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arxiv: 2505.03131 · v1 · submitted 2025-05-06 · ⚛️ physics.optics

Enhanced timing of a 113 km O-TWTFT link with digital maximum likelihood estimation process

Pith reviewed 2026-05-22 17:19 UTC · model grok-4.3

classification ⚛️ physics.optics
keywords O-TWTFTComplex Least Squaresmaximum likelihood estimationfree-space optical linkfrequency combtime extractionquantum limitoptical clock synchronization
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The pith

A Complex Least Squares estimator that uses both amplitude and phase data extracts timing from optical sampling signals at received powers ten times lower than prior records.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper shows how to improve time extraction in optical two-way time-frequency transfer by replacing phase-only methods with a maximum likelihood estimator that processes both amplitude and phase information from linear optical sampling. This change matters because time extraction error had been the main barrier to sensitivity once received power drops below a few nanowatts. Experiments over a 113 km free-space link with losses up to 100 dB demonstrate stable operation at 0.1 nW minimum received power. The resulting timing precision approaches the quantum limit set by photon statistics. The result directly supports practical long-distance optical clock networks that must tolerate high loss.

Core claim

The authors introduce the Complex Least Squares method as a maximum-likelihood estimator for time extraction in O-TWTFT. Unlike earlier approaches that rely only on phase, the new estimator incorporates both amplitude and phase of the sampled frequency-comb signals. Over a 113 km free-space link the method sustains operation at an average received power of 0.1 nW, more than ten times lower than previous benchmarks, while the achieved precision nears the quantum limit.

What carries the argument

The Complex Least Squares (CLS) estimator, a maximum-likelihood technique that jointly fits amplitude and phase information from the linear optical sampling waveform.

If this is right

  • Time extraction error ceases to dominate system sensitivity at ultra-low received powers.
  • O-TWTFT links remain functional with average losses up to 100 dB.
  • Timing precision reaches levels set by the quantum limit rather than algorithmic noise.
  • Minimum received power of 0.1 nW enables tenfold reduction compared with earlier free-space demonstrations.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The same estimator could be tested on other comb-based optical sampling tasks to check whether amplitude-plus-phase fitting improves sensitivity there as well.
  • Pairing the method with real-time turbulence compensation might push the operating range even farther without increasing transmitter power.
  • Lower required received power reduces the size and cost of ground stations needed for a continental-scale optical clock network.

Load-bearing premise

The actual noise statistics of the free-space channel, including turbulence and detector effects, match the statistical model used to derive the Complex Least Squares estimator as the true maximum-likelihood solution.

What would settle it

A direct comparison of measured timing jitter at 0.1 nW received power against the photon-shot-noise quantum limit calculated for the same integration time and link parameters.

Figures

Figures reproduced from arXiv: 2505.03131 by Cheng-Zhi Peng, Hai-Feng Jiang, Jian-Wei Pan, Jian-Yu Guan, Ji-Gang Ren, Jin-Jian Han, Lei Hou, Meng-Zhe Lian, Qiang Zhang, Qi Shen, Wei-Yue Liu, Yong Wang, Yu-Chen Fang.

Figure 1
Figure 1. Figure 1: FIG. 1: (a) The time domain picture of O-TWTFT: The two [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2: Experimental Setup: The schematic illustrates two free-space links, with the 1,545-nm link in yellow and the 1,563-nm link in [PITH_FULL_IMAGE:figures/full_fig_p004_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3: (a) Time deviation (TDEV) curves for the CLS and [PITH_FULL_IMAGE:figures/full_fig_p005_3.png] view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5: Illustration of the CLS algorithm in action, applied to [PITH_FULL_IMAGE:figures/full_fig_p007_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: FIG. 6: The distribution of received optical power. [PITH_FULL_IMAGE:figures/full_fig_p009_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: FIG. 7: The distribution of time differences between the actual [PITH_FULL_IMAGE:figures/full_fig_p010_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: FIG. 8: The relationship between the energy of the interferogram [PITH_FULL_IMAGE:figures/full_fig_p010_8.png] view at source ↗
Figure 9
Figure 9. Figure 9: FIG. 9: Depiction of the relationship between the received optical [PITH_FULL_IMAGE:figures/full_fig_p011_9.png] view at source ↗
read the original abstract

Optical two-way time-frequency transfer (O-TWTFT), employing linear optical sampling and based on frequency combs, is a promising approach for future large-scale optical clock synchronization. It offers the dual benefits of high temporal resolution and an extensive unambiguous range. A critical challenge in establishing long-distance free-space optical links is enhancing detection sensitivity. Particularly at ultra-low received power levels, the error caused by time extraction algorithms for linear optical sampling becomes a significant hindrance to system sensitivity, surpassing the constraints imposed by quantum limitations. In this work, we introduce the Complex Least Squares (CLS) method to enhance both the accuracy and sensitivity of time extraction. Unlike most previous methods that relied solely on phase information, our scheme utilizes a maximum likelihood estimation technique incorporating both amplitude and phase data. Our experiments, conducted over a 113 km free-space link with an average link loss of up to 100 dB, achieved a record minimum received power of 0.1 nW, which is over ten times lower than previous benchmarks. The precision also approaches the quantum limitation.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The paper reports an experimental demonstration of optical two-way time-frequency transfer (O-TWTFT) over a 113 km free-space link using a Complex Least Squares (CLS) estimator framed as a maximum-likelihood method that incorporates both amplitude and phase information from linear optical sampling. The central result is a record minimum received power of 0.1 nW under up to 100 dB average link loss, with timing precision stated to approach the quantum limit.

Significance. If validated, the reported sensitivity improvement would represent a meaningful advance for practical long-distance free-space optical clock synchronization by enabling operation at received powers an order of magnitude below prior benchmarks. The experimental scale (113 km link) adds value, though the attribution of the gain specifically to the CLS approach requires stronger support.

major comments (2)
  1. [CLS derivation and noise model] The section deriving the Complex Least Squares estimator as the maximum-likelihood solution assumes complex circular Gaussian noise statistics. Over a 113 km link with 100 dB loss, atmospheric turbulence introduces multiplicative scintillation and non-Gaussian intensity fluctuations that are not modeled or validated against measured data in the manuscript. This assumption is load-bearing for the claim that the 0.1 nW sensitivity and approach to the quantum limit are due to the amplitude-plus-phase estimator rather than other experimental factors.
  2. [Experimental results] The experimental results section reports the 0.1 nW minimum received power and near-quantum-limited precision but provides no quantitative error bars, details on averaging or statistical significance, or direct baseline comparisons to prior phase-only extraction methods under identical link conditions. These omissions weaken the quantitative support for the record sensitivity claim.
minor comments (2)
  1. [Experimental setup] Clarify the exact procedure used to determine the 100 dB link loss and 0.1 nW received power values, including any calibration steps or averaging windows.
  2. [Discussion] Add a brief discussion or citation addressing how the quantum limit is computed for this specific comb-based O-TWTFT configuration.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their careful reading and constructive comments on our manuscript. We address each major comment below and describe the revisions we will incorporate.

read point-by-point responses
  1. Referee: [CLS derivation and noise model] The section deriving the Complex Least Squares estimator as the maximum-likelihood solution assumes complex circular Gaussian noise statistics. Over a 113 km link with 100 dB loss, atmospheric turbulence introduces multiplicative scintillation and non-Gaussian intensity fluctuations that are not modeled or validated against measured data in the manuscript. This assumption is load-bearing for the claim that the 0.1 nW sensitivity and approach to the quantum limit are due to the amplitude-plus-phase estimator rather than other experimental factors.

    Authors: We agree that the maximum-likelihood derivation of the CLS estimator assumes complex circular Gaussian noise, which is standard for heterodyne detection with a strong local oscillator in linear optical sampling. While atmospheric turbulence induces scintillation, the post-mixing sampled complex amplitudes remain approximately Gaussian due to the dominant shot-noise contribution from the local oscillator. Nevertheless, we acknowledge that explicit discussion and validation would strengthen the manuscript. In revision we will add a dedicated subsection on the noise model, its applicability under turbulence, and comparison to measured intensity statistics from the 113 km link. revision: yes

  2. Referee: [Experimental results] The experimental results section reports the 0.1 nW minimum received power and near-quantum-limited precision but provides no quantitative error bars, details on averaging or statistical significance, or direct baseline comparisons to prior phase-only extraction methods under identical link conditions. These omissions weaken the quantitative support for the record sensitivity claim.

    Authors: We accept that additional quantitative details are needed to support the sensitivity claims. In the revised manuscript we will include error bars derived from repeated measurements, specify the number of samples and averaging intervals used, report statistical significance, and add direct side-by-side comparisons of CLS versus phase-only extraction performed on the same 113 km link data sets. These additions will clarify the contribution of the amplitude-plus-phase estimator. revision: yes

Circularity Check

0 steps flagged

No significant circularity; experimental result is self-contained

full rationale

The paper reports an experimental demonstration of record 0.1 nW sensitivity over a 113 km free-space O-TWTFT link using the Complex Least Squares estimator, presented as a maximum-likelihood method that incorporates amplitude and phase. No derivation chain reduces a claimed prediction or first-principles result to its own inputs by construction, and the central performance claims are validated by direct measurement rather than by fitting parameters to the target outcomes or by load-bearing self-citations. The noise-model assumptions are stated explicitly but do not create a self-referential loop within the reported work.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The work rests on standard assumptions of linear optical sampling and Gaussian noise statistics in the detection process; no new free parameters, invented entities, or ad-hoc axioms are introduced beyond the choice of the CLS estimator itself.

axioms (1)
  • domain assumption The received optical sampling signal follows a statistical model for which the Complex Least Squares estimator is the maximum-likelihood solution.
    Invoked when the authors state that the method incorporates both amplitude and phase data under a maximum-likelihood framework.

pith-pipeline@v0.9.0 · 5763 in / 1359 out tokens · 38087 ms · 2026-05-22T17:19:05.258242+00:00 · methodology

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Lean theorems connected to this paper

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  • IndisputableMonolith/Cost/FunctionalEquation.lean washburn_uniqueness_aczel unclear
    ?
    unclear

    Relation between the paper passage and the cited Recognition theorem.

    we apply a least squares fitting method to the complex results of the Fourier-transformed interferograms, which is equivalent to MLE in this context... helical curve is defined by three parameters: the attenuation coefficient β, the initial phase difference term γ, and the common difference α

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Reference graph

Works this paper leans on

35 extracted references · 35 canonical work pages

  1. [20]

    Dmitrieva, J

    M. Dmitrieva, J. Lefebvre, K. delas Penas, H. L. Zen- ner, J. Richens, D. St Johnston, and J. Rittscher, Short trajectory segmentation with 1d unet framework: Appli- cation to secretory vesicle dynamics, in2020 IEEE 17th International Symposium on Biomedical Imaging (ISBI) (IEEE, 2020) pp. 891–894

  2. [27]

    M. A. Richardset al.,Fundamentals of radar signal pro- cessing, Vol. 1 (Mcgraw-hill New York, 2005). 1 Supplemental Material CLS ALGORITHM Comprehensive Description of the CLS Algorithm FIG. 4: Depiction of initial frame data points on the complex plane post-Fourier transformation. Green points A1, A2, A3, A4, A5, . . .are presented with their respective ...

  3. [28]

    The results exhibit a normal distribution, indicat- ing that outliers are uncommon

  4. [29]

    Bias is absent in the estimation of delay time, en- suring the reliability of the estimation

  5. [30]

    Among all possible unbiased algorithms, CLS achieves the lowest error variance, signifying its su- perior precision. . DA T A FIL TERING In our experiment, due to the introduction of attenua- tors, the link loss for the 1,545-nm link was increased, po- tentially obscuring the interference patterns generated by 3 the optical comb with environmental noise. ...

  6. [31]

    Select high-SNR interferograms (signal power above 5 nW) and calculate the delay

  7. [32]

    Estimate the one-way delay of each sampling time by interpolating the high-SNR delay data

  8. [33]

    First, we justify the feasibility of selecting high SNR interferograms

    Calculate the one-way delay for each interferogram; if it deviates by more than 1000 fs from the delay estimated from the sampling timestamp of that in- terferogram, it is deemed a noise frame. First, we justify the feasibility of selecting high SNR interferograms. According to the findings in [12], the received power is log-normally distributed due to at...

  9. [34]

    S. M. Brewer, J.-S. Chen, A. M. Hankin, E. R. Clements, C.-w. Chou, D. J. Wineland, D. B. Hume, and D. R. Leibrandt, Al+ 27 quantum-logic clock with a systematic uncertainty below 10- 18, Physical review letters123, 033201 (2019)

  10. [35]

    Bothwell, D

    T. Bothwell, D. Kedar, E. Oelker, J. M. Robinson, S. L. Bromley, W. L. Tew, J. Ye, and C. J. Kennedy, Jila sri optical lattice clock with uncertainty of, Metrologia56, 065004 (2019)

  11. [36]

    T. L. Nicholson, S. Campbell, R. Hutson, G. E. Marti, B. Bloom, R. L. McNally, W. Zhang, M. Barrett, M. S. Safronova, G. Strouse,et al., Systematic evaluation of an atomic clock at 2×10- 18 total uncertainty, Nature communications6, 1 (2015)

  12. [37]

    Huntemann, C

    N. Huntemann, C. Sanner, B. Lipphardt, C. Tamm, and E. Peik, Single-ion atomic clock with 3×10- 18 sys- tematic uncertainty, Physical review letters116, 063001 (2016)

  13. [38]

    Aeppli, K

    A. Aeppli, K. Kim, W. Warfield, M. S. Safronova, and J. Ye, Clock with 8×10-19 systematic uncertainty, Phys- ical Review Letters133, 023401 (2024)

  14. [39]

    Dimarcq, M

    N. Dimarcq, M. Gertsvolf, G. Mileti, S. Bize, C. Oates, E. Peik, D. Calonico, T. Ido, P. Tavella, F. Meynadier, et al., Roadmap towards the redefinition of the second, Metrologia61, 012001 (2024)

  15. [40]

    T. E. Mehlst¨ aubler, G. Grosche, C. Lisdat, P. O. Schmidt, and H. Denker, Atomic clocks for geodesy, Re- ports on Progress in Physics81, 064401 (2018)

  16. [41]

    Lisdat, G

    C. Lisdat, G. Grosche, N. Quintin, C. Shi, S. Raupach, C. Grebing, D. Nicolodi, F. Stefani, A. Al-Masoudi, S. D¨ orscher,et al., A clock network for geodesy and fundamental science, Nature communications7, 12443 (2016)

  17. [42]

    Exertier, E

    P. Exertier, E. Samain, P. Bonnefond, and P. Guillemot, Status of the t2l2/jason2 experiment, Advances in Space Research46, 1559 (2010)

  18. [43]

    Exertier, E

    P. Exertier, E. Samain, N. Martin, C. Courde, M. Laas- Bourez, C. Foussard, and P. Guillemot, Time transfer by laser link: data analysis and validation to the ps level, Advances in Space Research54, 2371 (2014)

  19. [44]

    F. R. Giorgetta, W. C. Swann, L. C. Sinclair, E. Bau- mann, I. Coddington, and N. R. Newbury, Optical two- way time and frequency transfer over free space, Nature Photonics7, 434 (2013)

  20. [45]

    Shen, J.-Y

    Q. Shen, J.-Y. Guan, J.-G. Ren, T. Zeng, L. Hou, M. Li, Y. Cao, J.-J. Han, M.-Z. Lian, Y.-W. Chen,et al., Free- space dissemination of time and frequency with 10- 19 instability over 113 km, Nature610, 661 (2022)

  21. [46]

    E. D. Caldwell, L. C. Sinclair, N. R. Newbury, and J.- D. Deschenes, The time-programmable frequency comb and its use in quantum-limited ranging, Nature610, 667 (2022)

  22. [47]

    E. D. Caldwell, J.-D. Deschenes, J. Ellis, W. C. Swann, B. K. Stuhl, H. Bergeron, N. R. Newbury, and L. C. Sinclair, Quantum-limited optical time transfer for future geosynchronous links, Nature618, 721 (2023)

  23. [48]

    Bergeron, L

    H. Bergeron, L. C. Sinclair, W. C. Swann, I. Khader, K. C. Cossel, M. Cermak, J.-D. Deschˆ enes, and N. R. Newbury, Femtosecond time synchronization of optical clocks off of a flying quadcopter, Nature communications 10, 1819 (2019)

  24. [49]

    L. Kong, K. Cui, J. Shi, M. Zhu, and S. Li, 1d phase un- wrapping based on the quasi-gramian matrix and deep learning for interferometric optical fiber sensing applica- tions, Journal of Lightwave Technology40, 252 (2022)

  25. [50]

    Itoh, Analysis of the phase unwrapping algorithm, Applied optics21, 2470 (1982)

    K. Itoh, Analysis of the phase unwrapping algorithm, Applied optics21, 2470 (1982)

  26. [51]

    Zhang, M

    Y. Zhang, M. Xiao, Z. Wang, H. Fu, and Y. Wu, Robust three-stage unscented kalman filter for mars entry phase navigation, Information Fusion51, 67 (2019)

  27. [52]

    Kulkarni and P

    R. Kulkarni and P. Rastogi, Simultaneous unwrapping and low pass filtering of continuous phase maps based on autoregressive phase model and wrapped kalman fil- tering, Optics and Lasers in Engineering124, 105826 (2020)

  28. [53]

    Dmitrieva, J

    M. Dmitrieva, J. Lefebvre, K. delas Penas, H. L. Zen- ner, J. Richens, D. St Johnston, and J. Rittscher, Short trajectory segmentation with 1d unet framework: Appli- cation to secretory vesicle dynamics, in2020 IEEE 17th 6 International Symposium on Biomedical Imaging (ISBI) (IEEE, 2020) pp. 891–894

  29. [54]

    Shen, J.-Y

    Q. Shen, J.-Y. Guan, T. Zeng, Q.-M. Lu, L. Huang, Y. Cao, J.-P. Chen, T.-Q. Tao, J.-C. Wu, L. Hou,et al., Experimental simulation of time and frequency transfer via an optical satellite–ground link at 10-18 instability, Optica8, 471 (2021)

  30. [55]

    Charnes, E

    A. Charnes, E. L. Frome, and P.-L. Yu, The equivalence of generalized least squares and maximum likelihood esti- mates in the exponential family, Journal of the American Statistical Association71, 169 (1976)

  31. [56]

    Casella and R

    G. Casella and R. L. Berger,Statistical inference(Cen- gage Learning, 2021)

  32. [57]

    Oelker, R

    E. Oelker, R. Hutson, C. Kennedy, L. Sonderhouse, T. Bothwell, A. Goban, D. Kedar, C. Sanner, J. Robin- son, G. Marti,et al., Demonstration of 4.8×10- 17 sta- bility at 1 s for two independent optical clocks, Nature Photonics13, 714 (2019)

  33. [58]

    Schioppo, R

    M. Schioppo, R. C. Brown, W. F. McGrew, N. Hinkley, R. J. Fasano, K. Beloy, T. Yoon, G. Milani, D. Nicolodi, J. Sherman,et al., Ultrastable optical clock with two cold-atom ensembles, Nature Photonics11, 48 (2017)

  34. [59]

    J. L. Ellis, M. I. Bodine, W. C. Swann, S. A. Steven- son, E. D. Caldwell, L. C. Sinclair, N. R. Newbury, and J.-D. Deschˆ enes, Scaling up frequency-comb-based opti- cal time transfer to long terrestrial distances, Physical Review Applied15, 034002 (2021)

  35. [60]

    M. A. Richardset al.,Fundamentals of radar signal pro- cessing, Vol. 1 (Mcgraw-hill New York, 2005)