LIM Near IR from a minisatellite Dani Maoz

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LIM: Near IR from a mini-satellite Dani Maoz

LIM: Near IR from a mini-satellite Dani Maoz

HST WFC 3 IR channel: 1 k x 1 k Hg. Cd. Te detector,

HST WFC 3 IR channel: 1 k x 1 k Hg. Cd. Te detector, QE 80% 18 micron pixels (0. 13”/pix), ~2’x 2’ FOV Detector sensitivity engineered to cut off above 1. 7 micron, so can operate at -128 C (6 -stage thermoelectric cooler) without thermal noise from telescope and detector. J (1. 1 micron) and H (1. 6 microns) bands. Dominant background: zodiacal light: 0. 6 -1. 3 e/s/pix Sensitivity: J=27 (ABmag, S/N=5) in 45 min (point src. ), 1. 4 hr (1” diam src. ) H=26. 4 53 min 1. 5 hr Sensitivity: J=26 (ABmag, S/N=5) in 10 min (point src. ), 18 min (1” diam. src. ) H=25. 4 12 min 19 min

HAWK-I on VLT: 0. 1”/pixel, 7. 5’ FOV 1 hr exposure : J=24. 9,

HAWK-I on VLT: 0. 1”/pixel, 7. 5’ FOV 1 hr exposure : J=24. 9, H=23. 9 (S/N=5) i. e. 100 hrs exposure needed to reach WFC 3 1 -orbit depth! No place like space for NIR! 4 k pixels , 7. 4 cm

Why not make a “mini” (HST+WFC 3 -IR)/10? 2. 4 m 24 cm =

Why not make a “mini” (HST+WFC 3 -IR)/10? 2. 4 m 24 cm = 9. 5 in

For 24 cm aperture @ 1. 6 micron, diffraction limit: ~1. 3”. f/10 mirror,

For 24 cm aperture @ 1. 6 micron, diffraction limit: ~1. 3”. f/10 mirror, 18 -micron pixels 1. 5”/ pixel. Need ~100 hrs to get to HST-WFC 3 depth (same as VLT) BUT FOV can be much bigger! With 4 k x 4 k detector (like HAWK-I) FOV=1. 66 x 1. 66=2. 8 degree^2 = 2500 X WFC 3 ! A unique instrument for deep and wide NIR surveying. Science: Surveys for transients in NIR – High z and obscured regions

Survey Mode Examples: 1. All sky (1. 3 hr exposures): in 2 years, 2.

Survey Mode Examples: 1. All sky (1. 3 hr exposures): in 2 years, 2. to J=23. 4, H=22. 5 3. Ideal complement to LSST 2. 500 deg^2 transient search (180 fields, 1. 3 hr exposures), every 10 days to J=23. 4, H=22. 5. 3. 1 year: 10, 000 SNe Ia, 10, 000 CC-SNe 3. 30 deg^2 (10 fields, 30 -hr exposure), every 13 days to J=26, H=25. 4 1 year: 10, 000 SNe Ia, 10, 000 CC-SNe, z>1, z>2

Type-Ia SN delay time distribution

Type-Ia SN delay time distribution

Two approved HST MC Treasury programs (1400 orbits) predictions by K. Sharon

Two approved HST MC Treasury programs (1400 orbits) predictions by K. Sharon

predictions by K. Sharon

predictions by K. Sharon

Payload logistics: Telescope Weight: Off-shelf Celestron 10” telescope ~40 kg -- can shave off

Payload logistics: Telescope Weight: Off-shelf Celestron 10” telescope ~40 kg -- can shave off with custom lightweight mirror Camera: few kg? To keep it simple/light/cheap: minimum optics, minimum moving parts, fixed filters on chips: J H H J H J H J J H Thermoelectric cooler: Weight ~0 Power consumption: ~250 W