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J/AJ/131/2089       Planetary nebulae in NGC 3379 and NGC 3384    (Sluis+, 2006)

Uncovering planetary nebulae in early-type galaxies using the Rutgers Fabry-Perot. Sluis A.P.N., Williams T.B. <Astron. J., 131, 2089-2104 (2006)> =2006AJ....131.2089S
ADC_Keywords: Planetary nebulae ; Galaxies, nearby; Radial velocities Keywords: galaxies: elliptical and lenticular, cD - galaxies: kinematics and dynamics - instrumentation: spectrographs - planetary nebulae: general Abstract: We report on observations of four early-type galaxies performed with the Rutgers Fabry-Perot in order to search for planetary nebulae (PNe) in these systems. The aim is to use the PNe as kinematic tracers of the galaxy potential. We describe our data reduction and analysis procedure and show that the proper calibration of our detection statistic is crucial in getting down to our limiting magnitude of m5007=26.1. In the case of the two Leo galaxies, we find moderately sized samples: 54 PNe in NGC 3379 and 50 PNe in NGC 3384; NGC 4636 (two PNe) and NGC 1549 (six PNe) are included for completeness. We present our samples in tabular form, as well as the spectrum for each PN. Description: We observed the four galaxies in our sample with the Rutgers Fabry-Perot over the course of two runs at the Cerro Tololo Inter-American Observatory (CTIO) 4m Blanco telescope. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5.dat 85 54 NGC 3379 planetary nebulae table6.dat 85 50 NGC 3384 planetary nebulae
See also: J/ApJ/344/715 : Planetary nebulae as standard candles. IV. (Ciardullo+, 1989) J/ApJ/414/454 : NGC 3379 planetary nebulae radial velocities (Ciardullo+ 1993) J/ApJ/449/592 : NGC 5128 PN. III. (Hui+ 1995) J/ApJ/602/685 : NGC 5128 planetary nebulae (Peng+, 2004) Byte-by-byte Description of file: table5.dat table6.dat
Bytes Format Units Label Explanations
1- 3 A3 --- ID Source identification (1) 5- 6 I2 h RAh Hour of Right Ascension (J2000) (2) 8- 9 I2 min RAm Minute of Right Ascension (J2000) (2) 11- 15 F5.2 s RAs Second of Right Ascension (J2000) (2) 16 A1 --- DE- Sign of the Declination (J2000) (2) 17- 18 I2 deg DEd Degree of Declination (J2000) (2) 20- 21 I2 arcmin DEm Arcminute of Declination (J2000) (2) 23- 26 F4.1 arcsec DEs Arcsecond of Declination (J2000) (2) 28- 33 F6.1 0.1nm lambda Peak wavelength in Angstroms 35- 38 I4 km/s HRV Heliocentric line-of-sight velocity 40- 41 I2 km/s e_HRV Uncertainty in HRV 43- 46 F4.2 10-19W/m2 Flux Emission line flux in units of 10-16erg/s/cm2 48- 52 F5.2 mag 5007mag Emission line magnitude (3) 54- 57 F4.2 mag e_5007mag Uncertainty in 5007mag 59- 63 F5.1 --- S The likelihood ratio test statistic (4) 65- 66 I2 --- Num ? Number of data points in spectrum 68- 71 F4.1 --- S/N Signal-to-noise ratio 73- 74 I2 --- C89ID ? Ciardullo et al. (1989, J/ApJ/344/715) identification 76- 80 F5.2 mag C89mag ? Ciardullo et al. (1989, J/ApJ/344/715) emission line magnitude 82- 85 I4 km/s C89HRV ? Ciardullo et al. (1989, J/ApJ/344/715) heliocentric line-of-sight velocity
Note (1): E and W denote PNe found in the East and West fields, respectively. Nomenclature in Simbad: Table 5: [SW2006] NGC 3379 WNN Table 6: [SW2006] NGC 3384 WNN Note (2): Where the uncertainty in each coordinate is 0.4" (includes random and systematic uncertainty); Note (3): 5007mag=-2.5log(Flux)+13.74 (no extinction correction was made). Note (4): The spectra have a wide range in their number of data points and we determine Sc(α) for regions with one, two, or three pointings separately. Hence, the values of S listed in Table 6 are not always directly comparable.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 22-May-2007
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

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