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Arp 118


Above from Brown et al. (2014): Galaxy SEDs from the ultraviolet to the mid-infrared. In the left panel the observed and model spectra are shown in black and gray respectively, while the photometry used to constrain and verify the spectra is shown with red dots. In the right panel we plot (where applicable) the photometric aperture (thick white rectangle), the Akari extraction aperture (blue rectangle), the Spitzer SL extraction aperture (green rectangle) and the Spitzer LL extraction aperture (yellow rectangle). For galaxies with Spitzer stare mode spectra, we show a region corresponding to a quarter of the slit length. For scale, the horizontal bar denotes 1 arcmin.

Products:

Arp 118 Spectrum
hlsp_galsedatlas_2mass_imager_arp-118_h_v1_img.fits
hlsp_galsedatlas_2mass_imager_arp-118_j_v1_img.fits
hlsp_galsedatlas_2mass_imager_arp-118_ks_v1_img.fits
hlsp_galsedatlas_galex_fuv_arp-118_fuv_v1_img.fits
hlsp_galsedatlas_galex_nuv_arp-118_nuv_v1_img.fits
hlsp_galsedatlas_spitzer_irac_arp-118_i1_v1_img.fits
hlsp_galsedatlas_spitzer_irac_arp-118_i2_v1_img.fits
hlsp_galsedatlas_spitzer_irac_arp-118_i3_v1_img.fits
hlsp_galsedatlas_spitzer_irac_arp-118_i4_v1_img.fits
hlsp_galsedatlas_spitzer_mips_arp-118_m1_v1_img.fits
hlsp_galsedatlas_sdss_imager_arp-118_g_v1_img.fits
hlsp_galsedatlas_sdss_imager_arp-118_i_v1_img.fits
hlsp_galsedatlas_sdss_imager_arp-118_r_v1_img.fits
hlsp_galsedatlas_sdss_imager_arp-118_u_v1_img.fits
hlsp_galsedatlas_sdss_imager_arp-118_z_v1_img.fits
hlsp_galsedatlas_swift_imager_arp-118_u_v1_img.fits
hlsp_galsedatlas_swift_imager_arp-118_uvm2_v1_img.fits
hlsp_galsedatlas_swift_imager_arp-118_uvw2_v1_img.fits
hlsp_galsedatlas_wise_imager_arp-118_w1_v1_img.fits
hlsp_galsedatlas_wise_imager_arp-118_w2_v1_img.fits
hlsp_galsedatlas_wise_imager_arp-118_w3_v1_img.fits
hlsp_galsedatlas_wise_imager_arp-118_w4_v1_img.fits