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Samuel Oschin telescopePalomar Observatory18-inch Schmidt cameraSan Diego meetup May 2019Hale TelescopeGeorge Ellery Hale bust by Marian BreckenridgeCarolyn ShoemakerDigitized Sky Survey NGC objects

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Digitized Sky Survey

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California Institute of Technology

Analyzing Network Connections...

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Network Profile

Overall Strength
i
5.71% of network
(896)
Strength Breakdown
  • This Post (5.71%)
  • George Ellery Hale bust by Marian Breckenridge (5.71%)
  • 18-inch Schmidt camera (1.43%)
  • Carolyn Shoemaker (1.43%)
  • Hale Telescope (1.43%)
  • Samuel Oschin telescope (1.43%)
  • San Diego meetup May 2019 (1.43%)
  • Digitized Sky Survey NGC objects (1.43%)
Dominant nodes (excluded from chart)
Palomar Observatory 80.00%
Influence Score
i
10.94% of network
(1.14)
Influence Breakdown
  • This Post (10.94%)
  • Palomar Observatory (12.50%)
  • 18-inch Schmidt camera (10.94%)
  • Carolyn Shoemaker (10.94%)
  • George Ellery Hale bust by Marian Breckenridge (10.94%)
  • Hale Telescope (10.94%)
  • Samuel Oschin telescope (10.94%)
  • San Diego meetup May 2019 (10.94%)
  • Digitized Sky Survey NGC objects (10.94%)
Direct Connections 4

Node & Network Details

How is this calculated?

The math continuously tracks how strongly this post is connected to the rest of the network. Every tag forms a 2-way link. The base stats determine personal node strength, and the pie charts below show this node's share against its direct neighbours.

// 1. Base variables (floored at 1 to prevent zero-multiplication math errors)
$inbound = max(1, 2) = 2
$outbound = max(1, 2) = 2

// 2. Node Base Values (Local connection strength)
Base_Strength (PV) = $inbound * $outbound = 2 * 2 = 4
Base_Influence (IV) = $inbound / $outbound = 2 / 2 = 1

// 3. Exponential Network Values (accumulating 8 direct neighbours)
Network_Strength (CV) = Base_PV * (Neighbour_1_PV * Neighbour_2_PV * ...)
                         = 4 *
                           ( 56 [Palomar Observatory] *
                            1 [18-inch Schmidt camera] *
                            1 [Carolyn Shoemaker] *
                            4 [George Ellery Hale bust by Marian Breckenridge] *
                            1 [Hale Telescope] *
                            1 [Samuel Oschin telescope] *
                            1 [San Diego meetup May 2019] *
                            1 [Digitized Sky Survey NGC objects]
                           )

                         = 896

Network_Influence (TV) = Base_IV * (Neighbour_1_IV * Neighbour_2_IV * ...)
                         = 1 *
                           ( 1.14 [Palomar Observatory] *
                            1 [18-inch Schmidt camera] *
                            1 [Carolyn Shoemaker] *
                            1 [George Ellery Hale bust by Marian Breckenridge] *
                            1 [Hale Telescope] *
                            1 [Samuel Oschin telescope] *
                            1 [San Diego meetup May 2019] *
                            1 [Digitized Sky Survey NGC objects]
                           )

                         = 1.14
Outbound 2 Tags on post
Inbound 2 Posts tagging this
Connections 8 Total nodes
Base Node Strength 4
Base Node Influence 1
Strength Share (vs Direct Neighbours)
5.71% (896 overall)
  • This Post (5.71%)
  • George Ellery Hale bust by Marian Breckenridge (5.71%)
  • 18-inch Schmidt camera (1.43%)
  • Carolyn Shoemaker (1.43%)
  • Hale Telescope (1.43%)
  • Samuel Oschin telescope (1.43%)
  • San Diego meetup May 2019 (1.43%)
  • Digitized Sky Survey NGC objects (1.43%)
Dominant nodes (excluded from chart)
Palomar Observatory 80.00%
Influence Share (vs Direct Neighbours)
10.94% (1.14 overall)
  • This Post (10.94%)
  • Palomar Observatory (12.50%)
  • 18-inch Schmidt camera (10.94%)
  • Carolyn Shoemaker (10.94%)
  • George Ellery Hale bust by Marian Breckenridge (10.94%)
  • Hale Telescope (10.94%)
  • Samuel Oschin telescope (10.94%)
  • San Diego meetup May 2019 (10.94%)
  • Digitized Sky Survey NGC objects (10.94%)

Connected Network Hierarchy

Sort list by:
Top Network Boosters (Highest Multipliers)
Palomar Observatory ↗
Str: 56Inf: 1.14
18-inch Schmidt camera ↗
Str: 1Inf: 1
Carolyn Shoemaker ↗
Str: 1Inf: 1
George Ellery Hale bust by Marian Breckenridge ↗
Str: 4Inf: 1
Hale Telescope ↗
Str: 1Inf: 1
Samuel Oschin telescope ↗
Str: 1Inf: 1
San Diego meetup May 2019 ↗
Str: 1Inf: 1
Digitized Sky Survey NGC objects ↗
Str: 1Inf: 1
Weakest Connections (Lowest Multipliers)
Digitized Sky Survey NGC objects ↗
Str: 1Inf: 1
San Diego meetup May 2019 ↗
Str: 1Inf: 1
Samuel Oschin telescope ↗
Str: 1Inf: 1
Hale Telescope ↗
Str: 1Inf: 1
George Ellery Hale bust by Marian Breckenridge ↗
Str: 4Inf: 1
Carolyn Shoemaker ↗
Str: 1Inf: 1
18-inch Schmidt camera ↗
Str: 1Inf: 1
Palomar Observatory ↗
Str: 56Inf: 1.14

Connection Health Audit (Red = broken 1-way link)

Outbound Tags (2)
Digitized Sky Survey NGC objects
Palomar Observatory
Inbound Posts (2)
Palomar Observatory
Digitized Sky Survey NGC objects
Last calculated: Jun 17, 5:16 PM
14

Related Content

Locations

  • Palomar Observatory

Topics

  • 18-inch Schmidt camera
  • Carolyn Shoemaker
  • George Ellery Hale bust by Marian Breckenridge
  • Hale Telescope
  • Samuel Oschin telescope
  • San Diego meetup May 2019
  • Digitized Sky Survey NGC objects