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These are the user uploaded subtitles that are being translated: 1 00:00:00,240 --> 00:00:02,220 last week we got into stacking with 2 00:00:02,220 --> 00:00:05,100 Cyril using scripts this week let's take 3 00:00:05,100 --> 00:00:06,779 a look at how to stack with xero without 4 00:00:06,779 --> 00:00:09,120 scripts using serial is pretty 5 00:00:09,120 --> 00:00:10,920 straightforward and this won't take long 6 00:00:10,920 --> 00:00:13,019 and while a lot of people say they find 7 00:00:13,019 --> 00:00:15,179 stacking without scripts to be somewhat 8 00:00:15,179 --> 00:00:17,039 daunting it's straightforward once you 9 00:00:17,039 --> 00:00:19,140 learn it and the detailed control yields 10 00:00:19,140 --> 00:00:21,119 the best results you're going to start 11 00:00:21,119 --> 00:00:23,760 by going to the home icon top left go 12 00:00:23,760 --> 00:00:25,680 into the select folder window and 13 00:00:25,680 --> 00:00:27,359 navigate to the folder of astrophoto 14 00:00:27,359 --> 00:00:29,640 images that you want to process click on 15 00:00:29,640 --> 00:00:32,220 the folder and select to open Ciro only 16 00:00:32,220 --> 00:00:34,140 works with fits files which are common 17 00:00:34,140 --> 00:00:36,300 in astrophotography so if you did not 18 00:00:36,300 --> 00:00:38,340 record with fits files you can convert 19 00:00:38,340 --> 00:00:40,440 them in the conversion tab the 20 00:00:40,440 --> 00:00:42,360 conversion tab is the leftmost tab and 21 00:00:42,360 --> 00:00:44,219 the control panel on the right now 22 00:00:44,219 --> 00:00:45,840 navigate to the plus button in the 23 00:00:45,840 --> 00:00:47,760 control panel and Explorer window will 24 00:00:47,760 --> 00:00:50,399 pop up select all the relevant files and 25 00:00:50,399 --> 00:00:52,920 click add the files will be added into 26 00:00:52,920 --> 00:00:56,399 the control panel ready for manipulation 27 00:00:56,399 --> 00:00:58,260 now choose a name for your converted 28 00:00:58,260 --> 00:00:59,940 files or you can leave it the same if 29 00:00:59,940 --> 00:01:01,920 you want and you can even convert to a 30 00:01:01,920 --> 00:01:04,260 fit sequence or an Ser sequence if you 31 00:01:04,260 --> 00:01:05,159 prefer 32 00:01:05,159 --> 00:01:06,900 our purposes here we're just going to 33 00:01:06,900 --> 00:01:09,780 convert to fits images once ready hit 34 00:01:09,780 --> 00:01:12,060 the convert button unless you're using a 35 00:01:12,060 --> 00:01:13,860 much older computer zero will convert 36 00:01:13,860 --> 00:01:15,780 the files very quickly we're going to 37 00:01:15,780 --> 00:01:18,960 blaze through 386 Tiff images here in 38 00:01:18,960 --> 00:01:20,159 seconds 39 00:01:20,159 --> 00:01:22,560 next up is the sequence tab in the 40 00:01:22,560 --> 00:01:24,299 control panel just to the right of the 41 00:01:24,299 --> 00:01:25,979 conversion tab but we don't have much 42 00:01:25,979 --> 00:01:27,840 use for it here that's mainly for 43 00:01:27,840 --> 00:01:29,820 manipulating large sets of images that 44 00:01:29,820 --> 00:01:31,439 will turn into something like a dark 45 00:01:31,439 --> 00:01:33,600 master in this example we won't be using 46 00:01:33,600 --> 00:01:36,420 calibration frames such as darks biases 47 00:01:36,420 --> 00:01:38,579 or flats at all we're just going to keep 48 00:01:38,579 --> 00:01:40,320 it really simple 49 00:01:40,320 --> 00:01:42,060 beside the sequence tab is the 50 00:01:42,060 --> 00:01:44,460 calibration tab as I noted earlier we're 51 00:01:44,460 --> 00:01:46,439 not going to use calibration frames this 52 00:01:46,439 --> 00:01:48,060 time if you don't already know 53 00:01:48,060 --> 00:01:51,479 calibration frames are your dark biases 54 00:01:51,479 --> 00:01:53,880 flats and potentially dark flat frames 55 00:01:53,880 --> 00:01:55,680 they are used to remove any 56 00:01:55,680 --> 00:01:57,920 imperfections in your lenses or camera 57 00:01:57,920 --> 00:02:00,479 next we need to go to the registration 58 00:02:00,479 --> 00:02:02,700 tab here is where zero will align your 59 00:02:02,700 --> 00:02:04,680 images in the control panel you'll see 60 00:02:04,680 --> 00:02:06,719 the sequence stacking options the first 61 00:02:06,719 --> 00:02:08,640 thing to choose is your method there are 62 00:02:08,640 --> 00:02:10,560 five options we won't go through them 63 00:02:10,560 --> 00:02:12,420 all here but if you hold your cursor 64 00:02:12,420 --> 00:02:14,580 over the five options for a moment a 65 00:02:14,580 --> 00:02:16,379 dynamic description will pop up that 66 00:02:16,379 --> 00:02:18,000 will show you the pros and cons of each 67 00:02:18,000 --> 00:02:20,580 option Zero's full of these Dynamic 68 00:02:20,580 --> 00:02:22,560 menus they make it very user friendly 69 00:02:22,560 --> 00:02:24,720 they're well worth stopping and taking a 70 00:02:24,720 --> 00:02:26,220 moment to read in order for you to 71 00:02:26,220 --> 00:02:28,080 understand what the various options do 72 00:02:28,080 --> 00:02:31,080 and if you're unsure experiment try 73 00:02:31,080 --> 00:02:33,000 stacking one way in then another or 74 00:02:33,000 --> 00:02:34,980 aligning one way and then another and 75 00:02:34,980 --> 00:02:36,660 you'll learn a lot about how it works 76 00:02:36,660 --> 00:02:39,060 for our purposes here we're going to go 77 00:02:39,060 --> 00:02:41,640 with two pass Global alignment it uses 78 00:02:41,640 --> 00:02:43,739 multiple stars to give a very accurate 79 00:02:43,739 --> 00:02:45,780 alignment and it also allows us to 80 00:02:45,780 --> 00:02:47,580 choose which frame we want to use as our 81 00:02:47,580 --> 00:02:49,560 frame of reference for stacking 82 00:02:49,560 --> 00:02:51,840 personally I find this to be the most 83 00:02:51,840 --> 00:02:53,700 useful option and use it pretty much as 84 00:02:53,700 --> 00:02:55,019 my default 85 00:02:55,019 --> 00:02:57,060 having picked two-star alignments we're 86 00:02:57,060 --> 00:02:59,220 going to pop back over to the sequence 87 00:02:59,220 --> 00:03:02,220 Tab and pick open frame list and from 88 00:03:02,220 --> 00:03:03,720 there we're going to choose which frame 89 00:03:03,720 --> 00:03:06,360 is best or at least seems best to use as 90 00:03:06,360 --> 00:03:08,400 the reference frame this video is only 91 00:03:08,400 --> 00:03:10,200 for demonstration purposes so I'm not 92 00:03:10,200 --> 00:03:12,180 going to put too much effort into this I 93 00:03:12,180 --> 00:03:14,580 think frame 17 looks pretty good just a 94 00:03:14,580 --> 00:03:16,260 little bit more contrast detail there 95 00:03:16,260 --> 00:03:18,659 probably just due to momentary favorable 96 00:03:18,659 --> 00:03:21,120 atmospheric conditions but whatever that 97 00:03:21,120 --> 00:03:22,739 frame is good enough for here for 98 00:03:22,739 --> 00:03:24,420 registration Channel while we're working 99 00:03:24,420 --> 00:03:26,040 with a monochrome image so our only 100 00:03:26,040 --> 00:03:28,260 option here is luminance if you are 101 00:03:28,260 --> 00:03:29,879 working with color you could pick one of 102 00:03:29,879 --> 00:03:32,040 the color channels as well for the 103 00:03:32,040 --> 00:03:33,720 transformation Channel you have four 104 00:03:33,720 --> 00:03:36,599 options the default is homography with 105 00:03:36,599 --> 00:03:38,940 eight degrees of freedom moving up you 106 00:03:38,940 --> 00:03:41,879 have a fine or a fiend similarity and 107 00:03:41,879 --> 00:03:44,640 shift at the very top each one of those 108 00:03:44,640 --> 00:03:47,099 removes two degrees of freedom and each 109 00:03:47,099 --> 00:03:49,080 has less and less tolerance for error 110 00:03:49,080 --> 00:03:51,060 we're going to go with the shift option 111 00:03:51,060 --> 00:03:53,459 which is ideal for images with no 112 00:03:53,459 --> 00:03:55,560 scaling Distortion or field rotation 113 00:03:55,560 --> 00:03:57,480 none of which are in our set of images 114 00:03:57,480 --> 00:04:00,060 but if the images that you wish to stack 115 00:04:00,060 --> 00:04:02,340 have lost precise mapping you might want 116 00:04:02,340 --> 00:04:04,200 to use tomography or one of the other 117 00:04:04,200 --> 00:04:06,120 options below shift 118 00:04:06,120 --> 00:04:08,159 in the image selection section you can 119 00:04:08,159 --> 00:04:09,959 choose to use all the images in your 120 00:04:09,959 --> 00:04:11,939 stack or you can navigate back to the 121 00:04:11,939 --> 00:04:13,799 sequence Tab and go to the open frame 122 00:04:13,799 --> 00:04:16,139 list again and remove any images you 123 00:04:16,139 --> 00:04:18,479 consider entirely unsuitable once you've 124 00:04:18,479 --> 00:04:20,579 made your selection go ahead and hit go 125 00:04:20,579 --> 00:04:22,740 register Cyril will now begin the 126 00:04:22,740 --> 00:04:24,479 process of aligning all the images in 127 00:04:24,479 --> 00:04:26,639 your stack this could take only a few 128 00:04:26,639 --> 00:04:28,560 moments or a few minutes it depends on 129 00:04:28,560 --> 00:04:30,780 how many you have in our case it'll take 130 00:04:30,780 --> 00:04:32,220 a minute or two so we'll just go ahead 131 00:04:32,220 --> 00:04:34,560 and jump ahead when it's done you can go 132 00:04:34,560 --> 00:04:36,000 ahead and jump to the plotting if you're 133 00:04:36,000 --> 00:04:37,259 curious and see if there are any 134 00:04:37,259 --> 00:04:38,940 particular images you may want to remove 135 00:04:38,940 --> 00:04:40,560 from the sequence before you begin 136 00:04:40,560 --> 00:04:43,080 stacking I see a few rough ones in mind 137 00:04:43,080 --> 00:04:44,759 but none I'm going to bother with for 138 00:04:44,759 --> 00:04:46,320 the purposes of this informational 139 00:04:46,320 --> 00:04:49,979 session now at last the stacking under 140 00:04:49,979 --> 00:04:51,840 the stacking tab the first option is to 141 00:04:51,840 --> 00:04:53,880 pick your method you could go with some 142 00:04:53,880 --> 00:04:56,759 method many persons do and it works okay 143 00:04:56,759 --> 00:04:58,860 but it's not quite the same thing as 144 00:04:58,860 --> 00:05:01,259 saying it works well what we want to use 145 00:05:01,259 --> 00:05:03,660 here is average with rejection which 146 00:05:03,660 --> 00:05:05,580 performs several types of clipping that 147 00:05:05,580 --> 00:05:08,040 will work as error correction and do a 148 00:05:08,040 --> 00:05:09,960 heck of a lot to clean up the noise in 149 00:05:09,960 --> 00:05:12,300 the slow information set of images after 150 00:05:12,300 --> 00:05:13,680 you've picked through method you have to 151 00:05:13,680 --> 00:05:15,479 choose your normalization you have 152 00:05:15,479 --> 00:05:18,180 additive multiplicative and additive and 153 00:05:18,180 --> 00:05:20,699 multiplicative with scaling the scaling 154 00:05:20,699 --> 00:05:22,259 versions give us a better signal to 155 00:05:22,259 --> 00:05:24,060 noise ratio so we're going to go with 156 00:05:24,060 --> 00:05:26,340 additive with scaling we generally 157 00:05:26,340 --> 00:05:27,900 always want to choose to increase the 158 00:05:27,900 --> 00:05:29,759 signal to noise ratio 159 00:05:29,759 --> 00:05:31,320 from there you'll have to pick your 160 00:05:31,320 --> 00:05:33,720 preferred pixel rejection technique once 161 00:05:33,720 --> 00:05:35,699 again the dynamic menus give you an idea 162 00:05:35,699 --> 00:05:37,380 of which you should use as we are 163 00:05:37,380 --> 00:05:38,520 working with several hundred images 164 00:05:38,520 --> 00:05:40,320 we'll use the generalized extreme 165 00:05:40,320 --> 00:05:42,360 student deviate test 166 00:05:42,360 --> 00:05:44,520 and last we have to pick our weighing 167 00:05:44,520 --> 00:05:46,800 method as always the dynamic menu should 168 00:05:46,800 --> 00:05:48,360 give you a good idea which option will 169 00:05:48,360 --> 00:05:50,400 work best for you I'll pick noise since 170 00:05:50,400 --> 00:05:52,380 I want to minimize the noise in this low 171 00:05:52,380 --> 00:05:55,199 information image and that's it now we 172 00:05:55,199 --> 00:05:57,419 can stack here's where the magic happens 173 00:05:57,419 --> 00:06:00,419 and that hard one sequence of dozens 174 00:06:00,419 --> 00:06:02,520 maybe hundreds perhaps even thousands of 175 00:06:02,520 --> 00:06:04,919 images transforms into an 176 00:06:04,919 --> 00:06:06,600 astrophotograph 177 00:06:06,600 --> 00:06:08,580 this is going to take a few minutes so 178 00:06:08,580 --> 00:06:10,080 we'll go ahead and Skip ahead and take a 179 00:06:10,080 --> 00:06:12,240 look at the final results 180 00:06:12,240 --> 00:06:14,160 so our stack is just now coming to 181 00:06:14,160 --> 00:06:16,380 completion when it completes we'll go to 182 00:06:16,380 --> 00:06:18,960 the open Button top left click it and 183 00:06:18,960 --> 00:06:21,120 find the appropriate file you'll know it 184 00:06:21,120 --> 00:06:23,160 because it'll bear the suffix underscore 185 00:06:23,160 --> 00:06:26,160 stacked dot fit now deep Sky objects are 186 00:06:26,160 --> 00:06:28,139 dim so you'll still have to develop the 187 00:06:28,139 --> 00:06:29,940 image to properly see it but at the 188 00:06:29,940 --> 00:06:31,979 bottom center right of zero we can go to 189 00:06:31,979 --> 00:06:34,139 the display mode options and pick Auto 190 00:06:34,139 --> 00:06:36,360 stretch which gives us a quick rough 191 00:06:36,360 --> 00:06:38,699 idea of what our finished image can look 192 00:06:38,699 --> 00:06:39,479 like 193 00:06:39,479 --> 00:06:42,300 there we go we just saw that dim little 194 00:06:42,300 --> 00:06:44,940 hazy spot in the sky turn into a Galaxy 195 00:06:44,940 --> 00:06:46,620 now I'm going to crop out the 196 00:06:46,620 --> 00:06:48,960 imperfections along the Ridge and do a 197 00:06:48,960 --> 00:06:50,460 really quick edit on this to show you 198 00:06:50,460 --> 00:06:52,919 that with Cyril with some basic stacking 199 00:06:52,919 --> 00:06:54,660 technique even without calibration 200 00:06:54,660 --> 00:06:56,880 frames and even without a heck of a lot 201 00:06:56,880 --> 00:06:59,039 of captured information you can get some 202 00:06:59,039 --> 00:07:01,440 very beautiful final results so we're 203 00:07:01,440 --> 00:07:03,000 just going to pop up to the histogram 204 00:07:03,000 --> 00:07:05,039 transformation option and do a quick 205 00:07:05,039 --> 00:07:07,319 auto stretch this will give us a good 206 00:07:07,319 --> 00:07:08,940 sense of what the light of our galaxy 207 00:07:08,940 --> 00:07:10,620 should look like it's pretty close I 208 00:07:10,620 --> 00:07:12,240 think to the maximum that we want the 209 00:07:12,240 --> 00:07:14,039 light now we're going to play with the 210 00:07:14,039 --> 00:07:16,080 black level a bit via the generalized 211 00:07:16,080 --> 00:07:18,660 hyperbolic stretch transformation option 212 00:07:18,660 --> 00:07:20,520 and then adjust the Black Level just a 213 00:07:20,520 --> 00:07:23,280 little bit more via the Asin or a side 214 00:07:23,280 --> 00:07:24,660 option I'm not quite sure how to 215 00:07:24,660 --> 00:07:26,340 pronounce it 216 00:07:26,340 --> 00:07:28,440 I started to run a noise removal routine 217 00:07:28,440 --> 00:07:30,720 but quickly removed it the routine 218 00:07:30,720 --> 00:07:32,340 mistooks some of the beautiful contrast 219 00:07:32,340 --> 00:07:35,039 and detail within the Galaxy for noise 220 00:07:35,039 --> 00:07:37,319 so instead I'm just going to fine tune 221 00:07:37,319 --> 00:07:39,900 my black level just a little bit then 222 00:07:39,900 --> 00:07:41,460 we'll apply just a few more quick 223 00:07:41,460 --> 00:07:43,740 touch-ups and it's starting to look 224 00:07:43,740 --> 00:07:46,199 about like we want it to look stacked in 225 00:07:46,199 --> 00:07:49,319 developing zero in just about 15 minutes 226 00:07:49,319 --> 00:07:51,120 so next time you're stacking you could 227 00:07:51,120 --> 00:07:52,800 use scripts if you want the scripts are 228 00:07:52,800 --> 00:07:54,840 fast and convenient but if you really 229 00:07:54,840 --> 00:07:57,180 want to maximize the power of serum 230 00:07:57,180 --> 00:07:59,340 cereal is an incredibly powerful tool 231 00:07:59,340 --> 00:08:01,680 learn how to stack manually it's not 232 00:08:01,680 --> 00:08:04,199 that hard and for the detail and control 233 00:08:04,199 --> 00:08:06,300 that it gives you with a little practice 234 00:08:06,300 --> 00:08:07,860 you can really get some incredible 235 00:08:07,860 --> 00:08:09,000 results 236 00:08:09,000 --> 00:08:10,979 thank you for watching and if you 237 00:08:10,979 --> 00:08:12,840 appreciate these tutorials and the 238 00:08:12,840 --> 00:08:15,060 educational materials on astronomy via 239 00:08:15,060 --> 00:08:17,039 the sky story Channel don't forget to 240 00:08:17,039 --> 00:08:18,840 hit that like button and please take a 241 00:08:18,840 --> 00:08:21,740 moment to subscribe17248

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