1. Legacy Program “title/name of project” Part 1Instrument used: Observing Mode (example : MIRACLE broad-band filter imaging ) # of objects or size of survey area Net observing time required(example: 1hour x 100 objects = 100 hours) Required telescope specification(example: diameter >3m, T=6.0K or below) Wavelength specification (example: core =20-40  m, R>500) Sensitivity requirement (example: <50  Jy @ 20  m, 100  Jy@40  m) Data Volume, generation rate(example: 250MB / day, 0.25Mbps in realtime) Comments if any ** Outline ** (describe scientific target briefly, then give summary of your observing plan like the statement in “scientific target” in MRD. Applicable Scientific Target # in MRD : Goal of this Legacy program :

2. Part 2Instrument used: Observing Mode (example : MIRACLE broad-band filter imaging ) # of objects or size of survey area Net observing time required(example: 1hour x 100 objects = 100 hours) Required telescope specification(example: diameter >3m, T=6.0K or below) Wavelength specification (example: core =20-40  m, R>500) Sensitivity requirement (example: <50  Jy @ 20  m, 100  Jy@40  m) Data Volume, generation rate(example: 250MB in total, 0.25Mbps in average) Comments if any Part 3Instrument used: Observing Mode (example : MIRACLE broad-band filter imaging ) # of objects or size of survey area Net observing time required(example: 1hour x 100 objects = 100 hours) Required telescope specification(example: diameter >3m, T=6.0K or below) Wavelength specification (example: core =20-40  m, R>500) Sensitivity requirement (example: <50  Jy @ 20  m, 100  Jy@40  m) Data Volume, generation rate(example: 250MB in total, 0.25Mbps in average) Comments if any

3. ** Outline ** (describe scientific target briefly, then give summary of your observing plan like the statement in “scientific target” in MRD. Numb er ItemHST Subaru a (8 － 10m Ground based) Akari Spitzer Herschel Planck ALMAJWSTELTOthers A Same Observations (Purpose, method, ・ Performance [wavelength, resolution, sensitivity]) B Similar observations (method, performance are different, but the purpose is the same) CFoV DSpatial Resolution ESensitivity F Wavelength Resolution or filter band width G Contrast (Coronagraph) Legacy Program “title/name of project”(2)

4. GoodBad Intern al StrengthWeakness Exter nal OpportunitiesThreat Legacy Program “title/name of project” (3) SWOT Analysis