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These are the user uploaded subtitles that are being translated: 1 00:00:00,120 --> 00:00:00,960 What I want to do now is let's 2 00:00:00,960 --> 00:00:02,820 go through some photographs that we photographed of 3 00:00:02,820 --> 00:00:05,340 Lisa and Dylan, and these are the shots. 4 00:00:05,460 --> 00:00:06,540 They're straight out of the camera. 5 00:00:06,700 --> 00:00:07,260 They're all raw. 6 00:00:07,380 --> 00:00:09,380 Nothing's been done to these photographs whatsoever. 7 00:00:10,040 --> 00:00:13,340 But what actually is a histogram, and what 8 00:00:13,340 --> 00:00:14,120 does it represent? 9 00:00:14,180 --> 00:00:16,340 Because as far as we're concerned, it's just 10 00:00:16,340 --> 00:00:18,540 peaks and valleys, and it's all confusing. 11 00:00:18,800 --> 00:00:20,060 So what do we, what do we need 12 00:00:20,060 --> 00:00:20,420 to know? 13 00:00:20,780 --> 00:00:22,220 Well, let's go a little bit closer, and 14 00:00:22,220 --> 00:00:22,740 let's have a look. 15 00:00:23,320 --> 00:00:25,340 So, what is a histogram? 16 00:00:25,540 --> 00:00:27,700 Well, it's a graphic representation of the number 17 00:00:27,700 --> 00:00:31,100 of pixels at each luminance value in an 18 00:00:31,100 --> 00:00:31,380 image. 19 00:00:31,700 --> 00:00:33,660 Now, here we've got different values. 20 00:00:33,840 --> 00:00:35,660 As you can see, we've got the value 21 00:00:35,660 --> 00:00:38,940 from all the way from black, which is 22 00:00:38,940 --> 00:00:41,100 0, and then 255 is white. 23 00:00:41,400 --> 00:00:43,380 So even though we've got 0 to 255, 24 00:00:43,460 --> 00:00:46,220 there's not 255 levels of brightness. 25 00:00:46,400 --> 00:00:49,080 It's actually 256, because we have to count 26 00:00:49,080 --> 00:00:53,440 0 as black, 255 as white, and that's 27 00:00:53,440 --> 00:00:53,840 how we go. 28 00:00:53,980 --> 00:00:57,020 Now, here we see the actual histogram. 29 00:00:57,820 --> 00:00:59,300 Of course, as you can see, the left 30 00:00:59,300 --> 00:01:01,720 side indicates shadow clipping. 31 00:01:02,400 --> 00:01:03,879 All right, so in other words, clipping basically 32 00:01:03,879 --> 00:01:05,720 means that we have no detail in blacks. 33 00:01:06,300 --> 00:01:08,680 On the right-hand side, we have the 34 00:01:08,680 --> 00:01:11,540 actual, it indicates highlight clipping, or it's, this 35 00:01:11,540 --> 00:01:12,140 is the highlights. 36 00:01:12,240 --> 00:01:13,860 The way I like to remember it is 37 00:01:13,860 --> 00:01:16,580 SH, shadow highlights. 38 00:01:16,740 --> 00:01:19,200 Remember, shh, remember, remember that. 39 00:01:19,360 --> 00:01:20,980 That'll actually really help you understand it. 40 00:01:21,780 --> 00:01:23,300 And of course, now the height of the 41 00:01:23,300 --> 00:01:24,720 peaks, what does that represent? 42 00:01:24,900 --> 00:01:26,800 Well, that's actually how many pixels you have 43 00:01:26,800 --> 00:01:28,440 in a particular range. 44 00:01:29,220 --> 00:01:31,120 So, a common suggestion is to spread the 45 00:01:31,120 --> 00:01:34,920 pixel values evenly across the, the way here, 46 00:01:35,020 --> 00:01:36,540 and I'm thinking, well, you know what, that's 47 00:01:36,540 --> 00:01:37,280 not always the case. 48 00:01:37,400 --> 00:01:39,040 It's nice to have a nice little peak 49 00:01:39,760 --> 00:01:41,900 of a little mountain, and then coming all 50 00:01:41,900 --> 00:01:44,100 the way down, but your histogram will never 51 00:01:44,100 --> 00:01:44,700 be perfect. 52 00:01:45,260 --> 00:01:46,660 So, we have to understand that. 53 00:01:46,700 --> 00:01:48,320 Now, what about this red, green, blue? 54 00:01:48,420 --> 00:01:49,540 What does that basically mean? 55 00:01:49,700 --> 00:01:52,420 Well, it's made up of three colors, and 56 00:01:52,420 --> 00:01:54,420 red, green, and blue are the color channels. 57 00:01:55,000 --> 00:01:57,980 Now, where red and green actually overlap, you 58 00:01:57,980 --> 00:01:58,580 get yellow. 59 00:01:59,140 --> 00:02:01,360 Where red and blue overlap, you get magenta. 60 00:02:01,580 --> 00:02:03,060 And of course, blue and green is cyan. 61 00:02:03,640 --> 00:02:06,400 And white appears when all three channels overlap. 62 00:02:06,400 --> 00:02:08,000 So, as you can see, all of these 63 00:02:08,000 --> 00:02:08,820 sections over here. 64 00:02:09,300 --> 00:02:11,140 So, what we'll do at times is actually 65 00:02:11,140 --> 00:02:15,540 remove the RGB histogram to reveal just the 66 00:02:15,540 --> 00:02:17,960 exposure part of it, and that'll actually help 67 00:02:17,960 --> 00:02:18,940 us even further. 68 00:02:19,900 --> 00:02:21,880 So, what we have to do, guys, it 69 00:02:21,880 --> 00:02:23,400 depends on how you've actually photographed. 70 00:02:23,680 --> 00:02:26,560 As far as I'm concerned, I prefer to 71 00:02:26,560 --> 00:02:28,280 look at the back of the camera, or 72 00:02:28,280 --> 00:02:30,220 in my case, because I'm shooting mirrorless, I'm 73 00:02:30,220 --> 00:02:32,660 looking in the viewfinder, and I am seeing 74 00:02:32,660 --> 00:02:35,980 detail in the highlights and detail in the 75 00:02:35,980 --> 00:02:36,540 skin tones. 76 00:02:36,680 --> 00:02:38,100 Of course, the brightest part of an image 77 00:02:38,100 --> 00:02:39,840 of a person usually should be of that 78 00:02:39,840 --> 00:02:40,560 person's face. 79 00:02:40,960 --> 00:02:43,840 Then, that is where the detail should be, 80 00:02:44,060 --> 00:02:46,000 and everything will take care of itself. 81 00:02:46,460 --> 00:02:48,660 See, in the film days, you would expose 82 00:02:48,660 --> 00:02:51,340 for shadows, develop for the highlights, and with 83 00:02:51,340 --> 00:02:53,420 digital and transparency, for that matter, it's a 84 00:02:53,420 --> 00:02:54,300 very different scenario. 85 00:02:54,800 --> 00:02:56,200 So, what we're trying to do here, guys, 86 00:02:56,220 --> 00:02:58,880 is get detail in the brightest highlight in 87 00:02:58,880 --> 00:02:59,320 the face. 88 00:02:59,320 --> 00:03:02,380 And once you do that, or the dress, 89 00:03:02,840 --> 00:03:04,520 they both take care of each other. 90 00:03:04,600 --> 00:03:05,220 Does that make sense? 91 00:03:05,620 --> 00:03:07,780 So, here we've got out-of-camera exposure. 92 00:03:07,900 --> 00:03:09,160 Yes, she's a little bit shiny. 93 00:03:09,300 --> 00:03:10,900 That doesn't mean that this is a bad 94 00:03:10,900 --> 00:03:12,720 exposure, nor does it mean it's a bad 95 00:03:12,720 --> 00:03:14,300 exposure if we have a deep shadow on 96 00:03:14,300 --> 00:03:14,700 her face. 97 00:03:14,780 --> 00:03:17,320 Of course, if you remember, this is actually 98 00:03:17,320 --> 00:03:18,620 photographing in full sun. 99 00:03:19,320 --> 00:03:21,180 So, what I want to do now is 100 00:03:21,180 --> 00:03:22,280 let's flick this. 101 00:03:22,340 --> 00:03:24,480 You can see we can actually go to 102 00:03:24,480 --> 00:03:26,620 black and white, and if you look at 103 00:03:26,620 --> 00:03:28,920 these points here, the levels of brightness will 104 00:03:28,920 --> 00:03:29,620 be revealed. 105 00:03:30,500 --> 00:03:33,080 But I'm going to click my picker here. 106 00:03:33,300 --> 00:03:35,200 Now, do you see where my mouse is 107 00:03:35,200 --> 00:03:36,820 going, the little picker? 108 00:03:37,280 --> 00:03:40,320 And as we're doing that, you've got those 109 00:03:40,320 --> 00:03:41,340 levels of brightness. 110 00:03:42,700 --> 00:03:45,280 It's giving us like that 25. 111 00:03:45,440 --> 00:03:46,940 Do you see how that's very, very dark? 112 00:03:47,040 --> 00:03:48,700 It's not exactly black. 113 00:03:48,820 --> 00:03:49,620 It's not zero. 114 00:03:49,840 --> 00:03:50,580 Zero is black. 115 00:03:50,680 --> 00:03:51,280 No detail. 116 00:03:51,400 --> 00:03:52,140 It's pure black. 117 00:03:52,620 --> 00:03:54,620 If we go to the highlights, you'll start 118 00:03:54,620 --> 00:03:57,060 to see where it's getting closer to that 119 00:03:57,060 --> 00:03:58,100 255 back. 120 00:03:58,680 --> 00:04:00,780 So, let's see if I've actually blown out 121 00:04:00,780 --> 00:04:01,200 anything. 122 00:04:01,380 --> 00:04:02,160 I'm just trying to see. 123 00:04:02,280 --> 00:04:03,860 As soon as we get the 255, let's 124 00:04:03,860 --> 00:04:04,500 look at that area. 125 00:04:05,120 --> 00:04:06,940 No, let me put my glasses on, actually. 126 00:04:07,460 --> 00:04:08,900 I can see this a lot better. 127 00:04:09,860 --> 00:04:11,720 So, it looks like we have pretty much 128 00:04:11,720 --> 00:04:12,560 detail everywhere. 129 00:04:12,940 --> 00:04:14,540 Now, you might say, Jerry, well, why don't 130 00:04:14,540 --> 00:04:16,600 I just shoot aperture priority in and then 131 00:04:16,600 --> 00:04:18,200 hope for the best, and then I can 132 00:04:18,200 --> 00:04:20,500 just get detail in my shadows and highlights 133 00:04:20,500 --> 00:04:22,560 and things like that. 134 00:04:22,680 --> 00:04:23,580 Well, of course you can. 135 00:04:23,700 --> 00:04:25,580 You can get more details in shadows only. 136 00:04:26,080 --> 00:04:27,440 You can lift up the mid-tones and 137 00:04:27,440 --> 00:04:28,220 all that kind of stuff. 138 00:04:28,540 --> 00:04:30,680 But can you see how we're starting to 139 00:04:30,680 --> 00:04:32,460 lose a bit of detail and we get 140 00:04:32,460 --> 00:04:33,300 a lot of grain? 141 00:04:33,920 --> 00:04:36,700 So, nothing beats an in-camera good exposure 142 00:04:36,700 --> 00:04:39,540 rather than just trying to do it after 143 00:04:39,540 --> 00:04:40,000 the fact. 144 00:04:40,260 --> 00:04:42,760 Excuse my dog barking in the background there. 145 00:04:44,020 --> 00:04:45,360 He's probably missing daddy there. 146 00:04:45,700 --> 00:04:47,920 But again, this is a good exposure. 147 00:04:48,040 --> 00:04:49,320 We have detail in skin tones. 148 00:04:49,320 --> 00:04:50,720 We have detail in highlights. 149 00:04:51,280 --> 00:04:52,120 Life is good. 150 00:04:52,600 --> 00:04:54,120 Let's go down a little bit further. 151 00:04:54,700 --> 00:04:56,460 This one here of Lisa and Dylan, I 152 00:04:56,460 --> 00:04:58,500 love the way the light is skimming off 153 00:04:58,500 --> 00:04:59,120 Dylan there. 154 00:04:59,220 --> 00:05:01,620 We've got beautiful highlights over there as well, 155 00:05:01,760 --> 00:05:03,880 deep shadows, but you can see quite clearly 156 00:05:03,880 --> 00:05:05,780 the detail in them. 157 00:05:06,240 --> 00:05:08,360 But again, if you want to increase the 158 00:05:08,360 --> 00:05:09,940 exposure, you can, but of course you're going 159 00:05:09,940 --> 00:05:10,840 to blow out the highlights. 160 00:05:11,260 --> 00:05:14,520 So, if you expose well, that exposure slider 161 00:05:14,520 --> 00:05:15,600 will hardly be touched. 162 00:05:15,600 --> 00:05:17,760 You might just want to put some detail 163 00:05:17,760 --> 00:05:18,880 in those shadows. 164 00:05:19,160 --> 00:05:22,900 Personally, I love deep, dark shadows. 165 00:05:23,100 --> 00:05:24,940 It gives us beautiful depth and dimension and 166 00:05:24,940 --> 00:05:25,280 drama. 167 00:05:25,640 --> 00:05:27,220 It's one of the signatures to my work, 168 00:05:27,280 --> 00:05:28,120 which I really love. 169 00:05:28,220 --> 00:05:29,880 Let's just keep on going down and find 170 00:05:29,880 --> 00:05:31,180 some different shots here as well. 171 00:05:31,800 --> 00:05:33,020 So again, I love the fact that we're 172 00:05:33,020 --> 00:05:33,740 playing with shadows. 173 00:05:33,880 --> 00:05:36,040 Those half shadows underneath a guy's eyes, very 174 00:05:36,040 --> 00:05:36,920 masculine, looks good. 175 00:05:37,200 --> 00:05:38,460 I wouldn't do that for a girl, so 176 00:05:38,460 --> 00:05:40,100 I make sure her eye sock is completely 177 00:05:40,100 --> 00:05:40,440 lit. 178 00:05:40,840 --> 00:05:42,960 Love the shadow on her lips. 179 00:05:42,960 --> 00:05:44,560 It makes her lips look fuller, as well 180 00:05:44,560 --> 00:05:46,440 as the shadow underneath her top lip, which 181 00:05:46,440 --> 00:05:46,980 is amazing. 182 00:05:47,440 --> 00:05:48,300 Now, let's go to this. 183 00:05:48,340 --> 00:05:49,980 This is going to be almost impossible to 184 00:05:49,980 --> 00:05:53,080 get a perfect exposure, short of actually using 185 00:05:53,080 --> 00:05:56,100 off-camera flash, balancing that light that's hitting 186 00:05:56,100 --> 00:05:57,460 behind her veil and so on. 187 00:05:57,580 --> 00:05:59,060 Now, let's put our little picker here. 188 00:05:59,680 --> 00:06:01,340 So again, let's look at the RGB there. 189 00:06:01,440 --> 00:06:04,240 So again, although I'm going to flick it 190 00:06:04,240 --> 00:06:05,780 to black and white, it still gives us 191 00:06:05,780 --> 00:06:09,240 the luminance values from 0 to 255. 192 00:06:09,660 --> 00:06:11,160 So if you can sort of see there, 193 00:06:11,260 --> 00:06:12,460 well, there's some mid-tones, right? 194 00:06:12,460 --> 00:06:13,780 Mid-tones, it's going a bit darker. 195 00:06:13,900 --> 00:06:15,280 As you can see, it's going darker and 196 00:06:15,280 --> 00:06:15,560 darker. 197 00:06:16,280 --> 00:06:18,420 Now, let's put it on the veil. 198 00:06:18,960 --> 00:06:19,400 All right. 199 00:06:19,520 --> 00:06:22,020 Do you see how it's 255? 200 00:06:22,160 --> 00:06:23,800 We actually got some clipping. 201 00:06:24,360 --> 00:06:26,880 What that basically means, clipping means that if 202 00:06:26,880 --> 00:06:29,340 you go to the end here, like you 203 00:06:29,340 --> 00:06:33,900 want to contain usually your histogram within this 204 00:06:33,900 --> 00:06:34,160 way. 205 00:06:34,260 --> 00:06:36,760 You do not want this particular part of 206 00:06:36,760 --> 00:06:39,100 the mountain, so to speak, to clip and 207 00:06:39,100 --> 00:06:40,640 to hit that side of the histogram. 208 00:06:40,640 --> 00:06:43,000 Remember, shadows, highlights. 209 00:06:43,180 --> 00:06:45,400 Remember, like you're shushing someone. 210 00:06:45,720 --> 00:06:47,580 That makes you remember that the shadows are 211 00:06:47,580 --> 00:06:49,120 on the left and the highlights on the 212 00:06:49,120 --> 00:06:49,340 right. 213 00:06:49,880 --> 00:06:53,320 Now, does this make this a disposable photograph? 214 00:06:53,460 --> 00:06:54,380 This is a bad photograph. 215 00:06:54,480 --> 00:06:55,420 Do I just get rid of it? 216 00:06:55,880 --> 00:06:57,740 Well, as far as I'm concerned, I eliminated 217 00:06:57,740 --> 00:06:59,220 distraction by cropping closer. 218 00:06:59,680 --> 00:07:01,620 Yes, these are white and bright. 219 00:07:01,780 --> 00:07:05,160 If I exposed for the highlight here, in 220 00:07:05,160 --> 00:07:07,600 other words, I want detail in that veil. 221 00:07:07,600 --> 00:07:09,260 Well, of course, that light is going to 222 00:07:09,260 --> 00:07:11,520 be nowhere near as beautiful because we actually 223 00:07:11,520 --> 00:07:13,740 use light, the sun bouncing off a wall, 224 00:07:13,880 --> 00:07:14,640 hitting her face. 225 00:07:15,420 --> 00:07:18,420 Now, yes, if you entered into this competition, 226 00:07:19,080 --> 00:07:20,580 photographers would say, well, there's no detail on 227 00:07:20,580 --> 00:07:21,000 the highlights. 228 00:07:21,220 --> 00:07:21,940 That's terrible. 229 00:07:22,160 --> 00:07:24,880 Well, don't forget that most of the time, 230 00:07:24,980 --> 00:07:26,800 guys, well, most of the time we should 231 00:07:26,800 --> 00:07:29,080 be photographing for our clients. 232 00:07:29,140 --> 00:07:31,120 We're not there to actually photograph for other 233 00:07:31,120 --> 00:07:31,560 photographers. 234 00:07:31,920 --> 00:07:33,900 So just know what you're shooting for. 235 00:07:33,900 --> 00:07:35,860 And yes, if you want to be more 236 00:07:35,860 --> 00:07:40,020 critical and actually make sure that the judges 237 00:07:40,020 --> 00:07:41,460 in a competition say, well, this is a 238 00:07:41,460 --> 00:07:42,120 perfect exposure. 239 00:07:42,580 --> 00:07:44,680 Well, is there such a thing as a 240 00:07:44,680 --> 00:07:45,540 perfect exposure? 241 00:07:45,700 --> 00:07:48,740 I believe a perfect exposure is pretty much 242 00:07:48,740 --> 00:07:51,340 the execution of your desired result. 243 00:07:51,920 --> 00:07:54,220 In this case, I'm picking the lesser of 244 00:07:54,220 --> 00:07:54,700 the evils. 245 00:07:54,860 --> 00:07:56,440 I don't care about the detail here. 246 00:07:56,800 --> 00:07:58,240 All I care about is her face looking 247 00:07:58,240 --> 00:08:01,220 amazing and having a beautiful direction of light. 248 00:08:01,220 --> 00:08:03,680 Now, can I get detail in shadows? 249 00:08:04,860 --> 00:08:07,280 You see how I'm going over here now 250 00:08:07,280 --> 00:08:08,600 that looks a little bit fake. 251 00:08:08,780 --> 00:08:10,360 You can sort of see what's happening on 252 00:08:10,360 --> 00:08:13,300 the on the fringe of that highlight there. 253 00:08:13,500 --> 00:08:15,620 I would probably say you can certainly do 254 00:08:15,620 --> 00:08:15,880 that. 255 00:08:15,960 --> 00:08:17,080 That actually looks pretty good. 256 00:08:17,400 --> 00:08:19,260 But then I would massage this in Photoshop 257 00:08:19,260 --> 00:08:21,880 later on so I don't get that unrealistic 258 00:08:21,880 --> 00:08:23,680 sort of glow that's on the outside. 259 00:08:24,160 --> 00:08:25,780 So you can see, of course, that the 260 00:08:25,780 --> 00:08:27,760 the latitude that we have when it comes 261 00:08:27,760 --> 00:08:30,400 to digital processing after the fact is just 262 00:08:30,400 --> 00:08:32,880 it makes our life so much easier. 263 00:08:33,280 --> 00:08:35,679 But I'm saying don't rely on it because 264 00:08:35,679 --> 00:08:37,820 the quality will never be as good and 265 00:08:37,820 --> 00:08:41,179 compared to a good exposure in camera under 266 00:08:41,179 --> 00:08:42,900 the circumstances and what you're photographing. 267 00:08:43,320 --> 00:08:46,220 So, like I said, we've got no no 268 00:08:46,220 --> 00:08:48,340 detail on those whites, but we can bring 269 00:08:48,340 --> 00:08:48,680 it back. 270 00:08:48,720 --> 00:08:50,020 And that's quite amazing that we can do 271 00:08:50,020 --> 00:08:50,240 that. 272 00:08:50,760 --> 00:08:52,080 Let's keep on going here. 273 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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