J/A+A/408/67    LSB galaxies in near-infrared. II.     (Monnier-Ragaigne+, 2003)

A search for Low Surface Brightness galaxies in the near-infrared. II. Arecibo HI line observations. Monnier-Ragaigne D., van Driel W., O'Neil K., Schneider S.E., Balkowski C., Jarrett T.H. <Astron. Astrophys. 408, 67 (2003)> =2003A&A...408...67M 2003A&A...408...67M
ADC_Keywords: Galaxy catalogs ; Galaxies, photometry ; Photometry, infrared ; H I data Keywords: galaxies: distances and redshifts - galaxies: general - galaxies: ISM - infrared: galaxies - radio lines: galaxies Abstract: A total of 367 Low Surface Brightness galaxies detected in the 2MASS all-sky near-infrared survey have been observed in the 21 cm H I line using the Arecibo telescope. All have a Ks-band mean central surface brightness, measured within a 5" radius, fainter than 18mag/arcsec2. We present global H I line parameters for the 107 clearly detected objects and the 21 marginal detections, as well as upper limits for the undetected objects. The 107 clear detections comprise 15 previously uncatalogued objects and 36 with a PGC entry only. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 100 24 Comparison with published HI data table3a.dat 50 107 Detected objects - identifications and coordinates table4a.dat 47 21 Marginal detections - identifications and coordinates table5a.dat 50 237 Undetected objects - identifications and coordinates table3b.dat 133 108 Detected objects - basic data table4b.dat 114 21 Marginal detections - basic data table5b.dat 84 271 Undetected objects - basic data fig2a.ps 76 5112 Arecibo 21-cm H I line spectra of the clearly detected objects fig2b.ps 76 5267 Figure 2 continued fig2c.ps 76 6152 Figure 2 continued fig2d.ps 76 6044 Figure 2 continued fig2e.ps 76 3246 Figure 2 continued fig3.ps 76 5304 Arecibo 21-cm H I line spectra of marginal detections -------------------------------------------------------------------------------- See also: J/A+A/405/99 : LSB galaxies in near-infrared. I. (Monnier-Ragaigne+, 2003) J/A+A/408/465 : LSB galaxies in near-infrared. III. (Monnier-Ragaigne+, 2003) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- ID Identification of the galaxy 11- 23 A13 --- OName Other name 26- 29 I4 km/s V(HI) Heliocentric central radial velocity of 21cm line profile 32- 36 F5.2 Jy.km/s I(HI) ? Integrated 21cm line flux 40- 42 I3 km/s W(50) ? Width velocity at 50% of peak maximum 47 A1 --- Tel [AN] Telescopes, Arecibo (A) or Nancay (N) 53-102 A50 --- Ref Reference -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3a.dat table4a.dat table5a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- ID Identification of the galaxy 7 A1 --- n_ID [)] Source names in brackets are not found in later versions of the public 2MASS database 9- 22 A14 --- 2MASXi 2MASS name (hhmmsss+ddmmss, J2000.0) 24 A1 --- f_ID [*] *: S396N has no entry in table3b.dat 26- 32 I7 --- PGC ? PGC number 35- 54 A20 --- OName Other name -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- --- [(] 2- 7 A6 --- ID Identification of the galaxy 8 A1 --- m_ID [ab] Multiplicity index on ID, when two line profiles detected in the same spectrum 9 A1 --- --- [)] Source names in brackets are not found in later versions of the public 2MASS database 11- 15 F5.2 mag K20 ? Total magnitude measured within the rK20 isophotal aperture 17- 20 F4.2 mag J-Ks ? J-Ks colour index 22- 26 F5.2 mag/arcsec+2 SuBrK5 ? Mean central surface brightness measured within a radius of 5" around the source's center in the Ks band 28- 31 F4.2 --- b/a ? b/a ratio (ellipticity) 33- 36 F4.1 arcsec r(K20) ? Fiducial aperture in the Ks band 38- 42 F5.2 mag BTc ? Total apparent B-band magnitude (G1) 44- 47 F4.2 arcmin D25 ? Isophotal B-band diameter measured at a surface brightness level of 25mag/arcsec2 49- 53 F5.2 mag/arcsec+2 SuBrB25 ? Mean B-band surface brightness within the 25mag/arcsec2 isophote 55- 61 A7 --- MType Morphological type 63- 66 F4.2 mJy rms rms noise level in a spectrum 68 A1 --- l_I(HI) Limit flag on I(HI) 69- 72 F4.2 Jy.km/s I(HI) Integrated 21cm line flux 74 A1 --- l_V(HI) Limit flag on V(HI) 75- 79 I5 km/s V(HI) ? Heliocentric central radial velocity of 21cm line profile 81- 82 I2 km/s e_V(HI) ? rms uncertainty on V(HI) 84- 88 I5 km/s V(opt) ? Mean heliocentric optical radial velocity 90- 92 I3 km/s W(50) ? Velocity widths at 50% of peak maximum 94- 96 I3 km/s W(20) ? Velocity widths at 20% of peak maximum 98 A1 --- n_Dist [(] Note (1) 99-103 F5.1 Mpc Dist Distance 105 A1 --- n_logM(HI) [(] Note (2) 106-110 F5.2 [solMass] logM(HI) Total HI mass 112-116 F5.2 [solLum] logL(K) Absolute magnitude in the Ks band (G2) 118-122 F5.2 [solLum] logL(B) ? Absolute magnitude in the B band (G2) 124-127 F4.2 --- M(HI)/LK Mass-to-Ks luminosity ratio 129-132 F4.2 --- M(HI)/LB ? Mass-to-blue luminosity ratio 133 A1 --- --- [)] -------------------------------------------------------------------------------- Note (1): For L224O: Our H I spectrum of the target galaxy, NGC 464, shows two detections, at 5803 and 6673km/s. It is impossible to assign the detections to the objects, as neither has a known optical redshift. For the distance dependent parameters listed for L224Oa and L224Ob it was assumed that the H I is associated with NGC 464. Note (2): For S490P: H I profile partially outside our search range. For S2834O: Two H I lines were detected in our spectrum, at 5615 and 9802km/s. For the distance dependent parameters listed for S2834Oa/b it was assumed that the H I is associated with the target galaxy. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- ID Identification of the galaxy 8- 12 F5.2 mag K20 Total magnitude measured within the rK20 isophotal aperture 14- 17 F4.2 mag J-Ks J-Ks colour index 19- 23 F5.2 mag/arcsec+2 SuBrK5 Mean central surface brightness measured within a radius of 5" around the source's center in the Ks band 25- 28 F4.2 --- b/a b/a ratio 30- 33 F4.1 arcsec r(K20) Fiducial aperture in the Ks band 35- 39 F5.2 mag BTc ? Total apparent B-band magnitude (G1) 41- 44 F4.2 arcmin D25 ? Isophotal B-band diameter measured at a surface brightness level of 25mag/arcsec2 46- 50 F5.2 mag/arcsec+2 SuBrB25 ? Mean B-band surface brightness within the 25mag/arcsec2 isophote 52- 56 A5 --- MType Morphological type 58- 61 F4.2 mJy rms rms noise level in a spectrum 63- 66 F4.2 Jy.km/s I(HI) Integrated line flux 68- 72 I5 km/s V(HI) Heliocentric central radial velocity of a line profile 74- 77 I4 km/s V(opt) ? Mean heliocentric optical radial velocity 79- 81 I3 km/s W(50) Velocity widths at 50% of peak maximum 83- 87 F5.1 Mpc Dist Distance 89- 92 F4.2 [solMass] logM(HI) Total HI mass 94- 98 F5.2 [solLum] logL(K) Absolute magnitude in the Ks band (G2) 100-104 F5.2 [solLum] logL(B) ? Absolute magnitude in the B band (G2) 106-109 F4.2 --- M(HI)/LK Mass-to-Ks luminosity ratio 111-114 F4.2 --- M(HI)/LB ? Mass-to-blue luminosity ratio -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- ID Identification of the galaxy 8- 12 F5.2 mag K20 Total magnitude measured within the rK20 isophotal aperture 14- 17 F4.2 mag J-Ks J-Ks colour index 19- 22 F4.2 mag H-Ks H-Ks colour index 24- 28 F5.2 mag/arcsec+2 SuBrK5 Mean central surface brightness measured within a radius of 5" around the source's center in the Ks band 30- 33 F4.2 --- b/a b/a ratio 35- 38 F4.1 arcsec r(K20) Fiducial aperture in the Ks band 40- 44 F5.2 mag BTc ? Total apparent B-band magnitude (1) 46- 49 F4.2 arcmin D25 ? Isophotal B-band diameter measured at a surface brightness level of 25mag/arcsec2 51- 55 F5.2 mag/arcsec+2 SuBrB25 ? Mean B-band surface brightness within the 25mag/arcsec2 isophote 57- 60 A4 --- MType Morphological type 62- 65 F4.2 mJy rms rms noise level in a spectrum 67- 70 F4.2 Jy.km/s I(HI) Integrated line flux (2) 72- 75 F4.2 --- M(HI)/LK Mass-to-Ks luminosity ratio 77- 80 F4.2 --- M(HI)/LB ? Mass-to-blue luminosity ratio 83- 84 A2 --- Search Search mode (3) -------------------------------------------------------------------------------- Note (1): Reduced to the RC3 system and corrected for galactic extinction, inclination and redshift effects. Note (2): Estimated upper limits to I(HI) are for 250km/s wide, flat-topped profiles Note (3): 3 different line search modes were used: lo in the -500 to 11000km/s range, hi in the 9500 to 21000km/s range kv for objects with previously known redshifts; -------------------------------------------------------------------------------- Global notes: Note (G1): Reduced to the RC3 system and corrected for galactic extinction, inclination and redshift effects. Note (G2): LK (resp. LB) is expressed in L_☉,K (resp. L☉,B), and calculated using an absolute solar Ks (resp. B) -band magnitude of 3.33 (resp. 5.48) (Allen, 1973, Astrophysical Quantities). -------------------------------------------------------------------------------- Acknowledgements: Wim van Driel
(End) Patricia Bauer [CDS] 12-Sep-2003
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