Color management in Resolve, actually explained.

It’s the math that converts your log footage into whatever space you work in, then converts that into your output space. That’s it. Any camera-manufacturer LUT that takes S-Log3 to Rec.709 is doing this: a crude, one-step version of it. The node-level setup below is the same idea, done in two deliberate steps instead of one, so you get a working space to grade in between them.

This guide covers node-level color management: you build the CST yourself, on the clip or the group. Resolve also has a project-level mode that automates this. Node-level is worth learning first because it shows you what project-level is automating for you, and that’s its own guide.

Project Settings → Color Management is where you set the working space every input CST in your node trees will target. In this project that’s DaVinci Wide Gamut / DaVinci Intermediate (DWG/DI), set as the Timeline Color Space. You can use others, but whatever you pick here has to match every input CST’s output, or the math downstream is wrong.

Input CST = camera log space → working space. Output CST = working space → delivery space. Also referred to as an IDT (Input Device Transform), and ODT (Output Device Transform).

One setting worth changing while you’re in there: 3D lookup table interpolation sometimes defaults to Trilinear. Set it to Tetrahedral instead: better LUT interpolation, no downside.

Nearly every modern camera has its own log space: S-Log3, LogC3, whatever. The CST (color space transform) maps that into your working space, so footage from different cameras can be graded, shot-matched, and balanced the same way. (You can use “Use Timeline” on the CST’s output to automate matching it to your project’s timeline color space. I have trust issues, so I set it manually.)

The CST is a per-camera fact, not a per-shot decision: every clip from the same camera needs the identical transform. Set it on one clip, then apply it to the rest without touching each one by hand: select every clip from that camera (a saved smart filter makes this a one-click selection, see Lightbox below), right-click the one you set up, Apply Active Layer. Or right-click the CST node and set it as a shared node before applying it: every clip sharing that node updates together the moment you change it, no reapplying needed later.

A group gives you two extra node trees around the clip: a pre-clip that runs before every shot’s own corrections, and a post-clip that runs after. With the CST already handled by the node stack above, groups are free for one job: the look.

Click a node: this is the actual node tree, left to right, the way it reads in Resolve.

Because every clip lands in the same DWG/DI space before the group ever touches it, the post-clip can treat a red-camera shot and a Sony shot identically. That’s the payoff: one look decision covers a whole scene, mixed cameras included, because by the time the look sees any of them, they’re already speaking the same language.

This is what the group post-clip and the timeline node are actually for, and it borrows straight from how a film lab works: different scenes get shot on different negative stocks depending on what they need, then the whole reel gets printed through one consistent print stock. The negative can vary. The print doesn’t.

In Resolve, the negative is the group post-clip: run EMBR in Digital to Negative, then pick a stock for that scene. Because every clip in the group already arrived in DWG/DI regardless of camera, that one stock choice grades the whole scene at once, and different scenes can carry different negatives without looking like they belong to different projects. The look doesn’t stop at the stock, either: scene-level adjustments, printer lights, an overall balance or contrast move for that scene, live here too, inside EMBR or in extra nodes in the same group post-clip tree.

A print LUT isn’t the only way to keep a piece cohesive across scenes, you can grade for consistency scene to scene without ever touching one. What it buys you is a single, mechanical way to lay one consistent DNA over everything downstream of it, e.g. Resolve’s bundled Rec.709 Kodak 2383 (pick a white point, D55, D60, D65), even across scenes that were graded differently at the group level.

The print also does more than add a look: properly prepped, it performs the working-space-to-display transform too, the same job the output CST does. That’s why the typical DWG/DI → Rec709/Cineon CST doesn’t hold up as a terminal step on its own; Resolve’s Film LUTs are not meant for Rec709 primaries, which is why the colors don’t map as cleanly as the Digital to Negative transform built into EMBR’s DCTL and OFX. Use a properly prepped print LUT as your last node and you don’t need a separate output CST after it. The two usually aren’t paired, pick one.

Where it sits changes what it touches. At the timeline level, one print LUT catches everything downstream, including graphics and titles, which isn’t always what you want. Make it a shared node instead and drop it as the last node in each scene group’s post-clip, and it does the same job scoped to just that group’s clips, protecting anything at the timeline level that shouldn’t get the print treatment.

None of this is mandatory. You can finish a look entirely at the scene level and skip film emulation altogether, or do the whole grade at the timeline level with no groups at all. This is one way to work, the way that’s been working, not the only correct shape for the node tree.

Top right corner. Lightbox shows every clip in the timeline as a grid you can size, inspect, and sort: the fast way to find which clips belong to which camera before you start assigning groups, especially once a timeline has more than a handful of shots.

The left-side panel sorts and filters: by media pool bin, by flag or color tag you set on clips, or by a smart filter you build. One worth setting up: a filter for “no group” (every clip that hasn’t been assigned to a group yet). Run it after you think you’re done and it catches anything you missed.

From here, select every clip that shares a camera (click first, shift-click last, or sort by bin first) and add them into a group in one pass, instead of hunting through the timeline shot by shot.

The export matching what you see in Resolve comes down to three things: how you’re viewing the image, whether Resolve’s viewer matches your display, and what the file says about itself on the way out. The first two are this section. The third is output tagging, next.

The third thing: what the file says about itself. A tag tells whatever opens it which curve to assume. You set it on the Deliver page.

An NCLC tag isn’t “what space is this file in.” It’s an instruction to whatever decodes the file: assume this transfer curve. Two tags matter for most delivery:

Becasue there are so many different potential hardware and software and delivery combinations, its worth testing on your own setup before treating a particular combination as law: render a test file, upload it to the platform you’re delivering to, and check it on the devices you expect your audience to use. If you see a shift, swap the tags. Simple as that.

To confirm what actually landed on an exported file, check it in Finder: select the file, Get Info, Color profile.

Keep this to the tag, not the pixels. Grade and monitor at true Rec.709 gamma 2.4, calibrated, same as always, and render at that same 2.4. The only thing that changes for a 1-13-1 delivery is the Gamma Tag, set to sRGB. That’s an instruction, not a pixel remap: you’re not baking a different curve into the file, you’re telling whatever decodes it to assume one. Switching Resolve’s actual output curve to its own sRGB option instead of leaving it at 2.4 does the remap for real, which skips the tag doing its job and isn’t necessary for a safe 1-13-1 delivery.

One trap on the Deliver page: “Same as Project” follows the Timeline Color Space in a DaVinci YRGB project, so with a DWG/DI timeline it does not give you a Rec.709 tag. Set the Color Space Tag and Gamma Tag explicitly, as above. In a color-managed project, Same as Project follows the Output Color Space instead.

On Instagram: sRGB as the output gamma tag (2.2 gamma) can read slightly more accurate on Instagram and a few other apps that decode a little differently than YouTube does. If your Instagram exports look more contrasty and darker than what you graded, that’s the first thing to try.

None of this guarantees pixel-identical playback everywhere. YouTube, Vimeo, Instagram, and TikTok all decode slightly differently, and that’s not fixable from your end. The goal is a calibrated, zero baseline: tag correctly, and whatever drift remains is the platform’s, not a mistake you made.

This is node-level setup: you build the CST and manage the transforms by hand, into whatever working space you land on. That’s the same idea EMBR’s OFX tool uses for its own Input Color Space setting. Point it at the space you built your CST into (DWG or otherwise) and the tool receives exactly what it expects, no extra transform needed. The DCTL kit is narrower: those are built and locked to DWG/DI specifically, so if you’re working with the DCTLs, that’s the working space to standardize your project on. See how EMBR manages color or go see what EMBR does.