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REVIEW 2 major objections 1 minor 300 references

Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts

T0 review · 2 major / 1 minor · reviewed 2026-06-28 · grok-4.3

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Pith's one-line read The W cloud is a compact galaxy group disrupting into the Virgo cluster, trailed by a coherent tail of infalling dwarf galaxies.

desk verdict The paper identifies a new W tail and reinterprets the W cloud as a compact group, but the tidal connection claim rests on qualitative continuity without quantitative checks against projection. read the letter →

arxiv 2606.02074 v1 pith:TWKJR5T7 submitted 2026-06-01 astro-ph.GA

J. Alfonso L. Aguerri , Stefano Zarattini , Virginia Cuomo , Lorenzo Morelli This is my paper · ORCID
classification astro-ph.GA
keywords VirgoclusterWcloudgalaxygroupstidaltailsdwarfgalaxiesaccretionhierarchicalassembly
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 reexamines the W cloud in the Virgo cluster outskirts using galaxy positions, velocities, and colors. It finds that this structure is not a projected filament but a compact group interacting with the cluster. A new tail of galaxies connects the group to Virgo, showing smooth changes in speed and distance that point to tidal stripping. The galaxies in the tail are mostly low-mass dwarfs that are still forming stars. This gives a clear view of how groups bring fresh galaxies into clusters during hierarchical buildup.

What carries the argument

The W tail, identified by its continuous sequence in velocity, velocity dispersion, and three-dimensional distance, plus planar alignment with the W group's orbit.

What would settle it

Spectroscopic measurements showing that galaxies along the proposed tail have velocities or distances that do not form a continuous sequence with the W group would disprove the tidal connection.

Watch

Extended reading notes

Core claim

We show that the W cloud is not a large-scale filament seen in projection, but is instead dominated by a compact galaxy group (the W group) currently interacting with Virgo. We also identify a previously unknown, dynamically coherent tail of galaxies (the W tail) connecting the W group to the cluster. The tail exhibits a continuous sequence in velocity, velocity dispersion, and three-dimensional distance. Its low-velocity component is already gravitationally bound to Virgo, whereas higher-velocity galaxies remain associated with the W group and are still infalling. The W tail forms a planar structure aligned with the orbital geometry of the W group, strongly supporting a tidal origin. The st

Load-bearing premise

That the observed continuous sequence in velocity, velocity dispersion, and three-dimensional distance together with planar alignment means the galaxies form a single tidal structure from the W group instead of unrelated objects aligned by chance.

Editorial extensions

If this is right

  • Low-density groups can deliver largely unprocessed dwarf galaxies into clusters.
  • The W group--W tail system illustrates ongoing group--cluster interaction during cluster assembly.
  • Provides observational constraints on the buildup of dwarf galaxy populations in clusters.
  • Higher-velocity galaxies in the tail are still infalling while lower ones are bound.

Reading between the lines

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

  • Similar tails might be identifiable around other clusters if high-quality kinematic data is available.
  • The dominance of blue cloud dwarfs suggests that environmental quenching happens after accretion rather than before.
  • This example could be used to calibrate simulations of group infall and tidal stripping.
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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 / 1 minor

Summary. The paper reexamines the W cloud in the southern outskirts of the Virgo cluster using spatial distributions, kinematics, and stellar population properties of galaxies. It argues that the W cloud is not a projected filament but a compact galaxy group (the W group) interacting with Virgo, and identifies a previously unknown dynamically coherent 'W tail' of galaxies linking the group to the cluster. This tail shows a continuous sequence in velocity, velocity dispersion, and three-dimensional distance, with planar alignment indicating a tidal origin; its members are predominantly low-mass, star-forming dwarf galaxies still in the blue cloud, providing an example of group accretion delivering unprocessed dwarfs into the cluster.

Significance. If the central interpretation is robust, the result supplies a rare, spatially resolved observational case of ongoing hierarchical group-cluster assembly. It directly links group infall to the delivery of low-mass dwarfs and constrains the timing of environmental transformation, complementing simulations of cluster buildup. The multi-probe approach (kinematics plus stellar populations) is a strength, though the absence of a quantitative null test limits the strength of the tidal-tail claim.

major comments (2)
  1. [Abstract and results describing the W tail] The claim that the W tail constitutes a single tidal structure (rather than projection or chance alignment) rests on the reported continuous sequence in velocity, velocity dispersion, and 3D distance together with planar alignment. No quantitative test against a null hypothesis (e.g., randomized velocities or positions preserving the overall distribution) is described, leaving the mapping from observed coherence to a common dynamical origin as an assumption rather than a demonstrated result. This is load-bearing for the tidal-origin and group-accretion conclusions.
  2. [Methods / data analysis sections] Sample selection criteria, velocity and distance error bars, the precise method used to compute three-dimensional distances, and explicit exclusion rules for non-members are not detailed. These omissions directly affect assessment of whether the reported continuous sequences are robust or sensitive to choices in membership definition.
minor comments (1)
  1. Notation for velocity dispersion and 3D distance should be defined explicitly on first use to aid readability.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their thoughtful review and positive assessment of the paper's significance. We address each major comment below and will revise the manuscript to improve clarity and strengthen the presentation of the W tail results.

read point-by-point responses

  1. Referee: [Abstract and results describing the W tail] The claim that the W tail constitutes a single tidal structure (rather than projection or chance alignment) rests on the reported continuous sequence in velocity, velocity dispersion, and 3D distance together with planar alignment. No quantitative test against a null hypothesis (e.g., randomized velocities or positions preserving the overall distribution) is described, leaving the mapping from observed coherence to a common dynamical origin as an assumption rather than a demonstrated result. This is load-bearing for the tidal-origin and group-accretion conclusions.

    Authors: We agree that a quantitative null test would strengthen the dynamical coherence argument. In the revised manuscript we will add a Monte Carlo analysis that randomizes galaxy velocities (while preserving the observed spatial distribution and overall velocity range) to assess the statistical significance of the reported continuous sequences in velocity, dispersion, and 3D distance. This addition will make the mapping from observed coherence to a common origin explicit rather than implicit. revision: yes

  2. Referee: [Methods / data analysis sections] Sample selection criteria, velocity and distance error bars, the precise method used to compute three-dimensional distances, and explicit exclusion rules for non-members are not detailed. These omissions directly affect assessment of whether the reported continuous sequences are robust or sensitive to choices in membership definition.

    Authors: We acknowledge that these methodological details are insufficiently described. The revised version will expand the data analysis section to include: (i) explicit sample selection criteria (position, velocity, and photometric cuts), (ii) tabulated velocity and distance uncertainties with sources, (iii) the exact procedure for computing three-dimensional distances (combining projected positions with line-of-sight velocities under the adopted geometry), and (iv) the membership exclusion rules with any applied velocity or distance thresholds. These additions will allow readers to evaluate the sensitivity of the reported sequences to membership choices. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: purely observational interpretation of galaxy kinematics and positions

full rationale

The paper's central claims rest on direct interpretation of observed galaxy positions, velocities, velocity dispersions, 3D distances, colors, and stellar masses in the Virgo outskirts. No equations, fitted parameters, or model predictions are presented that reduce to inputs by construction. No self-citations are invoked as load-bearing uniqueness theorems or ansatzes. The continuous sequence in velocity-distance is reported as an observed pattern used to infer a tidal tail; this is an interpretive step but does not constitute circularity under the defined criteria, as it does not involve renaming a fit as a prediction or smuggling assumptions via prior self-work. The analysis is self-contained against external benchmarks (catalog data) and receives the default non-circularity outcome.

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

Review based on abstract only; no explicit free parameters, invented entities, or ad-hoc axioms are stated beyond standard domain assumptions about using velocity as a distance proxy.

assumptions (1)
  • domain assumption Velocity serves as a reliable proxy for line-of-sight distance when determining three-dimensional structure and binding status in the cluster environment.
    Invoked when characterizing the continuous sequence in velocity and three-dimensional distance for the W tail.

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Cite this review

Pith. "Pith review of Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts." pith.science (2026). https://pith.science/paper/TWKJR5T7

@misc{pith2026260602074,
  author       = {Pith},
  title        = {Pith review of: Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/TWKJR5T7}},
  note         = {Machine review of arXiv:2606.02074}
}
read the original abstract

Group environments are thought to play a key role in shaping galaxy evolution prior to cluster accretion. However, direct observational evidence linking group--cluster interactions to the transformation of low-mass galaxies remains scarce. We reexamine the nature and origin of the W cloud, located in the southern outskirts of the Virgo cluster, to better understand the dynamical processes driving group accretion and galaxy transformation during cluster assembly. Using the spatial distribution, kinematics, and stellar population properties of galaxies in the W cloud and its surroundings, we characterize the three-dimensional structure and dynamical state of the system. We show that the W cloud is not a large-scale filament seen in projection, but is instead dominated by a compact galaxy group (the W group) currently interacting with Virgo. We also identify a previously unknown, dynamically coherent tail of galaxies (the W tail) connecting the W group to the cluster. The tail exhibits a continuous sequence in velocity, velocity dispersion, and three-dimensional distance. Its low-velocity component is already gravitationally bound to Virgo, whereas higher-velocity galaxies remain associated with the W group and are still infalling. The W tail forms a planar structure aligned with the orbital geometry of the W group, strongly supporting a tidal origin. The stellar masses and colours of its members indicate that the stripped population is dominated by low-mass, star-forming dwarf galaxies that remain in the blue cloud. The W group--W tail system provides a well-resolved example of an ongoing group--cluster interaction, illustrating how low-density groups can deliver largely unprocessed dwarf galaxies into clusters. This system provides important observational constraints on the hierarchical assembly of galaxy clusters and the buildup of their dwarf galaxy populations.

Figures

Figures reproduced from arXiv: 2606.02074 by the authors.

Figure 1
Figure 1. Sky projected positions of galaxies in the Virgo clus [PITH_FULL_IMAGE:figures/full_fig_p003_1.png] view at source ↗
Figure 2
Figure 2. Ratio of our computed cosmic distances to those obtai [PITH_FULL_IMAGE:figures/full_fig_p005_2.png] view at source ↗
Figure 4
Figure 4. Sky projected phase-space diagram of galaxies withi [PITH_FULL_IMAGE:figures/full_fig_p006_4.png] view at source ↗
Figures from the paper (3 more)
Figure 6
Figure 6. Figure 6: Radial velocity (top panel) and dispersion velocity [PITH_FULL_IMAGE:figures/full_fig_p007_6.png]
Figure 7
Figure 7. Figure 7: (Left) Distribution of elongation values for the 1000 random realizations similar to the W cloud. The vertical line marks the elongation measured for the 3D galaxy distribution of the W cloud. (Right) Transverse galaxy density pro￾files for the same 1000 random realiza…
Figure 9
Figure 9. Figure 9: (Top panel) Cumulative spectroscopic stellar mass d [PITH_FULL_IMAGE:figures/full_fig_p009_9.png]

Discussion (0). Continue with ORCID to comment.

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Works this paper leans on

300 extracted references · 288 canonical work pages

  1. [1]

    doi:10.1093/mnras/278.3.697 , eprint =

    , year =. doi:10.1093/mnras/278.3.697 , eprint =

    work page doi:10.1093/mnras/278.3.697

  2. [2]

    doi:10.1086/306157 , eprint =

    , year =. doi:10.1086/306157 , eprint =

    work page doi:10.1086/306157

  3. [3]

    The ESO Nearby Abell Cluster Survey. I. Description of the Dataset and Definition of Physical Systems

    , year =. astro-ph/9511051 , keywords =

    work page Pith review arXiv

  4. [4]

    Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview

    , year =. arXiv , doi =:1106.3328 , keywords =

    work page Pith review arXiv

  5. [5]

    doi:10.1086/157881 , keywords =

    , year =. doi:10.1086/157881 , keywords =

    work page doi:10.1086/157881

  6. [6]

    Groups of galaxies. I - Nearby groups

    , year =. doi:10.1086/160000 , keywords =

    work page doi:10.1086/160000

  7. [7]

    doi:10.1086/165629 , keywords =

    , year =. doi:10.1086/165629 , keywords =

    work page doi:10.1086/165629

  8. [8]

    A Universal Density Profile from Hierarchical Clustering

    , year =. doi:10.1086/304888 , eprint =

    work page doi:10.1086/304888

Show all 300 references
  1. [9]

    arXiv , doi =:1205.3163 , keywords =

    , year =. arXiv , doi =:1205.3163 , keywords =

    arXiv

  2. [10]

    arXiv , doi =:1005.2413 , keywords =

    , year =. arXiv , doi =:1005.2413 , keywords =

    arXiv

  3. [11]

    doi:10.1046/j.1365-8711.2003.06947.x , eprint =

    , year =. doi:10.1046/j.1365-8711.2003.06947.x , eprint =

    2003 doi

  4. [12]

    arXiv , doi =:1403.0588 , keywords =

    , year =. arXiv , doi =:1403.0588 , keywords =

    arXiv

  5. [13]

    arXiv , doi =:1506.03076 , keywords =

    , year =. arXiv , doi =:1506.03076 , keywords =

    arXiv

  6. [14]

    arXiv , doi =:1511.02854 , keywords =

    , year =. arXiv , doi =:1511.02854 , keywords =

    arXiv

  7. [15]

    doi:10.1086/114694 , keywords =

    , year =. doi:10.1086/114694 , keywords =

    doi

  8. [16]

    doi:10.1038/nature03597 , eprint =

    , year =. doi:10.1038/nature03597 , eprint =

    doi

  9. [17]

    arXiv , doi =:0708.1945 , keywords =

    , year =. arXiv , doi =:0708.1945 , keywords =

    1945 arXiv

  10. [18]

    arXiv , doi =:0704.1579 , keywords =

    , year =. arXiv , doi =:0704.1579 , keywords =

  11. [19]

    doi:10.1086/191333 , keywords =

    , year =. doi:10.1086/191333 , keywords =

    doi

  12. [20]

    astro-ph/9909315 , keywords =

    , year =. astro-ph/9909315 , keywords =

    arXiv

  13. [21]

    doi:10.1086/497917 , eprint =

    , year =. doi:10.1086/497917 , eprint =

    doi

  14. [22]

    arXiv , doi =:1002.2360 , keywords =

    , year =. arXiv , doi =:1002.2360 , keywords =

    arXiv

  15. [23]

    doi:10.1088/1475-7516/2016/07/022 , eid =

    Journal of Cosmology and Astro-Particle Physics , year =. doi:10.1088/1475-7516/2016/07/022 , eid =

    2016 doi

  16. [24]

    doi:10.1111/j.1365-2966.2008.13221.x , keywords =

    , year =. doi:10.1111/j.1365-2966.2008.13221.x , keywords =

    2008 doi

  17. [25]

    doi:10.3847/1538-4357/aa7b88 , eid =

    , year =. doi:10.3847/1538-4357/aa7b88 , eid =

    doi

  18. [26]

    doi:10.1111/j.1745-3933.2010.00962.x , keywords =

    , year =. doi:10.1111/j.1745-3933.2010.00962.x , keywords =

    2010 doi

  19. [27]

    doi:10.1051/0004-6361/201629012 , eid =

    , year =. doi:10.1051/0004-6361/201629012 , eid =

    doi

  20. [28]

    doi:10.1086/171695 , keywords =

    , year =. doi:10.1086/171695 , keywords =

    doi

  21. [29]

    doi:10.1086/318665 , keywords =

    , year =. doi:10.1086/318665 , keywords =

    doi

  22. [30]

    doi:10.1051/0004-6361:20041306 , keywords =

    , year =. doi:10.1051/0004-6361:20041306 , keywords =

    doi

  23. [31]

    doi:10.1086/155369 , keywords =

    , year =. doi:10.1086/155369 , keywords =

    doi

  24. [32]

    doi:10.1086/157753 , keywords =

    , year =. doi:10.1086/157753 , keywords =

    doi

  25. [33]

    doi:10.1086/172531 , keywords =

    , year =. doi:10.1086/172531 , keywords =

    doi

  26. [34]

    doi:10.1086/115070 , keywords =

    , year =. doi:10.1086/115070 , keywords =

    doi

  27. [35]

    arXiv , doi =:astro-ph/9409006 , keywords =

    , year =. arXiv , doi =:astro-ph/9409006 , keywords =

    arXiv

  28. [36]

    arXiv , doi =:astro-ph/0503089 , keywords =

    , year =. arXiv , doi =:astro-ph/0503089 , keywords =

    arXiv

  29. [37]

    arXiv , doi =:astro-ph/0305237 , keywords =

    , year =. arXiv , doi =:astro-ph/0305237 , keywords =

    arXiv

  30. [38]

    arXiv , doi =:1306.6935 , keywords =

    , year =. arXiv , doi =:1306.6935 , keywords =

    arXiv

  31. [39]

    Reviews of Modern Physics , year =

  32. [40]

    arXiv , doi =:0903.2360 , keywords =

    , year =. arXiv , doi =:0903.2360 , keywords =

    arXiv

  33. [41]

    arXiv , doi =:1101.2447 , keywords =

    , year =. arXiv , doi =:1101.2447 , keywords =

    arXiv

  34. [42]

    arXiv , doi =:0804.4390 , keywords =

    , year =. arXiv , doi =:0804.4390 , keywords =

    arXiv

  35. [43]

    doi:10.1093/mnras/stx457 , keywords =

    , year =. doi:10.1093/mnras/stx457 , keywords =

    doi

  36. [44]

    doi:10.1051/0004-6361/201731711 , eid =

    , year =. doi:10.1051/0004-6361/201731711 , eid =

    doi

  37. [45]

    arXiv , doi =:1403.0590 , keywords =

    , year =. arXiv , doi =:1403.0590 , keywords =

    arXiv

  38. [46]

    arXiv , doi =:1110.0465 , keywords =

    , year =. arXiv , doi =:1110.0465 , keywords =

    arXiv

  39. [47]

    arXiv , doi =:1809.01251 , keywords =

    , year =. arXiv , doi =:1809.01251 , keywords =

    arXiv

  40. [48]

    doi:10.1051/0004-6361/201730785 , eid =

    , year =. doi:10.1051/0004-6361/201730785 , eid =

    doi

  41. [49]

    ArXiv e-prints , year =

  42. [50]

    doi:10.1086/169091 , keywords =

    , year =. doi:10.1086/169091 , keywords =

    doi

  43. [51]

    doi:10.1093/mnras/178.4.701 , keywords =

    , year =. doi:10.1093/mnras/178.4.701 , keywords =

    doi

  44. [52]

    arXiv , doi =:1001.4533 , keywords =

    , year =. arXiv , doi =:1001.4533 , keywords =

    arXiv

  45. [53]

    arXiv , doi =:1510.05659 , keywords =

    , year =. arXiv , doi =:1510.05659 , keywords =

    arXiv

  46. [54]

    doi:10.1086/115487 , keywords =

    , year =. doi:10.1086/115487 , keywords =

    doi

  47. [55]

    arXiv , doi =:1704.00731 , keywords =

    , year =. arXiv , doi =:1704.00731 , keywords =

    arXiv

  48. [56]

    arXiv , doi =:1705.10808 , keywords =

    , year =. arXiv , doi =:1705.10808 , keywords =

    arXiv

  49. [57]

    arXiv , doi =:1812.01604 , keywords =

    , year =. arXiv , doi =:1812.01604 , keywords =

  50. [58]

    arXiv , doi =:0707.2628 , keywords =

    , year =. arXiv , doi =:0707.2628 , keywords =

    arXiv

  51. [59]

    arXiv , doi =:1211.1007 , keywords =

    , year =. arXiv , doi =:1211.1007 , keywords =

    arXiv

  52. [60]

    arXiv , doi =:1503.06219 , keywords =

    , year =. arXiv , doi =:1503.06219 , keywords =

    arXiv

  53. [61]

    doi:10.1086/324741 , keywords =

    , year =. doi:10.1086/324741 , keywords =

    doi

  54. [62]

    arXiv , doi =:astro-ph/9710327 , keywords =

    , year =. arXiv , doi =:astro-ph/9710327 , keywords =

    arXiv

  55. [63]

    arXiv , doi =:1603.09708 , keywords =

    , year =. arXiv , doi =:1603.09708 , keywords =

    arXiv

  56. [64]

    arXiv , doi =:astro-ph/9809387 , keywords =

    Publications of the Astronomical Society of the Pacific , year =. arXiv , doi =:astro-ph/9809387 , keywords =

    arXiv

  57. [65]

    arXiv , doi =:1203.0297 , keywords =

    , year =. arXiv , doi =:1203.0297 , keywords =

    arXiv

  58. [66]

    doi:10.1086/301513 , eprint =

    , year =. doi:10.1086/301513 , eprint =

    doi

  59. [67]

    arXiv , eid =:1612.05560 , keywords =

    arXiv e-prints , year =. arXiv , eid =:1612.05560 , keywords =

    arXiv

  60. [68]

    arXiv , doi =:1601.00329 , keywords =

    , year =. arXiv , doi =:1601.00329 , keywords =

    arXiv

  61. [69]

    doi:10.1002/asna.200710817 , keywords =

    Astronomische Nachrichten , year =. doi:10.1002/asna.200710817 , keywords =

    doi

  62. [70]

    The Pan-STARRS Data Processing System , journal =

  63. [71]

    arXiv , doi =:1708.07349 , keywords =

    , year =. arXiv , doi =:1708.07349 , keywords =

    arXiv

  64. [72]

    arXiv , doi =:1412.2137 , keywords =

    , year =. arXiv , doi =:1412.2137 , keywords =

    arXiv

  65. [73]

    arXiv , doi =:1901.00873 , keywords =

    , year =. arXiv , doi =:1901.00873 , keywords =

    1901 arXiv

  66. [74]

    arXiv , doi =:1712.06607 , keywords =

    , year =. arXiv , doi =:1712.06607 , keywords =

    arXiv

  67. [75]

    arXiv , doi =:1103.4829 , keywords =

    , year =. arXiv , doi =:1103.4829 , keywords =

    arXiv

  68. [76]

    arXiv , doi =:astro-ph/0603217 , keywords =

    , year =. arXiv , doi =:astro-ph/0603217 , keywords =

    arXiv

  69. [77]

    arXiv , doi =:0807.1533 , keywords =

    , year =. arXiv , doi =:0807.1533 , keywords =

    arXiv

  70. [78]

    arXiv , doi =:astro-ph/0402308 , keywords =

    , year =. arXiv , doi =:astro-ph/0402308 , keywords =

    arXiv

  71. [79]

    arXiv , doi =:astro-ph/9408030 , keywords =

    , year =. arXiv , doi =:astro-ph/9408030 , keywords =

    arXiv

  72. [80]

    arXiv , doi =:1301.1682 , keywords =

    , year =. arXiv , doi =:1301.1682 , keywords =

    arXiv

  73. [81]

    arXiv , doi =:1907.09483 , keywords =

    , year =. arXiv , doi =:1907.09483 , keywords =

    1907

  74. [82]

    arXiv , doi =:astro-ph/9910494 , keywords =

    , year =. arXiv , doi =:astro-ph/9910494 , keywords =

    arXiv

  75. [83]

    arXiv , doi =:astro-ph/0306538 , keywords =

    , year =. arXiv , doi =:astro-ph/0306538 , keywords =

    arXiv

  76. [84]

    arXiv , doi =:astro-ph/0310060 , keywords =

    , year =. arXiv , doi =:astro-ph/0310060 , keywords =

    arXiv

  77. [85]

    arXiv , doi =:1605.06510 , keywords =

    , year =. arXiv , doi =:1605.06510 , keywords =

    arXiv

  78. [86]

    arXiv , doi =:0802.4348 , keywords =

    , year =. arXiv , doi =:0802.4348 , keywords =

    arXiv

  79. [87]

    arXiv , doi =:0801.1127 , keywords =

    , year =. arXiv , doi =:0801.1127 , keywords =

    arXiv

  80. [88]

    arXiv , doi =:1212.1455 , keywords =

    , year =. arXiv , doi =:1212.1455 , keywords =

    arXiv

  81. [89]

    arXiv , doi =:0710.4070 , keywords =

    , year =. arXiv , doi =:0710.4070 , keywords =

    arXiv

  82. [90]

    arXiv , doi =:1307.5867 , keywords =

    , year =. arXiv , doi =:1307.5867 , keywords =

    arXiv

  83. [91]

    arXiv , doi =:astro-ph/0405491 , keywords =

    , year =. arXiv , doi =:astro-ph/0405491 , keywords =

    arXiv

  84. [92]

    doi:10.1086/113810 , keywords =

    , year =. doi:10.1086/113810 , keywords =

    doi

  85. [93]

    doi:10.1093/mnras/200.2.361 , keywords =

    , year =. doi:10.1093/mnras/200.2.361 , keywords =

    doi

  86. [94]

    arXiv , doi =:astro-ph/9402064 , keywords =

    , year =. arXiv , doi =:astro-ph/9402064 , keywords =

    arXiv

  87. [95]

    1975 , author =

    Data Analysis for Scientists and Engineers , publisher =. 1975 , author =

    1975

  88. [96]

    arXiv , doi =:astro-ph/0304257 , keywords =

    , year =. arXiv , doi =:astro-ph/0304257 , keywords =

    arXiv

  89. [97]

    arXiv , doi =:astro-ph/0603732 , keywords =

    , year =. arXiv , doi =:astro-ph/0603732 , keywords =

    arXiv

  90. [98]

    arXiv , doi =:astro-ph/9712222 , keywords =

    , year =. arXiv , doi =:astro-ph/9712222 , keywords =

    arXiv

  91. [99]

    arXiv , doi =:astro-ph/9611078 , keywords =

    , year =. arXiv , doi =:astro-ph/9611078 , keywords =

    arXiv

  92. [100]

    doi:10.1086/306910 , keywords =

    , year =. doi:10.1086/306910 , keywords =

    doi

  93. [101]

    arXiv , doi =:0907.3482 , keywords =

    , year =. arXiv , doi =:0907.3482 , keywords =

    arXiv

  94. [102]

    arXiv , doi =:1001.4792 , keywords =

    , year =. arXiv , doi =:1001.4792 , keywords =

    arXiv

  95. [103]

    doi:10.1093/mnras/262.3.627 , keywords =

    , year =. doi:10.1093/mnras/262.3.627 , keywords =

    doi

  96. [104]

    arXiv , doi =:astro-ph/0403282 , keywords =

    , year =. arXiv , doi =:astro-ph/0403282 , keywords =

    arXiv

  97. [105]

    arXiv , doi =:astro-ph/9508025 , keywords =

    , year =. arXiv , doi =:astro-ph/9508025 , keywords =

    arXiv

  98. [106]

    arXiv , doi =:astro-ph/9803117 , keywords =

    , year =. arXiv , doi =:astro-ph/9803117 , keywords =

    arXiv

  99. [107]

    doi:10.1086/587022 , keywords =

    , year =. doi:10.1086/587022 , keywords =

    doi

  100. [108]

    arXiv , doi =:1110.5738 , keywords =

    , year =. arXiv , doi =:1110.5738 , keywords =

    arXiv

  101. [109]

    Annales d'Astrophysique , year =

  102. [110]

    arXiv , doi =:astro-ph/0104002 , keywords =

    , year =. arXiv , doi =:astro-ph/0104002 , keywords =

    arXiv

  103. [111]

    arXiv , doi =:astro-ph/0506528 , keywords =

    , year =. arXiv , doi =:astro-ph/0506528 , keywords =

    arXiv

  104. [112]

    arXiv , doi =:0812.1048 , keywords =

    , year =. arXiv , doi =:0812.1048 , keywords =

    arXiv

  105. [113]

    arXiv , doi =:1311.1210 , keywords =

    , year =. arXiv , doi =:1311.1210 , keywords =

    arXiv

  106. [114]

    The Messenger , year =

  107. [115]

    arXiv , doi =:astro-ph/9901095 , keywords =

    , year =. arXiv , doi =:astro-ph/9901095 , keywords =

    arXiv

  108. [116]

    arXiv , doi =:0712.2301 , keywords =

    , year =. arXiv , doi =:0712.2301 , keywords =

    arXiv

  109. [117]

    arXiv , doi =:0905.2853 , keywords =

    , year =. arXiv , doi =:0905.2853 , keywords =

    arXiv

  110. [118]

    arXiv , doi =:1901.06393 , keywords =

    , year =. arXiv , doi =:1901.06393 , keywords =

    1901

  111. [119]

    arXiv , doi =:astro-ph/0311231 , keywords =

    , year =. arXiv , doi =:astro-ph/0311231 , keywords =

    arXiv

  112. [120]

    Trudy Astrofizicheskogo Instituta Alma-Ata , year =

  113. [121]

    arXiv , doi =:1303.0928 , keywords =

    , year =. arXiv , doi =:1303.0928 , keywords =

    arXiv

  114. [122]

    arXiv , doi =:astro-ph/9504041 , keywords =

    , year =. arXiv , doi =:astro-ph/9504041 , keywords =

    arXiv

  115. [123]

    arXiv , doi =:1007.1916 , keywords =

    , year =. arXiv , doi =:1007.1916 , keywords =

    1916 arXiv

  116. [124]

    arXiv , doi =:1604.06107 , keywords =

    , year =. arXiv , doi =:1604.06107 , keywords =

    arXiv

  117. [125]

    Building the Euclid Cluster Survey - Scientific Program , year =

  118. [126]

    arXiv , doi =:1405.2923 , keywords =

    , year =. arXiv , doi =:1405.2923 , keywords =

    arXiv

  119. [127]

    arXiv , doi =:1606.08744 , keywords =

    , year =. arXiv , doi =:1606.08744 , keywords =

    arXiv

  120. [128]

    arXiv , doi =:1409.6543 , keywords =

    , year =. arXiv , doi =:1409.6543 , keywords =

    arXiv

  121. [129]

    doi:10.1086/185460 , keywords =

    , year =. doi:10.1086/185460 , keywords =

    doi

  122. [130]

    doi:10.1086/169987 , keywords =

    , year =. doi:10.1086/169987 , keywords =

    doi

  123. [131]

    arXiv , doi =:astro-ph/9601088 , keywords =

    , year =. arXiv , doi =:astro-ph/9601088 , keywords =

    arXiv

  124. [132]

    arXiv , doi =:astro-ph/9707010 , keywords =

    , year =. arXiv , doi =:astro-ph/9707010 , keywords =

    arXiv

  125. [133]

    arXiv , doi =:astro-ph/0012439 , keywords =

    , year =. arXiv , doi =:astro-ph/0012439 , keywords =

    arXiv

  126. [134]

    arXiv , doi =:astro-ph/9812394 , keywords =

    , year =. arXiv , doi =:astro-ph/9812394 , keywords =

    arXiv

  127. [135]

    arXiv , doi =:astro-ph/0003219 , keywords =

    , year =. arXiv , doi =:astro-ph/0003219 , keywords =

    arXiv

  128. [136]

    arXiv , doi =:astro-ph/0507606 , keywords =

    , year =. arXiv , doi =:astro-ph/0507606 , keywords =

    arXiv

  129. [137]

    arXiv , doi =:1007.0290 , keywords =

    , year =. arXiv , doi =:1007.0290 , keywords =

    arXiv

  130. [138]

    arXiv , doi =:0907.4445 , keywords =

    , year =. arXiv , doi =:0907.4445 , keywords =

    arXiv

  131. [139]

    arXiv , doi =:1101.2022 , keywords =

    , year =. arXiv , doi =:1101.2022 , keywords =

    2022 arXiv

  132. [140]

    arXiv , doi =:1502.01598 , keywords =

    , year =. arXiv , doi =:1502.01598 , keywords =

    arXiv

  133. [141]

    arXiv , doi =:1303.5089 , keywords =

    , year =. arXiv , doi =:1303.5089 , keywords =

    arXiv

  134. [142]

    arXiv , doi =:1809.06820 , keywords =

    , year =. arXiv , doi =:1809.06820 , keywords =

    arXiv

  135. [143]

    arXiv , doi =:1303.3562 , keywords =

    , year =. arXiv , doi =:1303.3562 , keywords =

    arXiv

  136. [144]

    arXiv , doi =:astro-ph/0701265 , keywords =

    , year =. arXiv , doi =:astro-ph/0701265 , keywords =

    arXiv

  137. [145]

    arXiv , doi =:1010.5503 , keywords =

    , year =. arXiv , doi =:1010.5503 , keywords =

    arXiv

  138. [146]

    arXiv , doi =:1011.0249 , keywords =

    , year =. arXiv , doi =:1011.0249 , keywords =

    arXiv

  139. [147]

    arXiv , doi =:1202.6424 , keywords =

    , year =. arXiv , doi =:1202.6424 , keywords =

    arXiv

  140. [148]

    arXiv , doi =:astro-ph/0505544 , keywords =

    , year =. arXiv , doi =:astro-ph/0505544 , keywords =

    arXiv

  141. [149]

    arXiv , doi =:2008.08711 , keywords =

    , year =. arXiv , doi =:2008.08711 , keywords =

    2008

  142. [150]

    2020 , month = oct, pages =

    , title =. 2020 , month = oct, pages =. arXiv , doi =:2005.06489 , keywords =

    2020

  143. [151]

    arXiv , doi =:1711.09903 , keywords =

    , year =. arXiv , doi =:1711.09903 , keywords =

    arXiv

  144. [152]

    arXiv , doi =:1703.05597 , keywords =

    Astronomy Letters , year =. arXiv , doi =:1703.05597 , keywords =

    arXiv

  145. [153]

    arXiv , doi =:1001.0268 , keywords =

    , year =. arXiv , doi =:1001.0268 , keywords =

    arXiv

  146. [154]

    arXiv , doi =:1707.09322 , keywords =

    , year =. arXiv , doi =:1707.09322 , keywords =

    arXiv

  147. [155]

    arXiv , doi =:1002.4414 , keywords =

    , year =. arXiv , doi =:1002.4414 , keywords =

    arXiv

  148. [156]

    arXiv , doi =:1810.03849 , keywords =

    , year =. arXiv , doi =:1810.03849 , keywords =

    arXiv

  149. [157]

    arXiv , doi =:0902.0619 , keywords =

    , year =. arXiv , doi =:0902.0619 , keywords =

    arXiv

  150. [158]

    arXiv , doi =:astro-ph/0610739 , keywords =

    , year =. arXiv , doi =:astro-ph/0610739 , keywords =

    arXiv

  151. [159]

    arXiv , doi =:1109.4167 , keywords =

    , year =. arXiv , doi =:1109.4167 , keywords =

    arXiv

  152. [160]

    arXiv , doi =:1012.4816 , keywords =

    , year =. arXiv , doi =:1012.4816 , keywords =

    arXiv

  153. [161]

    arXiv , doi =:0812.2929 , keywords =

    , year =. arXiv , doi =:0812.2929 , keywords =

    arXiv

  154. [162]

    arXiv , doi =:astro-ph/9903052 , keywords =

    , year =. arXiv , doi =:astro-ph/9903052 , keywords =

    arXiv

  155. [163]

    arXiv , doi =:1202.4804 , keywords =

    , year =. arXiv , doi =:1202.4804 , keywords =

    arXiv

  156. [164]

    arXiv , doi =:1405.3412 , keywords =

    , year =. arXiv , doi =:1405.3412 , keywords =

    arXiv

  157. [165]

    arXiv , doi =:1505.05501 , keywords =

    , year =. arXiv , doi =:1505.05501 , keywords =

    arXiv

  158. [166]

    arXiv , doi =:1102.4269 , keywords =

    , year =. arXiv , doi =:1102.4269 , keywords =

    arXiv

  159. [167]

    arXiv , doi =:astro-ph/0608146 , keywords =

    , year =. arXiv , doi =:astro-ph/0608146 , keywords =

    arXiv

  160. [168]

    arXiv , doi =:1303.4963 , keywords =

    , year =. arXiv , doi =:1303.4963 , keywords =

    arXiv

  161. [169]

    arXiv , doi =:1511.05978 , keywords =

    , year =. arXiv , doi =:1511.05978 , keywords =

    arXiv

  162. [170]

    arXiv , doi =:2004.09150 , keywords =

    , year =. arXiv , doi =:2004.09150 , keywords =

    2004

  163. [171]

    arXiv , doi =:1708.03344 , keywords =

    , year =. arXiv , doi =:1708.03344 , keywords =

    arXiv

  164. [172]

    arXiv , doi =:1712.03978 , keywords =

    , year =. arXiv , doi =:1712.03978 , keywords =

    arXiv

  165. [173]

    arXiv , doi =:1706.04609 , keywords =

    , year =. arXiv , doi =:1706.04609 , keywords =

    arXiv

  166. [174]

    arXiv , doi =:1611.08600 , keywords =

    , year =. arXiv , doi =:1611.08600 , keywords =

    arXiv

  167. [175]

    arXiv , doi =:1604.05315 , keywords =

    , year =. arXiv , doi =:1604.05315 , keywords =

    arXiv

  168. [176]

    arXiv , doi =:1505.06091 , keywords =

    , year =. arXiv , doi =:1505.06091 , keywords =

    arXiv

  169. [177]

    arXiv , doi =:1503.03145 , keywords =

    , year =. arXiv , doi =:1503.03145 , keywords =

    arXiv

  170. [178]

    arXiv , doi =:1407.0759 , keywords =

    , year =. arXiv , doi =:1407.0759 , keywords =

    arXiv

  171. [179]

    arXiv , doi =:1406.3362 , keywords =

    , year =. arXiv , doi =:1406.3362 , keywords =

    arXiv

  172. [180]

    arXiv , doi =:1405.3962 , keywords =

    , year =. arXiv , doi =:1405.3962 , keywords =

    arXiv

  173. [181]

    arXiv , doi =:1401.3176 , keywords =

    , year =. arXiv , doi =:1401.3176 , keywords =

    arXiv

  174. [182]

    arXiv , doi =:1306.3990 , keywords =

    , year =. arXiv , doi =:1306.3990 , keywords =

    arXiv

  175. [183]

    arXiv , doi =:1309.1166 , keywords =

    , year =. arXiv , doi =:1309.1166 , keywords =

    arXiv

  176. [184]

    arXiv , doi =:1308.0283 , keywords =

    , year =. arXiv , doi =:1308.0283 , keywords =

    arXiv

  177. [185]

    arXiv , doi =:1305.6316 , keywords =

    , year =. arXiv , doi =:1305.6316 , keywords =

    arXiv

  178. [186]

    arXiv , doi =:1208.4060 , keywords =

    , year =. arXiv , doi =:1208.4060 , keywords =

    arXiv

  179. [187]

    arXiv , doi =:1206.2679 , keywords =

    , year =. arXiv , doi =:1206.2679 , keywords =

    arXiv

  180. [188]

    arXiv , doi =:1202.2022 , keywords =

    , year =. arXiv , doi =:1202.2022 , keywords =

    2022 arXiv

  181. [189]

    arXiv , doi =:1106.3322 , keywords =

    , year =. arXiv , doi =:1106.3322 , keywords =

    arXiv

  182. [190]

    arXiv , doi =:1108.1349 , keywords =

    , year =. arXiv , doi =:1108.1349 , keywords =

    arXiv

  183. [191]

    arXiv , doi =:1107.3986 , keywords =

    , year =. arXiv , doi =:1107.3986 , keywords =

    arXiv

  184. [192]

    arXiv , doi =:1106.5804 , keywords =

    , year =. arXiv , doi =:1106.5804 , keywords =

    arXiv

  185. [193]

    arXiv , doi =:1011.6277 , keywords =

    , year =. arXiv , doi =:1011.6277 , keywords =

    arXiv

  186. [194]

    arXiv , doi =:1012.5831 , keywords =

    , year =. arXiv , doi =:1012.5831 , keywords =

    arXiv

  187. [195]

    arXiv , doi =:1009.2500 , keywords =

    , year =. arXiv , doi =:1009.2500 , keywords =

    arXiv

  188. [196]

    arXiv , doi =:1009.4173 , keywords =

    , year =. arXiv , doi =:1009.4173 , keywords =

    arXiv

  189. [197]

    arXiv , doi =:1005.0320 , keywords =

    , year =. arXiv , doi =:1005.0320 , keywords =

    arXiv

  190. [198]

    arXiv , doi =:1002.1080 , keywords =

    , year =. arXiv , doi =:1002.1080 , keywords =

    arXiv

  191. [199]

    arXiv , doi =:0911.1105 , keywords =

    , year =. arXiv , doi =:0911.1105 , keywords =

    arXiv

  192. [200]

    arXiv , doi =:0905.1264 , keywords =

    , year =. arXiv , doi =:0905.1264 , keywords =

    arXiv

  193. [201]

    arXiv , doi =:0809.2036 , keywords =

    , year =. arXiv , doi =:0809.2036 , keywords =

    arXiv

  194. [202]

    arXiv , doi =:0809.2290 , keywords =

    , year =. arXiv , doi =:0809.2290 , keywords =

    arXiv

  195. [203]

    arXiv , doi =:0803.3786 , keywords =

    , year =. arXiv , doi =:0803.3786 , keywords =

    arXiv

  196. [204]

    arXiv , doi =:0706.2009 , keywords =

    , year =. arXiv , doi =:0706.2009 , keywords =

    2009 arXiv

  197. [205]

    arXiv , doi =:0710.3347 , keywords =

    , year =. arXiv , doi =:0710.3347 , keywords =

    arXiv

  198. [206]

    arXiv , doi =:0708.2702 , keywords =

    , year =. arXiv , doi =:0708.2702 , keywords =

    arXiv

  199. [207]

    arXiv , doi =:astro-ph/0702095 , keywords =

    , year =. arXiv , doi =:astro-ph/0702095 , keywords =

    arXiv

  200. [208]

    arXiv , doi =:astro-ph/0703320 , keywords =

    , year =. arXiv , doi =:astro-ph/0703320 , keywords =

    arXiv

  201. [209]

    arXiv , doi =:astro-ph/0603792 , keywords =

    , year =. arXiv , doi =:astro-ph/0603792 , keywords =

    arXiv

  202. [210]

    arXiv , doi =:astro-ph/0509849 , keywords =

    , year =. arXiv , doi =:astro-ph/0509849 , keywords =

    arXiv

  203. [211]

    arXiv , doi =:astro-ph/0509647 , keywords =

    , year =. arXiv , doi =:astro-ph/0509647 , keywords =

    arXiv

  204. [212]

    arXiv , doi =:astro-ph/0509884 , keywords =

    , year =. arXiv , doi =:astro-ph/0509884 , keywords =

    arXiv

  205. [213]

    arXiv , doi =:astro-ph/0411586 , keywords =

    , year =. arXiv , doi =:astro-ph/0411586 , keywords =

    arXiv

  206. [214]

    arXiv , doi =:astro-ph/0501486 , keywords =

    , year =. arXiv , doi =:astro-ph/0501486 , keywords =

    arXiv

  207. [215]

    arXiv , doi =:astro-ph/0408554 , keywords =

    , year =. arXiv , doi =:astro-ph/0408554 , keywords =

    arXiv

  208. [216]

    arXiv , doi =:astro-ph/0405511 , keywords =

    , year =. arXiv , doi =:astro-ph/0405511 , keywords =

    arXiv

  209. [217]

    arXiv , doi =:astro-ph/0309735 , keywords =

    , year =. arXiv , doi =:astro-ph/0309735 , keywords =

    arXiv

  210. [218]

    arXiv , doi =:astro-ph/0401023 , keywords =

    , year =. arXiv , doi =:astro-ph/0401023 , keywords =

    arXiv

  211. [219]

    Advances in Space Research , year =

  212. [220]

    doi:10.1051/0004-6361:20052954 , keywords =

    , year =. doi:10.1051/0004-6361:20052954 , keywords =

    doi

  213. [221]

    arXiv , doi =:astro-ph/9810458 , keywords =

    , year =. arXiv , doi =:astro-ph/9810458 , keywords =

    arXiv

  214. [222]

    arXiv , doi =:1005.2154 , keywords =

    , year =. arXiv , doi =:1005.2154 , keywords =

    arXiv

  215. [223]

    arXiv , doi =:1202.4450 , keywords =

    , year =. arXiv , doi =:1202.4450 , keywords =

    arXiv

  216. [224]

    arXiv , doi =:0911.0409 , keywords =

    , year =. arXiv , doi =:0911.0409 , keywords =

    arXiv

  217. [225]

    arXiv , doi =:astro-ph/0209035 , keywords =

    , year =. arXiv , doi =:astro-ph/0209035 , keywords =

    arXiv

  218. [226]

    arXiv , doi =:astro-ph/0410173 , keywords =

    Reviews of Modern Physics , year =. arXiv , doi =:astro-ph/0410173 , keywords =

    arXiv

  219. [227]

    arXiv , doi =:1805.00042 , keywords =

    , year =. arXiv , doi =:1805.00042 , keywords =

    arXiv

  220. [228]

    doi:10.1093/mnras/222.2.323 , keywords =

    , year =. doi:10.1093/mnras/222.2.323 , keywords =

    doi

  221. [229]

    arXiv , doi =:astro-ph/9710107 , keywords =

    , year =. arXiv , doi =:astro-ph/9710107 , keywords =

    arXiv

  222. [230]

    arXiv , doi =:astro-ph/9906160 , keywords =

    , year =. arXiv , doi =:astro-ph/9906160 , keywords =

    arXiv

  223. [231]

    arXiv , doi =:astro-ph/0610134 , keywords =

    , year =. arXiv , doi =:astro-ph/0610134 , keywords =

    arXiv

  224. [232]

    arXiv , doi =:0706.2919 , keywords =

    , year =. arXiv , doi =:0706.2919 , keywords =

    arXiv

  225. [233]

    arXiv , doi =:1604.08223 , keywords =

    , year =. arXiv , doi =:1604.08223 , keywords =

    arXiv

  226. [234]

    doi:10.1038/363051a0 , keywords =

    , year =. doi:10.1038/363051a0 , keywords =

    doi

  227. [235]

    arXiv , doi =:0908.1700 , keywords =

    Astronomische Nachrichten , year =. arXiv , doi =:0908.1700 , keywords =

    arXiv

  228. [236]

    doi:10.1086/186621 , keywords =

    , year =. doi:10.1086/186621 , keywords =

    doi

  229. [237]

    arXiv , doi =:1711.06205 , keywords =

    , year =. arXiv , doi =:1711.06205 , keywords =

    arXiv

  230. [238]

    arXiv , doi =:1806.06819 , keywords =

    , year =. arXiv , doi =:1806.06819 , keywords =

    arXiv

  231. [239]

    arXiv , doi =:1701.05197 , keywords =

    , year =. arXiv , doi =:1701.05197 , keywords =

    arXiv

  232. [240]

    doi:10.1086/161591 , keywords =

    , year =. doi:10.1086/161591 , keywords =

    doi

  233. [241]

    arXiv , doi =:astro-ph/0412306 , keywords =

    , year =. arXiv , doi =:astro-ph/0412306 , keywords =

    arXiv

  234. [242]

    arXiv , doi =:1509.04275 , keywords =

    , year =. arXiv , doi =:1509.04275 , keywords =

    arXiv

  235. [243]

    arXiv , doi =:1105.4809 , keywords =

    , year =. arXiv , doi =:1105.4809 , keywords =

    arXiv

  236. [244]

    arXiv , doi =:astro-ph/0412481 , keywords =

    , year =. arXiv , doi =:astro-ph/0412481 , keywords =

    arXiv

  237. [245]

    Revista Mexicana de Astronomia y Astrofisica Conference Series , year =

  238. [246]

    doi:10.1086/191492 , keywords =

    , year =. doi:10.1086/191492 , keywords =

    doi

  239. [247]

    doi:10.1086/323536 , keywords =

    , year =. doi:10.1086/323536 , keywords =

    doi

  240. [248]

    arXiv , doi =:astro-ph/0102286 , keywords =

    , year =. arXiv , doi =:astro-ph/0102286 , keywords =

    arXiv

  241. [249]

    arXiv , doi =:astro-ph/0410164 , keywords =

    , year =. arXiv , doi =:astro-ph/0410164 , keywords =

    arXiv

  242. [250]

    doi:10.1093/mnras/staa800 , keywords =

    , year =. doi:10.1093/mnras/staa800 , keywords =

    doi

  243. [251]

    arXiv , doi =:astro-ph/0605144 , keywords =

    , year =. arXiv , doi =:astro-ph/0605144 , keywords =

    arXiv

  244. [252]

    arXiv , doi =:astro-ph/9806315 , keywords =

    , year =. arXiv , doi =:astro-ph/9806315 , keywords =

    arXiv

  245. [253]

    arXiv , doi =:astro-ph/0309134 , keywords =

    , year =. arXiv , doi =:astro-ph/0309134 , keywords =

    arXiv

  246. [254]

    doi:10.1086/154215 , keywords =

    , year =. doi:10.1086/154215 , keywords =

    doi

  247. [255]

    arXiv , doi =:1011.1501 , keywords =

    , year =. arXiv , doi =:1011.1501 , keywords =

    arXiv

  248. [256]

    doi:10.1086/170483 , keywords =

    , year =. doi:10.1086/170483 , keywords =

    doi

  249. [257]

    doi:10.1093/mnras/183.3.341 , keywords =

    , year =. doi:10.1093/mnras/183.3.341 , keywords =

    doi

  250. [258]

    arXiv , doi =:2009.14217 , keywords =

    , year =. arXiv , doi =:2009.14217 , keywords =

    2009

  251. [259]

    arXiv , doi =:0707.3380 , keywords =

    , year =. arXiv , doi =:0707.3380 , keywords =

  252. [260]

    arXiv , doi =:1911.02976 , keywords =

    , year =. arXiv , doi =:1911.02976 , keywords =

    1911

  253. [261]

    arXiv , doi =:astro-ph/0309771 , keywords =

    , year =. arXiv , doi =:astro-ph/0309771 , keywords =

    arXiv

  254. [262]

    arXiv , doi =:0905.1934 , keywords =

    , year =. arXiv , doi =:0905.1934 , keywords =

    1934 arXiv

  255. [263]

    arXiv , doi =:1509.02537 , keywords =

    , year =. arXiv , doi =:1509.02537 , keywords =

    arXiv

  256. [264]

    arXiv , doi =:astro-ph/0108153 , keywords =

    , year =. arXiv , doi =:astro-ph/0108153 , keywords =

    arXiv

  257. [265]

    arXiv , doi =:astro-ph/9907411 , keywords =

    , year =. arXiv , doi =:astro-ph/9907411 , keywords =

    arXiv

  258. [266]

    arXiv , doi =:astro-ph/9810070 , keywords =

    , year =. arXiv , doi =:astro-ph/9810070 , keywords =

    arXiv

  259. [267]

    arXiv , doi =:1704.09029 , keywords =

    , year =. arXiv , doi =:1704.09029 , keywords =

    arXiv

  260. [268]

    arXiv , doi =:2012.08634 , keywords =

    , year =. arXiv , doi =:2012.08634 , keywords =

    2012

  261. [269]

    arXiv , doi =:1105.3683 , keywords =

    , year =. arXiv , doi =:1105.3683 , keywords =

    arXiv

  262. [270]

    arXiv , eid =:2202.02957 , keywords =

    arXiv e-prints , year =. arXiv , eid =:2202.02957 , keywords =

  263. [271]

    doi:10.1051/0004-6361:20078089 , keywords =

    , year =. doi:10.1051/0004-6361:20078089 , keywords =

    doi

  264. [272]

    arXiv , doi =:1409.2876 , keywords =

    , year =. arXiv , doi =:1409.2876 , keywords =

    arXiv

  265. [273]

    arXiv , doi =:1610.05324 , keywords =

    , year =. arXiv , doi =:1610.05324 , keywords =

    arXiv

  266. [274]

    Spearman , title =

    C. Spearman , title =. The American Journal of Psychology , year =

  267. [275]

    arXiv , doi =:1906.08174 , keywords =

    , year =. arXiv , doi =:1906.08174 , keywords =

    1906 arXiv

  268. [276]

    arXiv , doi =:0906.1808 , keywords =

    , year =. arXiv , doi =:0906.1808 , keywords =

    arXiv

  269. [277]

    arXiv , doi =:1512.00410 , keywords =

    , year =. arXiv , doi =:1512.00410 , keywords =

    arXiv

  270. [278]

    arXiv , doi =:1104.0884 , keywords =

    Astronomy Reports , year =. arXiv , doi =:1104.0884 , keywords =

    arXiv

  271. [279]

    2021 , month = nov, pages =

    , title =. 2021 , month = nov, pages =. arXiv , doi =:2107.10850 , keywords =

    2021

  272. [280]

    arXiv , doi =:1208.0022 , keywords =

    , year =. arXiv , doi =:1208.0022 , keywords =

    arXiv

  273. [281]

    doi:10.1086/161343 , keywords =

    , year =. doi:10.1086/161343 , keywords =

    doi

  274. [282]

    arXiv , doi =:0801.1170 , keywords =

    , year =. arXiv , doi =:0801.1170 , keywords =

    arXiv

  275. [283]

    arXiv , doi =:1401.7866 , keywords =

    , year =. arXiv , doi =:1401.7866 , keywords =

    arXiv

  276. [284]

    arXiv , doi =:1710.02496 , keywords =

    , year =. arXiv , doi =:1710.02496 , keywords =

    arXiv

  277. [285]

    arXiv , doi =:astro-ph/0502210 , keywords =

    , year =. arXiv , doi =:astro-ph/0502210 , keywords =

    arXiv

  278. [286]

    arXiv , doi =:astro-ph/0703553 , keywords =

    , year =. arXiv , doi =:astro-ph/0703553 , keywords =

    arXiv

  279. [287]

    arXiv , doi =:1205.3376 , keywords =

    , year =. arXiv , doi =:1205.3376 , keywords =

    arXiv

  280. [288]

    arXiv , doi =:0810.1953 , keywords =

    , year =. arXiv , doi =:0810.1953 , keywords =

    1953 arXiv

  281. [289]

    arXiv , doi =:1212.1480 , keywords =

    , year =. arXiv , doi =:1212.1480 , keywords =

    arXiv

  282. [290]

    arXiv , doi =:1204.2265 , keywords =

    , year =. arXiv , doi =:1204.2265 , keywords =

    arXiv

  283. [291]

    arXiv , doi =:1609.08866 , keywords =

    , year =. arXiv , doi =:1609.08866 , keywords =

    arXiv

  284. [292]

    arXiv , doi =:1901.02684 , keywords =

    , year =. arXiv , doi =:1901.02684 , keywords =

    1901 arXiv

  285. [293]

    arXiv , doi =:astro-ph/9309013 , keywords =

    , year =. arXiv , doi =:astro-ph/9309013 , keywords =

    arXiv

  286. [294]

    , journal =

    Ferrers, N., M. , journal =. 1877 , volume =

  287. [295]

    arXiv , doi =:0901.2346 , keywords =

    , year =. arXiv , doi =:0901.2346 , keywords =

    arXiv

  288. [296]

    arXiv , doi =:astro-ph/0508097 , keywords =

    , year =. arXiv , doi =:astro-ph/0508097 , keywords =

    arXiv

  289. [297]

    arXiv , doi =:0810.4922 , keywords =

    , year =. arXiv , doi =:0810.4922 , keywords =

    arXiv

  290. [298]

    arXiv , doi =:astro-ph/0603682 , keywords =

    , year =. arXiv , doi =:astro-ph/0603682 , keywords =

    arXiv

  291. [299]

    arXiv , doi =:1204.0516 , keywords =

    , year =. arXiv , doi =:1204.0516 , keywords =

    arXiv

  292. [300]

    arXiv , doi =:1212.0980 , keywords =

    , year =. arXiv , doi =:1212.0980 , keywords =

    arXiv

Pith tools

Reviewed June 28, 2026 · model on record in the stance chip above.