you know
712
00:23:38,460 --> 00:23:40,540
that you're about one click out, as in
713
00:23:40,540 --> 00:23:42,800
one third stop increment out of your exposure.
714
00:23:43,140 --> 00:23:45,880
And you need to either under or overexpose
715
00:23:45,880 --> 00:23:48,000
deliberately by what the camera is saying.
716
00:23:48,740 --> 00:23:49,880
Take that shot.
717
00:23:50,420 --> 00:23:50,660
Done.
718
00:23:51,080 --> 00:23:52,860
Shoot that whole scene in that environment.
719
00:23:53,260 --> 00:23:53,680
You're done.
720
00:23:54,520 --> 00:23:56,420
If you shoot with aperture priority with one
721
00:23:56,420 --> 00:23:58,420
subject and the minute you widen your angle
722
00:23:58,420 --> 00:24:00,680
of view, you start to get your exposure
723
00:24:00,680 --> 00:24:02,980
changes with every element that is added into
724
00:24:02,980 --> 00:24:03,480
that photograph.
725
00:24:03,640 --> 00:24:05,260
But you just want that skin to be
726
00:24:05,260 --> 00:24:07,280
beautiful, that white dress to be beautiful.
727
00:24:08,320 --> 00:24:10,580
So that's what I'm saying is shooting manually
728
00:24:10,580 --> 00:24:12,420
is going to be more consistent.
729
00:24:13,160 --> 00:24:15,820
And when you're converting your files, for example.
730
00:24:15,820 --> 00:24:18,160
So when you're correcting your files, if you
731
00:24:18,160 --> 00:24:20,660
shoot aperture priority, you'll find your exposures are
732
00:24:20,660 --> 00:24:21,180
spiking.
733
00:24:21,320 --> 00:24:23,140
They're going forward and back just by shooting
734
00:24:23,140 --> 00:24:23,900
that one scene.
735
00:24:24,420 --> 00:24:25,340
Here's the thing.
736
00:24:25,700 --> 00:24:28,400
If you shoot manual and you forget to
737
00:24:28,400 --> 00:24:30,660
actually fix your exposure after you've tested it
738
00:24:30,660 --> 00:24:31,880
originally and something's happened.
739
00:24:32,320 --> 00:24:34,560
Let's say you've got a chunk of 50
740
00:24:34,560 --> 00:24:36,700
photographs that are over or underexposed.
741
00:24:36,840 --> 00:24:37,400
Well, guess what?
742
00:24:37,880 --> 00:24:41,180
You can globally grab them and globally fix
743
00:24:41,180 --> 00:24:42,180
them with a couple of clicks.
744
00:24:42,730 --> 00:24:44,480
If it was aperture priority, you would have
745
00:24:44,480 --> 00:24:47,240
to literally go into every image, every two
746
00:24:47,240 --> 00:24:49,320
or three images and change the exposure.
747
00:24:49,500 --> 00:24:50,560
That is a pain in the butt.
748
00:24:51,220 --> 00:24:52,500
So make your life easy.
749
00:24:52,760 --> 00:24:54,880
Understand what the camera is doing.
750
00:24:55,700 --> 00:24:56,540
Understand exposure.
751
00:24:56,780 --> 00:24:59,200
Certainly, you might want to understand the techniques
752
00:24:59,200 --> 00:24:59,820
of a histogram.
753
00:25:00,560 --> 00:25:02,840
But when we mash that all in, this
754
00:25:02,840 --> 00:25:05,060
should be no different to a calculator to
755
00:25:05,060 --> 00:25:05,500
an accountant.
756
00:25:06,020 --> 00:25:06,780
Know your craft.
757
00:25:06,920 --> 00:25:07,840
Know the tool of your trade.
758
00:25:08,080 --> 00:25:09,700
Exposure should be the last thing you care
759
00:25:09,700 --> 00:25:09,960
about.
760
00:25:09,960 --> 00:25:12,260
You should be worrying about connecting with your
761
00:25:12,260 --> 00:25:15,440
clients, your creativity and just getting the job
762
00:25:15,440 --> 00:25:15,720
done.
763
00:25:15,980 --> 00:25:16,920
Hope you enjoyed that.
764
00:25:17,060 --> 00:25:18,620
Hopefully that was one of the easiest ways
765
00:25:18,620 --> 00:25:21,400
you've ever been explained about how to expose
766
00:25:21,400 --> 00:25:21,780
correctly.
767
00:25:22,220 --> 00:25:23,340
Enjoy guys and practice.
52734
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