MC SNR Database References
[C76]: Clarke, J. N. Little, A. G., & Mills, B. Y. 1976, AuJPA, 40 1 (C76)
[DEM76]: Davies, R. D., Elloitt, K. H., & Meaburn, J 1976, MemRAS, 81, 89 (DEML, DEMS)
[D01]: Dickel, J. R., Williams, R. M., Carter, L. M., Milne, D. K., Petre, R., & Amy, S. W. 2001, AJ, 122, 849
[DW09]: Dickel, J. R. & Williams, R.M. 2009, in "Supernova Remnants and Pulsar Wind Nebulae in the Chandra Era", Boston, MA
[F08] Filipovic, M. D., Haberl, F., Winkler, P. F., Pietsch, W., Payne, J., Crawford, E. J., De Horta, A. Y., Stootman, F. H., & Reaser, B. E. 2008, A&A, 485, 63
[H04]: Heyden K. J. van der, Bleeker, J. A. M., & Kaastra, J. S. 2004 A&A, 421, 1031
[HFPK00]: Haberl, F., Filipovic, M. D., Pietsch, W., & Kahabka, P . 2000 A&AS 142, 41 (HFPK)
[H56]: Henize, K. 1956 ApJS, 2, 315 (LHa 120-, LHa 115-)
[IKT83]: Inoue, H., Koyama, K., & Tanaka, Y. 1983 Supernova Remnants and their X-Ray Emission, IAU Symposium 35, ed. By J. Danziger & P. Gorenstein 540 (IKT)
[K+09]: Klimek et al. 2009 (to be submitted to ApJ) (XMM data)
[M83]: Mathewson, D. S., Ford, V. L., Dopita, M. A., tuohy, I. R., Long, K. s., & Helfand, D. 1983 ApJS, 51 345
[M84]: Mathewson, D S., Ford, V. L., Dopita, M. A., Tuohy, I. R., Mills, b. Y., & Turtle, A. J. 1984 ApJS, 55, 189
[P04]: Payne, J., Filipovic, M. D., Reid, W., Jones, P. A., Staveley-Smith, L., & White, G. L. 2004 MNRAS, 355, 44
[P07]: Payne, J., White, g. L., Filipovic, M. D., & Pannuti, T. G. 2007 MNRAS, 376, 1793
[RI+08]: Reyes-Iturbide, J., Rosado, M., & Velázquez, P. F. 2008, AJ, 136, 2011 (XMM data)
[SW81]: Seward, F. D. & Mitchell, M. 1981 ApJ, 243, 736 (SW81 and IE designations)
[S-catlg]: Seward et al. Chandra SNR Catalog, http://hea-www.harvard.edu/ChandraSNR/
[W+99]: Williams et al. 1999, ApJ, 514, 798 (ROSAT data)
[W+04]: Williams et al. 2004, ApJ, 613, 948 (XMM data)
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Reference Notes
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"2 cm" radio fluxes for the LMC were from Milne, Caswell, Haynes 1980, MNRAS,
191, 469.
"3 cm" and "6 cm" values are all from the present study (DW09).
"13 cm" values for the LMC are from various publications, most frequently from
Dickel & Milne 1995, AJ, 109, 200 or 1998, AJ, 115, 1057. For the SMC, these are
taken from both Dickel et al. 2001, AJ, 122, 849 and Payne et al. 2004 MNRAS,
355, 44.
"20 cm" radio fluxes are usually in fact from 22 cm radio data. For the LMC,
most such values are measurements by DW09 from Hughes et al. For the SMC, these
are taken from both Dickel et al. 2001, AJ, 122, 849 and Payn eet al. 2004
MNRAS, 355, 44.
"36 cm" radio fluxes for the LMC are almost all SUMSS - Mauch et al. 2003,
MNRAS, 342, 1117. For the SMC, these are from the Mathewson et al. papers in
1983-85 and from Payne et al. 2007 MNRAS, 376, 1793.
"74 cm" radio fluxes for the LMC are various but mostly the Mathewson et al.
papers in 1983-85. For the SMC, these are from Clarke, Little, & Mills 1976,
AuJPA, 40 1.
[SII]/Ha ratios for the LMC were measured by DW09 from MCELS images. For the
SMC, values were taken from Payne et al. 2007 MNRAS, 376, 1793.
X-ray fluxes were largely taken from the literature as noted by the references
in the database, and converted to a common range of 0.5-2.0 keV unabsorbed
fluxes using the HEASARC PIMMS software.
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