Title: Host Galaxy Properties of the Swift BAT Ultra Hard X-ray Selected AGN Authors: Koss M., Mushotzky R., Veilleux S., Winter L.M., Baumgartner W., Tueller J., Gehrels N., Valencic L. Table: Summary of Morphological Properties ================================================================================ Byte-by-byte Description of file: apj399721t6_mrt.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 23 A23 --- Name Galaxy name 25- 30 F6.2 arcsec Rp ? Petrosian radius (1) 32- 35 F4.2 --- C ? Concentration index (2) 37- 39 A3 --- Class Galaxy Zoo class (3) 41- 44 F4.2 --- b/a Observed axial ratio (4) 46 A1 --- Broad Broad-line AGN? (5) -------------------------------------------------------------------------------- Note (1): The Petrosian radius was determined following the SDSS see http:// www.sdss.org/dr7/algorithms/photometry.html. Blank values indicate that the Petrosian radius and concentration failed to converge. This happened more often for close mergers or in a broad-line AGN where the AGN was imperfectly subtracted. Note (2): The concentration index is defined as the ratio of the radii containing 90 and 50 per cent of the Petrosian r-band galaxy light. Blank values indicate that the Petrosian radius and concentration failed to converge. This happened more often for close mergers or in a broad-line AGN where the AGN was imperfectly subtracted. Note (3): Where E stands for ellipticals, I, for intermediates, S, for spirals, and M for mergers/peculiars. For the Kitt Peak data, which has no Galaxy Zoo data, we use the Hubble Types from the RC3 with T = -6 to -4 corresponding to ellipticals, T = -3 to 0 to intermediates, T > 0 to spirals. Note (4): We use b/a as a proxy for inclination. An b/a = 1 corresponds to a face-on galaxy. We use the g band and fit to the 25th mag/arcsecond^2^ isophote. Note (5): Whether the galaxy has a broad-line AGN based on SDSS galaxy class or the available optical spectra. While we excluded these broad-line measurements from the morphological analysis, we have provided them for completeness. We subtracted the AGN model for these galaxies before determining the Petrosian radius and concentration index. However, the difficulty of perfectly subtracting the AGN light distribution makes these values more uncertain. -------------------------------------------------------------------------------- 2MASX J00253292+6821442 M 0.43 2MASX J01064523+0638015 12.8 3.1 S 0.8 2MASX J03534246+3714077 8.66 3.03 I 0.56 2MASX J04440903+2813003 30.8 2.92 I 0.91 2MASX J05054575-2351139 7.14 3.37 I 0.87 2MASX J06411806+3249313 9.11 2.93 M 0.82 2MASX J07595347+2323241 15.7 2.8 S 0.49 2MASX J09112999+4528060 9.22 2.9 I 0.7 2MASX J12005792+0648226 17.9 3.3 I 0.55 2MASX J16174158+0607100 9.53 2.83 S 0.25 2MFGC 02280 15.4 2.99 S 0.21 ARK 347 11.2 3.26 I 0.6 ARP 102B 12.1 3.55 E 0.79 CGCG 102-048 10.5 3.04 S 0.36 CGCG 300-062 14. 2.73 S 0.77 CGCG 312-012 8.52 3.04 E 0.95 CGCG 420-015 13.7 3.27 E 0.77 CGCG 427-028 14.6 2.58 I 0.22 ESO 506-G027 44.9 3.74 S 0.31 FAIRALL 272 18.6 3.21 M 0.61 IC 0486 17.5 3.04 S 0.65 IC 0751 16.9 2.85 S 0.28 IC 2461 29.2 3. S 0.22 IC 2515 16.6 3.42 S 0.22 LEDA 170194 16.7 2.66 S 0.9 LEDA 214543 10.6 3.13 I 0.87 M106 216. 3.01 S 0.38 MCG -01-05-047 66.1 2.87 S 0.13 MCG -01-24-012 27.9 2.75 S 0.56 MCG -01-40-001 39.6 2.65 S 0.34 MCG -02-08-014 11.9 3.09 S 0.16 MCG -02-12-050 24.1 2.88 M/S 0.89 MCG -05-14-012 15.6 3.39 M/I 0.86 MCG -05-23-016 15.4 3.26 I 0.45 MCG +02-21-013 22. 2.65 I 0.43 MCG +04-48-002 20.8 2.73 M/S 0.36 MCG +05-28-032 12.9 2.88 S 0.51 MCG +06-24-008 17. 2.44 S 0.26 MCG +06-49-019 18.4 3.18 S 0.64 MCG +11-11-032 11.8 3.02 S 0.45 MCG+10-17-061 8.52 2.67 I 0.92 Mrk 1210 15.6 2.93 E 0.86 Mrk 18 8.5 3.15 I 0.15 Mrk 198 7.71 3.31 S 0.86 Mrk 268 12.8 3.31 I 0.45 Mrk 348 55. 3.19 S 0.97 Mrk 417 9.1 3.18 E 0.77 Mrk 463E 12.6 2.24 M 0.41 Mrk 477 6.19 2.56 M 0.71 Mrk 732 16.5 3.17 I 0.87 Mrk 78 I 0.61 NGC 0835 24.3 2.99 M/S 0.45 NGC 1012 47.8 2.57 S 0.51 NGC 1052 44. 3.06 E 0.56 NGC 1142 28. 2.87 M 0.48 NGC 1194 35.8 3.22 I 0.47 NGC 1275 52.1 3.02 M 0.74 NGC 2110 53.9 3.35 E 0.74 NGC 235A 11.5 3.09 M 0.52 NGC 2992 41.4 3.09 M 0.3 NGC 3079 119. 3.12 S 0.15 NGC 3081 41.8 2.69 S 0.77 NGC 3281 70.4 2.21 S 0.5 NGC 3718 106. 2.65 S 0.42 NGC 4102 51.8 2.6 S 0.41 NGC 4388 81.7 3.13 S 0.18 NGC 452 23.6 2.94 S 0.28 NGC 4686 21.4 3.47 I 0.29 NGC 4992 19.8 2.62 I 0.57 NGC 5106 14.2 2.87 M/S 0.69 NGC 513 13.9 2.27 M/S 0.51 NGC 5231 26. 2.44 S 0.51 NGC 5252 25.1 3.2 I 0.56 NGC 5290 53.4 2.86 S 0.27 NGC 5506 56.2 2.3 I 0.23 NGC 5610 26.5 2.32 S 0.33 NGC 5728 82.3 2.58 S 0.57 NGC 5899 57. 2.6 S 0.43 NGC 5995 21.1 3.43 I 0.32 NGC 6240 36.5 2.95 M 0.51 NGC 7319 M/S 0.55 NGC 7682 37.1 2.78 S 0.89 NGC 788 31.7 3.01 S 0.75 NGC 973 S 0.14 UGC 02724 40.8 1.87 S 0.65 UGC 03995A 45.2 2.37 S 0.44 UGC 05881 10.6 3.19 S 0.38 UGC 06527 NED03 7. 3.65 M/S 0.32 UGC 07064 20.7 2.56 S 0.88 UGC 08327 NED02 18. 3.94 M/S 0.62 UGC 11185 NED02 M/S 0.96 UGC 12741 13.6 3.18 S 0.28 2MASX J09043699+5536025 4.74 3.56 M 0.61 Y 2MASX J21355399+4728217 S 0.18 Y ARP 151 4.94 3.15 M 0.16 Y CGCG 031-072 10.5 3.04 I 0.59 Y CGCG 046-033 11.3 2.5 S 0.75 Y CGCG 122-055 12.9 2.97 I 0.75 Y CGCG 198-020 20.6 2.45 I 0.71 Y CGCG 319-007 12.2 2.68 I 0.61 Y ESO 490-IG026 28.9 3.59 M 0.68 Y ESO 511-G030 75. 3.34 S 0.7 Y IC 4329A S 0.27 Y KAZ 320 2.68 2.76 I 0.79 Y KUG 1141+371 12.2 2.67 I 0.87 Y KUG 1208+386 11.9 3.26 E 0.94 Y MCG -01-13-025 16.8 3.19 E 0.61 Y MCG -03-34-064 11.2 3.37 E 0.81 Y MCG +01-57-016 7.12 3.78 S 0.86 Y MCG +04-06-043 13.9 2.91 S 0.92 Y MCG +04-22-042 15.2 2.92 S 0.56 Y MCG +08-11-011 1.36 2.47 S 0.7 Y Mrk 10 31.8 2.64 S 0.41 Y Mrk 1018 11.1 3.72 M 0.52 Y Mrk 110 4.64 3.68 M 0.62 Y Mrk 1392 18.4 3.04 S 0.51 Y Mrk 1469 8.82 3.26 I 0.35 Y Mrk 279 19. 2.73 M/S 0.58 Y Mrk 352 I 0.83 Y Mrk 464 2.6 3.23 I 0.76 Y Mrk 50 8.03 2.94 E 0.6 Y Mrk 520 15. 3.63 S 0.62 Y Mrk 590 29.3 2.92 M/S 0.97 Y Mrk 595 7.2 3.24 M/E 0.62 Y Mrk 705 5.14 3.5 I 0.88 Y Mrk 728 7.08 3.08 E 0.64 Y Mrk 739E 14.2 2.18 M/S 0.87 Y Mrk 766 20.4 2.78 S 0.78 Y Mrk 79 39.4 2.49 S 0.9 Y Mrk 817 9.04 3.42 S 0.87 Y Mrk 915 14.7 2.97 S 0.35 Y Mrk 926 18.8 2.87 S 0.82 Y NGC 2885 13.1 3. S 0.69 Y NGC 3227 81. 2.52 M/S 0.56 Y NGC 3516 E 0.77 Y NGC 3786 38.4 2.68 M/S 0.59 Y NGC 4051 S 0.68 Y NGC 4138 41.3 2.59 S 0.65 Y NGC 4235 48.2 3.29 S 0.22 Y NGC 4395 S 0.83 Y NGC 4593 92.1 2.38 S 0.74 Y NGC 5273 58.2 2.26 I 0.92 Y NGC 5548 36. 3.25 S 0.87 Y NGC 5674 31.1 1.7 S 0.92 Y NGC 5683 8.35 3.23 I 0.52 Y NGC 5940 22. 2.11 S 0.98 Y NGC 6814 76.2 2.31 S 0.93 Y NGC 7314 92.1 2.38 S 0.45 Y NGC 7469 17. 3.29 M/S 0.72 Y NGC 7603 2.21 2.78 M/S 0.65 Y NGC 7679 17. 3.29 S 0.64 Y NGC 931 48.6 3.45 M/S 0.21 Y NGC 985 22.1 3.2 M 0.71 Y SBS 1301+540 5.93 3.11 S 0.42 Y UGC 03142 28.8 2. S 0.78 Y UGC 03601 13.4 3.02 I 0.74 Y UGC 12282 34.3 3.08 I 0.27 Y UM 614 4.9 3.44 I 0.51 Y VII Zw 073 7.36 2.58 S 0.91 Y