Galaxy-scale and CGM-scale spectra for MID = 1141. Left: Spectrum extracted from the original minicube (black line) with a $0\stackrel{″}{.}8$ aperture (radius) around the HST center. The gray solid line indicates the continuum. The gray shade shows 1σ uncertainties. The vertical red and blue lines indicate the rest-frame wavelength of Si II absorption and Si II* emission (EW_abs(Si IIλ1527) = 1.6 ± 0.2 Å and EW_em(Si II* λ1533) = 1.1 ± 0.1 Å). Right: Spectrum extracted from a $2\stackrel{″}{.}4$ aperture around the HST center (EW_em(Si II* λ1533) = 1.8 ± 0.4 Å). The spectra indicate that the photon conservation works on the CGM scales.