# 2007/09/18 # JD Smith # # All Herschel KP galaxies which are within 2.5 FWHM's of the "perfectly # bad" 8 pixel separation from foreground v=0 line emission. The # estimated foreground CII surface brightness is compared to the # estimated nuclear SB. Galaxies which have contamination with the line # itself (as opposed to the 8 pixel wavelength beam) are not included # (as they would be contaminants with chopping as well). [OIII] and # [NII] are not included, as they are likely weak in the cirrus # emission. Galaxy v Line Wave FWHM Range Beam Sep. Fore_CII Src_NUC_CII Cont. Frac (nuc) km/s um pix km/s FWHM's 1.e-10 W/m^2/sr percent ========================================================================================= m101 241 [CII] 157.7 2.4 1576.9 2.3 3.5 257.7 1.3 ngc0855 610 [CII] 157.7 2.4 1576.9 0.7 9.6 133.6 7.2 ngc0855 610 [OI] 63.2 1.3 1047.2 1.0 9.6 133.6 7.2 ngc3773 987 [CII] 157.7 2.4 1576.9 0.8 7.2 156.3 4.6 ngc5866 692 [CII] 157.7 2.4 1576.9 0.4 4.2 428.1 1.0 ngc5866 692 [OI] 63.2 1.3 1047.2 1.9 4.2 428.1 1.0 ngc1291 839 [CII] 157.7 2.4 1576.9 0.2 4.6 115.5 4.0 ngc1512 896 [CII] 157.7 2.4 1576.9 0.4 3.8 255.2 1.5 ngc3190 1271 [CII] 157.7 2.4 1576.9 2.0 6.8 331.5 2.1 ngc4594 1091 [CII] 157.7 2.4 1576.9 1.3 9.4 112.0 8.4 ngc4826 408 [CII] 157.7 2.4 1576.9 1.6 7.9 1781.1 0.4 ngc4826 408 [OI] 63.2 1.3 1047.2 1.3 7.9 1781.1 0.4 ngc1097 1275 [CII] 157.7 2.4 1576.9 2.0 5.4 3002.3 0.2 ngc2841 638 [CII] 157.7 2.4 1576.9 0.6 4.7 95.0 4.9 ngc2841 638 [OI] 63.2 1.3 1047.2 1.3 4.7 95.0 4.9 ngc3351 778 [CII] 157.7 2.4 1576.9 0.0 7.3 1645.0 0.4 ngc3521 805 [CII] 157.7 2.4 1576.9 0.1 8.9 370.4 2.4 ngc5055 504 [CII] 157.7 2.4 1576.9 1.2 4.4 595.8 0.7 ngc5055 504 [OI] 63.2 1.3 1047.2 0.2 4.4 595.8 0.7 ngc7331 816 [CII] 157.7 2.4 1576.9 0.1 11.3 646.0 1.7 ngc0024 554 [CII] 157.7 2.4 1576.9 1.0 5.6 52.5 10.6 ngc0024 554 [OI] 63.2 1.3 1047.2 0.3 5.6 52.5 10.6 ngc0628 657 [CII] 157.7 2.4 1576.9 0.5 9.8 87.6 11.2 ngc0628 657 [OI] 63.2 1.3 1047.2 1.5 9.8 87.6 11.2 ngc3184 592 [CII] 157.7 2.4 1576.9 0.8 5.0 328.1 1.5 ngc3184 592 [OI] 63.2 1.3 1047.2 0.8 5.0 328.1 1.5 ngc3198 663 [CII] 157.7 2.4 1576.9 0.5 4.1 313.6 1.3 ngc3198 663 [OI] 63.2 1.3 1047.2 1.6 4.1 313.6 1.3 ngc3938 809 [CII] 157.7 2.4 1576.9 0.1 5.4 110.3 4.9 ngc4559 816 [CII] 157.7 2.4 1576.9 0.1 5.3 133.8 4.0 ngc5474 273 [CII] 157.7 2.4 1576.9 2.2 3.4 28.1 12.2 ngc0925 553 [CII] 157.7 2.4 1576.9 1.0 9.6 92.0 10.4 ngc0925 553 [OI] 63.2 1.3 1047.2 0.3 9.6 92.0 10.4 ngc3621 727 [CII] 157.7 2.4 1576.9 0.3 11.4 292.5 3.9 ngc3621 727 [OI] 63.2 1.3 1047.2 2.3 11.4 292.5 3.9 ngc4631 606 [CII] 157.7 2.4 1576.9 0.8 5.0 3166.2 0.2 ngc4631 606 [OI] 63.2 1.3 1047.2 0.9 5.0 3166.2 0.2 tol89 1216 [CII] 157.7 2.4 1576.9 1.8 12.3 189.4 6.5 ngc7793 230 [CII] 157.7 2.4 1576.9 2.3 5.0 217.9 2.3 ngc2915 468 [CII] 157.7 2.4 1576.9 1.3 16.9 85.1 19.9 ngc2915 468 [OI] 63.2 1.3 1047.2 0.6 16.9 85.1 19.9 ngc4625 609 [CII] 157.7 2.4 1576.9 0.8 5.1 58.4 8.7 ngc4625 609 [OI] 63.2 1.3 1047.2 1.0 5.1 58.4 8.7 ngc5408 509 [CII] 157.7 2.4 1576.9 1.2 12.8 259.0 4.9 ngc5408 509 [OI] 63.2 1.3 1047.2 0.2 12.8 259.0 4.9 ic4710 741 [CII] 157.7 2.4 1576.9 0.2 13.1 29.4 44.7 ic4710 741 [OI] 63.2 1.3 1047.2 2.5 13.1 29.4 44.7 ngc4552 340 [CII] 157.7 2.4 1576.9 1.9 7.8 15.6 50.0 ngc4552 340 [OI] 63.2 1.3 1047.2 2.1 7.8 15.6 50.0 ngc4569 -235 [CII] 157.7 2.4 1576.9 2.3 8.0 543.0 1.5 ngc4725 1206 [CII] 157.7 2.4 1576.9 1.7 4.5 162.9 2.8 ngc4736 308 [CII] 157.7 2.4 1576.9 2.0 4.4 1263.3 0.3 ngc4736 308 [OI] 63.2 1.3 1047.2 2.5 4.4 1263.3 0.3 ngc3627 727 [CII] 157.7 2.4 1576.9 0.3 7.1 1076.7 0.7 ngc3627 727 [OI] 63.2 1.3 1047.2 2.3 7.1 1076.7 0.7 ngc5033 875 [CII] 157.7 2.4 1576.9 0.4 4.1 519.9 0.8