Searching For Ceiling Effects in NASA MDP Components - Part I - Undersampling

Defect distribution visualization can be found here among components. These are verified by components flagged to be used/ignored based on the median number of defects. Components whose defects exceed in number the median are first filtered for selection. These components can be seen below.

Component ID	Use/Ignore
22295	ignore
22296	ignore
22297	ignore
22298	ignore
22299	ignore
22302	ignore
22303	ignore
22305	ignore
22306	ignore
24952	ignore
24954	ignore
24958	ignore
24959	ignore
24960	ignore
24962	ignore
24964	ignore
24967	ignore
24970	ignore
24971	ignore
25	ignore
25492	ignore
26	ignore
27	ignore
28	ignore
29	ignore
30	ignore
31	ignore
32	ignore
33132	ignore
33135	ignore
33137	ignore
33138	ignore
33139	ignore
33140	ignore
33142	ignore
33143	ignore
33146	ignore
33147	ignore
33148	ignore
34753	ignore
34754	ignore
34755	ignore
34756	ignore
34757	ignore
34758	ignore
34759	ignore
34760	ignore
34761	ignore
34762	ignore
34763	ignore
34764	ignore
34765	ignore
34766	ignore
34767	ignore
34768	ignore
34769	ignore
70812	ignore
70814	ignore
70815	ignore
70818	ignore
70820	ignore
70821	ignore
70822	ignore
70823	ignore
70824	ignore
17	use
18	use
19	use
20	use
21	use
22	use
22292	use
22293	use
22294	use
22300	use
22301	use
22304	use
22307	use
22308	use
22309	use
23	use
24	use
24953	use
24955	use
24956	use
24957	use
24961	use
24963	use
24965	use
24966	use
24968	use
24969	use
25493	use
33133	use
33134	use
33136	use
33141	use
33144	use
33145	use
33149	use
33150	use
34752	use
70816	use
70817	use
70819	use

Plots of the potential ceiling effects can be found here using subsampling, where M=N (#defective = #non-defective). A 10X10-way cross-validation was used in the experiment.