The Wiper Gold competes against the Capintec Caprac and other single-well counters on form factor, footprint, and bench presence. What separates them is qualitative — capabilities that a spec column can’t convey but that change the actual work. Here are four of them, made visceral.
Interactive Walkthrough8 min readLTI Engineering — for buyers comparing the Wiper Gold to a Capintec Caprac
Two single-well wipe-test counters can look identical on a desk. Buyers who don’t use one every day often default to the lower-priced option. This walkthrough is for that buyer — the four capabilities below are the differences that show up after the purchase order is signed, and the differences that justify the choice up front.
01
Resolution that matters.
4096 channels vs. the competitive deck
A multi-channel analyzer (MCA) divides the 0–1 MeV energy range into individual “channels.” More channels = finer resolution = sharper peaks, cleaner identifications, more reliable analysis. The Wiper Gold has 4096 channels. Most competitors at this price point have 256 or 64. Here’s the difference, applied to a thing your eyes already know how to evaluate.
4096 channels — the Wiper Gold. You can read the antenna on Willis Tower. You can see the windows on the Marina City corncobs. You can pick out the bridge structure over the river. This is what the Wiper Gold sees in your wipe spectrum.
Click the buttons above to see what 256 and 64 channels do to the same image. The detail you lose isn’t cosmetic — in a real spectrum it’s the difference between resolving Tc-99m (140 keV) cleanly from a Mo-99 breakthrough sitting next to it, or seeing them as one indistinct hump. It’s the difference between identifying an unknown contamination from its photopeak signature, or shrugging.
02
More crystal mass below the well — where stopping power lives.
1″¼ deep well in a 2″⅛ long crystal vs. 1.5″ deep well in a 1.75″ long crystal — and why F-18 cares
Gamma rays don’t deposit their energy in a crystal by magic. They have to travel through enough crystal mass to interact — the higher the energy, the more crystal it takes. Stopping power is everything at high energies. The Wiper Gold uses a 1″⅛ × 2″⅛ NaI(Tl) crystal with a 0.67″ wide × 1″¼-deep well, leaving ⅞ of an inch of crystal directly below the sample. The Capintec Caprac uses a 1.5″×1.75″ detector with a 0.67″×1.5″ well — the well runs nearly the full length of the crystal, leaving only 0.25″ of crystal below the sample. 3.5× more stopping mass where it matters most.
The asymmetric design is deliberate. The Wiper Gold detector is longer than it is wide — while Capintec’s is wider than it is long. Capintec’s extra side-of-well crystal might sound like an advantage, but side mass stops contributing usefully above I-125 (35 keV). At clinical-isotope energies — Tc-99m (140 keV), F-18 (511 keV), Cs-137 (662 keV), Co-57 (122 keV) — gammas going out the side interact even in a thin crystal. So Capintec’s extra side mass is wasted at every energy you actually count. What matters at high energies is the crystal mass below the sample, where gammas heading downward have to travel through enough material to be stopped. LTI puts the crystal where it does the most work.
Capintec Caprac — 1.5″×1.75″ detector, 0.67″×1.5″ well
~8% stopped — 1 of 12
0.25 in. of crystal below the sample
The well runs nearly the full length of the detector. Almost no crystal mass below the sample to stop high-energy gammas. F-18, Cs-137, and Co-57 photons pass straight through the thin crystal floor without interacting. Lost counts. Lower DPM accuracy. Underreported activity at the energies that matter for PET work.
Wiper Gold — 1″⅛×2″⅛ detector, 0.67″×1″¼ well
~25% stopped — 3 of 12
⅞ in. of crystal below the sample
3.5× the stopping mass below the well. High-energy gammas have meaningfully more material to interact with on their way through. The result: > 80 % efficiency on Co-57 and meaningfully better F-18 / 511 keV performance than the wider-but-shorter Capintec design.
This isn’t marketing. It’s the geometry of how a NaI(Tl) crystal actually works. Look at the crystal-mass numbers on any single-well counter spec sheet — the ones that publish them. Then look at the published efficiency curves at 511 keV. The math always lines up. We’re just one of the few willing to put both numbers on the page.
03
Real DPM, on any isotope — not a fudge factor.
AutoSpect™ Spectrum Compensation vs. flat-percentage approximations
Most counters report DPM by applying a single flat percentage efficiency per isotope — a fudge factor the manufacturer pre-calculated for the isotopes shipped in the library. Want to count an isotope not in the library? You can manually enter your own fudge factor — and live with whatever accuracy that produces. The Wiper Gold doesn’t work that way.
The flat-fudge-factor approach
Most counters at this price point
Manufacturer assigns one efficiency number per isotope
Same fudge factor across the entire energy range
Doesn’t account for crystal-efficiency variation between isotope energies
Doesn’t account for per-isotope gamma abundance
Counting an isotope not in the library? Enter your own number and hope.
Result: approximate DPM. Often good enough for Pass/Fail at trigger. Not good enough for inspector-grade reporting on isotopes the manufacturer didn’t pre-calibrate.
AutoSpect™ + Spectrum Compensation — two stages, real physics
Wiper Gold
Stage 1 — AutoSpect™ corrects the spectrum per keV. A NaI(Tl) crystal isn’t equally efficient at every energy. AutoSpect compensates for that loss across the entire energy range, so the corrected spectrum represents what would be captured as if the sample were encapsulated inside the crystal and every gamma emitted was detected.
Stage 2 — Spectrum Compensation applies gamma abundance per peak. Most isotopes emit gammas at multiple energies (Na-22 at 511 and 1274 keV; I-131 at 364, 637, 723 keV; etc.). Each peak has its own gamma abundance — the fraction of decays that produce a gamma at that specific energy. The Wiper Gold's library entry windows around one peak and applies that peak’s abundance — back-calculating from the windowed count rate to true DPM for the whole isotope. (Example: I-131’s 364 keV peak has 81% abundance; entering 81% in the library lets the system convert 364 keV counts into total I-131 decays.)
The output: true DPM — the actual decay rate of the sample, not a count rate adjusted by a fudge factor.
Works on any gamma-emitting isotope from 1 keV to 1 MeV — including isotopes the lab adds itself. Add the energy windows and the gamma abundance, and the Wiper Gold gives you accurate DPM immediately.
Same calibration source (Cs-137, Na-22, or Co-57) drives the whole thing.
Result: real DPM on any isotope you put in. Inspector-grade. Defensible against any audit. No isotope-specific calibrated-source purchase required for routine work.
The Co-60 case — DPM on isotopes whose main peaks are above the Wiper Gold’s 1 MeV range.
The Wiper Gold’s MCA tops out at 1 MeV. Co-60’s dominant photopeaks (1173 keV and 1332 keV) are both above that range — so most counters would say “Co-60 is out of scope.” The Wiper Gold quantifies it anyway, by counting the 511 keV annihilation peak that Co-60 produces inside the crystal via pair production. (Co-60’s high-energy gammas convert into electron-positron pairs in the NaI; the positron annihilates and produces two 511 keV photons that the detector sees.) The effective abundance of that peak is empirically calibrated for the Wiper Gold’s specific crystal geometry and stored in the isotope library. The result: real DPM on Co-60, on an instrument whose direct measurement range tops out below Co-60’s primary emissions.
The visible difference shows up on the spectrum itself. Below: the same Cs-137 measurement with and without AutoSpect applied. The corrected version is what the spectrum would look like if the sample were perfectly captured by the crystal at every energy — that’s the spectrum your inspector and your isotope-ID software actually want to see. From there, the per-isotope Spectrum Compensation step does the math from gammas to disintegrations, and the result is DPM you can trust.
Raw spectrum Cs-137, no compensationAutoSpect™ compensated
04
A multi-channel analyzer that would otherwise cost $20,000+.
Full PHA toolkit — built into the wipe counter
A standalone laboratory MCA — a dedicated rack-mount instrument with full Pulse Height Analysis (PHA), Region of Interest (ROI) selection, peak identification, FWHM calculation, baseline subtraction, and dead-time correction — runs $15,000 to $25,000 on the open market. Most labs that need MCA-grade analysis budget for a separate piece of equipment, on a separate bench, with separate maintenance. The Wiper Gold has all of that built into the wipe counter itself.
📊
Region of Interest (ROI)
Drag region edges across the live spectrum, define multiple ROIs simultaneously, get integrated counts and net activity per region.
🔍
Peak ID
Identify peaks against the stored isotope library. Useful for unknown-contamination forensics on routine wipes.
📐
FWHM
Full Width at Half Maximum measurement on any peak in the spectrum. Resolution diagnostics, calibration verification, detector aging tracking.
📉
Baseline subtraction
Automated background subtraction across user-defined regions. Cleaner peak integration, more accurate net counts.
⏱️
Dead-time correction
Automatic correction at high count rates. The Wiper Gold handles count rates well into the hundreds of thousands of cps without paralysis.
🎯
Marker positioning
Cursor-driven energy/channel readout. Useful for spectrum interpretation, calibration verification, peak identification on the fly.
The MCA isn’t a feature on a feature list. It’s a separate instrument’s worth of capability shipping in the same chassis as the wipe counter — for the same total cost as a single-well wipe counter without an MCA. Customers who don’t need PHA capability never use it. Customers who do (radiation safety officers, university research labs, nuclear pharmacies handling unusual contamination) report it as the single feature that justifies the purchase.
None of this is on a spec sheet.
Spec sheets compare on numbers that are easy to print — channel count, well dimensions, weight, dimensions, calibration source. The four capabilities above are the differences that matter day-to-day, after the instrument is on the bench. They’re harder to explain in a column-vs-column comparison, which is why most buyers default to price.
If you want to talk through your specific application — what isotopes you count, what energy range you actually need, whether the MCA capability matters for your QA program — call us. We’re the people who designed the instrument, not a sales channel.
Sources: Wiper Gold Operator's Manual 2.0.0; LTI Engineering specifications; published Capintec Caprac product datasheet (Mirion / Capintec). Capintec® and Caprac® are trademarks of Mirion Technologies; LTI is not affiliated with Mirion.Wiper Gold product page →