J/A+A/542/A39    NIR photometry in 10 nearby spiral galaxies   (Grosboel+, 2012)

Star formation in grand-design, spiral galaxies. Young, massive clusters in NIR. Grosbol P., Dottori H. <Astron. Astrophys. 542, A39 (2012)> =2012A&A...542A..39G 2012A&A...542A..39G
ADC_Keywords: Galaxies, nearby ; Clusters, open ; Photometry, infrared Keywords: galaxies: spiral - galaxies: structure - galaxies: star clusters: general - galaxies: star formation - infrared: galaxies - techniques: photometry Abstract: Spiral structure is a prominent feature in many disk galaxies and is often outlined by bright, young objects. We study the distribution of young stellar clusters in grand-design spiral galaxies and thereby determine whether strong spiral perturbations can influence star formation. Description: Near-infrared (NIR) aperture photometry of sources in 7 arcmin fields around 10 nearby, grand-design spiral galaxies is presented based on HAWK-I/VLT observations. The sources were identified using Sextractor (Bertin & Amouts, 1996A&AS..117..393B 1996A&AS..117..393B) and measured with an aperture of 1 arcsec diameter. The sources numbers are those of the original Sextractor search on the Ks maps and are not strictly sequential. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 89 10 List of galaxies n0157c.dat 133 2254 NIR sources in NGC 157 with Ks<20.2mag n1232c.dat 133 3177 NIR sources in NGC 1232 with Ks<20.6mag n1300c.dat 133 614 NIR sources in NGC 1300 with Ks<19.8mag n1365c.dat 133 2417 NIR sources in NGC 1365 with Ks<20.2mag n1566c.dat 133 969 NIR sources in NGC 1566 with Ks<19.3mag n2997c.dat 152 5313 NIR sources in NGC 2997 with Ks<20.1mag n4030c.dat 133 1196 NIR sources in NGC 4030 with Ks<19.7mag n4321c.dat 133 1184 NIR sources in NGC 4321 with Ks<19.3mag n5247c.dat 133 2259 NIR sources in NGC 5247 with Ks<19.8mag n7424c.dat 113 6137 NIR sources in NGC 7424 with Ks<20.8mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- --- [NGC] 5- 8 I04 --- NGC Galaxy NGC number 10- 19 A10 --- MType Morphological Hubble type of galaxy 21- 27 A7 --- Band Observed bands (Brg for Brγ) 29- 32 F4.2 arcsec FWHM Seeing in the final, stacked K-band image expressed as the full-width at half-maximum 34- 37 F4.1 mag/pix mu5 Ks surface brightness for which a signal-to-noise ratio of five was reached 39- 43 F5.2 mag MOD Distance modulus (m-M) 45- 48 F4.1 Mpc Dist Distance 50- 51 I2 pc Ds Linear resolution corresponding to distance 53- 55 I3 deg PA position angle adopted for the galaxy 56 A1 --- r_PA Reference for PA (1) 58- 59 I2 deg IA Inclination angle adopted for the galaxy 60 A1 --- r_IA Reference for IA (1) 62- 66 F5.2 mag Klim Limiting K magnitude to a completeness of ∼90% 68- 72 F5.2 mag Hlim Limiting H magnitude to a completeness of ∼90% 74- 78 F5.2 mag Jlim Limiting J magnitude to a completeness of ∼90% 80- 84 F5.2 mag Ylim ?=- Limiting Y magnitude to a completeness of ∼90% 86- 89 I4 --- Ns Total number of sources in the galaxy disk for which aperture magnitudes could be estimated is given -------------------------------------------------------------------------------- Note (1): References to the projection parameters adopted as follows: a = Zurita et al. (2002A&A...386..801Z 2002A&A...386..801Z) b = van Zee & Bryant (1999AJ....118.2172V 1999AJ....118.2172V) c = Lindblad et al. (1997A&A...317...36L 1997A&A...317...36L) d = Pence et al. (1990ApJ...357..415P 1990ApJ...357..415P) e = Hess et al. (2009ApJ...699...76H 2009ApJ...699...76H) f = Ganda et al. (2006MNRAS.367...46G 2006MNRAS.367...46G) g = Knapen et al. (1993ApJ...416..563K 1993ApJ...416..563K) h = Kuno et al. (2007PASJ...59..117K 2007PASJ...59..117K) i = Becker et al. (1988A&A...203...21B 1988A&A...203...21B) -------------------------------------------------------------------------------- Byte-by-byte Description of file: n*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Seq Source number within galaxy 7- 16 F10.5 deg RAdeg Right ascension J2000 18- 27 F10.5 deg DEdeg Declination J2000 29- 34 F6.1 arcsec X0 X coordinate on chip relative to galaxy 36- 41 F6.1 arcsec Y0 Y coordinate on chip relative to galaxy 43- 47 I5 --- npix Number of pixels associated to source 49- 52 F4.2 --- cs [0,1] Sextractor class_star index (0=extended, 1=stellar) 54- 59 F6.2 mag Ksmag Aperture magnitude Ks 61- 65 F5.2 mag e_Ksmag Internal error in Ksmag 67- 72 F6.2 mag/arcsec+2 bgKsmag ? Background surface brightness in Ks 74- 79 F6.2 mag Hmag ? Aperture magnitude H 81- 85 F5.2 mag e_Hmag ? Internal error in Hmag 87- 92 F6.2 mag/arcsec+2 bgHmag ? Background surface brightness in H 94- 99 F6.2 mag Jmag ? Aperture magnitude J 101-105 F5.2 mag e_Jmag ? Internal error in Jmag 107-112 F6.2 mag/arcsec+2 bgJmag ? Background surface brightness in J 114-119 F6.2 mag Ymag ? Aperture magnitude Y 121-125 F5.2 mag e_Ymag ? Internal error in Ymag 127-132 F6.2 mag/arcsec+2 bgYmag ? Background surface brightness in Y 134-139 F6.2 mag Brg ? Aperture magnitude Brγ 141-145 F5.2 mag e_Brg ? Internal error in Brg 147-152 F6.2 mag/arcsec+2 bgBrg ? Background surface brightness in Brg -------------------------------------------------------------------------------- Acknowledgements: Preben Grosbol, pgrosbol(at)eso.org Horacio Dottori, dottori(at)ufrgs.br
(End) Preben Grosboel [ESO], Patricia Vannier [CDS] 05-Apr-2012
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