deletions | additions       diff --git a/sample_states.json b/sample_states.json  index 9afd512..af297ba 100644  --- a/sample_states.json  +++ b/sample_states.json 
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"grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Early M dwarfs",  "caption" : "", "This just shows the early M dwarfs.",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K", 
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}  ]  },  { "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Mid M dwarfs",  "caption" : "Now we just show the mid M dwarfs",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K",  "yAxis" : "H-K"  },  {   "gridPosition" : [0,1],  "xAxis" : "H-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,2],  "xAxis" : "J-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,3],  "xAxis" : "H2OK2 Index",  "yAxis" : "H2OK2 Index" ,   "selection" : {"xRange" : [0.83, 0.9],  "yRange" : [0.83, 0.9]}  }  ]  },  {  "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Late M dwarfs",  "caption" : "Now we just show the late M dwarfs",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K",  "yAxis" : "H-K"  },  {   "gridPosition" : [0,1],  "xAxis" : "H-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,2],  "xAxis" : "J-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,3],  "xAxis" : "H2OK2 Index",  "yAxis" : "H2OK2 Index" ,   "selection" : {"xRange" : [0.65, 0.83],  "yRange" : [0.65, 0.83]}  }  ]  },  {  "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" :  "All the stars and their iron abundances", [Fe/H]",  "colorAxis" : "[Fe/H]", "EW NA",  "colorMap" : ["blue", "red"],  "caption" : "In this plot, the near-infrared colors of the M dwarfs remain the same. However, now the stars are colored by their iron abundance, [Fe/H]. The [Fe/H] of each star was inferred following the methods described in Newton et al. (2013), which use the equivalent width of the Na line near 2.2 microns as a proxy for metallicity. You can see that a metal-rich star is seen to have a different color than a more metal-poor star of the same spectral type. This allowed us to calibrate a relation for iron abundance using 2MASS photometry.",  "plots" : [ {  
...
"yAxis" : "H2OK2 Index"  }  ]  },  {  "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Early M dwarfs and their [Fe/H]",  "colorAxis" : "EW NA",  "colorMap" : ["blue", "red"],  "caption" : "Early M and iron abundance",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K",  "yAxis" : "H-K"  },  {   "gridPosition" : [0,1],  "xAxis" : "H-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,2],  "xAxis" : "J-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,3],  "xAxis" : "H2OK2 Index",  "yAxis" : "H2OK2 Index",  "selection" : {"xRange" : [0.9, 1.2],  "yRange" : [0.9, 1.2]}  }  ]  },  {  "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Mid M dwarfs and their iron abundances",  "colorAxis" : "EW NA",  "colorMap" : ["blue", "red"],  "caption" : "Mid M and their [Fe/H]",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K",  "yAxis" : "H-K"  },  {   "gridPosition" : [0,1],  "xAxis" : "H-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,2],  "xAxis" : "J-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,3],  "xAxis" : "H2OK2 Index",  "yAxis" : "H2OK2 Index",  "selection" : {"xRange" : [0.83, 0.9],  "yRange" : [0.83, 0.9]}  }  ]  },  {  "grid" : { "nRows" : 1,  "nColumns" : 4},  "name" : "Late M dwarfs and their [Fe/H]",  "colorAxis" : "EW NA",  "colorMap" : ["blue", "red"],  "caption" : "Late M and iron abundance",  "plots" : [ {   "gridPosition" : [0,0],  "xAxis" : "J-K",  "yAxis" : "H-K"  },  {   "gridPosition" : [0,1],  "xAxis" : "H-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,2],  "xAxis" : "J-K",  "yAxis" : "J-H"  },  {   "gridPosition" : [0,3],  "xAxis" : "H2OK2 Index",  "yAxis" : "H2OK2 Index",  "selection" : {"xRange" : [0.1, 0.83],  "yRange" : [0.1, 0.83]}  }  ]  }