Wavelength (WL) References to Original Literature: S

Sulfur, Z = 16

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S I (WL)
  1. A1 - Alder, J. F., Bombelka, R. M., and Kirkbright, G. F. (1978), J. Phys. B 11, 235-238.
  2. E1 - Eriksson, K. B. S. (1978), Astrophys. J. 222, 398-399.
  3. F1 - Frerichs, R. (1933), Z. Phys. 80, 150-160.
  4. G1 - Gibson, S. T., Greene, J. P., Rui, B., and Berkowitz, J. (1986), J. Phys. B 19, 2825-2840.
  5. H2 - Haas, M. R., Hollenbach, D., and Erickson, E. F. (1991), Astrophys. J. 374, 555-563.
  6. J1 - Jakobsson, L. R. (1966), Ark. Fys. 34, 19-31.
  7. J2 - Joshi, Y. N., Mazzoni, M., Nencioni, A., Parkinson, W. H., and Cantu, A. (1987), J. Phys. B 20, 1203-1213.
  8. K1 - Kaufman, V. (1982), Phys. Scr. 26, 439-442.
  9. M1 - Meissner, K. W., Bartlet, O., and Eckstein, L. (1933), Z. Phys. 86, 54-76.
  10. S1 - Sarma, V. N. and Joshi, Y. N. (1984), Physica (Utrecht) 123C, 349-352.
  11. T1 - Tondello, G. (1972), Astrophys. J. 172, 771-783.
S II (WL)
  1. B2 - Bowen, I. S. (1955), Astrophys. J. 121, 306-311.
  2. B3 - Bowen, R. A. (1983), Astrophys. J. 268, L47-L30.
  3. B4 - Bartlet, O. and Eckstein, L. (1933), Z. Phys. 86, 77-81.
  4. B5 - Bloch, L. and Bloch, E. (1929), Ann. Phys. (Paris) 12, 1-22.
  5. H1 - Hunter, A. (1934), Phil. Trans. R. Soc. London, Ser. A 233, 303-326.
  6. P2 - Pettersson, J. E. (1983), Phys. Scr. 28, 421-434.
  7. T3 - Trauger, J. T., Munch, G., and Roesler, F. L. (1980), Astrophys. J. 236, 1035-1042.
S III (WL)
  1. B2 - Bowen, I. S. (1955), Astrophys. J. 121, 306-311.
  2. B9 - Bowen, I. S. (1960), Astrophys. J. 132, 1-17.
  3. B10- - Baluteau, J. P., Bussoletti, E., Anderegg, M., Moorwood, A. F. M., and Coron, N. (1976), Astrophys. J. 210, L45-L48.
  4. B11 - Bloch, L. and Bloch, E. (1935), J. Phys. (Paris) 6, 441-450.
  5. C1 - Colgan, S. W. J., Simpson, J. P., Rubin, R. H., Erickson, E. F., Haas, M. R., and Wolf, J. (1991), Astrophys. J. 366, 172-180. The accurate measurement of the S III 3s23p2 3P0-3P1 wavelength made in connection with the observations described in this reference was not published. The value obtained was 33.480 ñ 0.004 æm (Haas, M. R. (1989), private communication).
  6. G6 - Graf, P. H. (1988), A Fabry-Perot for Airborne Infrared Astronomy and the (Si II) Emission from the Galactic Center, Ph.D Thesis, Cornell Univ., CRSR 889. Graf obtained a wavelength of 33.482 ñ 0.002 æm for the S III 3P0-3P1 ground-term interval assuming VLSR=0 for the Omega Nebula source. Correction to VLSR=17 km/s for the central region of this nebula (Reifenstein, E. C., III et al., (1970), Astron. Astrophys. 4, 357-377) yields a rest wavelength of 33.480 ñ 0.002 æm.
  7. J8 - Johansson, L., Magnusson, C. E., Joelsson, I., and Zetterberg, P. O. (1992), Phys. Scr. 46, 221-224.
  8. J10 - Johansson, L. (1992), private communication.
  9. K5 - Kaufman, V. (1971), unpublished material.
  10. S5 - Smith, P. L., Magnusson, C. E., and Zetterberg, P. O. (1984), Astrophys. J. 277, L79-L81.
S IV (WL)
  1. E2 - Engstrom, L. (1991), unpublished material from an analysis of S IV in progress at the University of Lund, Sweden.
  2. L1 - Lacy, J. H. (1989), private communication. The line was measured in the spectra of several different planetary nebulae; see Beck, S. C., et al. (1981), Astrophys. J. 249, 592-601.
S V (WL)
  1. Engstrom, L. and Jupen, C. (1992), private communication.
  2. J4 - Joelsson, I., Zetterberg, P. O., and Magnusson, C. B. (1981), Phys. Scr. 23, 1087-1095.
S VI (WL)
  1. D4 - Dynefors, B. I. and Martinson, I. (1978), Phys. Scr. 17, 123-129.
  2. J5 - Joelsson, I., Zetterberg, P. O., and Magnusson, C. E. (1979), Phys. Scr. 20, 145-150.
  3. J6 - Jupen, C., Engstrom, L., Hutton, R., Reistad, N., and Westerlind, M. (1990), Phys. Scr. 42, 44-50.
  4. W2 - Westerlind, M., Engstrom, L., Jupen, C., and Bengtsson, P. (1991), Phys. Scr. 44, 582-586.
S VII (WL)
  1. F2 - Ferner, E. (1948), Ark. Mat., Astron. Fys. 36, 1-65.
  2. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  3. G2 - Garnir, H. P. (1979), J. Opt. Soc. Am. 69, 916-917.
  4. G5 - Garnir, H. P., Baudinet-Robinet, Y., and Dumont, P. D. (1976), Phys. Scr. 17, 463-465.
  5. J3 - Jupen, C., Litzen, U., and Trigueiros, A. (1984), Phys. Scr. 29, 317-318.
  6. J9 - Jupen, C. (1992), J. Phys. B 25, L237-L241.
  7. K2 - Kononov, E. Ya., Kramida, A. E., Podobedova, L. I., Ragozin, E. N., and Chirkov, V. A. (1983), Phys. Scr. 28, 496-500.
S VIII (WL)
  1. C1 - Cohen, L. and Martin, W. C. (1985), unpublished material.
  2. F2 - Ferner, E. (1948), Ark. Mat. Astron. Fys. 36, 1-65.
  3. R1 - Robinson, H. A. (1937), Phys. Rev. 52, 724-725.
  4. T2 - Trigueiros, A. and Jupen, C. (1985), Phys. Scr. 31, 359-363.
S IX (WL)
  1. D1 - Deutschman, W. A., and House, L. L. (1966), Astrophys. J. 144, 435-437.
  2. F2 - Ferner, E. (1948), Ark. Mat. Astron. Fys. 36, 1-65.
  3. F3 - Fawcett, B. C., and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  4. F4 - Fawcett, B. C., Cowan, R. D., and Hayes, R. W. (1974), Astrophys. J. 187, 377-383.
  5. F5 - Feldman, U. and Doschek, G. A. (1977), J. Opt. Soc. Am. 67, 726-734.
  6. F7 - Fawcett, B. C., Gabriel, A. H., and Paget, T. M. (1971), J. Phys. B 4, 986-994.
  7. K3 - Kononov, E. Ya. (1966), Opt. Spectrosc. (USSR) 20, 303-304.
  8. P1 - Podobedova, L. I., Kononov, E. Ya., and Koshelev, K. N. (1971), Opt. Spectrosc. (USSR) 30, 217-220.
  9. S2 - Sandlin, G. D., Brueckner, G. E., and Tousey, R. (1977), Astrophys. J. 214, 898-904.
S X (WL)
  1. C2 - Cohen, L. and Crooker, A. M. (1985), unpublished measurements.
  2. D2 - Deutschman, W. A., and House, L. L. (1967), Astrophys. J. 149, 451-452.
  3. F2 - Ferner, E. (1948), Ark. Mat. Astron. Fys. 36, 1-65.
  4. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  5. F5 - Feldman, U. and Doschek, G. A. (1977), J. Opt. Soc. Am. 67, 726-734.
  6. F6 - Fawcett, B. C. and Hayes, R. W. (1973), Phys. Scr. 8, 244-248.
  7. F7 - Fawcett, B. C., Gabriel, A. H., and Paget, T. M. (1971), J. Phys. B 4, 986-994.
  8. F9 - Fawcett, B. C., Hardcastle, R. A., and Tondello, G. (1970), J. Phys. B 3, 564-571.
  9. K3 - Kononov, E. Ya. (1966), Opt. Spectrosc. (USSR) 20, 303-304.
  10. K4 - Kastner, S. O., Bhatia, A. K. and Cohen, L. (1977), Phys. Scr. 15, 259-267.
  11. P1 - Podobedova, L. I., Kononov, E. Ya., and Koshelev, K. N. (1971), Opt. Spectrosc. (USSR) 30, 217-220.
  12. S2 - Sandlin, G. D., Brueckner, G. E., and Tousey, R. (1977), Astrophys. J. 214, 898-904.
S XI (WL)
  1. D2 - Deutschman, W. A. and House, L. L. (1967), Astrophys. J. 149, 451-452.
  2. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  3. F5 - Feldman, U. and Doschek, G. A. (1977), J. Opt. Soc. Am. 67, 726-734.
  4. F6 - Fawcett, B. C. and Hayes, R. W. (1973), Phys. Scr. 8, 244-248.
  5. F8 - Fawcett, B. C. (1975), At. Data Nucl. Data Tables 16, 135-164.
  6. F9 - Fawcett, B. C., Hardcastle, R. A., and Tondello, G. (1970), J. Phys. B 3, 564-571.
  7. P1 - Podobedova, L. I., Kononov, E. Ya., and Koshelev, K. N. (1971), Opt. Spectrosc. (USSR)30, 217-220.
  8. S2 - Sandlin, G. D., Brueckner, G. E., and Tousey, R. (1977), Astrophys. J. 214, 898-904.
S XII (WL)
  1. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  2. F8 - Fawcett, B. C. (1975), At. Data Nucl. Data Tables 16, 135-164.
  3. F10 - Fawcett, B. C. (1970), J. Phys. B 3, 1152-1163.
  4. J7 - Jefferies, J. T. (1969), Mem. Soc. R. Sci. Liege. Collect. 8, 17, 213-234.
  5. P1 - Podobedova, L. I., Kononov, E. Ya., and Koshelev, K. N. (1971), Opt. Spectrosc. (USSR) 30, 217-220.
S XIII (WL)
  1. D3 - Dere, K. P. (1978), Astrophys. J. 221, 1062-1067.
  2. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  3. F8 - Fawcett, B. C. (1975), At. Data Nucl. Data Tables 16, 135-164.
  4. P1 - Podobedova, L. I., Kononov, E. Ya., and Koshelev, K. N. (1971), Opt. Spectrosc. (USSR) 30, 217-220.
  5. S6 - Serpa, F. G. and Livingston, A. E. (1991), Phys. Rev. A 43, 6447-6450.
  6. W1 - Widing, K. G. (1978), Astrophys. J. 122, 735-739.
S XIV (WL)
  1. A2 - Aglitskii, E. V., Boiko, V. A., Zakharov, S. M., Pikuz, S. A., and Faenov, E. Ya. (1974), Sov. J. Quantum Electron. 4, 500-513.
  2. {b1 - Brown, C. M., Ekberg, J. O., Seely, J. E., and Feldman, U. (1989), J. Opt. Soc. Am. B 6, 1650-1651.
  3. B6 - Boiko, V. A., Pikuz, A. A., Safronova, U. I., and Faenov, A. Ya. (1978), Mon. Not. R. Astron. Soc. 185, 789-805.
  4. D3 - Dere, K. P. (1978), Astrophys. J. 221, 1062-1067.
  5. Edlen, B. (1979), Phys. Scr. 19, 255-266.
  6. F3 - Fawcett, B. C. and Hayes, R. W. (1987), Phys. Scr. 36, 80-87.
  7. F6 - Fawcett, B. C. and Hayes, R. W. (1973), Phys. Scr. 8, 244-248.
  8. G3 - Goldsmith, S., Oren, L., and Cohen, L. (1974), Astrophys. J. 188, 197-200.
  9. S3 - Sandlin, G. D., Brueckner, G. E., Scherrer, V. E., and Tousey, R. (1976), Astrophys. J. 205, L47-L50.
  10. Vainshtein, L. A. and Safronova, U. I. (1980), At. Data Nucl. Data Tables 25, 311-385.
  11. W2 - Widing, K. G. and Purcell, J. D. (1976), Astrophys. J. 204, L151-L153.
S XV (WL)
  1. A2 - Aglitskii, E. V., Boiko, V. A., Zakharov, S. M., Pikuz, S. A., and Faenov, A. Ya. (1974), Sov. J. Quantum Electron. 4, 500-513. The experimental wavelengths in this paper have been increased by 8 parts in 105; see Martin, W. C. (1981), Phys. Scr. 24, 725-731.
  2. A3 - Aglitsky, E. V., Antsiferov, P. S., Mandelstam, S. L., Panin, A. M., Safronova, U. I., Ulitin, S. A., and Vainshtein, L. A. (1988), Phys. Scr. 38, 136-142.
  3. B7 - Boiko, V. A., Faenov, A. Ya., Pikuz, S. A., and Safronova, U. I. (1977), Mon. Not. R. Astron. Soc. 181, 107-120. The experimental wavelength has been increased by 8 parts in 105; see Martin, W. C. (1981), Phys. Scr. 24, 725-731.
  4. B8 - Boiko, V. A., Faenov, A. Ya., Pikuz, S. A., Skobelev, I. Yu., Vinogradov, A. V., and Yukov, E. A. (1977), J. Phys. B 10, 3387-3394. The experimental wavelength has been increased by 8 parts in 105; see Martin, W. C. (1981), Phys. Scr. 24, 725-731.
  5. D5 - DeSerio, R., Berry, H. G., Brooks, R. L., Hardis, J., Livingston, A. E., and Hinterlong, S. J. (1981), Phys. Rev. A 24, 1872-1888.
  6. S4 - Schleinkofer, L., Bell, F., Betz, H. D., Trollmann, G., and Rothermel, J. (1982), Phys. Scr. 25, 917-923.
S XVI (WL)
  1. A2 - Aglitskii, E. V., Boiko, V. A., Zakharov, S. M., Pikuz, S. A., and Faenov, A. Ya. (1974), Sov. J. Quantum Electron. 4, 500-513. The experimental wavelengths in this paper have been increased by 8 parts in 105; see Martin, W. C. (1981), Phys. Scr. 24, 725-731.
  2. G4 - Georgiadis, A. P., Muller, D., Strater, H. D., Gassen, J., von Brentano, P., Sens, J. C., and Pape, A. (1986), Phys. Lett. A 115, 108-110.
  3. S4 - Schleinkofer, L., Bell, F., Betz, H. D., Trollman, G., and Rothermel, J. (1982), Phys. Scr. 25, 917-923.

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