SMAKCED
Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies


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Approved SMAKCED Proposals

NOT/NOTCam, 2012 (Toloba et al., 45-210) 4 nights  
TNG/NICS, 2012 (Toloba et al., CAT_155) 4 nights 85% outcome
NOT/NOTCam, 2012 (Janz et al., 44-036) 6 nights 75% outcome
NOT/NOTCam, 2012 (Toloba et al., 44-216) 1 night 75% outcome
WHT/ISIS, 2011 (Toloba et al., W11AC090) 4 nights 0% outcome
WHT/ISIS, 2011 (Peletier et al., W11AN014) 4 nights 60% outcome
NOT/NOTCam, 2011 (Janz et al., 43-038) 3 nights 44% outcome
NOT/NOTCam, 2011 (Toloba et al., 43-206) 4 nights 16% outcome
NOT/NOTCam, 2011 (Janz et al., 42-047) 6 nights 90% outcome
NOT/NOTCam, 2011 (Toloba et al., 42-212) 5 nights 50% outcome
TNG/NICS, 2011 (Toloba et al., CAT_102) 4 nights 40% outcome
ESO VLT/FORS, 2010 (Toloba et al., 085.A-1004) 40 hours 25% outcome
WHT/ISIS, 2010 (Toloba et al., W10AC060) 2 nights 100% outcome
WHT/ISIS, 2010 (Peletier et al., W10AN011) 6 nights 40% outcome
TNG/NICS, 2010 (Toloba et al., CAT_193) 4 nights 65% outcome
NOT/NOTCam, 2010 (Toloba et al., 41-217) 4 nights 50% outcome
ESO NTT/SOFI, 2010 (Janz et al., 085.B-0919) 5 nights 78% outcome

Near-infrared imaging: 50 nights (61% outcome)
Optical spectroscopy: 20 nights (39% outcome)

Outcome mostly affected by weather losses