GALEX (UV) SDSS (Optical) UKIDSS (NIR) YHK
Basic data
objid specobjid mjd plate fiberid
587722982288458063 84382943316803584 51671 299 6
ra dec z zerr zconf spectrum_snr
206.35488 -0.81053 0.151 0.000 0.948 12.563
Links
SDSS object page   Complete object RCSED data (VOTable)   FITS spectrum (incl. continuum model)

Search this object in: DECaLS UKIDSSSimbad 2'Vizier 20"XMM-NewtonCADC CAOM VOTableHyperLedaNED
Photometry
  FUV NUV u g r i z Y J H K
Integrated
mag ? 20.181 20.108 18.562 17.781 17.368 17.141 ? ? ? ?
err ? 0.060 0.168 0.017 0.014 0.014 0.036 ? ? ? ?
k-corr ? -0.060 0.270 0.203 0.043 -0.012 0.004 ? ? ? ?
3-arcsec aperture
mag ? 23.248 21.060 19.611 18.772 18.306 17.995 ? ? ? ?
err ? 0.238 0.097 0.013 0.009 0.008 0.020 ? ? ? ?
k-corr ? 0.185 0.258 0.247 0.063 0.020 0.032 ? ? ? ?
Fully corrected SED in 6 bands for SDSS J134525.17-004837.9 (objid=587722982288458063) galaxy Fully corrected SED in 6 bands for SDSS J134525.17-004837.9 (objid=587722982288458063) galaxy at redshift 0.1505. 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 = 1.51) , in units of 10-17 erg/s/cm2;
flux 14.29 13.74 55.50 8.93 39.78 9.87 38.90 253.69 125.23 48.81 39.31
err 5.61 4.20 4.61 4.96 5.41 5.62 4.68 4.58 4.64 6.21 5.94
S/N 2.55 3.27 12.04 1.80 7.35 1.76 8.31 55.40 26.96 7.85 6.62
Non-parametric fit (χ2 = 1.45) , in units of 10-17 erg/s/cm2;
flux 26.24 13.45 58.04 5.97 37.68 11.29 46.61 262.41 120.47 50.63 38.28
err 10.07 9.74 23.95 11.38 12.01 13.54 14.46 15.13 14.36 17.73 16.98
S/N 2.61 1.38 2.42 0.52 3.14 0.83 3.22 17.34 8.39 2.86 2.25
Nbursts full spectrum fitting for SDSS J134525.17-004837.9 (objid=587722982288458063) galaxy spectrum together with the emission lines fitting Nbursts full spectrum fitting for SDSS J134525.17-004837.9 (objid=587722982288458063) 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 0.40 9.14 0.06 9.00 0.08 0.04
Stellar populations
Radial velocity, km/s Velocity dispersion, km/s Age or exp-tau, Myr Metallicity, dex
Simple stellar population (SSP) fit (χ2 = 1.232)
Value 45094.90 164.85 4166 -0.09
Error 13.95 15.59 567 0.10
Exponentially declining SFH (exp-SFH) fit (χ2 = 1.023)
Value 45085.60 153.80 5111 0.08
Error 10.73 12.37 378 0.08
BPT diagram for SDSS J134525.17-004837.9 (objid=587722982288458063) galaxy
Position of SDSS J134525.17-004837.9 (objid=587722982288458063) 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
? ? ? ? ? ? ? ?
p_mg p_cs p_el_debiased p_cs_debiased spiral elliptical uncertain
? ? ? ? ? ? ?