var fDesc=new Array(); fDesc[0] = "This calculator determines the dark energy figure of merit, defined as 1/(σwaσwp), as well as the expected cluster counts, for a large cluster survey, with several user-specified parameters. It assumes either a single observable-mass relation with self-calibration or two different observable-mass relations with cross-calibration.

Additionally, the calculator optimizes follow ups to a large cluster survey using a simulated annealing algorithm, as described in Wu, Rozo, and Wechsler 2009 (W09)."; function tShowHide(id, show) { var s = document.getElementById("desc"); if ((s.innerHTML.length<=212 || show==1) && show!=2) { s.innerHTML = fDesc[id]; if (document.getElementById('m1')) document.getElementById('m1').style.display='none'; if (document.getElementById('m2')) document.getElementById('m2').style.display='none'; if (document.getElementById('more_txt')) document.getElementById('more_txt').style.display='inline'; } else { s.innerHTML = ''; } }