Table 2.

Global properties: Physical parameters of SDSS J1229+0001 grouped according to the results of different analyses. Columns 2–4 are the results of the SDSS r-band image analysis. The magnitudes are corrected for galactic and internal extinction. Rh is the half-light radius derived from the Petrosian method. The emission-line metallicity, 12 + log (O/H), is listed in column 6. The output of the best-fitting SED using magphys is presented in columns 7–11.

MrgiRhz12 + log (O/H)E(BV)M*MdustArlog [Z/Z]
(mag)(mag)(kpc)(dex)(mag)(M)(M)(mag)(dex)
SDSS J122958.84+000138.0−17.751.02 (1.35a)0.520.0088.50.851.8 × 1095.1 × 1050.710.008
MrgiRhz12 + log (O/H)E(BV)M*MdustArlog [Z/Z]
(mag)(mag)(kpc)(dex)(mag)(M)(M)(mag)(dex)
SDSS J122958.84+000138.0−17.751.02 (1.35a)0.520.0088.50.851.8 × 1095.1 × 1050.710.008

aBefore extinction correction.

Table 2.

Global properties: Physical parameters of SDSS J1229+0001 grouped according to the results of different analyses. Columns 2–4 are the results of the SDSS r-band image analysis. The magnitudes are corrected for galactic and internal extinction. Rh is the half-light radius derived from the Petrosian method. The emission-line metallicity, 12 + log (O/H), is listed in column 6. The output of the best-fitting SED using magphys is presented in columns 7–11.

MrgiRhz12 + log (O/H)E(BV)M*MdustArlog [Z/Z]
(mag)(mag)(kpc)(dex)(mag)(M)(M)(mag)(dex)
SDSS J122958.84+000138.0−17.751.02 (1.35a)0.520.0088.50.851.8 × 1095.1 × 1050.710.008
MrgiRhz12 + log (O/H)E(BV)M*MdustArlog [Z/Z]
(mag)(mag)(kpc)(dex)(mag)(M)(M)(mag)(dex)
SDSS J122958.84+000138.0−17.751.02 (1.35a)0.520.0088.50.851.8 × 1095.1 × 1050.710.008

aBefore extinction correction.

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