Filters & Calibration Frames

A filter wheel is only as usable as its labels. ARIS lets you name and color every slot, carry per-filter focus offsets so filter changes don’t cost you a focus run, and shoot calibration frames as ordinary sequence steps.

Filter slot names and colors

Edit each slot’s name and color in ARIS — “Ha”, “OIII”, “L” instead of “Slot 3”. The names and colors follow the filters everywhere: sequence plans, capture controls, file organization, and focus offsets all speak in your labels.

Where the edits persist depends on the rig type:

• INDI rigs — slot names and colors are saved in the rig’s equipment profile, on the rig itself.
• NINA rigs — edits persist into your NINA profile, so NINA and ARIS always agree on what lives in the wheel. See NINA Integration.

Per-filter focus offsets

Different filters focus at slightly different points. Store an offset per slot and ARIS applies it automatically on every filter change during a sequence — the focuser moves by the offset difference and imaging continues, no autofocus run required for the swap.

Offsets also power the autofocus filter-swap option: run autofocus through your chosen filter (typically luminance, where stars are brightest), then let the offset place narrowband filters at their correct focus. Sequences with an Ha/OIII/SII rotation stop paying a full focus run at every change.

Tip

Measure offsets on a night of decent seeing: run autofocus through each filter back-to-back and note the best-focus positions. The differences are your offsets, and they stay valid until the optical train changes.

Darks, flats, and bias in sequences

Calibration frames are first-class sequence steps. Add a dark, flat, or bias block to a plan just like a light block — count, exposure, binning, filter where relevant — and the runner executes it in order, waiting for every calibration frame to actually complete before moving on.

That completion-wait matters for unattended nights: an end-of-plan dark library shoots reliably after the last light, with no babysitting, and the frames land in your file tree organized by type. A common plan shape is lights through the night with a calibration block at the end, when you are asleep and the optics are still at temperature.

Flat wizard

Flats want a specific signal level, and dialing panel brightness and exposure per filter by hand is tedious. The flat wizard does it for you: with a flat panel connected, it measures the signal at multiple brightness levels and finds the brightness/exposure pair that hits the target level for each filter. The results are saved to your equipment profile, so future flat runs reuse the calibration instead of re-deriving it.

Cover guard

Some motorized flat-panel covers close themselves when they power up. ARIS guards against the resulting silent disaster: before light frames, it checks the cover and automatically opens a closed one — so a power blip at dusk cannot turn your imaging run into a night of exposures against the inside of a lid.

The same logic works in your favor for calibration: flats run against the closed, lit panel, and the cover state is managed as part of the sequence rather than by memory.