Isotopic Abundances of Dwarf Stars
Ian J. M. Crossfield, Becky E. Flores, Lothringer, Josh, Elisabeth A. C. Mills, Jessica Valverde, Richard Freedman, Coria, David
Abstract
Ian J. M. Crossfield, Becky E. Flores, Lothringer, Josh, Elisabeth A. C. Mills, Jessica Valverde, Richard Freedman, Coria, David
Abstract
GeoSnap is a new HgCdTe detector currently showing QE ~50% across 3-13?m. The device takes advantage of a ROIC currently operated at 85Hz full-frame readout across a 2048x1024 array, with larger sizes easily possible. This talk presents characterization of the first engineering-grade test device from Teledyne Imaging Systems, over the last year conducted at the Universities of Arizona and Michigan. I also describe science applications and planned deployment over the next year.
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GeoSnap is a new HgCdTe detector currently showing QE ~50% across 3-13?m. The device takes advantage of a ROIC currently operated at 85Hz full-frame readout across a 2048x1024 array, with larger sizes easily possible. This talk presents characterization of the first engineering-grade test device from Teledyne Imaging Systems, over the last year conducted at the Universities of Arizona and Michigan. I also describe science applications and planned deployment over the next year.
Key concepts: Stars, Astrophysics, Astronomy, Physics, White dwarf, Astrobiology