Lewis C. Roberts Jr, Emily L. Rice, Charles A. Beichman, Douglas Brenner, Rick Burruss, Justin R. Crepp, Richard G. Dekany, Lynne A. Hillenbrand, Sasha Hinkley, E. Robert Ligon, Thomas G. Lockhart, David King, Stanimir Metchev, Ben R. Oppenheimer, Ian R. Parry, Laurent Pueyo, Jennifer E. Roberts, Michael Shao, Anand Sivaramakrishnan, Rémi Soummer, Gautam Vasisht, Fred E. Vescelus, J. Kent Wallace, Neil T. Zimmerman, Chengxing Zhai
We used the Project 1640 near-infrared coronagraph and integral field spectrograph to observe 19 young solar type stars. Five of these stars are known binary stars and we detected the late-type secondaries and were able to measure their JH spectra with a resolution of R\sim30. The reduced, extracted, and calibrated spectra were compared to template spectra from the IRTF spectral library. With this comparison we test the accuracy and consistency of spectral type determination with the low-resolution near-infrared spectra from P1640. Additionally, we determine effective temperature and surface gravity of the companions by fitting synthetic spectra calculated with the PHOENIX model atmosphere code. We also present several new epochs of astrometry of each of the systems. Together these data increase our knowledge and understanding of the stellar make up of these systems. In addition to the astronomical results, the analysis presented helps validate the Project 1640 data reduction and spectral extraction processes and the utility of low-resolution, near-infrared spectra for characterizing late-type companions in multiple systems.
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http://arxiv.org/abs/1205.0998
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