Panchromatic properties of 99 000 galaxies detected by SDSS, and (some by) ROSAT, GALEX, 2MASS, IRAS, GB6, FIRST, NVSS and WENSS surveys

We discuss the panchromatic properties of 99,088 galaxies selected from the Sloan Digital Sky Survey Data Release 1 “main” spectroscopic sample (a flux-limited sample for 1360 deg 2 ). These galaxies are positionally matched to sources detected by ROSAT, GALEX, 2MASS, IRAS, GB6, FIRST, NVSS and WENSS. The matching fraction varies from < 1% for ROSAT and GB6 to �40% for GALEX and 2MASS. In addition to its size, the advantages of this sample are well controlled selection effects, faint flux limits and the wealth of measured parameters, including accurate X-ray to radio photometry, angular sizes, and optical spectra. We find strong correlations between the detection fraction at other wavelengths and optical properties such as flux, colors, and emission-line strengths. For example, �2/3 of SDSS “main” galaxies classified as AGN using emission-line strengths are detected by 2MASS, while the corresponding fraction for star-forming galaxies is only �1/10. Similarly, over 90% of galaxies detected by IRAS display strong emission lines in their optical spectra, compared to �50% for the whole SDSS sample. Using GALEX, SDSS, and 2MASS data, we construct the UV-IR broad-band spectral energy distributions for various types of galaxies, and find that they form a nearly one-parameter family. For example, the SDSS u- and r- band data, supplemented with redshift, can be used to “predict” K-band magnitudes measured by 2MASS with an rms scatter of only 0.2 mag. When a dust content estimate determined from SDSS spectra with the aid of models is also utilized, this scatter decreases to 0.1 mag and can be fully accounted for by measurement uncertainties. We demonstrate that this interstellar dust content, inferred from optical SDSS spectra by Kauffmann et al. (2003a), is indeed higher for galaxies detected by IRAS and that it can be used to “predict” measured IRAS 60 µm flux density within a factor of two using only SDSS data. We also show that the position of a galaxy in the emission-line-based Baldwin-Phillips-Terlevich diagram is correlated with the optical light concentration index and u r color determined from the SDSS broad-band imaging data, and discuss changes in the morphology of this diagram induced by requiring detections at other wavelengths. Notably, we find that SDSS “main” galaxies detected by GALEX include a non-negligible fraction (10-30%) of AGNs, and hence do not represent a clean sample of starburst galaxies. We study the IR-radio correlation and find evidence that its slope