J/ApJS/125/349      Morphology of 12micron Seyfert Galaxies  (Hunt+, 1999)

Morphology of the 12 Micron Seyfert Galaxies. II. Optical and Near-Infrared Image Atlas Hunt L. K., Malkan M. A., Rush B., Bicay M. D., Nelson B. O., Stanga R. M., Webb W. <Astrophys. J. Suppl. Ser. 125, 349 (1999)> =1999ApJS..125..349H 1999ApJS..125..349H
ADC_Keywords: Atlases; Galaxies, Seyfert; Photometry, infrared Keywords: atlases-infrared: galaxies-galaxies: photometry-galaxies: Seyfert-galaxies: structure Abstract: We present 263 optical and near-infrared (NIR) images for 42 1s and 48 Seyfert 2s, selected from the Extended 12µm Galaxy Sample. Elliptically averaged profiles are derived from the images, and isophotal radii and magnitudes are calculated from these. We also report virtual aperture photometry that, judging from comparison with previous work, is accurate to roughly 0.05 mag in the optical, and 0.07 mag in the NIR. Our B-band isophotal magnitude and radii, obtained from ellipse fitting, are in good agreement with those of Third Reference Catalogue of Bright Galaxies. When compared with the B band, V, I, J, and K isophotal diameters show that the colors in the outer regions of Seyfert galaxies are consistent with the colors of normal spirals. Differences in the integrated isophotal colors and comparison with a simple model show that the active nucleus+bulge are stronger and redder in the NIR than in the optical. Finally, roughly estimated Seyfert disk surface brightnesses are significantly brighter in B and K than those in normal spirals of similar morphological type. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 109 263 Morphology Seyferts at 12 microns -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- SType Seyfert type 5- 17 A13 --- Name Source name 19 A1 --- n_Name Profile extraction note (1) 21- 29 A9 --- Oname Other name 31- 50 A20 --- Mtype Morphological type (from NED & RC3) 52- 57 F6.4 --- z Redshift (from NED) 60 A1 --- Filt Filter 63- 67 F5.2 mag Dia10 Aperture photometry 10'' diameter in Filt 69- 73 F5.2 mag Dia20 Aperture photometry 20'' diameter in Filt 75- 79 F5.2 mag Dia30 Aperture photometry 30'' diameter in Filt 81- 85 F5.2 mag IntMag Integrated isophotal magnitude 88 A1 --- n_IntMag Indicates that the radius used in calculation is extrapolated, not interpolated 90- 94 F5.1 arcsec Radius Isophotal radius (2) 96 A1 --- n_Radius Note indicating that the radius used is extrapolated, not interpolated 99-102 F4.1 mag/arcsec2 SurfB Central surface brightness fit by an exponential to the outer profile 104 A1 --- n_SurfB Note indicating that the radius used in calculation is extrapolated, not interpolated 107-109 A3 --- Code Observing run code (3) -------------------------------------------------------------------------------- Note (1): Sources for which B and V profiles extracted with I- or J-band ellipse parameters. Note (2): B evaluated at 25 mag.arcsec-2 V evaluated at 24 mag.arcsec-2 I evaluated at 23 mag.arcsec-2 J evaluated at 22 mag.arcsec-2 H evaluated at 21.5 mag.arcsec-2 K evaluated at 21 mag.arcsec-2 Note (3): See Col.7 of Table 1. An ``X'' signifies images that were not acquired in the context of an observing run. J and K images for NGC 2639 were taken at Palomar, and for NGC 3227 at Mt. Hopkins. -------------------------------------------------------------------------------- History: From ApJ electronic edition
(End) Greg Schwarz (AAS), 26-Jan-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line