Pith. sign in

REVIEW 2 major objections 2 minor 298 references

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz

T0 review · 2 major / 2 minor · reviewed 2026-05-25 · grok-4.3

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read Galactic magnetic field models match polarization angles but not intensity because local structures dominate the polarized sky.

desk verdict The paper tests GMF models on combined S-PASS/C-BASS data after Faraday cuts and finds angles correlate on large scales while intensity morphology does not, but the exclusion step leaves open whether the retained sky fairly represents the full emission. read the letter →

arxiv 2605.23489 v1 pith:H7KGWRJ5 submitted 2026-05-22 astro-ph.GA astro-ph.HE

Vasundhara Shaw , S. E. Harper , C. Dickinson , J. P. Leahy , Gabriel A. Hoerning , R. Cepeda-Arroita , Gilles Weymann-Despres , Mike Peel
show 4 more authors
Angela C. Taylor T. J. Pearson Jamie Leech Michael Jones
This is my paper · ORCID
classification astro-ph.GAastro-ph.HE
keywords galacticmagneticfieldpolarizedsynchrotronemissionmicrowavefrequenciesFaradayrotationpolarizationanglesintensitylocalstructurestemplatefitting
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

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

The reading

The paper compares contemporary Galactic magnetic field models against polarized synchrotron observations from the S-PASS survey at 2.3 GHz and the C-BASS survey at 4.76 GHz. Pixels with potentially large Faraday rotation are excluded and small corrections are applied to the remainder before using a template fit to test how well each model reproduces observed polarization amplitudes and angles. Most models reproduce large-scale polarization angles reasonably well but fail to match the morphology of polarized intensity. The mismatch indicates that local foreground features such as the North Polar Spur and the Fan region shape a large portion of the polarized emission at microwave frequencies.

What carries the argument

Template-fitting approach that compares each model's predicted polarization amplitudes and angles to the survey data after Faraday corrections.

What would settle it

A polarized intensity map at 4.76 GHz in which a global magnetic field model without added local structures matches the observed morphology as closely as a model that includes the North Polar Spur and Fan region would falsify the central claim.

Watch

Extended reading notes

Core claim

Contemporary Galactic magnetic field models generally reproduce observed polarization angles on large scales but fail to match the morphology of polarized intensity. A significant fraction of the polarized sky is shaped by local foreground structures such as the North Polar Spur/Loop I and the Fan region. Accurate modeling of polarized synchrotron emission at microwave frequencies therefore requires incorporating these local structures.

Load-bearing premise

Excluding pixels with potentially large Faraday rotation and applying small corrections to the remainder does not introduce selection bias that affects the comparison between models and data.

Editorial extensions

If this is right

  • Most models reproduce polarization angles on large scales but not the morphology of polarized intensity.
  • There is a clear correlation between data and models for polarization angles but not for polarized intensity.
  • Local structures such as the North Polar Spur and the Fan region shape a large portion of the polarized sky.
  • Incorporating local structures is required for accurate modeling of polarized synchrotron emission at microwave frequencies.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Global magnetic field models alone may be insufficient without explicit local additions to describe microwave polarization data.
  • This result could influence how polarized foregrounds are subtracted in analyses of the cosmic microwave background.
  • Repeating the template comparison at additional frequencies would test whether the mismatch with intensity persists.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 2 minor

Summary. The paper compares several contemporary Galactic magnetic field (GMF) models against polarized synchrotron emission from the S-PASS survey at 2.3 GHz and C-BASS at 4.76 GHz. Pixels with potentially large Faraday rotation are excluded and small (<80°) corrections are applied to the remainder; a template-fitting analysis then evaluates model performance on polarization angles and amplitudes. The authors report that most models reproduce large-scale polarization angles reasonably well but fail to match the morphology of polarized intensity, and conclude that local structures such as the North Polar Spur/Loop I and the Fan region must be incorporated into models for accurate reproduction of microwave polarized synchrotron emission. A combined 4.76 GHz full-sky map is also presented.

Significance. If the template-fit comparison after pixel selection is unbiased, the result would be significant for Galactic astrophysics and CMB foreground modeling: it would demonstrate that global GMF models are insufficient for polarized intensity at these frequencies and motivate inclusion of local features. The use of two independent surveys and published models (rather than internally fitted parameters) is a methodological strength.

major comments (2)
  1. [Abstract and Methods] Abstract and Methods (pixel exclusion and Faraday correction procedure): the description of excluding pixels with large Faraday rotation and applying corrections to the rest does not include a quantitative test (e.g., sky-fraction overlap or correlation statistics) of whether the retained pixels are biased away from the local structures (North Polar Spur/Loop I, Fan) invoked in the conclusion. This selection step is load-bearing for the central claim that global models fail on intensity morphology because of missing local features.
  2. [Results] Results section (template-fitting evaluation): the claims that models 'match the polarization angles reasonably well' but 'often fail to reproduce the morphology of the polarized intensity' are presented without reported quantitative statistics (correlation coefficients, reduced chi-squared values, or error budgets on the fits). This leaves the strength of the angle-intensity discrepancy unquantified and weakens support for the conclusion.
minor comments (2)
  1. [Abstract] The abstract states that a reconstructed 4.76 GHz map is created but does not specify the exact weighting or combination method used; this should be clarified in the main text for reproducibility.
  2. [Figures and Methods] Figure captions and text should explicitly state the number of pixels retained after exclusion and the sky fraction covered, to allow readers to assess the scope of the comparison.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive comments, which help clarify and strengthen the presentation of our results. We address each major comment below and will incorporate revisions to provide the requested quantitative support.

read point-by-point responses

  1. Referee: [Abstract and Methods] Abstract and Methods (pixel exclusion and Faraday correction procedure): the description of excluding pixels with large Faraday rotation and applying corrections to the rest does not include a quantitative test (e.g., sky-fraction overlap or correlation statistics) of whether the retained pixels are biased away from the local structures (North Polar Spur/Loop I, Fan) invoked in the conclusion. This selection step is load-bearing for the central claim that global models fail on intensity morphology because of missing local features.

    Authors: We agree that explicitly demonstrating the absence of selection bias is important for the robustness of our central claim. In the revised manuscript we will add a quantitative comparison of the retained pixel set against the full sky, including sky-fraction overlap statistics and spatial correlation measures specifically evaluated within the North Polar Spur/Loop I and Fan regions. This analysis will confirm that the local structures remain well represented after the Faraday-based selection and will be presented in an expanded Methods section. revision: yes

  2. Referee: [Results] Results section (template-fitting evaluation): the claims that models 'match the polarization angles reasonably well' but 'often fail to reproduce the morphology of the polarized intensity' are presented without reported quantitative statistics (correlation coefficients, reduced chi-squared values, or error budgets on the fits). This leaves the strength of the angle-intensity discrepancy unquantified and weakens support for the conclusion.

    Authors: We accept that the manuscript would benefit from explicit quantitative metrics. We will revise the Results section to report Pearson correlation coefficients and reduced chi-squared values for both the polarization-angle and polarized-intensity template fits, together with a brief error budget derived from the fit residuals. These statistics will be shown for each GMF model and will directly quantify the reported difference in performance between angles and amplitudes. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity; comparison uses independent data and models

full rationale

The paper's central result follows from a template-fit comparison of published GMF models against independent S-PASS and C-BASS survey data after described pixel exclusions and Faraday corrections. No equations reduce any prediction to a fitted parameter defined inside the paper, no self-citation chain bears the load of the conclusion, and the mismatch in polarized intensity morphology is an empirical observation not forced by the inputs. The derivation is self-contained against external benchmarks.

Assumptions & free parameters 0 free parameters · 1 assumptions · 0 invented entities

Abstract supplies no explicit free parameters or invented entities; the only identifiable assumption is the accuracy of the applied Faraday corrections.

assumptions (1)
  • domain assumption Faraday rotation corrections derived at the survey frequencies can be applied without introducing significant residual bias to the polarization comparison.
    Abstract states that small corrections are applied after excluding high-rotation pixels.

how reviews work

0 comments
Cite this review

Pith. "Pith review of A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz." pith.science (2026). https://pith.science/paper/H7KGWRJ5

@misc{pith2026260523489,
  author       = {Pith},
  title        = {Pith review of: A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/H7KGWRJ5}},
  note         = {Machine review of arXiv:2605.23489}
}
abstract

We compare a set of contemporary Galactic magnetic field (GMF) models with polarized synchrotron observations from the S-PASS and C-BASS radio surveys and combine them to create a reconstructed 4.76~GHz full sky map. Pixels that potentially have a large Faraday rotation are excluded while small ($< 80\degree$) Faraday corrections derived at the respective frequencies of the two surveys are applied to the rest of the map. Using a template-fitting approach, we evaluate the ability of each model to reproduce the observed polarization amplitudes and polarization angles. We find that while most GMF models match the polarization angles reasonably well, they often fail to reproduce the morphology of the polarized intensity. We find that for most models there is a clear correlation between the data and models in polarization angles on large scales, but this does not hold true for polarized intensity. Our results show that a large portion of the polarized sky is shaped by local ``foreground'' features such as the North Polar Spur/Loop\,I and the Fan region. We conclude that incorporating such local structures is essential for accurately modelling the polarized synchrotron emission at microwave frequencies.

Figures

Figures reproduced from arXiv: 2605.23489 by the authors.

Figure 1
Figure 1. The combined C-BASS and S-PASS polarized syn￾chrotron intensity map at 4.76 GHz shown in Galactic coordinates and rendered at HEALPix resolution Nside = 16 (G´orski et al. 2005a). the most complete and reliable reconstructed sky coverage currently possible at 4.76 GHz. 2.1 C-BASS North In this study we use the Data release 1 version of the C-Band All Sky Survey (C-BASS), an all-sky continuum survey mea￾suring total … view at source ↗
Figure 2
Figure 2. The Base map and additional masked regions shown above in Galactic coordinates and rendered at HEALPix resolution Nside = 16. The grey areas in the mask indicate excluded regions: a circular region of radius 30◦ centred on the Galactic Centre, where strong Faraday rotation leads to significant depolarization; a symmetric Galactic latitude cut of ±10◦ to remove bright disc emission; and high-latitude pixels with rota… view at source ↗
Figure 3
Figure 3. Polarized intensity (PI) synchrotron skymaps at 4.76 GHz, presented in Galactic coordinates at HEALPix resolution Nside = 16. The skymap in the top-left panel shows the combined C-BASS/S-PASS observational data, followed by synthetic PI maps generated from each GMF model. All maps have been processed using the same Base mask and have been rescaled by their respective fitted amplitudes obtained from fitting the full … view at source ↗
Figures from the paper (7 more)
Figure 4
Figure 4. Figure 4: Residual polarized intensity maps at 4.76 GHz, shown in Galactic coordinates at HEALPix resolution Nside = 16 with the Base mask applied (masked regions appear in grey). For reference, the C-BASS data in the same units but with a different colour map are displayed in t…
Figure 5
Figure 5. Figure 5: Polarization angles (PA) skymaps at 4.76 GHz, presented in Galactic coordinates at HEALPix resolution Nside = 16. The skymap in the top-left panel shows the combined C-BASS/S-PASS observational data, followed by synthetic PA maps generated from each GMF model. All maps…
Figure 6
Figure 6. Figure 6: Heatmaps showing the fitted amplitude (left) and Spearman’s rank correlation coefficient (right) for each GMF model across selected small sky regions, evaluated at HEALPix resolution Nside = 16. The fitted amplitude represents the scaling factor obtained from the linea…
Figure 7
Figure 7. Figure 7: Heatmaps showing the fitted amplitude (left) and Spearman’s rank correlation coefficient (right) for each GMF model across selected hemispheric regions, evaluated at HEALPix resolution Nside = 16. The fitted amplitude represents the scaling factor obtained from the lin…
Figure 8
Figure 8. Figure 8: Histograms of polarization angle (PA) differences between the C-BASS/S-PASS data and each GMF model, computed at HEALPix resolution Nside = 16. The distributions are fitted using the position angle difference model described by Naghizadeh-Khouei & Clarke (1993), which …
Figure 9
Figure 9. Figure 9: Polarization angle structure functions at NSIDE = 16 ( ≈ 3.7 ◦) for the North Polar Spur and high Galactic latitude regions of the reconstructed 4.76 GHz sky. The structure functions were calculated for the reconstructed 4.76 GHz sky and compared with polarization angl…
Figure 10
Figure 10. Figure 10: Left : T-T plot comparison between the data and the KST24 full Dragon model for regionsQ-NE, Q-1-NE, Q-2-NE. Right: T-T plot between the data and the UF23 cre10 model for regionsQ-SW, Q-3-SW, Q-4-SW. ated with the Orion–Eridanus superbubble, while Booth et al. (2025) …

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

298 extracted references · 298 canonical work pages

  1. [1]

    Jansson, Ronnie and Farrar, Glennys R. , year=. A NEW MODEL OF THE GALACTIC MAGNETIC FIELD , journal=

    work page

  2. [2]

    Galactic halo bubble magnetic fields and UHECR deflections

    work page

  3. [3]

    , title =

    , in prep. , title =

    work page

  4. [4]

    , keywords =

    , in prep. , keywords =

    work page

  5. [5]

    arXiv , author =:1610.02743 , journal =

    work page Pith review arXiv

  6. [6]

    CMB-S4 Science Case, Reference Design, and Project Plan

    CMB-S4 Science Case, Reference Design, and Project Plan. arXiv e-prints , keywords =. doi:10.48550/arXiv.1907.04473 , archivePrefix =. 1907.04473 , primaryClass =

    work page Pith review arXiv doi:10.48550/arxiv.1907.04473 1907

  7. [7]

    Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abernathy, M. R. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. and Ain, A. and Ajith, P. and Allen, B. and Allocca, A. and Altin, P. A. and A...

    work page doi:10.1103/physrevlett.116.061102 2016

  8. [8]

    doi:10.1016/j.newar.2003.09.016 , journal =

    work page doi:10.1016/j.newar.2003.09.016 2003

Show all 298 references
  1. [9]

    doi:10.3847/0067-0049/223/2/26 , eid =

    2016 , bdsk-url-1 =. doi:10.3847/0067-0049/223/2/26 , eid =. arXiv , author =:1602.07246 , journal =

    2016 doi arXiv

  2. [10]

    doi:10.1111/j.1365-2966.2009.14599.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2009.14599.x , eprint =

    2009 doi

  3. [11]

    SpDust/SpDust.2: Code to Calculate Spinning Dust Spectra , year =

    Ali-Ha. SpDust/SpDust.2: Code to Calculate Spinning Dust Spectra , year =. Astrophysics Source Code Library , month =

  4. [12]

    doi:10.1086/184494 , journal =

    doi

  5. [13]

    doi:10.1111/j.1365-2966.2012.20796.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2012.20796.x , eprint =

    2012 doi

  6. [14]

    doi:10.1093/mnras/stv751 , eprint =

    , keywords =. doi:10.1093/mnras/stv751 , eprint =

    doi

  7. [15]

    doi:10.1111/j.1365-2966.2011.18925.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2011.18925.x , eprint =

    2011 doi

  8. [16]

    doi:10.1111/j.1365-2966.2011.18755.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2011.18755.x , eprint =

    2011 doi

  9. [17]

    arXiv , author =:2103.10466 , journal =

    doi:10.3847/1538-4365/abef65 , eid =. arXiv , author =:2103.10466 , journal =

    doi

  10. [18]

    arXiv , author =:1108.1474 , journal =

    doi:10.1051/0004-6361/201117837 , eid =. arXiv , author =:1108.1474 , journal =

    doi arXiv

  11. [19]

    arXiv , author =:1910.06359 , journal =

    1910

  12. [20]

    doi:10.1111/j.1365-2966.2012.21314.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2012.21314.x , eprint =

    2012 doi

  13. [21]

    doi:10.1046/j.1365-8711.2000.03751.x , eprint =

    , keywords =. doi:10.1046/j.1365-8711.2000.03751.x , eprint =

    2000 doi

  14. [22]

    D. S. Proposed Array-Based Deep Space Network for NASA , volume =. Proceedings of the IEEE , keywords =. 2007 , bdsk-url-1 =. doi:10.1109/JPROC.2007.905046 , issn =

    2007 doi

  15. [23]

    doi:10.1093/mnras/115.6.690 , journal =

    1955 , bdsk-url-1 =. doi:10.1093/mnras/115.6.690 , journal =

    1955 doi

  16. [24]

    Radio Astronomy and the Galactic System , editor =

  17. [25]

    doi:10.1046/j.1365-8711.2003.07008.x , eprint =

    , keywords =. doi:10.1046/j.1365-8711.2003.07008.x , eprint =

    2003 doi

  18. [26]

    doi:10.1093/mnras/stt1158 , eprint =

    , keywords =. doi:10.1093/mnras/stt1158 , eprint =

    doi

  19. [27]

    Dark Energy: Observational and Theoretical Approaches , publisher =

  20. [28]

    E. S. Battistelli and E. Carretti and A. Cruciani and P. de Bernardis and R. Genova-Santos and S. Masi and A. Naldi and R. Paladini and F. Piacentini and C. T. Tibbs and L. Verstraete and N. Ysard , journal =. New Radio Observations of Anomalous Microwave Emission in the H II ...

    2015

  21. [29]

    doi:10.3847/2041-8213/ab21de , eid =

    2019 , bdsk-url-1 =. doi:10.3847/2041-8213/ab21de , eid =. arXiv , author =:1905.12276 , journal =

    2019 doi arXiv

  22. [30]

    doi:10.1093/mnras/stt1082 , eprint =

    , keywords =. doi:10.1093/mnras/stt1082 , eprint =

    doi

  23. [31]

    arXiv , author =:1803.04888 , keywords =

    The Cosmic Wheel and the Legacy of the AKARI Archive: From Galaxies and Stars to Planets and Life , editor =. arXiv , author =:1803.04888 , keywords =

    arXiv

  24. [32]

    2019 , bdsk-url-1 =

    , keywords =. 2019 , bdsk-url-1 =. doi:10.1093/pasj/psz110 , eprint =

    2019 doi

  25. [33]

    doi:10.1086/377252 , eprint =

    , keywords =. doi:10.1086/377252 , eprint =

    doi

  26. [34]

    doi:10.1086/377253 , eprint =

    , keywords =. doi:10.1086/377253 , eprint =

    doi

  27. [35]

    doi:10.1086/310075 , eprint =

    , keywords =. doi:10.1086/310075 , eprint =

    doi

  28. [36]

    arXiv , author =:1212.5225 , journal =

    doi:10.1088/0067-0049/208/2/20 , eid =. arXiv , author =:1212.5225 , journal =

    doi arXiv

  29. [37]

    doi:10.1086/186505 , journal =

    doi

  30. [38]

    BEYONDPLANCK. I. Global Bayesian analysis of the Planck Low Frequency Instrument data. , keywords =. doi:10.1051/0004-6361/202244953 , archivePrefix =. 2011.05609 , primaryClass =

    2011 doi

  31. [39]

    arXiv , author =:1407.2973 , keywords =

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII , doi =. arXiv , author =:1407.2973 , keywords =

    arXiv

  32. [40]

    , year = 1971, month = sep, volume =

    Are the galactic loops supernova remnants?. , year = 1971, month = sep, volume =

    1971

  33. [41]

    Astronomy and Astrophysics Supplement Series , month = Mar, pages =

  34. [42]

    doi:10.1111/j.1365-2966.2004.07797.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2004.07797.x , eprint =

    2004 doi

  35. [43]

    doi:10.1086/378398 , eprint =

    , keywords =. doi:10.1086/378398 , eprint =

    doi

  36. [44]

    Bock, J and R

    de Bernardis, P and Ade, Peter and J. Bock, J and R. Bond, J and Borrill, J and Boscaleri, A and Coble, K and R. Contaldi, C and P. Crill, B and De Troia, G and Farese, P and Ganga, Ken and Giacometti, M and Hivon, Eric and V. Hristov, V and Iacoangeli, A and Jaffe, AH and Jon...

    2008

  37. [45]

    L. S. Bernstein and F. O. Clark and J. A. Cline and D. K. Lynch , doi =. The Astrophysical Journal , month =

  38. [46]

    doi:10.1051/0004-6361/200911624 , eprint =

    , keywords =. doi:10.1051/0004-6361/200911624 , eprint =

    doi

  39. [47]

    arXiv , author =:1807.02199 , journal =

    arXiv

  40. [48]

    arXiv , author =:1606.01968 , journal =

    doi:10.3847/1538-4357/833/2/228 , eid =. arXiv , author =:1606.01968 , journal =

    doi arXiv

  41. [49]

    arXiv , author =:1403.3985 , journal =

    doi:10.1103/PhysRevLett.112.241101 , eid =. arXiv , author =:1403.3985 , journal =

    doi arXiv

  42. [50]

    doi:10.1086/590487 , eprint =

    , keywords =. doi:10.1086/590487 , eprint =

    doi

  43. [51]

    doi:10.1038/311517a0 , journal =

    doi

  44. [52]

    , journal =

    Bock, D. , journal =. Measurements of a scale-model ortho-mode transducer , year =

  45. [53]

    doi:10.1117/12.674051 , eid =

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , date-modified =. doi:10.1117/12.674051 , eid =

    doi

  46. [54]

    American Astronomical Society Meeting Abstracts , month = dec, pages =

  47. [55]

    astro-ph/0604101 , journal =

    arXiv

  48. [56]

    P. T. Boggs and J. E. Rogers , booktitle =. Orthogonal Distance Regression , volume =. Statistical analysis of measurement error models and applications: proceedings of the AMS-IMS-SIAM joint summer research conference held June 10-16, 1989 , month =

    1989

  49. [57]

    doi:10.1111/j.1365-2966.2007.12477.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2007.12477.x , eprint =

    2007 doi

  50. [58]

    arXiv , author =:1109.4175 , journal =

    doi:10.1088/0004-637X/744/2/129 , eid =. arXiv , author =:1109.4175 , journal =

    doi arXiv

  51. [59]

    2005 , bdsk-url-1 =

    , keywords =. 2005 , bdsk-url-1 =. doi:10.1051/0004-6361:20052990 , eprint =

    2005 doi

  52. [60]

    , keywords =

    The Distance and Radius of the Neutron Star PSR B0656+14. , keywords =. doi:10.1086/378184 , archivePrefix =. astro-ph/0306232 , primaryClass =

    doi arXiv

  53. [61]

    doi:10.1088/0004-637X/705/1/978 , eprint =

    , keywords =. doi:10.1088/0004-637X/705/1/978 , eprint =

    doi

  54. [62]

    doi:10.1016/S1384-1076(02)00105-7 , eprint =

    , month = jun, pages =. doi:10.1016/S1384-1076(02)00105-7 , eprint =

    doi

  55. [63]

    doi:10.1007/BF02639066 , journal =

    doi

  56. [64]

    arXiv , author =:astro-ph/9906360 , journal =

    arXiv

  57. [65]

    arXiv , author =:1310.2414 , journal =

    doi:10.1017/pasa.2013.36 , eid =. arXiv , author =:1310.2414 , journal =

    2013 doi arXiv

  58. [66]

    doi:10.1038/nature11734 , eprint =

    , month = jan, pages =. doi:10.1038/nature11734 , eprint =

    doi

  59. [67]

    doi:10.1111/j.1365-2966.2005.08761.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2005.08761.x , eprint =

    2005 doi

  60. [68]

    2019 , bdsk-url-1 =

    , keywords =. 2019 , bdsk-url-1 =. doi:10.1093/mnras/stz806 , eprint =

    2019 doi

  61. [69]

    doi:10.1111/j.1365-2966.2010.16608.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2010.16608.x , eprint =

    2010 doi

  62. [70]

    doi:10.1111/j.1365-2966.2008.13954.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2008.13954.x , eprint =

    2008 doi

  63. [71]

    doi:10.1086/499517 , eprint =

    , keywords =. doi:10.1086/499517 , eprint =

    doi

  64. [72]

    doi:10.1093/mnras/staa4016 , eprint =

    , keywords =. doi:10.1093/mnras/staa4016 , eprint =

    doi

  65. [73]

    Measuring Anomalous Microwave Emission with QUIJOTE , year =

    Roke Cepeda-Arroita , school =. Measuring Anomalous Microwave Emission with QUIJOTE , year =

  66. [74]

    , keywords =

    Detection of spectral variations of Anomalous Microwave Emission with QUIJOTE and C-BASS. , keywords =. doi:10.1093/mnras/stab583 , archivePrefix =. 2001.07159 , primaryClass =

    2001 doi

  67. [75]

    doi:10.1088/0004-637X/711/2/1123 , eprint =

    , keywords =. doi:10.1088/0004-637X/711/2/1123 , eprint =

    doi

  68. [76]

    doi:10.1093/mnras/stx1982 , eprint =

    , keywords =. doi:10.1093/mnras/stx1982 , eprint =

    doi

  69. [77]

    European Physical Journal Web of Conferences , doi =

  70. [78]

    doi:10.1111/j.1365-2966.2004.07737.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2004.07737.x , eprint =

    2004 doi

  71. [79]

    doi:10.1111/j.1365-2966.2005.09037.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2005.09037.x , eprint =

    2005 doi

  72. [80]

    arXiv , author =:1010.2769 , journal =

    doi:10.1051/0004-6361/201015292 , eid =. arXiv , author =:1010.2769 , journal =

    doi arXiv

  73. [81]

    doi:10.1086/116992 , journal =

    doi

  74. [82]

    doi:10.1086/152714 , journal =

    doi

  75. [83]

    doi:10.1086/162705 , journal =

    doi

  76. [84]

    doi:10.1086/300337 , journal =

    doi

  77. [85]

    The Southern C-BASS Instrument , volume =

    C Copley , date-modified =. The Southern C-BASS Instrument , volume =. , pages =

  78. [86]

    doi:10.1146/annurev-astro-081811-125514 , journal =

    2012 , bdsk-url-1 =. doi:10.1146/annurev-astro-081811-125514 , journal =

    2012 doi

  79. [87]

    doi:10.1086/307483 , journal =

    1999 , bdsk-url-1 =. doi:10.1086/307483 , journal =

    1999 doi

  80. [88]

    doi:10.1086/167620 , journal =

    doi

  81. [89]

    , keywords =

    Constraining the distance to the North Polar Spur with Gaia DR2. , keywords =. doi:10.1093/mnras/staa2702 , archivePrefix =. 2009.01320 , primaryClass =

    2009 doi

  82. [90]

    doi:10.1111/j.1365-2966.2006.10572.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2006.10572.x , eprint =

    2006 doi

  83. [91]

    doi:10.1088/1748-0221/4/12/T12002 , eprint =

    Journal of Instrumentation , month = dec, pages =. doi:10.1088/1748-0221/4/12/T12002 , eprint =

    doi

  84. [92]

    doi:10.1038/35010035 , eprint =

    , month = apr, pages =. doi:10.1038/35010035 , eprint =

    doi

  85. [94]

    doi:10.1086/312384 , eprint =

    , keywords =. doi:10.1086/312384 , eprint =

    doi

  86. [95]

    arXiv , author =:astro-ph/9705090 , keywords =

    Eighteenth Texas Symposium on Relativistic Astrophysics , editor =. arXiv , author =:astro-ph/9705090 , keywords =

    arXiv

  87. [96]

    doi:10.1086/310684 , eprint =

    , keywords =. doi:10.1086/310684 , eprint =

    doi

  88. [97]

    doi:10.1086/421293 , eprint =

    , keywords =. doi:10.1086/421293 , eprint =

    doi

  89. [98]

    2008 , bdsk-url-1 =

    , keywords =. 2008 , bdsk-url-1 =. doi:10.1111/j.1365-2966.2008.13376.x , eprint =

    2008 doi

  90. [99]

    doi:10.1007/s00159-009-0026-0 , eprint =

    , keywords =. doi:10.1007/s00159-009-0026-0 , eprint =

    doi

  91. [100]

    doi:10.1051/aas:1998119 , journal =

    doi

  92. [101]

    Data Analysis in Cosmology , doi =

  93. [102]

    arXiv , author =:astro-ph/0702198 , journal =

    arXiv

  94. [103]

    arXiv , author =:1706.04516 , journal =

    doi:10.1088/1475-7516/2018/04/014 , eid =. arXiv , author =:1706.04516 , journal =

    2018 doi

  95. [104]

    doi:10.1111/j.1365-2966.2003.07069.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2003.07069.x , eprint =

    2003 doi

  96. [105]

    arXiv , author =:1207.3675 , journal =

    doi:10.1051/0004-6361/201220019 , eid =. arXiv , author =:1207.3675 , journal =

    doi arXiv

  97. [106]

    Publications Astronomical Society of Australia , keywords =

  98. [107]

    Review of Scientific Instruments , local-url =

    Dicke, R H , date-added =. Review of Scientific Instruments , local-url =. 1946 , bdsk-url-1 =. doi:10.1063/1.1770483 , file =

    1946 doi

  99. [108]

    doi:10.1086/148306 , journal =

    doi

  100. [109]

    doi:10.1086/505299 , eprint =

    , keywords =. doi:10.1086/505299 , eprint =

    doi

  101. [110]

    doi:10.1088/0004-637X/690/2/1585 , eprint =

    , keywords =. doi:10.1088/0004-637X/690/2/1585 , eprint =

    doi

  102. [111]

    doi:10.1088/0004-637X/705/2/1607 , eprint =

    , keywords =. doi:10.1088/0004-637X/705/2/1607 , eprint =

    doi

  103. [112]

    doi:10.1111/j.1365-2966.2007.11967.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2007.11967.x , eprint =

    2007 doi

  104. [113]

    doi:10.1111/j.1365-2966.2004.08206.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2004.08206.x , eprint =

    2004 doi

  105. [114]

    doi:10.1111/j.1365-2966.2010.17079.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2010.17079.x , eprint =

    2010 doi

  106. [115]

    doi:10.1111/j.1745-3933.2011.01138.x , eprint =

    , keywords =. doi:10.1111/j.1745-3933.2011.01138.x , eprint =

    2011 doi

  107. [116]

    arXiv , author =:1501.00804 , keywords =

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , eid =. arXiv , author =:1501.00804 , keywords =

    arXiv

  108. [117]

    2019 , bdsk-url-1 =

    , keywords =. 2019 , bdsk-url-1 =. doi:10.1093/mnras/stz522 , eprint =

    2019 doi

  109. [118]

    doi:10.1016/j.newar.2018.02.001 , eprint =

    , keywords =. doi:10.1016/j.newar.2018.02.001 , eprint =

    2018 doi

  110. [119]

    doi:10.1046/j.1365-8711.2003.06439.x , eprint =

    , keywords =. doi:10.1046/j.1365-8711.2003.06439.x , eprint =

    2003 doi

  111. [120]

    arXiv , author =:1606.03606 , journal =

    arXiv

  112. [121]

    Observations of Anomalous Microwave Emission from HII Regions , volume =

    Dickinson, Clive , doi =. Observations of Anomalous Microwave Emission from HII Regions , volume =. Advances in Astronomy , month =. 2013 , bdsk-url-1 =

    2013

  113. [122]

    doi:10.1088/0004-637X/699/2/1374 , eprint =

    , keywords =. doi:10.1088/0004-637X/699/2/1374 , eprint =

    doi

  114. [123]

    doi:10.1086/587862 , eprint =

    , keywords =. doi:10.1086/587862 , eprint =

    doi

  115. [124]

    doi:10.1086/587863 , eprint =

    , keywords =. doi:10.1086/587863 , eprint =

    doi

  116. [125]

    2012 , bdsk-url-1 =

    , journal-added =. 2012 , bdsk-url-1 =. doi:10.1088/2041-8205/760/1/L8 , eid =. 1208.2690 , eprintclass =

    2012 doi arXiv

  117. [126]

    2012 , bdsk-url-1 =

    , keywords =. 2012 , bdsk-url-1 =. doi:10.1088/0004-637X/750/1/17 , eid =. 1109.4418 , eprintclass =

    2012 doi arXiv

  118. [127]

    doi:10.1088/0004-637X/717/2/825 , eprint =

    , keywords =. doi:10.1088/0004-637X/717/2/825 , eprint =

    doi

  119. [128]

    2002 , bdsk-url-1 =

    , keywords =. 2002 , bdsk-url-1 =. doi:10.1086/324631 , eprint =

    2002 doi

  120. [129]

    doi:10.1093/mnras/stx1136 , eprint =

    , keywords =. doi:10.1093/mnras/stx1136 , eprint =

    doi

  121. [130]

    doi:10.1086/311167 , eprint =

    , keywords =. doi:10.1086/311167 , eprint =

    doi

  122. [131]

    doi:10.1086/306387 , eprint =

    , keywords =. doi:10.1086/306387 , eprint =

    doi

  123. [132]

    doi:10.1086/306809 , eprint =

    , keywords =. doi:10.1086/306809 , eprint =

    doi

  124. [133]

    arXiv , author =:1205.7021 , journal =

    doi:10.1088/0004-637X/765/2/159 , eid =. arXiv , author =:1205.7021 , journal =

    doi arXiv

  125. [134]

    arXiv , author =:1205.6810 , journal =

    doi:10.1088/0004-637X/757/1/103 , eid =. arXiv , author =:1205.6810 , journal =

    doi arXiv

  126. [135]

    Physics of the Interstellar and Intergalactic Medium by Bruce T. Draine. Princeton University Press, 2011. ISBN: 978-0-691-12214-4 , date-modified =

    2011

  127. [136]

    , keywords =

    Quantum Suppression of Alignment in Ultrasmall Grains: Microwave Emission from Spinning Dust will be Negligibly Polarized. , keywords =. 2016. doi:10.3847/0004-637X/831/1/59 , archivePrefix =. 1605.06671 , primaryClass =

    2016 doi arXiv

  128. [137]

    doi:10.1088/1538-3873/128/969/115006 , eprint =

    , month = nov, number = 11, pages =. doi:10.1088/1538-3873/128/969/115006 , eprint =

    doi

  129. [138]

    doi:10.1088/0004-637X/701/2/1804 , eprint =

    , keywords =. doi:10.1088/0004-637X/701/2/1804 , eprint =

    doi

  130. [139]

    arXiv , author =:0811.3915 , keywords =

    American Institute of Physics Conference Series , doi =. arXiv , author =:0811.3915 , keywords =

    arXiv

  131. [140]

    , keywords =

    The Radio Sky at Meter Wavelengths: m-mode Analysis Imaging with the OVRO-LWA. , keywords =. doi:10.3847/1538-3881/aac721 , archivePrefix =. 1711.00466 , primaryClass =

    doi arXiv

  132. [141]

    , keywords =

    A parsec-scale Galactic 3D dust map out to 1.25 kpc from the Sun. , keywords =. doi:10.1051/0004-6361/202347628 , archivePrefix =. 2308.01295 , primaryClass =

    doi

  133. [142]

    arXiv , author =:1211.0041 , month = sep, primaryclass =

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , doi =. arXiv , author =:1211.0041 , month = sep, primaryclass =

    arXiv

  134. [143]

    doi:10.1071/AS98056 , journal =

    doi

  135. [144]

    Faraday tomography of LoTSS-DR2 data. II. Multi-tracer analysis in the high-latitude outer Galaxy. , keywords =. doi:10.1051/0004-6361/202348586 , archivePrefix =. 2404.19068 , primaryClass =

    doi

  136. [145]

    doi:10.1086/146421 , journal =

    doi

  137. [146]

    doi:10.1086/525277 , eprint =

    , keywords =. doi:10.1086/525277 , eprint =

    doi

  138. [147]

    doi:10.1086/526545 , eprint =

    , keywords =. doi:10.1086/526545 , eprint =

    doi

  139. [148]

    arXiv , author =:1203.5285 , journal =

    doi:10.1103/PhysRevD.85.083006 , eid =. arXiv , author =:1203.5285 , journal =

    doi arXiv

  140. [149]

    Journal of Cosmology and Astro-Particle Physics , keywords =

    Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization. Journal of Cosmology and Astro-Particle Physics , keywords =. 2016. doi:10.1088/1475-7516/2016/03/052 , archivePrefix =. 1509.06770 , primaryClass =

    2016 doi arXiv

  141. [150]

    , keywords =

    Magnetic Fields in Large-diameter H II Regions Revealed by the Faraday Rotation of Compact Extragalactic Radio Sources. , keywords =. doi:10.1088/0004-637X/736/2/83 , archivePrefix =. 1106.0931 , primaryClass =

    doi arXiv

  142. [151]

    BEYONDPLANCK. XV. Limits on large-scale polarized anomalous microwave emission from Planck LFI and WMAP. , keywords =. doi:10.1051/0004-6361/202243081 , archivePrefix =. 2201.03530 , primaryClass =

    doi

  143. [152]

    arXiv , author =:1008.3915 , journal =

    arXiv

  144. [153]

    arXiv , author =:1408.4788 , keywords =

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII , doi =. arXiv , author =:1408.4788 , keywords =

    arXiv

  145. [154]

    arXiv , author =:1201.5742 , journal =

    doi:10.1051/0004-6361/201016349 , eid =. arXiv , author =:1201.5742 , journal =

    doi arXiv

  146. [156]

    doi:10.1086/374411 , eprint =

    , keywords =. doi:10.1086/374411 , eprint =

    doi

  147. [157]

    doi:10.1086/307852 , eprint =

    , keywords =. doi:10.1086/307852 , eprint =

    doi

  148. [158]

    doi:10.1086/425165 , eprint =

    , keywords =. doi:10.1086/425165 , eprint =

    doi

  149. [159]

    doi:10.1086/423482 , eprint =

    , keywords =. doi:10.1086/423482 , eprint =

    doi

  150. [160]

    doi:10.1086/338225 , eprint =

    , keywords =. doi:10.1086/338225 , eprint =

    doi

  151. [161]

    doi:10.1088/0004-637X/734/1/5 , eid =

    2011 , bdsk-url-1 =. doi:10.1088/0004-637X/734/1/5 , eid =. arXiv , author =:0901.0555 , journal =

    2011 doi arXiv

  152. [162]

    doi:10.1086/344402 , journal =

    2002 , bdsk-url-1 =. doi:10.1086/344402 , journal =

    2002 doi

  153. [163]

    doi:10.1088/0004-637X/707/2/916 , eprint =

    , keywords =. doi:10.1088/0004-637X/707/2/916 , eprint =

    doi

  154. [164]

    arXiv , author =:1405.7351 , journal =

    arXiv

  155. [165]

    doi:10.1086/670067 , eprint =

    , month = mar, pages =. doi:10.1086/670067 , eprint =

    doi

  156. [166]

    doi:10.1051/0004-6361:20000432 , journal =

    doi

  157. [167]

    arXiv , author =:1106.3087 , journal =

    doi:10.1088/1475-7516/2013/04/047 , eid =. arXiv , author =:1106.3087 , journal =

    2013 doi arXiv

  158. [168]

    , keywords =

    Spatial Variations in the Spectral Index of Polarized Synchrotron Emission in the 9 yr WMAP Sky Maps. , keywords =. doi:10.1088/0004-637X/790/2/104 , archivePrefix =. 1404.5323 , primaryClass =

    doi arXiv

  159. [169]

    , keywords =

    Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data. , keywords =. doi:10.1051/0004-6361/202037629 , archivePrefix =. 1909.05923 , primaryClass =

    1909 doi

  160. [170]

    2008 , bdsk-url-1 =

    PASA , keywords =. 2008 , bdsk-url-1 =. doi:10.1071/AS08004 , eprint =

    2008 doi

  161. [171]

    arXiv , author =:1808.04493 , keywords =

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX , doi =. arXiv , author =:1808.04493 , keywords =

  162. [172]

    arXiv , author =:1607.06172 , keywords =

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII , doi =. arXiv , author =:1607.06172 , keywords =

    arXiv

  163. [173]

    arXiv , author =:1901.00631 , journal =

    1901 arXiv

  164. [174]

    doi:10.1086/323969 , eprint =

    , keywords =. doi:10.1086/323969 , eprint =

    doi

  165. [175]

    doi:10.1086/133729 , journal =

    doi

  166. [176]

    arXiv , author =:1109.4171 , journal =

    doi:10.1088/0004-637X/743/1/67 , eid =. arXiv , author =:1109.4171 , journal =

    doi arXiv

  167. [177]

    doi:10.1093/mnras/stw2503 , eprint =

    , keywords =. doi:10.1093/mnras/stw2503 , eprint =

    doi

  168. [178]

    arXiv , author =:1504.03514 , month = may, pages =

    Highlights of Spanish Astrophysics VIII , editor =. arXiv , author =:1504.03514 , month = may, pages =

    arXiv

  169. [179]

    doi:10.1111/j.1365-2966.2012.20875.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2012.20875.x , eprint =

    2012 doi

  170. [180]

    doi:10.1051/0004-6361:20020285 , eprint =

    , keywords =. doi:10.1051/0004-6361:20020285 , eprint =

    doi

  171. [181]

    doi:10.1088/0067-0049/180/2/265 , eprint =

    , keywords =. doi:10.1088/0067-0049/180/2/265 , eprint =

    doi

  172. [182]

    arXiv , author =:1001.4555 , journal =

    doi:10.1088/0067-0049/192/2/15 , eid =. arXiv , author =:1001.4555 , journal =

    doi arXiv

  173. [183]

    doi:10.2140/camcos.2010.5.65 , journal =

    2010 doi

  174. [184]

    doi:10.1086/427976 , eprint =

    , keywords =. doi:10.1086/427976 , eprint =

    doi

  175. [185]

    arXiv , author =:1607.04668 , keywords =

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII , doi =. arXiv , author =:1607.04668 , keywords =

    arXiv

  176. [186]

    2018 , bdsk-url-1 =

    Nature Astronomy , keywords =. 2018 , bdsk-url-1 =. doi:10.1038/s41550-018-0495-z , eprint =

    2018 doi

  177. [187]

    , keywords =

    Constraints on the distribution of supernova remnants with Galactocentric radius. , keywords =. doi:10.1093/mnras/stv1885 , archivePrefix =. 1508.02931 , primaryClass =

    doi arXiv

  178. [188]

    doi:10.1086/192282 , journal =

    doi

  179. [189]

    doi:10.1086/191863 , journal =

    1994 , bdsk-url-1 =. doi:10.1086/191863 , journal =

    1994 doi

  180. [190]

    Grimes, P K and King, O G and Yassin, G and Jones, M E , journal =

  181. [191]

    doi:10.1093/mnras/staa1572 , eprint =

    , keywords =. doi:10.1093/mnras/staa1572 , eprint =

    doi

  182. [192]

    arXiv , author =:0709.2012 , journal =

    2012 arXiv

  183. [193]

    Inner Space/Outer Space: The Interface between Cosmology and Particle Physics , editor =

  184. [194]

    arXiv , author =:1011.4298 , journal =

    doi:10.1051/0004-6361/200913628 , eid =. arXiv , author =:1011.4298 , journal =

    doi arXiv

  185. [195]

    doi:10.1111/j.1365-2966.2008.13515.x , journal =

    2008 doi

  186. [196]

    arXiv , author =:1008.0612 , keywords =

    The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey , editor =. arXiv , author =:1008.0612 , keywords =

    arXiv

  187. [197]

    doi:10.1086/378850 , eprint =

    , keywords =. doi:10.1086/378850 , eprint =

    doi

  188. [198]

    doi:10.1086/338879 , eprint =

    , keywords =. doi:10.1086/338879 , eprint =

    doi

  189. [199]

    arXiv , author =:1307.5830 , journal =

    doi:10.1103/PhysRevLett.111.141301 , eid =. arXiv , author =:1307.5830 , journal =

    doi arXiv

  190. [200]

    , month = oct, pages =

  191. [201]

    , keywords =

    The C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky. , keywords =. doi:10.1093/mnras/stac1210 , archivePrefix =. 2202.10411 , primaryClass =

    doi

  192. [202]

    , keywords =

    The C-Band All-Sky Survey (C-BASS): new constraints on the integrated radio spectrum of M 31. , keywords =. doi:10.1093/mnras/stad1539 , archivePrefix =. 2304.03875 , primaryClass =

    doi

  193. [203]

    , month = mar, pages =

  194. [204]

    Proceedings of the Astronomical Society of Australia , keywords =

  195. [205]

    doi:10.1086/306379 , eprint =

    , keywords =. doi:10.1086/306379 , eprint =

    doi

  196. [206]

    doi:10.1088/0004-6256/138/4/1032 , eprint =

    , keywords =. doi:10.1088/0004-6256/138/4/1032 , eprint =

    doi

  197. [207]

    Radiotekhnika , pages =

  198. [208]

    arXiv , author =:1505.02157 , journal =

    doi:10.3847/0004-637X/827/1/45 , eid =. arXiv , author =:1505.02157 , journal =

    doi arXiv

  199. [209]

    arXiv , author =:1709.07897 , journal =

    doi:10.3847/1538-4357/aaa489 , eid =. arXiv , author =:1709.07897 , journal =

    doi arXiv

  200. [210]

    arXiv , author =:1611.08597 , journal =

    doi:10.3847/1538-4357/aa5c37 , eid =. arXiv , author =:1611.08597 , journal =

    doi arXiv

  201. [211]

    , year = 1909, month = sep, volume =

    On new members of the system of the stars beta, gamma, delta, epsilon, zeta Ursae Majoris. , year = 1909, month = sep, volume =. doi:10.1086/141690 , adsurl =

    1909 doi

  202. [212]

    , month = sep, pages =

  203. [213]

    doi:10.1111/j.1365-2966.2007.12380.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2007.12380.x , eprint =

    2007 doi

  204. [214]

    Canadian Long Range Plan for Astronomy and Astrophysics White Papers , year = 2019, volume =

    CMB Science in Canada. Canadian Long Range Plan for Astronomy and Astrophysics White Papers , year = 2019, volume =. doi:10.5281/zenodo.3825611 , adsurl =

    2019 doi

  205. [215]

    2018 , bdsk-url-1 =

    NextBASS , url =. 2018 , bdsk-url-1 =

    2018

  206. [216]

    doi:10.1088/0067-0049/180/2/225 , eprint =

    , keywords =. doi:10.1088/0067-0049/180/2/225 , eprint =

    doi

  207. [217]

    Interplanetary Network Progress Report , month = nov, pages =

  208. [218]

    arXiv , author =:1112.3409 , journal =

    doi:10.1088/0004-637X/761/2/96 , eid =. arXiv , author =:1112.3409 , journal =

    doi arXiv

  209. [219]

    arXiv , author =:1305.0276 , journal =

    doi:10.1088/0004-637X/779/2/152 , eid =. arXiv , author =:1305.0276 , journal =

    doi arXiv

  210. [220]

    doi:10.1088/0004-637X/715/2/1462 , eprint =

    , keywords =. doi:10.1088/0004-637X/715/2/1462 , eprint =

    doi

  211. [221]

    arXiv , author =:1511.03691 , journal =

    doi:10.3847/0004-637X/821/2/91 , eid =. arXiv , author =:1511.03691 , journal =

    doi arXiv

  212. [222]

    arXiv , author =:1105.2302 , journal =

    doi:10.1088/0004-637X/741/2/87 , eid =. arXiv , author =:1105.2302 , journal =

    doi arXiv

  213. [223]

    doi:10.1086/668058 , eprint =

    , month = sep, pages =. doi:10.1086/668058 , eprint =

    doi

  214. [224]

    , date-added =

    Hogenauer, Eugene B. , date-added =. An economical class of digital filters for decimation and interpolation , volume =. IEEE Transactions on Acoustics, Speech and Signal Processing , pages =

  215. [225]

    doi:10.1109/TAP.2012.2219843 , journal =

    2012 doi

  216. [226]

    arXiv , author =:2211.11301 , journal =

    doi:10.1007/s11433-022-2039-8 , eid =. arXiv , author =:2211.11301 , journal =

    doi

  217. [227]

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , doi =

  218. [228]

    doi:10.1016/S1384-1076(97)00022-5 , eprint =

    , month = oct, pages =. doi:10.1016/S1384-1076(97)00022-5 , eprint =

    doi

  219. [229]

    , keywords =

    The Galactic Faraday depth sky revisited. , keywords =. doi:10.1051/0004-6361/201935479 , archivePrefix =. 1903.06735 , primaryClass =

    1903 doi

  220. [230]

    , keywords =

    The Galactic Faraday rotation sky 2020. , keywords =. doi:10.1051/0004-6361/202140486 , archivePrefix =. 2102.01709 , primaryClass =

    2020 doi

  221. [231]

    arXiv , author =:1308.2804 , journal =

    doi:10.1051/0004-6361/201322013 , eid =. arXiv , author =:1308.2804 , journal =

    doi arXiv

  222. [232]

    Progress of Theoretical and Experimental Physics , keywords =

    CMB foreground: A concise review. Progress of Theoretical and Experimental Physics , keywords =. doi:10.1093/ptep/ptu065 , adsurl =

    doi

  223. [233]

    doi:10.1086/497589 , journal =

    2005 , bdsk-url-1 =. doi:10.1086/497589 , journal =

    2005 doi

  224. [234]

    The local radio sky: high frequency-resolution single-dish studies of polarised Galactic synchrotron emission around 1.4 GHz , language =

    Leclercq, Indy , year =. The local radio sky: high frequency-resolution single-dish studies of polarised Galactic synchrotron emission around 1.4 GHz , language =

  225. [235]

    doi:10.1093/mnras/stv212 , eprint =

    , keywords =. doi:10.1093/mnras/stv212 , eprint =

    doi

  226. [236]

    Irfan, M. O. , month = 6, school =

  227. [237]

    Jaffe, T. R. and Leahy, J. P. and Banday, A. J. and Leach, S. M. and Lowe, S. R. and Wilkinson, A. , doi =. Monthly Notices of the Royal Astronomical Society , month =. 2010 , bdsk-url-1 =. https://academic.oup.com/mnras/article-pdf/401/2/1013/3958026/mnras0401-1013.pdf , issn =

    2010

  228. [238]

    doi:10.1111/j.1365-2966.2011.19114.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2011.19114.x , eprint =

    2011 doi

  229. [239]

    doi:10.1086/501343 , eprint =

    , keywords =. doi:10.1086/501343 , eprint =

    doi

  230. [240]

    doi:10.1111/j.1365-2966.2004.07169.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2004.07169.x , eprint =

    2004 doi

  231. [241]

    doi:10.1086/346080 , eprint =

    , keywords =. doi:10.1086/346080 , eprint =

    doi

  232. [242]

    doi:10.1111/j.1365-2966.2008.13634.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2008.13634.x , eprint =

    2008 doi

  233. [243]

    , keywords =

    The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization. , keywords =. doi:10.1093/mnras/stz2697 , archivePrefix =. 1907.11642 , primaryClass =

    1907 doi

  234. [244]

    C-Band All-Sky Survey (C-BASS) , year =

    Luke Jew , note =. C-Band All-Sky Survey (C-BASS) , year =

  235. [245]

    doi:10.1046/j.1365-8711.1998.01367.x , journal =

    1998 doi

  236. [246]

    doi:10.1051/0004-6361/200810621 , journal =

    doi

  237. [247]

    doi:10.1093/mnras/sty1956 , eprint =

    , keywords =. doi:10.1093/mnras/sty1956 , eprint =

    doi

  238. [248]

    , keywords =

    Suzaku observations of the Monogem Ring and the origin of the Gemini H ring. , keywords =. doi:10.1093/mnras/sty915 , adsurl =

    doi

  239. [249]

    arXiv e-prints , keywords =

    A new understanding of the Gemini-Monoceros X-ray enhancement from discoveries with eROSITA. arXiv e-prints , keywords =. doi:10.48550/arXiv.2401.17289 , archivePrefix =. 2401.17289 , primaryClass =

    doi

  240. [250]

    doi:10.1086/112957 , journal =

    doi

  241. [251]

    doi:10.1103/PhysRevD.55.7368 , eprint =

    , keywords =. doi:10.1103/PhysRevD.55.7368 , eprint =

    doi

  242. [252]

    doi:10.1146/annurev-astro-081915-023433 , eprint =

    Annual Review of Astronomy and Astrophysics , keywords =. doi:10.1146/annurev-astro-081915-023433 , eprint =

    doi

  243. [253]

    doi:10.3847/1538-4357/aadb3f , eid =

    2018 , bdsk-url-1 =. doi:10.3847/1538-4357/aadb3f , eid =. arXiv , author =:1808.05327 , journal =

    2018 doi arXiv

  244. [254]

    , month = dec, pages =

  245. [255]

    doi:10.1111/j.1365-2966.2005.09055.x , eprint =

    , keywords =. doi:10.1111/j.1365-2966.2005.09055.x , eprint =

    2005 doi

  246. [256]

    arXiv , author =:1503.02315 , journal =

    doi:10.1088/0004-637X/807/2/151 , eid =. arXiv , author =:1503.02315 , journal =

    doi arXiv

  247. [257]

    Modelling Of Solar Sidelobe Profiles For The C-Band All Sky Survey (C-BASS) North Telescope , year =

    Michael Kennedy , school =. Modelling Of Solar Sidelobe Profiles For The C-Band All Sky Survey (C-BASS) North Telescope , year =

  248. [258]

    King , school =

    O.G. King , school =. C-BASS: The C-Band All-Sky Survey , year =

  249. [259]

    doi:10.1093/mnras/stu2172 , eprint =

    , keywords =. doi:10.1093/mnras/stu2172 , eprint =

    doi

  250. [260]

    doi:10.1093/mnras/stt2359 , eprint =

    , keywords =. doi:10.1093/mnras/stt2359 , eprint =

    doi

  251. [261]

    arXiv , author =:1008.4082 , month = jul, primaryclass =

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , doi =. arXiv , author =:1008.4082 , month = jul, primaryclass =

    arXiv

  252. [262]

    C-BASS : the C-band all-sky survey , url =

    King, Oliver Gray , language =. C-BASS : the C-band all-sky survey , url =. 2009 , bdsk-url-1 =

    2009

  253. [263]

    arXiv , author =:0901.0562 , journal =

    doi:10.1088/0004-637X/734/1/4 , eid =. arXiv , author =:0901.0562 , journal =

    doi arXiv

  254. [264]

    doi:10.1086/310072 , eprint =

    , keywords =. doi:10.1086/310072 , eprint =

    doi

  255. [265]

    arXiv , author =:1205.4041 , journal =

    doi:10.1088/0004-637X/753/2/110 , eid =. arXiv , author =:1205.4041 , journal =

    doi arXiv

  256. [266]

    arXiv , author =:1105.2044 , journal =

    doi:10.1088/1475-7516/2011/07/025 , eid =. arXiv , author =:1105.2044 , journal =

    2011 doi arXiv

  257. [267]

    doi:10.1117/12.925204 , eid =

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , date-modified =. doi:10.1117/12.925204 , eid =

    doi

  258. [268]

    doi:10.1086/519754 , eprint =

    , keywords =. doi:10.1086/519754 , eprint =

    doi

  259. [269]

    doi:10.1093/mnras/stx2632 , eprint =

    , keywords =. doi:10.1093/mnras/stx2632 , eprint =

    doi

  260. [270]

    arXiv , author =:1001.4538 , journal =

    doi:10.1088/0067-0049/192/2/18 , eid =. arXiv , author =:1001.4538 , journal =

    doi arXiv

  261. [271]

    doi:10.1086/171264 , journal =

    doi

  262. [272]

    arXiv , author =:1802.01145 , journal =

    doi:10.1051/0004-6361/201832768 , eid =. arXiv , author =:1802.01145 , journal =

    doi arXiv

  263. [273]

    doi:10.1086/191952 , journal =

    doi

  264. [274]

    Lada and Marco Lombardi and Jo

    Charles J. Lada and Marco Lombardi and Jo. doi:10.1088/0004-637x/703/1/52 , journal =

    doi

  265. [275]

    doi:10.1051/0004-6361:20030545 , eprint =

    , keywords =. doi:10.1051/0004-6361:20030545 , eprint =

    doi

  266. [276]

    doi:10.1051/0004-6361/201834695 , eid =

    2019 , bdsk-url-1 =. doi:10.1051/0004-6361/201834695 , eid =. arXiv , author =:1902.04116 , journal =

    2019 doi arXiv

  267. [277]

    doi:10.1051/0004-6361/201832832 , eid =

    2018 , bdsk-url-1 =. doi:10.1051/0004-6361/201832832 , eid =. arXiv , author =:1804.06060 , journal =

    2018 doi arXiv

  268. [278]

    arXiv , author =:2203.01312 , journal =

  269. [279]

    arXiv , author =:1903.00426 , journal =

    doi:10.3847/1538-4357/ab7b6b , eid =. arXiv , author =:1903.00426 , journal =

    1903 doi

  270. [280]

    doi:10.1071/AS98070 , journal =

    1998 , bdsk-url-1 =. doi:10.1071/AS98070 , journal =

    1998 doi

  271. [281]

    arXiv , author =:1001.4635 , journal =

    doi:10.1088/0067-0049/192/2/16 , eid =. arXiv , author =:1001.4635 , journal =

    doi arXiv

  272. [282]

    doi:10.1086/312720 , eprint =

    , keywords =. doi:10.1086/312720 , eprint =

    doi

  273. [283]

    doi:10.1051/0004-6361:200810116 , eprint =

    , keywords =. doi:10.1051/0004-6361:200810116 , eprint =

    doi

  274. [284]

    doi:10.1093/mnras/226.2.433 , journal =

    doi

  275. [285]

    The Astrophysical Journal , month =

    Dukhang Lee and Kwang-Il Seon and Young-Soo Jo , doi =. The Astrophysical Journal , month =

  276. [286]

    doi:10.1086/310823 , eprint =

    , keywords =. doi:10.1086/310823 , eprint =

    doi

  277. [287]

    doi:10.1086/428825 , eprint =

    , keywords =. doi:10.1086/428825 , eprint =

    doi

  278. [288]

    Li and Risa H

    Tony Y. Li and Risa H. Wechsler and Kiruthika Devaraj and Sarah E. Church , journal =. Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly , url =. 2016 , bdsk-url-1 =

    2016

  279. [289]

    doi:10.1016/0370-2693(82)91219-9 , journal =

    doi

  280. [290]

    arXiv , author =:1404.1899 , journal =

    doi:10.1088/2041-8205/789/2/L29 , eid =. arXiv , author =:1404.1899 , journal =

    doi arXiv

  281. [291]

    doi:10.1007/s12036-014-9203-2 , journal =

    doi

  282. [292]

    arXiv , author =:1401.4690 , journal =

    arXiv

  283. [293]

    arXiv , author =:1011.1242 , journal =

    doi:10.1088/0004-637X/729/1/25 , eid =. arXiv , author =:1011.1242 , journal =

    doi arXiv

  284. [294]

    arXiv , author =:1109.5093 , journal =

    doi:10.1088/0004-637X/749/2/165 , eid =. arXiv , author =:1109.5093 , journal =

    doi arXiv

  285. [295]

    Cosmological Signature of New Parity-Violating Interactions , url =

    Lue, Arthur and Wang, Limin and Kamionkowski, Marc , doi =. Cosmological Signature of New Parity-Violating Interactions , url =. Phys. Rev. Lett. , month =. 1999 , bdsk-url-1 =

    1999

  286. [296]

    doi:10.1086/190072 , journal =

    doi

  287. [297]

    doi:10.1111/j.1365-2966.2011.19542.x , journal =

    2011 doi

  288. [298]

    doi:10.1086/165818 , journal =

    doi

  289. [299]

    arXiv , author =:0902.2850 , month = sep, pages =

    Astronomical Data Analysis Software and Systems XVIII , editor =. arXiv , author =:0902.2850 , month = sep, pages =

    arXiv

  290. [300]

    doi:10.1046/j.1365-2966.2003.06885.x , eprint =

    , keywords =. doi:10.1046/j.1365-2966.2003.06885.x , eprint =

    2003 doi

Pith tools

Reviewed May 25, 2026 · model on record in the stance chip above.