How long to image the M106 with the DwarfLab DWARF II

From a Bortle 6 suburban sky, the DwarfLab DWARF II needs about 3 h 42 min (887 subs of 15 s) for a solid image of the M106. A quick look takes 55 min; a showpiece 15 h. Under a Bortle 3 rural sky the solid figure drops to 1 h 53 min. At Bortle 6 the limit is a mix of skyglow and read noise. In this scope's field it fills 18% of the frame’s short side.

M106 with the DwarfLab DWARF II: 15 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site26 min103 subs1 h 42 min409 subs6 h 49 min1,635 subs
Bortle 2Typical dark site26 min106 subs1 h 46 min424 subs7 h 03 min1,694 subs
Bortle 3Rural28 min113 subs1 h 53 min452 subs7 h 31 min1,805 subs
Bortle 4Rural / suburban transition32 min130 subs2 h 10 min519 subs8 h 38 min2,074 subs
Bortle 5Suburban39 min157 subs2 h 36 min625 subs10 h2,500 subs
Bortle 6Bright suburban55 min222 subs3 h 42 min887 subs15 h3,546 subs
Bortle 7Suburban / urban transition1 h 27 min347 subs5 h 46 min1,385 subs23 h5,539 subs
Bortle 8City2 h 15 min540 subs9 h2,159 subs36 h8,634 subs
Bortle 9Inner city3 h 58 min953 subs16 h3,809 subs63 h15,234 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 4 h 48 min of run time. The DWARF II’s battery is rated at about 3 h, so the session needs an external power bank. (Bortle 6, solid image; we allow 30% over the integration time.)

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How it frames

The M106 is 19′ × 8′ across. The DWARF II frames 3.19° × 1.79° at 2.99″ per pixel, so it fills 18% of the frame’s short side.

About the M106

A big, bright spiral with anomalous red arms driven by its black hole. Dual-band brings the extra arms out.

NGC 4258 · Galaxy in Canes Venatici · magnitude 8.4 · 19′ × 8′ · best in Mar, Apr, May. Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.

Galaxies are broadband targets: their light is mostly starlight spread across the spectrum, so a dual-band filter throws most of it away and makes things slower, not faster. Shoot without a filter (or with a plain UV/IR cut) and rely on total time and a dark sky. The core of a galaxy is usually many times brighter than its outer disc, so a short stack shows the nucleus long before the arms; the figures here are for the arms and disc, not the core.

Field rotation in Alt-Az mode crops the edges of the stack over a long session, so on a big galaxy re-centre now and then or use EQ mode where your scope supports it.

About the DwarfLab DWARF II

The original pocket scope. 24 mm aperture and tiny 1.45 µm pixels mean it is slow per pixel, so bin or downsample and be patient.

15 s is the hard maximum in any mode; DwarfLab recommends EQ mode at 15 s. Two built-in filters, VIS and Astro (IR-pass); no dual-band. The optional UHC filter is no longer sold.

The DWARF II uses fixed 15 s subs, so the only levers you have are the sky you shoot from, the filter, and total time.

Stack across nights. Every smart scope app can continue a stack or you can combine the saved frames on a computer; the figures here are totals, not single-session limits.

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Imaged the M106 with your DWARF II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M106 from a DWARF II? Email it with your total time and sky to [email protected] and it goes here, credited.

Same target, other telescopes

All telescopes for the M106 · All targets for the DWARF II