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ZEMAX FILE FOR ECHELLE SPECTROGRAPH UPDATE
Mahadevan, S., Ramsey, L.W., Terrien, R., Halverson, S., Roy, A., Hearty, F., Levi, E., Stefansson, G.K., Robertson, P., Bender, C., Schwab, C., Nelson, M.: The Habitable-zone Planet Finder: A status update on the development of a stabilized fiber-fed nearinfrared spectrograph for the for the Hobby-Eberly telescope. In: Ground-based and Airborne Instrumentation for Astronomy III, Proc. Yuk, I.S., Jaffe, D.T., Barnes, S., Chun, M.Y., Park, C., Lee, S., Lee, H., Wang, W., Park, K.J., Pak, S., Strubhar, J., Deen, C., Oh, H., Seo, H., Pyo, T.S., Park, W.K., Lacy, J., Goertz, J., Rand, J., Gully-Santiago, M.: Preliminary design of IGRINS (Immersion GRating INfrared Spectrograph). In: Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Proc. Oliva, E., Origlia, L., Baffa, C., Biliotti, C., Bruno, P., D’Amato, F., Del Vecchio, C., Falcini, G., Gennari, S., Ghinassi, F., Giani, E., Gonzalez, M., Leone, F., Lolli, M., Lodi, M., Maiolino, R., Mannucci, F., Marcucci, G., Mochi, I., Montegriffo, P., Rossetti, E., Scuderi, S., Sozzi, M.: The GIANO-TNG spectrometer. Moorwood, A.: CRIRES: Context and status, pp 15–24. Pepe, F., Ehrenreich, D., Meyer, M.R.: Instrumentation for the detection and characterization of exoplanets. Reiners, A., Bean, J.L., Huber, K.F., Dreizler, S., Seifahrt, A., Czesla, S.: Detecting planets around very low mass stars with the radial velocity method. II, Henry, T.J., Hollingsworth, J.L., Joshi, M.M., Kilston, S., Liu, M.C., Meikle, E., Reid, I.N., Rothschild, L.J., Scalo, J., Segura, A., Tang, C.M., Tiedje, J.M., Turnbull, M.C., Walkowicz, L.M., Weber, A.L., Young, R.E.: A reappraisal of the habitability of planets around M dwarf stars.
Tarter, J.C., Backus, P.R., Mancinelli, R.L., Aurnou, J.M., Backman, D.E., Basri, G.S., Boss, A.P., Clarke, A., Deming, D., Doyle, L.R., Feigelson, E.D., Freund, F., Grinspoon, D.H., Haberle, R.M., Hauck, S.A., Heath, M.J. Vanderburg, A., Latham, D.W., Buchhave, L.A., Bieryla, A., Berlind, P., Calkins, M.L., Esquerdo, G.A., Welsh, S., Johnson, J.A.: Planetary candidates from the first year of the K2 mission. Perryman, M.: The Exoplanet Handbook (2011)Ĭrossfield, I.J.M., Ciardi, D.R., Petigura, E.A., Sinukoff, E., Schlieder, J.E., Howard, A.W., Beichman, C.A., Isaacson, H., Dressing, C.D., Christiansen, J.L., Fulton, B.J., Lépine, S., Weiss, L., Hirsch, L., Livingston, J., Baranec, C., Law, N.M., Riddle, R., Ziegler, C., Howell, S.B., Horch, E., Everett, M., Teske, J., Martinez, A.O., Obermeier, C., Benneke, B., Scott, N., Deacon, N., Aller, K.M., Hansen, B.M.S., Mancini, L., Ciceri, S., Brahm, R., Jordán, A., Knutson, H.A., Henning, T., Bonnefoy, M., Liu, M.C., Crepp, J.R., Lothringer, J., Hinz, P., Bailey, V., Skemer, A., Defrere, D.: 197 candidates and 104 validated planets in K2’s first five fields. Mayor, M., Queloz, D.: A Jupiter-mass companion to a solar-type star. In this paper, we present early results from the prototype of this spectrograph at ambient temperature. We obtain excellent resolution even when taking realistic manufacturing and alignment tolerances as well as thermal variations into account. To reduce the cost, we squeeze 42 spectral orders onto a 1K detector with a semi-cryogenic solution. The Tao Aiuc high Resolution (d) Y band Spectrograph (TARdYS) covers 0.843-1.117 μ m. The instrument is proposed for the University of Tokyo Atacama Observatory (TAO) 6.5 m telescope in Chile. We compare the best possible performance of quasi-Littrow and White Pupil setups, and prefer the latter because it achieves higher image quality. Our instrument is a high-resolution (R = 60,000) infrared spectrograph with a R6 Echelle grating and an image slicer. We present a new optical design, which leads to a cost-effective solution. An important factor in the scarcity of high precision IR spectrographs is the high cost of these instruments. One limitation in characterizing exoplanet candidates is the availability of infrared, high-resolution spectrographs.
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