J/ApJ/703/1569  Radial distribution in SINGS galaxies. I.  (Munoz-Mateos+, 2009)

Radial distribution of stars, gas, and dust in SINGS galaxies. I. Surface photometry and morphology. Munoz-Mateos J.C., Gil de Paz A., Zamorano J., Boissier S., Dale D.A., Perez-Gonzalez P.G., Gallego J., Madore B.F., Bendo G., Boselli A., Buat V., Calzetti D., Moustakas J., Kennicutt R.C. <Astrophys. J., 703, 1569-1596 (2009)> =2009ApJ...703.1569M 2009ApJ...703.1569M
ADC_Keywords: Galaxies, nearby ; Photometry, UBVRI ; Photometry, SDSS ; Photometry, infrared ; Photometry, ultraviolet ; Morphology Keywords: atlases - galaxies: fundamental parameters - galaxies: photometry - galaxies: structure Abstract: We present ultraviolet through far-infrared (FIR) surface brightness profiles for the 75 galaxies in the Spitzer Infrared Nearby Galaxies Survey (SINGS). The imagery used to measure the profiles includes Galaxy Evolution Explorer UV data, optical images from Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and Sloan Digital Sky Survey, near-IR data from Two Micron All Sky Survey, and mid- and FIR images from Spitzer. Along with the radial profiles, we also provide multi-wavelength asymptotic magnitudes and several nonparametric indicators of galaxy morphology: the concentration index (C42), the asymmetry (A), the Gini coefficient (G), and the normalized second-order moment of the brightest 20% of the galaxy's flux ({overline}M20). In this paper, the first of a series, we describe the technical aspects regarding the surface photometry, and present a basic analysis of the global and structural properties of the SINGS galaxies at different wavelengths. Description: The SINGS sample (Kennicutt et al. 2003PASP..115..928K 2003PASP..115..928K) consists of 75 nearby galaxies selected to cover the range in morphological-type, luminosity and FIR/optical luminosity observed in the local universe. The GALEX mission has observed nearly all SINGS galaxies in the FUV and the near-UV. Optical images for the SINGS galaxies were taken at the Kitt Peak National Observatory (KPNO) 2.1m telescope and the Cerro Tololo Inter-American Observatory (CTIO) 1.5m telescope, using Harris BVRI filters. We finally opted for using images from the Sloan Digital Sky Survey (SDSS-DR6; Adelman-McCarthy et al. 2008, Cat. II/282; superseded by II/294) for as many galaxies as possible. Since the SINGS galaxies are too large to fit into a single Two Micron All Sky Survey (2MASS) scan, the corresponding mosaics were retrieved from the 2MASS Large Galaxy Atlas (LGA; Jarrett et al. 2003AJ....125..525J 2003AJ....125..525J). Mid-IR images at 3.6, 4.5, 5.8, and 8.0um were obtained using the Infrared Array Camera (IRAC) on board Spitzer and MIPS for 24, 70 and 160um. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 93 75 Sample table2.dat 120 2206 UV, optical and NIR surface photometry profiles table3.dat 128 2161 UV, optical (SDSS) and NIR photometry profiles table4.dat 98 4319 IRAC and MIPS surface photometry table5.dat 130 43 UV, optical, and near-IR asymptotic magnitudes for SINGS galaxies lacking SDSS data table6.dat 138 32 UV, optical (SDSS), and near-IR asymptotic magnitudes table7.dat 102 75 IRAC and MIPS asymptotic magnitudes table8.dat 209 300 Non-parametrical morphological estimators -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) J/ApJS/190/233 : Spectroscopy and abundances of SINGS galaxies (Moustakas+, 2010) J/ApJ/701/1965 : Radial dust properties of SINGS galaxies (Munoz-Mateos+, 2009) J/ApJS/173/185 : GALEX ultraviolet atlas of nearby galaxies (Gil de Paz+, 2007) J/ApJ/669/959 : Warm molecular hydrogen in SINGS galaxies (Roussel+, 2007) J/ApJ/630/784 : UBVR observations of nearby galaxies (Taylor+, 2005) J/ApJS/156/345 : Surface photometry of BCD galaxies (Gil De Paz+, 2005) J/ApJS/126/271 : Surface photometry of nearby field galaxies (Jansen+ 2000) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Galaxy name 12 A1 --- f_Name [d] Flag for NGC 5194 (1) 14- 15 I2 h RAh Hour of right ascension (J2000) 17- 18 I2 min RAm Minute of right ascension (J2000) 20- 23 F4.1 s RAs Second of right ascension (J2000) 25 A1 --- DE- Sign of declination (J2000) 26- 27 I2 deg DEd Degree of declination (J2000) 29- 30 I2 arcmin DEm Arcminute of declination (J2000) 32- 35 F4.1 arcsec DEs Arcsecond of declination (J2000) 37- 40 F4.1 arcmin 2a Apparent major isophotal diameter (2) 42- 45 F4.1 arcmin 2b Apparent minor isophotal diameter (2) 47- 49 I3 deg PA [0,360] Position angle from RC3 51- 55 F5.3 mag E(B-V) Galactic color excess from Schlegel et al. (1998) 57- 61 F5.2 Mpc Dist Distance to the galaxy (3) 63- 66 F4.1 --- TType RC3 morphological type T 68- 82 A15 --- MType RC3 full description of the morphological type 84- 88 A5 --- Opt Optical data used for each galaxy (4) 90- 92 I3 arcsec rP ? Petrosian radius (5) 93 A1 --- f_rP [B] B if B-band images used for rP (5) -------------------------------------------------------------------------------- Note (1): d = The P.A. and axis ratio for NGC 5194 differ from those in the RC3, which are affected by the presence of NGC 5195. Note (2): Apparent major and minor isophotal diameters at µB=25mag/arcsec2 from the RC3 catalog. Note (3): Distance to the galaxy, rounded to the nearest Mpc when larger than 10Mpc, taken from Gil de Paz et al. (2007, Cat. J/ApJS/173/185) and Kennicutt et al. (2003PASP..115..928K 2003PASP..115..928K). Note (4): Optical data from the SDSS or recalibrated with compiled aperture photometry ("recal", see Section 2.2 and Appendix A). Galaxies lacking any label in this column have optical images with unreliable zero points. Neither surface brightness profiles nor asymptotic magnitudes are provided for these galaxies in the optical bands. However, we do provide morphological estimators, since they are not affected by zero-point errors. Note (5): Petrosian radius at η=0.2, measured on the 3.6um images (except for a few galaxies where no meaningful solution was found, and the B-band images were used instead). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Galaxy name 13- 16 I4 arcsec Arad Angular radius along semimajor axis 18- 21 F4.1 kpc Lrad Physical radius along semimajor axis 23- 27 F5.2 mag/arcsec2 FUV ? FUV 0.153 micron surface brightness (1) 29- 32 F4.2 mag/arcsec2 e_FUV ? Uncertainty in FUV (1) 34- 38 F5.2 mag/arcsec2 NUV ? NUV 0.227 micron surface brightness (1) 40- 43 F4.2 mag/arcsec2 e_NUV ? Uncertainty in NUV (1) 45- 49 F5.2 mag/arcsec2 B ? B (0.45 micron) band surface brightness (1) 51- 54 F4.2 mag/arcsec2 e_B ? Uncertainty in B (1) 56- 60 F5.2 mag/arcsec2 V ? V (0.55 micron) band surface brightness (1) 62- 65 F4.2 mag/arcsec2 e_V ? Uncertainty in V (1) 67- 71 F5.2 mag/arcsec2 R ? R (0.66 micron) band surface brightness (1) 73- 76 F4.2 mag/arcsec2 e_R ? Uncertainty in R (1) 78- 82 F5.2 mag/arcsec2 I ? I (0.81 micron) band surface brightness (1) 84- 87 F4.2 mag/arcsec2 e_I ? Uncertainty in I (1) 89- 93 F5.2 mag/arcsec2 J ? J (1.25 micron) band surface brightness (1) 95- 98 F4.2 mag/arcsec2 e_J ? Uncertainty in J (1) 100-104 F5.2 mag/arcsec2 H ? H (1.65 micron) band surface brightness (1) 106-109 F4.2 mag/arcsec2 e_H ? Uncertainty in H (1) 111-115 F5.2 mag/arcsec2 Ks ? Ks (2.17 micron) band surface brightness (1) 117-120 F4.2 mag/arcsec2 e_Ks ? Uncertainty in Ks (1) -------------------------------------------------------------------------------- Note (1): Expressed in AB magnitudes and corrected for foreground galactic extinction. The quoted uncertainties include photometric and sky errors, but not zero-point errors (see Section 3.2 for details). The optical values have been recalibrated to correct zero-point offsets present in the original data (see Appendix A). Again, the errors quoted here do not include the uncertainty resulting from the recalibration procedure. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Galaxy name 10- 13 I4 arcsec Arad Angular radius along semimajor axis 15- 18 F4.1 kpc Lrad Physical radius along semimajor axis 20- 24 F5.2 mag/arcsec2 FUV ? FUV 0.153 micron surface brightness (1) 26- 29 F4.2 mag/arcsec2 e_FUV ? Uncertainty in FUV (1) 31- 35 F5.2 mag/arcsec2 NUV ? NUV 0.227 micron surface brightness (1) 37- 40 F4.2 mag/arcsec2 e_NUV ? Uncertainty in NUV (1) 42- 46 F5.2 mag/arcsec2 u ? u (0.354 micron) band surface brightness (1) 48- 51 F4.2 mag/arcsec2 e_u ? Uncertainty in u (1) 53- 57 F5.2 mag/arcsec2 g ? g (0.477 micron) band surface brightness (1) 59- 62 F4.2 mag/arcsec2 e_g ? Uncertainty in g (1) 64- 68 F5.2 mag/arcsec2 r ? r (0.623 micron) band surface brightness (1) 70- 73 F4.2 mag/arcsec2 e_r ? Uncertainty in r (1) 75- 79 F5.2 mag/arcsec2 i ? i (0.762 micron) band surface brightness (1) 81- 84 F4.2 mag/arcsec2 e_i ? Uncertainty in i (1) 86- 90 F5.2 mag/arcsec2 z ? z (0.913 micron) band surface brightness (1) 92- 95 F4.2 mag/arcsec2 e_z ? Uncertainty in z (1) 97-101 F5.2 mag/arcsec2 J ? J (1.25 micron) band surface brightness (1) 103-106 F4.2 mag/arcsec2 e_J ? Uncertainty in J (1) 108-112 F5.2 mag/arcsec2 H ? H (1.65 micron) band surface brightness (1) 114-117 F4.2 mag/arcsec2 e_H ? Uncertainty in H (1) 119-123 F5.2 mag/arcsec2 Ks ? Ks (2.17 micron) band surface brightness (1) 125-128 F4.2 mag/arcsec2 e_Ks ? Uncertainty in Ks (1) -------------------------------------------------------------------------------- Note (1): Expressed in AB magnitudes. All values are corrected for foreground galactic extinction. The quoted uncertainties include photometric and sky errors, but not zero-point errors (see Section 3.2 for details). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Galaxy name 13- 16 I4 arcsec Arad Angular radius along semimajor axis 18- 21 F4.1 kpc Lrad Physical radius along semimajor axis 23- 27 F5.2 [Jy/arcsec2] I3.6 ? Log 3.6 micron band surface brightness (1) 29- 32 F4.2 [Jy/arcsec2] e_I3.6 ? Uncertainty in I3.6 (1) 34- 38 F5.2 [Jy/arcsec2] I4.5 ? Log 4.5 micron band surface brightness (1) 40- 43 F4.2 [Jy/arcsec2] e_I4.5 ? Uncertainty in I4.5 (1) 45- 49 F5.2 [Jy/arcsec2] I5.8 ? Log 5.8 micron band surface brightness (1) 51- 54 F4.2 [Jy/arcsec2] e_I5.8 ? Uncertainty in I5.8 (1) 56- 60 F5.2 [Jy/arcsec2] I8.0 ? Log 8.0 micron band surface brightness (1) 62- 65 F4.2 [Jy/arcsec2] e_I8.0 ? Uncertainty in I8.0 (1) 67- 71 F5.2 [Jy/arcsec2] I24 ? Log 24 micron band surface brightness (1) 73- 76 F4.2 [Jy/arcsec2] e_I24 ? Uncertainty in I24 (1) 78- 82 F5.2 [Jy/arcsec2] I70 ? Log 70 micron band surface brightness (1) 84- 87 F4.2 [Jy/arcsec2] e_I70 ? Uncertainty in I70 (1) 89- 93 F5.2 [Jy/arcsec2] I160 ? Log 160 micron band surface brightness (1) 95- 98 F4.2 [Jy/arcsec2] e_I160 ? Uncertainty in I160 (1) -------------------------------------------------------------------------------- Note (1): All values are corrected for foreground galactic extinction. The quoted uncertainties include photometric and sky errors, but not zero-point errors (see Section 3.2 for details). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- n_Name [R]? R: galaxies with recalibrated optical data 3- 13 A11 --- Name Galaxy name 15- 20 F6.3 mag FUV ? GALEX FUV 0.153um-band AB magnitude (1) 22- 26 F5.3 mag e_FUV ? FUV uncertainty (1) 28- 33 F6.3 mag NUV ? GALEX NUV 0.227um-band AB magnitude (1) 35- 39 F5.3 mag e_NUV ? NUV uncertainty (1) 41- 46 F6.3 mag Bmag ? B-band 0.45um AB magnitude (1) 48- 52 F5.3 mag e_Bmag ? Bmag uncertainty (1) 54- 59 F6.3 mag Vmag ? V-band 0.55um AB magnitude (1) 61- 65 F5.3 mag e_Vmag ? Vmag uncertainty (1) 67- 72 F6.3 mag Rmag ? R-band 0.66um AB magnitude (1) 74- 78 F5.3 mag e_Rmag ? Rmag uncertainty (1) 80- 85 F6.3 mag Imag ? I-band 0.81um AB magnitude (1) 87- 91 F5.3 mag e_Imag ? Imag uncertainty (1) 93- 98 F6.3 mag Jmag ? 2MASS J-band 1.25um AB magnitude (1) 100-104 F5.3 mag e_Jmag ? Jmag uncertainty (1) 106-111 F6.3 mag Hmag ? 2MASS H-band 1.65um AB magnitude (1) 113-117 F5.3 mag e_Hmag ? Hmag uncertainty (1) 119-124 F6.3 mag Ksmag ? 2MASS Ks-band 2.17um AB magnitude (1) 126-130 F5.3 mag e_Ksmag ? Ksmag uncertainty (1) -------------------------------------------------------------------------------- Note (1): All values are in AB magnitudes and corrected for foreground galactic extinction. The quoted uncertainties are just the statistical errors resulting from the fit applied to the growth curve, but do not include zero-point errors (see Section 4.1 for details). The optical values (Columns 5-8) have been recalibrated to correct zero-point offsets present in the original data (see Section A). Again, the errors quoted here do not include the uncertainty resulting from the recalibration procedure. -------------------------------------------------------------------------------- Byte-by-byte Description of file:table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Galaxy name 10- 15 F6.3 mag FUV ? GALEX FUV 0.153um-band AB magnitude (1) 17- 21 F5.3 mag e_FUV ? FUV uncertainty (1) 23- 28 F6.3 mag NUV GALEX NUV 0.227um-band AB magnitude (1) 30- 34 F5.3 mag e_NUV NUV uncertainty (1) 36- 41 F6.3 mag umag SDSS u-band 0.354um AB magnitude (1) 43- 47 F5.3 mag e_umag umag uncertainty (1) 49- 54 F6.3 mag gmag SDSS g-band 0.477um AB magnitude (1) 56- 60 F5.3 mag e_gmag gmag uncertainty (1) 62- 67 F6.3 mag rmag SDSS r-band 0.623um AB magnitude (1) 69- 73 F5.3 mag e_rmag rmag uncertainty (1) 75- 80 F6.3 mag imag SDSS i-band 0.762um AB magnitude (1) 82- 86 F5.3 mag e_imag imag uncertainty (1) 88- 93 F6.3 mag zmag ? SDSS z-band 0.913um AB magnitude (1) 95- 99 F5.3 mag e_zmag ? zmag uncertainty (1) 101-106 F6.3 mag Jmag 2MASS J-band 1.25um AB magnitude (1) 108-112 F5.3 mag e_Jmag Jmag uncertainty (1) 114-119 F6.3 mag Hmag 2MASS H-band 1.65um AB magnitude (1) 121-125 F5.3 mag e_Hmag Hmag uncertainty (1) 127-132 F6.3 mag Ksmag 2MASS Ks-band 2.17um AB magnitude (1) 134-138 F5.3 mag e_Ksmag Ksmag uncertainty (1) -------------------------------------------------------------------------------- Note (1): All values are in AB magnitudes and are corrected for foreground galactic extinction. The quoted uncertainties are just the statistical errors resulting from the fit applied to the growth curve, but do not include zero-point errors (see Section 4.1 for details). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Galaxy name 13- 18 F6.3 [Jy] logF3.6 ? Spiter/IRAC 3.6um flux density (1) 20- 24 F5.3 [Jy] e_logF3.6 ? logF3.6 uncertainty (1) 26- 31 F6.3 [Jy] logF4.5 ? Spiter/IRAC 4.5um flux density (1) 33- 37 F5.3 [Jy] e_logF4.5 ? logF4.5 uncertainty (1) 39- 44 F6.3 [Jy] logF5.8 ? Spiter/IRAC 5.8um flux density (1) 46- 50 F5.3 [Jy] e_logF5.8 ? logF5.8 uncertainty (1) 52- 57 F6.3 [Jy] logF8.0 ? Spiter/IRAC 8.0um flux density (1) 59- 63 F5.3 [Jy] e_logF8.0 ? logF8.0 uncertainty (1) 65- 70 F6.3 [Jy] logF24 ? Spiter/MIPS 24um flux density (1) 72- 76 F5.3 [Jy] e_logF24 ? logF24 uncertainty (1) 78- 83 F6.3 [Jy] logF70 ? Spiter/MIPS 70um flux density (1) 85- 89 F5.3 [Jy] e_logF70 ? logF70 uncertainty (1) 91- 96 F6.3 [Jy] logF160 ? Spiter/MIPS 160um flux density (1) 98-102 F5.3 [Jy] e_logF160 ? logF160 uncertainty (1) -------------------------------------------------------------------------------- Note (1): All values are in Jy, and are corrected for foreground galactic extinction. The quoted uncertainties are just the statistical errors resulting from the fit applied to the growth curve, but do not include zero-point errors (see Section 4.1 for details). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Galaxy name 17- 21 A5 --- Param Morphological parameter (1) 23 A1 --- l_FUV Limit flag on FUV (2) 24- 30 F7.3 --- FUV ? Param value in the FUV band 31 A1 --- u_FUV Uncertainty flag on FUV (3) 33 A1 --- l_NUV Limit flag on NUV (2) 34- 40 F7.3 --- NUV ? Param value in the NUV band 41 A1 --- u_NUV Uncertainty flag on NUV (3) 43 A1 --- l_B Limit flag on B (2) 44- 50 F7.3 --- B ? Param value in the B band 52 A1 --- l_V Limit flag on V (2) 53- 59 F7.3 --- V ? Param value in the V band 61 A1 --- l_R Limit flag on R (2) 62- 68 F7.3 --- R ? Param value in the R band 70 A1 --- l_I Limit flag on I (2) 71- 77 F7.3 --- I ? Param value in the I band 79 A1 --- l_u Limit flag on u (2) 80- 86 F7.3 --- u ? Param value in the u band 88- 93 F6.3 --- g ? Param value in the g band 95-100 F6.3 --- r ? Param value in the r band 102-107 F6.3 --- i ? Param value in the i band 109-114 F6.3 --- z ? Param value in the z band 116 A1 --- l_J Limit flag on J (2) 117-123 F7.3 --- J ? Param value in the J band 125 A1 --- l_H Limit flag on H (2) 126-132 F7.3 --- H ? Param value in the H band 134 A1 --- l_Ks Limit flag on Ks (2) 135-141 F7.3 --- Ks ? Param value in the Ks 143 A1 --- l_3.6 Limit flag on 3.6 (2) 144-150 F7.3 --- 3.6 ? Param value in the 3.6 micron band 152 A1 --- l_4.5 Limit flag on 4.5 (2) 153-159 F7.3 --- 4.5 ? Param value in the 4.5 micron band 161 A1 --- l_5.8 Limit flag on 5.8 (2) 162-168 F7.3 --- 5.8 ? Param value in the 5.8 micron band 170 A1 --- l_8.0 Limit flag on 8.0 (2) 171-177 F7.3 --- 8.0 ? Param value in the 8.0 micron band 179 A1 --- l_24 Limit flag on 24 (2) 180-186 F7.3 --- 24 ? Param value in the 24 micron band 187 A1 --- u_24 Uncertainty flag in 24 (3) 189 A1 --- l_70 Limit flag on 70 (2) 190-198 F9.3 --- 70 ? Param value in the 70 micron band 199 A1 --- u_70 Uncertainty flag in 70 (3) 201 A1 --- l_160 Limit flag on 160 (2) 202-208 F7.3 --- 160 ? Param value in the 160 micron band 209 A1 --- u_160 Uncertainty flag in 160 (3) -------------------------------------------------------------------------------- Note (1): The information for each galaxy is spread over 4 consecutive rows: the Concentration index (C42), asymmetry (A), Gini coefficient (G) and normalized second-order moment of the brightest 20% to the total galaxy flux (M20) at different wavelengths, respectively. Note (2): When the inner radius r20 needed to compute C42 is smaller than the innermost point in our profiles (or the PSF size, in the case of the 70 micron and 160 micron bands), the quoted values are just lower limits for the actual concentration indices. Note (3): : = Take with caution since at the particular distance of each galaxy, the FWHM of the PSF of the affected bands does not allow resolving structures smaller than 0.5kpc. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Munoz-Mateos et al. Paper II. 2009ApJ...701.1965M 2009ApJ...701.1965M Cat. J/ApJ/701/1965 Munoz-Mateos et al. Paper III. 2011ApJ...731...10M 2011ApJ...731...10M
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 26-Sep-2011
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