PHOTOMETRIC REDSHIFTS
Top PDF PHOTOMETRIC REDSHIFTS:
IDENTIFICATIONS AND PHOTOMETRIC REDSHIFTS OF THE 2 Ms CHANDRA DEEP FIELD SOUTH SOURCES
... high-quality photometric redshifts for the 462 X-ray sources in the ≈2 Ms Chandra Deep Field-South (CDF-S) ...master photometric catalog for the identified X-ray sources including up to 42 bands of ...
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The Multiwavelength Survey by Yale Chile (MUSYC): Deep Medium band Optical Imaging and High quality 32 band Photometric Redshifts in the ECDF S
... spectroscopic redshifts and high-S/N detections, in this case expected SED template fluxes of at least five times the detection limit for the ...these photometric offsets, listed in Table 6, before ...
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Introducing the photometric maximum likelihood method: galaxy luminosity functions at z < 1 2 in MUSYC ECDFS
... approach, photometric redshifts are increasingly being substituted for spectroscopic red- shifts even in the study of LFs (Benitez 2000; Bolzonella, Pell´o & Maccagni ...that photometric red- ...
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The cluster lensing and supernova survey with hubble (clash): strong lensing analysis of A383 from 16 BAND HST/WFC3/ACS imaging
... obtain photometric redshifts using BPZ (Bayesian photometric redshift; Ben´ıtez 2000; Ben´ıtez et ...spectroscopic redshifts from Wuyts et ...spectroscopic redshifts as described in ...
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Young Galaxy Candidates in the Hubble Frontier Fields II MACS,J0416 2403
... The galaxy cluster M0416 ( Ebeling et al. 2001; Mann & Ebeling 2012 ) lies at a redshift of z = 0.396 and has been extensively studied in recent years due to its inclusion in CLASH. While it does not have a ...
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AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale Structure
... Figure 7. 1.1 mm flux densities (medians in four redshift bins with 68% bootstrap errors are shown as thick crosses) and the 1.1 mm/1.4 GHz, 1.1 mm/24µm and 24 µm/1.4 GHz flux-density ratios plotted against redshift for ...
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LOW X RAY LUMINOSITY GALAXY CLUSTERS: MAIN GOALS, SAMPLE SELECTION, PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS
... selection, photometric and spectroscopic observations, and data ...reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at ...
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Clustering and descendants of MUSYC galaxies at z < 1 5
... and photometric redshifts in the volume- limited ECDF-S mock samples as solid triangles and open squares, ...of photometric or spectroscopic redshifts (except for the highest-redshift samples ...
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Southern cosmology survey ii massive optically selected clusters from 70 square degrees of the sunyaev zel'dovich effect common survey area
... The last decade has seen significant effort to produce large and well-selected optical catalogs of cluster of galaxies that can be used in cosmological, large-scale structure and galaxy evolution studies. The first ...
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XZ: Deriving redshifts from X ray spectra of obscured AGN
... 2004) detects gamma-ray bursts and observes X-ray spectra with XRT. Obtaining redshift constraints is crucial in order to probe massive star formation in the early Universe. Today, this requires timely follow-up and ...
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The ALHAMBRA survey: A large area multimedium band optical and near infrared photometric survey
... As was mentioned in Section 2.1, the ALHAMBRA filter set was devised following detailed simulations in order to optimize the quality and number of photometric redshifts for galaxies in our fields. ...
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Spitzer irac identification of Herschel atlas spire sources
... H-ATLAS ID-827, shown in Figure 8, is the most complex system in our sample. In this case there are four IRAC coun- terparts identified on the basis of their colors and magnitudes. The four galaxies have a wide range of ...
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The multiwavelength survey by Yale Chile (Musyc): Deep near infrared imaging and the selection of distant galaxies
... and photometric redshifts of galaxies that are selected using common color selection techniques, including distant red galaxies ( DRGs), star-forming and passive BzKs, and the rest-frame UV-selected BM, BX, ...
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The VANDELS ESO public spectroscopic survey: Observations and first data release
... multiwavelength photometric catalogs were assembled using the publicly avail- able ...multiwavelength photometric catalogs were generated using the publicly available imaging in 12 filters for UDS-GROUND ...
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Southern cosmology survey I Optical cluster detections and predictions for the southern common area millimeter wave experiments
... accurate photometric redshifts, and detect optical ...filter, photometric redshift probability distributions and rich- ness ...present photometric redshifts, richness estimates, ...
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Detection of Non Stationary Photometric Perturbations on Projection Screens
... detect photometric perturbations in projected images in real ...preliminary photometric calibration process among projectors, cameras, and the screen is ...global photometric calibration is ...
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First "Winged" and X Shaped Radio Source Candidates II New Redshifts
... The majority of double-lobed radio galaxies can be classified into one of two morphological classes: edge-dimmed and edge- brightened, corresponding to the Fanaroff & Riley (1974) type I and II sources, respectively. ...
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Galaxías débiles en el entorno de grupos fósiles
... Para realizar los mismos estudios pero en tiempos m´as tempranos, primero iden- tificamos nuestras muestras en los diferentes redshifts. Para esto buscamos la galaxia m´as brillante de los grupos en z = 0, y luego ...
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A Photometric and Spectroscopic Evaluation of the Site at Tonantzintla Observatory
... absolute photometric cal- ibration of standard stars of apparent magnitudes from (9–15) and (8–14) in the B and I bands, respec- tively, yielded no significant systematic shift of the zero points and color terms ...
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PHOTOMETRIC STUDY OF THREE SHORT PERIOD VARIABLE STARS
... we must locate the determined unreddened points in some theoretical grids such as those of Lester, Gray and Kurucz (1986, hereinafter LGK86) developed for uvby − β photometric data for several metallicities. ...
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