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List of Figures

  1. Echellogram of the zJ-band when echelle setting parameter (ESP) = 2240 and cross-disperser setting parameter (XSP) = 2000. The background is the badpixel image.
  2. Response function of the zJ-band when ESP = 2240 and XSP = 2000.
  3. Echellogram of the J-band when ESP = 2240 and XSP = -830. The background image shows the sky OH emission lines.
  4. Response function of the J-band when ESP = 2240 and XSP = -830.
  5. Echellogram for part of the H-band when ESP = 3610 and XSP = -300. The background image shows the sky OH emission lines.
  6. Response function for a part of the H-band when ESP = 3610 and XSP = -300.
  7. Echellogram for part of the H-band when ESP = 1490 and XSP = -180. The background is the bad pixel image.
  8. Response function for part of the H-band when ESP = 1490 and XSP = -180.
  9. Echellogram for part of the K-band when ESP = 6450 and XSP = -470. The background image is the bad pixel image.
  10. Response function for part of the K-band when ESP = 6450 and XSP = -470.
  11. Echellogram for part of the K-band when ESP = -270 and XSP = 200. The background is the bad pixel image.
  12. Response function for part of the K-band when ESP = -270 and XSP = 200.
  13. Echellogram for part of the L-band when ESP = 10500 and XSP = -200. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  14. Response function for part of the L-band when ESP = 10500 and XSP = -200.
  15. Echellogram for part of the L-band when ESP = 2500 and XSP = 500. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  16. Response function for part of the L-band when ESP = 2500 and XSP = 500.
  17. Echellogram for part of the L-band when ESP = -4500 and XSP = 1300. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  18. Response function for part of the L-band when ESP = -4500 and XSP = 1300.
  19. Echellogram for part of the L-band when ESP = 10500 and XSP = 2600. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  20. Response function for part of the L-band when ESP = 10500 and XSP = 2600.
  21. Echellogram for part of the L-band when ESP = 2500 and XSP = 3400. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  22. Response function for part of the L-band when ESP = 2500 and XSP = 3400.
  23. Echellogram for part of the L-band when ESP = -4500 and XSP = 4100. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  24. Response function for part of the L-band when ESP = -4500 and XSP = 4100.
  25. Echellogram for part of M-band when ESP = 12000 and XSP = -5500. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  26. Response function for part of M-band when ESP = 12000 and XSP = -5500.
  27. Echellogram for part of the M-band when ESP = 4000 and XSP = -5500. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  28. Response function for part of the M-band when ESP = 4000 and XSP = -5500.
  29. Echellogram for part of the M-band when ESP = -4000 and XSP = -5500. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  30. Response function for part of the M-band when ESP = -4000 and XSP = -5500.
  31. Echellogram for part of the M-band when ESP = -1100 and XSP = -5500. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines.
  32. Response function for part of the M-band when ESP = -1100 and XSP = -5500.
  33. Echellogram of the zJ-band when ESP = 2240 and XSP = 2000. The background image shows the emission lines of a Th-Ar lamp.
  34. Response function of the zJ-band when ESP = 2240 and XSP = 2000.
  35. Echellogram of the J-band when ESP = 2240 and XSP = -830. The background is the bad pixel image.
  36. Response function of the J-band when ESP = 2240 and XSP = -830.
  37. Echellogram for part of the H-band when ESP = 3610 and XSP = -300. The background image shows the emission lines of a Th-Ar lamp.
  38. Response function for a part of the H-band when ESP = 3610 and XSP = -300.
  39. Echellogram for part of the H-band when ESP = 1490 and XSP = -180. The background is the bad pixel image.
  40. Response function for part of the H-band when ESP = 1490 and XSP = -180.
  41. Echellogram for part of the K-band when ESP = 6450 and XSP = -470. The background image is the bad pixel image.
  42. Response function for part of the K-band when ESP = 6450 and XSP = -470.
  43. Echellogram for part of the K-band when ESP = -270 and XSP = 200. The background is the bad pixel image.
  44. Response function for part of the K-band when ESP = -270 and XSP = 200.

Tae-Soo Pyo 2003-05-21