ITM03; LHO ITMx Post O2 inspection LIGO-T v1

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ITM03; LHO ITMx Post O2 inspection LIGO-T1800013-v1 A feature was found at the location predicted by TCS. This feature is highly absorbing. This feature was present in the scans of the optic as received from the coater. No other absorbers over 20 ppm were found in the center 60 mm of the optic. Authors: G. Billingsley, L. Zhang January 2018 G Scatter

Experimental process Scatter measurement - The map before installation: measured after First Contact cleaning with ion gun. The map after O2: measured as-returned from LHO, no cleaning Cleaning with ion gun because there was some dust visible when checking with a flash light. Gentle absorption: the measurement was carried out with a beam of 0.3mm in diameter and 0.9W, i.e. 12.7W/mm^2. The lower limit of sensitivity for this scan was about 20ppm. High resolution probe of the high absorption spot. The measurement was done with a beam of 60 um in diameter at 25 mW, i.e. 8.8 W/mm^2. All scatter and absorption data are referenced from LIGO-E1000766

ITM03 scatter In chamber view, before install, after removal Scatter before installation: 5.6 ppm. Scatter after installation 6.3 ppm Spot # 2 found to be the high absorber, Present in “before” and “after” scatter scans

Features found within a radius of ~60 mm of center. Interesting 1 Features found within a radius of ~60 mm of center. 1 mm ∅ field Center scale squares are 50 µm Absorbing Interesting 2 Interesting 3

Interesting 1 (5, -27) Branch-like center structure

Interesting 2 (-8, -39) Shown in bright field ~80 µm in diameter

Interesting 3 (-60, -43) Center is filled

Absorption spot noise floor ~20 ppm

Probe absorption with smaller beam

absorber: 155 µm across bright center

absorber: 155 µm across bright center

Absorption spot seen in figure data? Polished and coated data 60 mm mask (orange circle) 0.06 nm rms polished, PV 0.49 nm 0.08 nm rms coated, PV 1.06 nm - 1 pixel = 400 µm Interesting point #1 is in a similar, though not exact location to the point seen low right.