GW name GWTC run M1 source M2 source Luminosity distance Spin Total mass Chirp mass Redshift 85 GW200302 3 37.80 20.00 1480 0.01 57.80 23.400 0.28 86 GW200306 28.30 14.80 2100 0.32 43.90 17.500 0.38 87 GW200308 36.40 13.80 5400 0.65 50.60 19.000 0.83 88 GW200311 3 34.20 27.70 1170 -0.02 61.90 26.600 0.23 89 GW200316 13.10 7.80 1120 0.13 21.20 8.750 0.22 90 GW200322 3 34.00 14.00 3600 0.24 55.00 15.500 0.60This EMA covers some interesting data related to Gravitational Wave [(GW) events. The detection of gravitational waves, which are ripples in space-time, make it possible to detect events such as black hole mergers that can not be seen through conventional telescopes. There have been 93 such events recorded to date, 90 are used in this data set. These GW events are mostly black hole mergers, but one of the more widely recorded events GW1T0817, is the merger of two neutron stars, the only such event recorded to date. In this EMA, you will analyse data relating gravitational wave events, all the initial data for this EMA are given in the file GW Data.mwx. The stubsequent data tables used in this EMA are subsets or summaries of these initial data. In this GW Data.mwx file there are the [ollowing variables: + GW Name: the name of the gravitational wave event, this is in the form GW followed by the year, month day, for instance GW1T05817 is the gravitational wave event recorded on the 17th August 2017, If there were two or more events on the same date, these have been labeled as "a', b, GWTC run: the run in which the GW event was recorded. run 1 took place between 2015 and 2017, run 2 between April 2019 and Sept 2019 and rmn 3 took place between November 2019 and March 2020, + M1 source: the mass of source object 1, measured in units of solar masses the mass of the sun denoted as Mq. * M2 source: the mass of source object 2, measured in solar masses, M. + Luminosity distance: the distance to the GW event, based on it's Inminesity messured in Mpe, + Spin: the effective spin of the GW event. + Total mass: the total mass of the GW event (in solar masses, Mz ). + Chirp mass: a measure of the effective mass of the binary system that produces the GW event {in solar masses, M2 ). * Redshift: a measure of how much the light from the GW event is shifted towards the red part of the electromagnetic spectrum. + Final mass: the final mass after the GW event merger (in solar masses, M. You are strongly recommended to use Minitab where appropriate, but you are not required to do so. Please round vour results to a suitable aceuracy as appropriate lor the question. By looking at the data file GW Data.mwx, answer the following. You might find the Minitab commands Subset worksheet and Sort (or Rank) useful from the Data menu. In your answers you don't necessarily need to use the symbol Mo, mentioning the unit as 'solar masses' is sufficient. (a) Write down the GW event that has the smallest MI source mass for GWTC run 3. What was the MI source mass for this GW event? [1] "b) For this GW event, what is the chirp mass? Again for GWTC run 3, does this GW event have the smallest chirp mass? [1] (c) A boxplot of the spin for the GW events by GWCT run is shown in Figure 1. Boxplot of Spin GWTC run WM .04 -0.2 0.0 0.2 04 016 0.8 Spin Figure 1 Spin value for GW events by GWTC run (i) Using only the boxplot, is the shape of the boxplot for the GWTC run 3 left-skew, right-skew or neither? Give your reasons. [2] (ii) The left-hand edge of the box section of the boxplot for GWTC run 3 has a value of -0.04. How is this value calculated? 2 (iii) Using the boxplots, compare the ranges, interquartile ranges, and medians of the distributions for the different GWTC runs. [3] (iv) For GWTC run 3, the median spin value is 0.05. Is the mean spin value for this GWTC run likely to be higher or lower than or equal to this median? Why is this? You should not need to calculate the mean to answer this. [1]