The Echellograms and Response Functions from zj to M bands Calculated by Echelle Simulator V0.9 for IRCS
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- Ευτροπια Φωτόπουλος
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1 The Echellograms and Response Functions from zj to M bands Calculated by Echelle Simulator V0.9 for IRCS Tae-Soo Pyo pyo@subaru.naoj.org Subaru Telescope National Astronomical Observatory of Japan April
2 This report represents echelle spectral formats (echellograms) and response functions of Infrared Camera and Spectrograph (IRCS) from zj to M bands. The response function of each setting in this report includes the transmittance of atmosphere, blaze functions of echelle and cross-disperser gratings, and transmittance of the filter. The infrared spectral lines shown on echellograms and response functions are as follows: (a) OH lines (Steed & Baker, 1979) (b) Ar lines (Rao, Humphreys, & Rank, 1966) (c) [Fe ii] lines (Nussbaumer & Storey, 1988) (d) Atomic Hydrogen lines (Hummer & Storey, 1987) (e) Molecular Hydrogen lines (UKIRT Homepage) 1 (f) He I and He II lines (UKIRT Homepage) (g) 12 C 16 O and 13 C 16 O bandheads (UKIRT Homepage) (h) 12 C 16 O and 13 C 16 O fundamental (1-0) band lines µm (UKIRT Homepage) Each line group is marked with different color as indicated at lower-left corner of each echellogram. Each value in Intensity column of tables in this report indicates as follows: (a) Intensities in kr for OH lines (Steed & Baker, 1979) (b) Einstein coefficients for [Fe II] lines (Nussbaumer & Storey, 1988) (c) Relative intensities of I(line)/I(Hβ) for atomic Hydrogen lines(hummer & Storey, 1987) (d) Relative intensities of I(line)/I(1-0S(1)) at LTE (T=4000 K) for H 2 lines (UKIRT homepage) The accuracies of X and Y columns are about ±10 pixels The current version of echelle simulator calculates echellograms without correction of optical abbretions. We will correct the optical abbretions for the higher fitting accuracies in the next version. 2
3 Bibliography Hummer, D. G., & Storey, P. J. 1987, MNRAS, 224, 801 Nussbaumer, H., and Storey, P. J. 1988, A&A, 193, 327 Rao, K. N., Humphreys, C. J., & Rank, D. H. 1966, in Wavelength Standards in the Infrared (NewYork; London: Acad. Press) Steed, A. J., & Baker, D. J. 1979, Appl. Opt., 18,
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5 Contents 1 zj- to K-bands : OH lines and other infrared lines 11 2 zj- to K-bands : Ar lines and other infrared lines 39 3 L- and M-bands 63 5
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7 List of Figures 1.1 Echellogram of the zj-band when echelle setting parameter (ESP) = 2240 and cross-disperser setting parameter (XSP) = The background is the badpixel image Response function of the zj-band when ESP = 2240 and XSP = Echellogram of the J-band when ESP = 2240 and XSP = 830. The background image shows the sky OH emission lines Response function of the J-band when ESP = 2240 and XSP = Echellogram for part of the H-band when ESP = 3610 and XSP = 300. The background image shows the sky OH emission lines Response function for a part of the H-band when ESP = 3610 and XSP = Echellogram for part of the H-band when ESP = 1490 and XSP = 180. The background is the bad pixel image Response function for part of the H-band when ESP = 1490 and XSP = Echellogram for part of the K-band when ESP = 6450 and XSP = 470. The background image is the bad pixel image Response function for part of the K-band when ESP = 6450 and XSP = Echellogram for part of the K-band when ESP = 270 and XSP = 200. The background is the bad pixel image Response function for part of the K-band when ESP = 270 and XSP = Echellogram of the zj-band when ESP = 2240 and XSP = The background image shows the emission lines of a Th-Ar lamp Response function of the zj-band when ESP = 2240 and XSP =
8 2.3 Echellogram of the J-band when ESP = 2240 and XSP = 830. The background is the bad pixel image Response function of the J-band when ESP = 2240 and XSP = 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 Response function for a part of the H-band when ESP = 3610 and XSP = Echellogram for part of the H-band when ESP = 1490 and XSP = 180. The background is the bad pixel image Response function for part of the H-band when ESP = 1490 and XSP = Echellogram for part of the K-band when ESP = 6450 and XSP = 470. The background image is the bad pixel image Response function for part of the K-band when ESP = 6450 and XSP = Echellogram for part of the K-band when ESP = 270 and XSP = 200. The background is the bad pixel image Response function for part of the K-band when ESP = 270 and XSP = Echellogram for part of the L-band when ESP = and XSP = 200. The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the L-band when ESP = and XSP = 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 Response function for part of the L-band when ESP = 2500 and XSP = Echellogram for part of the L-band when ESP = 4500 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the L-band when ESP = 4500 and XSP =
9 3.7 Echellogram for part of the L-band when ESP = and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the L-band when ESP = and XSP = Echellogram for part of the L-band when ESP = 2500 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the L-band when ESP = 2500 and XSP = Echellogram for part of the L-band when ESP = 4500 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the L-band when ESP = 4500 and XSP = Echellogram for part of M-band when ESP = and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of M-band when ESP = and XSP = Echellogram for part of the M-band when ESP = 4000 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the M-band when ESP = 4000 and XSP = Echellogram for part of the M-band when ESP = 4000 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the M-band when ESP = 4000 and XSP = Echellogram for part of the M-band when ESP = 1100 and XSP = The backgraound image shows the spectra of a standard star and sky. Telluric lines are revealed as emission lines Response function for part of the M-band when ESP = 1100 and XSP =
10 List of Tables 1.1 List of spectral lines displayed on zj-band (Figures 1.1 and 1.2) List of spectral lines displayed on J-band (Figures 1.3 and 1.4) List of spectral lines displayed on H-band (H-: Figures 1.5 and 1.6) List of spectral lines displayed on H-band (H+: Figures 1.7 and 1.8) List of spectral lines displayed on K-band (K-: Figures 1.9 and 1.10) List of spectral lines displayed on K-band (K+: Figures 1.11 and 1.12) List of spectral lines displayed on zj-band (Figures 2.1 and 2.2) List of spectral lines displayed on J-band (Figures 2.3 and 2.4) List of spectral lines displayed on H-band (H-: Figures 2.5 and 2.6) List of spectral lines displayed on H-band (H+: Figures 2.7 and 2.8) List of spectral lines displayed on K-band (K-: Figures 2.9 and 2.10) List of spectral lines displayed on K-band (K+: Figures 2.11 and 2.12) List of spectral lines displayed on L-band (LA-: Figures 3.1 and 3.2) List of spectral lines displayed on L-band (LA*: Figures 3.3 and 3.4) List of spectral lines displayed on L-band (LA+: Figures 3.5 and 3.6) List of spectral lines displayed on L-band (LB-: Figures 3.7 and 3.8) List of spectral lines displayed on L-band (LB*: Figures 3.9 and 3.10) List of spectral lines displayed on L-band (LB+: Figures 3.11 and 3.12) List of spectral lines displayed on M-band (M : Figures 3.13 and 3.14) List of spectral lines displayed on M-band (M-: Figures 3.15 and 3.16) List of spectral lines displayed on M-band (M+: Figures 3.17 and 3.18) List of spectral lines displayed on M-band (M++: Figures 3.19 and 3.20)
11 Chapter 1 zj- to K-bands : OH lines and other infrared lines 11
12 Figure 1.1: Echellogram of the zj-band when echelle setting parameter (ESP) = 2240 and cross-disperser setting parameter (XSP) = The background is the badpixel image. 12
13 Figure 1.2: Response function of the zj-band when ESP = 2240 and XSP =
14 Figure 1.3: Echellogram of the J-band when ESP = 2240 and XSP = 830. The background image shows the sky OH emission lines. 14
15 Figure 1.4: Response function of the J-band when ESP = 2240 and XSP =
16 Figure 1.5: Echellogram for part of the H-band when ESP = 3610 and XSP = 300. The background image shows the sky OH emission lines. 16
17 Figure 1.6: Response function for a part of the H-band when ESP = 3610 and XSP =
18 Figure 1.7: Echellogram for part of the H-band when ESP = 1490 and XSP = 180. The background is the bad pixel image. 18
19 Figure 1.8: Response function for part of the H-band when ESP = 1490 and XSP =
20 Figure 1.9: Echellogram for part of the K-band when ESP = 6450 and XSP = 470. The background image is the bad pixel image. 20
21 Figure 1.10: Response function for part of the K-band when ESP = 6450 and XSP =
22 Figure 1.11: Echellogram for part of the K-band when ESP = 270 and XSP = 200. The background is the bad pixel image. 22
23 Figure 1.12: Response function for part of the K-band when ESP = 270 and XSP =
24 Table 1.1: List of spectral lines displayed on zj-band (Figures 1.1 and 1.2). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) e-6 6D(9/2)-4D(5/2) e-6 6D(9/2)-4D(5/2) e-6 6D(7/2)-4D(3/2) Paδ(7-3) Paγ(6-3) HEII HEII HEI HEII HEI HEI HEI HEI HEI HEI HEI HEI HEII HEI HEI HEI
25 Table 1.1: List of spectral lines displayed on zj-band (Figures 1.1 and 1.2) HEI HEII HEII HEI HEII HEII HEI (end) 25
26 Table 1.2: List of spectral lines displayed on J-band (Figures 1.3 and 1.4). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) e-6 6D(9/2)-4D(5/2) e-6 6D(9/2)-4D(5/2) e-6 6D(7/2)-4D(3/2) e-5 6D(5/2)-4D(3.2)
27 Table 1.2: List of spectral lines displayed on J-band (Figures 1.3 and 1.4) e-4 6D(7/2)-4D(5/2) e-4 6D(3/2)-4D(1/2) e-3 6D(9/2)-4D(7/2) e-3 6D(1/2)-4D(1/2) e-3 6D(1/2)-4D(1/2) e-3 6D(3/2)-4D(3/2) e-3 6D(5/2)-4D(5/2) e-3 6D(1/2)-4D(3/2) e-3 6D(1/2)-4D(3/2) e-3 6D(7/2)-4D(7/2) e-3 6D(3/2)-4D(5/2) e-4 6D(5/2)-4D(7/2) Paβ(5-3) HEII HEII HEII HEI HEII HEII HEII HEI HEII HEI HEI HEII HEI HEII HEI HEI HEI HEI HEI HEII HEI HEII (end) 27
28 Table 1.3: List of spectral lines displayed on H-band (H-: Figures 1.5 and 1.6). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels)
29 Table 1.3: List of spectral lines displayed on H-band (H-: Figures 1.5 and 1.6) e-3 4F(9/2)-4D(5/2) e-3 4F(7/2)-4D(3/2) e-3 4F(9/2)-4D(7/2) e-3 4F(5/2)-4D(1/2) e-4 4F(5/2)-4D(3/2) e-3 4F(3/2)-4D(1/2) e-3 4D(7/2)-4P(3/2) e-3 4F(5/2)-4D(5/2) e-3 4F(7/2)-4D(7/2) e-3 4D(7/2)-4P(5/2) e-3 4D(5/2)-4P(1/2) Br(20-4) Br(19-4) Br(18-4) Br(17-4) Br(16-4) Br(15-4) Br(14-4) Br(13-4) Br(12-4) Br(10-4) Br(9-4) HEII HEII HEI HEII HEII HEII HEII HEII HEI
30 Table 1.3: List of spectral lines displayed on H-band (H-: Figures 1.5 and 1.6) HEII HEII HEII HEII HEII C16O C16O C16O C16O C16O C16O (end) 30
31 Table 1.4: List of spectral lines displayed on H-band (H+: Figures 1.7 and 1.8). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels)
32 Table 1.4: List of spectral lines displayed on H-band (H+: Figures 1.7 and 1.8) e-3 4F(9/2)-4D(5/2) e-3 4F(7/2)-4D(3/2) e-3 4F(5/2)-4D(1/2) e-3 4F(7/2)-4D(5/2) e-4 4F(5/2)-4D(3/2) e-3 4F(7/2)-4D(7/2) e-3 4D(7/2)-4P(5/2) e-3 4D(5/2)-4P(1/2) Br(20-4) Br(19-4) Br(18-4) Br(17-4) Br(16-4) Br(15-4) Br(14-4) Br(13-4) Br(11-4) Br(10-4) Br(9-4) HEII HEII HEII HEII HEII HEII HEI HEII HEII HEII HEII HEII HEII
33 Table 1.4: List of spectral lines displayed on H-band (H+: Figures 1.7 and 1.8) HEII C16O C16O C16O C16O (end) 33
34 Table 1.5: List of spectral lines displayed on K-band (K-: Figures 1.9 and 1.10). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) e-4 4D(3/2)-4P(1/2) e-4 4D(5/2)-4P(5/2) e-4 4D(1/2)-4P(1/2) e-4 4D(3/2)-4P(3/2) e-4 4D(1/2)-4P(3/2) e-4 4D(3/2)-4P(5/2) e-5 4D(1/2)-4P(5/2) Brδ(8-4) Brγ(7-4) Pf(22-5) Pf(21-5) Pf(20-5) Pf(19-5)
35 Table 1.5: List of spectral lines displayed on K-band (K-: Figures 1.9 and 1.10) HEI HEI HEI HEI HEI HEII HEII HEI HEI HeI HEI HEII HeI HEII HEI HEI HEII HEII C16O C16O C16O C16O C16O C16O C16O C16O (end) 35
36 Table 1.6: List of spectral lines displayed on K-band (K+: Figures 1.11 and 1.12). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) e-4 4F(5/2)-4D(7/2) e-4 4D(5/2)-4P(5/2) e-4 4D(1/2)-4P(1/2) e-4 4D(3/2)-4P(5/2) Brδ(8-4) Brγ(7-4) Pf(n-4) Pf(25-5) Pf(24-5) Pf(23-5) Pf(19-5) Pf(18-5) Pf(17-5)
37 Table 1.6: List of spectral lines displayed on K-band (K+: Figures 1.11 and 1.12) HEI HEII HEI HEI HeI HEI HEII HEII HeI HEII HEI HEII HEII HEII HEII HEII HEII HEII HEI C16O C16O C16O C16O C16O C16O C16O C16O (end) 37
38 38
39 Chapter 2 zj- to K-bands : Ar lines and other infrared lines 39
40 Figure 2.1: Echellogram of the zj-band when ESP = 2240 and XSP = The background image shows the emission lines of a Th-Ar lamp. 40
41 Figure 2.2: Response function of the zj-band when ESP = 2240 and XSP =
42 Figure 2.3: Echellogram of the J-band when ESP = 2240 and XSP = 830. The background is the bad pixel image. 42
43 Figure 2.4: Response function of the J-band when ESP = 2240 and XSP =
44 Figure 2.5: 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. 44
45 Figure 2.6: Response function for a part of the H-band when ESP = 3610 and XSP =
46 Figure 2.7: Echellogram for part of the H-band when ESP = 1490 and XSP = 180. The background is the bad pixel image. 46
47 Figure 2.8: Response function for part of the H-band when ESP = 1490 and XSP =
48 Figure 2.9: Echellogram for part of the K-band when ESP = 6450 and XSP = 470. The background image is the bad pixel image. 48
49 Figure 2.10: Response function for part of the K-band when ESP = 6450 and XSP =
50 Figure 2.11: Echellogram for part of the K-band when ESP = 270 and XSP = 200. The background is the bad pixel image. 50
51 Figure 2.12: Response function for part of the K-band when ESP = 270 and XSP =
52 Table 2.1: List of spectral lines displayed on zj-band (Figures 2.1 and 2.2). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) B e-6 6D(9/2)-4D(5/2) e-6 6D(9/2)-4D(5/2) e-6 6D(7/2)-4D(3/2) Paδ(7-3) Paγ(6-3) HEII HEII HEI HEII HEI HEI HEI HEI HEI HEI HEI HEI HEII HEI HEI HEI HEI HEII HEII HEI HEII HEII HEI (end) 52
53 Table 2.2: List of spectral lines displayed on J-band (Figures 2.3 and 2.4). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) B B e-6 6D(9/2)-4D(5/2) e-6 6D(9/2)-4D(5/2) e-6 6D(7/2)-4D(3/2) e-5 6D(5/2)-4D(3.2)
54 Table 2.2: List of spectral lines displayed on J-band (Figures 2.3 and 2.4) e-4 6D(7/2)-4D(5/2) e-4 6D(3/2)-4D(1/2) e-3 6D(9/2)-4D(7/2) e-3 6D(1/2)-4D(1/2) e-3 6D(1/2)-4D(1/2) e-3 6D(3/2)-4D(3/2) e-3 6D(5/2)-4D(5/2) e-3 6D(1/2)-4D(3/2) e-3 6D(1/2)-4D(3/2) e-3 6D(7/2)-4D(7/2) e-3 6D(3/2)-4D(5/2) e-4 6D(5/2)-4D(7/2) Paβ(5-3) HEII HEII HEII HEI HEII HEII HEII HEI HEII HEI HEI HEII HEI HEII HEI HEI HEI HEI HEI HEII HEI HEII (end) 54
55 Table 2.3: List of spectral lines displayed on H-band (H-: Figures 2.5 and 2.6). Line Number Order Wavelength (µm) Intensity Label X(pixels) Y(pixels) B e-3 4F(9/2)-4D(5/2) e-3 4F(7/2)-4D(3/2) e-3 4F(9/2)-4D(7/2) e-3 4F(5/2)-4D(1/2) e-4 4F(5/2)-4D(3/2) e-3 4F(3/2)-4D(1/2) e-3 4D(7/2)-4P(3/2) e-3 4F(5/2)-4D(5/2) e-3 4F(7/2)-4D(7/2) e-3 4D(7/2)-4P(5/2) e-3 4D(5/2)-4P(1/2) Br(20-4) Br(19-4) Br(18-4) Br(17-4) Br(16-4) Br(15-4) Br(14-4) Br(13-4) Br(12-4) Br(10-4) Br(9-4) HEII HEII HEI HEII HEII HEII HEII HEII HEI HEII HEII HEII HEII HEII C16O C16O
56 Table 2.3: List of spectral lines displayed on H-band (H-: Figures 2.5 and 2.6) C16O C16O C16O C16O (end) 56
Si + Al Mg Fe + Mn +Ni Ca rim Ca p.f.u
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