This data server provides access to the ALHAMBRA Final Catalogue. The ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift Astronomical) survey (Moles et al. 2008) has observed 8 different regions of the sky, including sections of the COSMOS, DEEP2, ELAIS, GOODS-N, SDSS and Groth fields using a new photometric system with 20 contiguous, non-overlapping, equal width (~ 300A) filters, covering the optical range (3500A-9700A), plus the standard broadband NIR J, H and Ks filters. The observations were carried out with the Calar Alto (CAHA) 3.5m telescope using the wide field, 0.25 deg2 FOV optical camera LAICA and the NIR instrument Omega-2000. The ALHAMBRA survey dataset represents a ~700hrs of total exposure time, gathered in between the 2005 and 2012.Further information on the project
can be found at the ALHAMBRA web page.Right Ascension (degrees)Declination (degrees)Search radiusAllowed values for verbosity: 1=minimum, 2=default, 3=maximumMinimum value for F814W. Isophotal magnitude [AB]Maximum value for F814W. Isophotal magnitude [AB]Minimum value for Satur_Flag. Photometric Saturation-Flag [0:Good Detection, 1:Saturated Detection]Maximum value for Satur_Flag. Photometric Saturation-Flag [0:Good Detection, 1:Saturated Detection]Minimum value for Stellar_Flag. Statistical STAR/GALAXY Discriminator [0:Pure-Galaxy,0.5:Unknown,1:Pure-Star]Maximum value for Stellar_Flag. Statistical STAR/GALAXY Discriminator [0:Pure-Galaxy,0.5:Unknown,1:Pure-Star]Minimum value for zb_1. BPZ most likely redshift for the First PeakMaximum value for zb_1. BPZ most likely redshift for the First PeakBPZ most likely spectral type for the First PeakMinimum value for Odds_1. P(z) contained within zb +/- 2*0.01*(1+z) for the First PeakMaximum value for Odds_1. P(z) contained within zb +/- 2*0.01*(1+z) for the First PeakRight Ascension (degrees)Declination (degrees)Distance from ConeSearch center positionObject ID Number [814+Field+Pointing+CCD+ColorProindex]ALHAMBRA fieldPointing within the fieldDetector within the pointingX-pixel coordinateY-pixel coordinateIsophotal aperture area (pixels)Full width at half maximum for detection image (arcsec)SExtractor stellarity (1 = star; 0 = galaxy)Ellipticity = 1 - B/AProfile RMS along major axis (pixels)Profile RMS along minor axis (pixels)Position Angle (CCW/x)Kron apertures in units of A or B (pixels)Fraction-of-light radii (pixels)Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)SExtractor Photometric FlagIsophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Isophotal magnitude uncertainty [AB]Isophotal magnitude [AB]Number Filters Detected (out of 24)X-Ray Source [0:NO,1:YES] (2XMM;Watson et al. 2009;A&A493,339-373)Percentual Photometric Weight (on detection image).Photometric Saturation-Flag [0:Good Detection, 1:Saturated Detection]Statistical STAR/GALAXY Discriminator [0:Pure-Galaxy,0.5:Unknown,1:Pure-Star]BPZ most likely redshift for the First PeakLower limit (95p confidence) for the First PeakUpper limit (95p confidence) for the First PeakBPZ most likely spectral type for the First PeakP(z) contained within zb +/- 2*0.01*(1+z) for the First PeakPoorness of BPZ fit: observed vs. model fluxesStellar Mass for the First Peak (log10(M_sun))Absolute Magnitude [AB] (B_JOHNSON) for the First PeakOptical-Quality-Flag. Number of Optical Filters with PercW < 0.8NIR-Quality-Flag. Number of NIR Filters with PercW < 0.8Link to F814W Image