SDSS J153209.95+010945.0
GALEX (UV) SDSS (Optical) UKIDSS (NIR) YHK
Basic data
objid specobjid mjd plate fiberid
587726014555291875 831711419278819328 54561 2954 87
ra dec z zerr zconf spectrum_snr
233.04147 1.16251 0.052 0.000 0.994 13.827
Links
SDSS object page   Complete object RCSED data (VOTable)   FITS spectrum (incl. continuum model)

Search this object in: DECaLS UKIDSS,  Simbad 2',  Vizier 20",  XMM-Newton,  CADC CAOM VOTable,  HyperLeda,  NED
Photometry
  FUV NUV u g r i z Y J H K
Integrated
mag 19.959 19.301 19.079 18.116 17.781 17.522 17.491 17.030 17.196 16.770 16.994
err 0.144 0.081 0.079 0.012 0.013 0.016 0.056 0.049 0.071 0.067 0.075
k-corr -0.040 0.009 0.122 0.007 0.032 -0.041 -0.012 -0.017 -0.014 -0.004 -0.112
3-arcsec aperture
mag 22.245 21.133 19.834 18.857 18.562 18.325 18.208 17.746 17.677 17.575 17.693
err 0.571 0.221 0.054 0.008 0.008 0.011 0.034 0.021 0.026 0.029 0.030
k-corr 0.021 0.004 0.121 -0.002 0.032 -0.052 -0.007 -0.049 -0.023 0.004 -0.116
Fully corrected SED in 11 bands for SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy Fully corrected SED in 11 bands for SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy at redshift 0.0518. Blue and red symbols represent total (Petrosian) and 3-arcsec fiber magnitudes correspondingly. The rest framed SDSS spectrum is overplotted and demonstrates a typical good agreement with the corrected fiber magnitudes for that galaxy. The inset shows an 36x36 arcsec optical SDSS false color image.
Emission lines
[O II] λ3727 Hγ λ4340 Hβ λ4861 [O III] λ4959 [O III] λ5007 [O I] λ6300 [N II] λ6548 Hα λ6563 [N II] λ6583 [S II] λ6716 [S II] λ6731
Gaussian fit (χ2 = 0.69) , in units of 10-17 erg/s/cm2/Å
flux 310.33 119.58 282.16 101.56 308.87 31.32 77.51 1037.04 228.84 193.13 136.13
err 13.30 5.08 5.69 4.42 6.08 2.88 3.47 9.56 4.38 3.97 3.57
S/N 23.34 23.56 49.59 22.97 50.78 10.89 22.36 108.45 52.19 48.69 38.18
Non-parametric fit (χ2 = 0.72) , in units of 10-17 erg/s/cm2/Å
flux 318.36 121.22 286.35 104.85 320.35 32.50 79.08 1037.19 240.99 203.08 142.06
err 22.47 12.37 12.23 15.72 14.78 11.53 19.98 19.73 20.63 12.52 11.41
S/N 14.17 9.80 23.41 6.67 21.68 2.82 3.96 52.57 11.68 16.22 12.45
Nbursts full spectrum fitting for SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy spectrum together with the emission lines fitting Nbursts full spectrum fitting for SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy spectrum together with the emission lines fitting (gaussian model). Central panel shows an observed galaxy spectrum (black), the best fitting template (red) and residuals (blue). The observed and rest-frame wavelength are shown in the bottom and top of the plot respectively. Panels on the sides demonstrate recovered profiles after the continuum subtraction of individual emission lines (black) and the best-fitting models (red). Blue lines show emission line flux uncertainties. Vertical red dashed lines represent the galaxy redshift in the SDSS database. See also this spectrum with best-fit models in the interactive spectrum viewer.
E(B-V) 12+logO/H1 12+logO/H1 err 12+logO/H2, 3 12+logO/H2, 3 err low 12+logO/H2, 3 err high
Value 0.21 8.67 0.01 8.87 0.14 0.02
Stellar populations
Radial velocity, km/s Velocity dispersion, km/s Age or exp-tau, Myr Metallicity, dex
Simple stellar population (SSP) fit (χ2 = 0.586)
Value 15521.90 73.00 2987 -1.06
Error 12.01 15.81 512 0.07
Exponentially declining SFH (exp-SFH) fit (χ2 = 0.536)
Value 15507.00 90.86 20275 -0.82
Error 10.33 13.13 -0 0.11
BPT diagram for SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy
Position of SDSS J153209.95+010945.0 (objid=587726014555291875) galaxy (shown as a star) on the BPT diagram with the color coded Hα equivalent width. Two or more stars mean that there are several spectra for this galaxy in the database. Here we display in the background only those galaxies from RCSED catalog where all emission lines used in the plot have signal-to-noise ratio S/N > 3. The contours correspond to the galaxy density smoothed with a moving average based on a 4-pixels window. The number of galaxies kept in the sample is indicated on the top left. The full and dashed lines correspond to starforming and transitional galaxies in Kewley et al. (2006).
Galaxy Zoo morphology
ra dec nvote p_el p_cw p_acw p_edge p_dk
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p_mg p_cs p_el_debiased p_cs_debiased spiral elliptical uncertain
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