Astronomical Spectroscopy - Physics - University of Cincinnati

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$1 Ch. 22 â Reflection and Refraction of Light 22.1 The ... - Physics$

– 84 – Tonry, J., & Davis, M. 1979, AJ, 84, 1511 Turnshek, D. E., Turnshek, D. A., Craine, E. R., & Boeshaar, P. C., An Atlas of Digitial Spectra of Cool Stars (Types G, K, M, S, and C), (Tucson: Western Research Company) Valdivielso, L., Esparza, P., Martin, E. L., Maukonen, D, & Peale, R. E. 2010, ApJ, 715, 1366 Wagner, R. M. 1992, in Astronomical CCD Observing and Reductions Techniques, ASP Conf. 23, ed. S. B. Howell (San Francisco: ASP), 160 Walborn, N. R., & Fitzpatrick, E. L. 1990, PASP, 102, 379 Walker, G. 1987, Astronomical Observations: An Optical Perspective (Cambridge: Press Syndicate of the University of Cambridge) Woodgate, B. E. et al. 1998, PASP, 110, 1183 Wynne, C. G. 1993, MNRAS, 262, 741 This preprint was prepared with the AAS L A TEX macros v5.2.
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Astronomical Spectroscopy Philip Ma
Page 3 and 4:
- 3 - Similarly the emphasis here w
Page 5 and 6:
- 5 - could see 8000Å light from f
Page 7 and 8:
- 7 - ratio of the focal lengths of
Page 9 and 10:
- 9 - Fig. 2.— The overlap of var
Page 11 and 12:
- 11 - 2.1.2. Choosing a grating Wh
Page 13 and 14:
- 13 - 4-Meter Telescope - RC Spect
Page 15 and 16:
- 15 - gratings blazed at the red.
Page 17 and 18:
- 17 - each order (Equation 9). Thi
Page 19 and 20:
- 19 - wants can be a real challeng
Page 21 and 22:
- 21 - Fig. 7.— Multi-object mask
Page 23 and 24:
- 23 - Fig. 8.— Optical layout of
Page 25 and 26:
- 25 - Fig. 9.— View of the focal
Page 27 and 28:
- 27 - Fig. 10.— Optical design o
Page 29 and 30:
- 29 - When built twenty years ago,
Page 31 and 32:
- 31 - corrected” image cube is c
Page 33 and 34: - 33 - • The data frames themselv
Page 35 and 36: - 35 - Fig. 11.— Three examples o
Page 37 and 38: - 37 - bumps and wiggles are presen
Page 39 and 40: - 39 - Fig. 13.— The spatial prof
Page 41 and 42: - 41 - one might want to do this on
Page 43 and 44: - 43 - The steps involved in this r
Page 45 and 46: - 45 - be obtained for each grating
Page 47 and 48: - 47 - the flat-field division. Alt
Page 49 and 50: - 49 - night. More about this is di
Page 51 and 52: - 51 - can be answered given a comp
Page 53 and 54: - 53 - that it degraded the signal-
Page 55 and 56: - 55 - 3.2.6. Long-Slit Flat-Fieldi
Page 57 and 58: - 57 - over the “perfect” flat-
Page 59 and 60: - 59 - 3.2.7. Radial velocities and
Page 61 and 62: - 61 - A good general line list (id
Page 63 and 64: - 63 - the only overlap would be wi
Page 65 and 66: - 65 - a far better job at matching
Page 67 and 68: - 67 - dispersion. Going to the par
Page 69 and 70: - 69 - red (including at least 7770
Page 71 and 72: - 71 - Exposures of the dome flat q
Page 73 and 74: - 73 - A bright star was seen just
Page 75 and 76: - 75 - 500 stars. Figure 20 shows t
Page 77 and 78: - 77 - So, attempt to select a tell
Page 79 and 80: - 79 - Fig. 21.— Output from the
Page 81 and 82: - 81 - Wrap-Up and Acknowledgements
Page 83: - 83 - Massey, P., DeVeny, J., Jann
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