Sony DSC HX95
Response
- red (R)
- green (G)
- blue (B)
Astro mode
Emission-line overlay on the active single-profile plot. Values are the source's own native samples (or a labelled linear interpolation).
About this spectrum5 notes
- Warning: Response scope is unknown; do not interpret this response as a bare-sensor measurement. Dataset interpretation
- Warning: Physical configuration is not documented; the response cannot be assigned to a confirmed optical configuration. Dataset interpretation
- Warning: Estimated response; not a primary measurement. Sources and attribution
- Warning: Normalization is unknown; amplitude comparisons are not established. Dataset interpretation
- Warning: Uncertainty is not documented. Missing uncertainty does not mean zero uncertainty. Dataset interpretation
Source & details
- Source category: estimated
- Estimated response: not a primary measurement (e.g. diffraction-grating closed-form recovery, model prediction). Independent of profile_type and quality/confidence grades.
- Type: estimated
- Estimated response, not a direct measurement; quality and confidence are assessed separately.
- Quality: unassessed
- Quality has not been assessed; no grade is inferred. Canonical release: no per-leaf scientific-quality assessment is asserted; the source-side claim is preserved verbatim.
- Confidence: unassessed
- Confidence has not been assessed; no confidence level is inferred. Canonical release: no claim about the per-leaf measurement precision is asserted; the upstream 'as is' wording (where present) is preserved.
- Author
- Solomatov
- Source
- Solomatov & Akkaynak, ICCP 2023, 'Spectral Sensitivity Estimation Without a Camera' (link)
- Source category
estimated(estimated response; not a primary measurement)- Methodology
- Solomatov & Akkaynak, ICCP 2023, 'Spectral Sensitivity Estimation Without a Camera' — model output.
- As-is
- Samples rendered verbatim: no smoothing, no interpolation, no zero-padding, no gap bridging in the browser. Documented null sparse cells render as visible gaps.
- Optical configuration
cfg-prf-solomatov-pred-sony-dsc-hx95-d3b9510b35d8(unknown) — unknown- Normalisation
- unknown (original: unknown)
- Response unit / scale
unknown/unknown- Sample count
- 31 samples from 400–700 nm, Δ 10 nm
- Profile ID
prf-solomatov-pred-sony-dsc-hx95-d3b9510b35d8@1- Profile checksum
sha256:549e0171f8f878d1…- Processing
- source_column=predicted-Sony-DSC-HX95.csv
- Scientific notes
- Canonical release: native grid and native R/G/B samples are preserved verbatim; sparse cells (wavelengths absent in the upstream CSV / JSON) are preserved as null; the parser never invents a value.
- Citation
- Solomatov & Akkaynak, ICCP 2023, 'Spectral Sensitivity Estimation Without a Camera', data/predictions/.
- Known limitations
- source_category=estimated
- permission_status is 'unknown' on the canonical License record (no independent operational clearance granted).
Graph tools
Inspect, zoom, export, and share the current chart. Native samples only — no interpolation, no averaging.
Channels
Zoom (nm)
Data details
- Dataset version
recovered-2026-09-29-all-available-with-ie-202404- Manifest digest
8f960e18d6c9dbef…- Manifest schema
0.1.0-draft- Release kind
full- Linked profiles / sessions
- 1 profile revision
Raw samples (R/G/B at native wavelengths)
prf-solomatov-pred-sony-dsc-hx95-d3b9510b35d8(revision 1)Raw samples for prf-solomatov-pred-sony-dsc-hx95-d3b9510b35d8 (revision 1): R/G/B response at native wavelengths. λ (nm) R G B 400 0.0036923704 0.0048783747 0.012816464 410 0.006002437 0.007686759 0.031255536 420 0.0051772166 0.014525072 0.07422822 430 0.0003578306 0.023119137 0.12599078 440 0.000258329 0.032546017 0.15804763 450 0.00007623297 0.039247446 0.17691717 460 0.00077762856 0.050888807 0.18989854 470 0.008284084 0.07438631 0.18523179 480 0.0197316 0.105453685 0.16470715 490 0.019451478 0.13924962 0.13354266 500 0.01645744 0.17979743 0.096538424 510 0.013468557 0.22732179 0.06472398 520 0.011155673 0.2610531 0.041409533 530 0.0024243128 0.27385345 0.028428001 540 0.001140465 0.2696118 0.026344473 550 0.0016179517 0.25357032 0.026658854 560 0.0012493185 0.22743163 0.029418262 570 0.06629737 0.19113004 0.029892808 580 0.16806649 0.15152818 0.026294472 590 0.21479207 0.11279603 0.02143506 600 0.20608154 0.08136224 0.017368445 610 0.18691862 0.056476016 0.012993329 620 0.16131933 0.04303932 0.007436973 630 0.14180233 0.032443903 0.0020059273 640 0.122867115 0.024170369 0.0000040473647 650 0.10283878 0.01606528 0.0000039502706 660 0.08327824 0.012412207 0.0000020887724 670 0.05787124 0.0069912085 0.0000015964258 680 0.03228541 0.004574064 0.0000017347093 690 0.012871163 0.0030695803 0.0000051858956 700 0.0086068455 0.001436221 0.000001434696