ALMA Lensing Cluster Survey: and Photometry of 33 Lensed Fields Built with CHArGE
arXiv:2207.07125 · doi:10.3847/1538-4365/ac9909
Abstract
We present a set of multi-wavelength mosaics and photometric catalogs in the ALMA lensing cluster survey (ALCS) fields. The catalogs were built by reprocessing of archival data from the CHArGE compilation, taken by the () in the RELICS, CLASH and Hubble Frontier Fields. Additionally we have reconstructed the IRAC 3.6 and 4.5 m mosaics, by utilising all the available archival IRSA/SHA exposures. To alleviate the effect of blending in such a crowded region, we have modelled the photometry by convolving the detection image with the PSF using the novel software. The final catalogs contain 218,000 sources, covering a combined area of 690 arcmin. These catalogs will serve as an important tool in aiding the search of the sub-mm galaxies in future ALMA surveys, as well as follow ups of the dark - IRAC sources. Coupled with the available photometry the addition of the 3.6 and 4.5 m bands will allow us to place a better constraint on photometric redshifts and stellar masses of these objects, thus giving us an opportunity to identify high-redshift candidates for spectroscopic follow ups and answer the important questions regarding the epoch of reionization and formation of first galaxies.
41 pages, 16 figures, 8 tables. Accepted to ApJS. Mosaics and photometric catalogs can be accessed online https://github.com/dawn-cph/alcs-clusters
References in corpus (38)
- The Gaia mission
- Cosmic Star Formation History
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- EAZY: A Fast, Public Photometric Redshift Code
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
- Detection of quiescent galaxies in a bicolor sequence from z=0-2
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
- The Relation Between SFR and Stellar Mass for Galaxies at 3.5 6.5 in CANDELS
- Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties
- Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high redshift studies
- The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
- The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts
- The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
- Hubble Frontier Fields First Complete Cluster Data: Faint Galaxies at for UV Luminosity Functions and Cosmic Reionization
- New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
- ALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies
- A Geometrically Supported Candidate Multiply-Imaged by the Hubble Frontier Fields Cluster Abell 2744
- An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
- Hubble Frontier Fields : A High Precision Strong Lensing Analysis of Galaxy Cluster MACSJ0416.1-2403 using ~200 Multiple Images
- The sizes of lensed galaxies from the Hubble Frontier Fields Abell 2744 data
- The quenching of the star formation activity in cluster galaxies
- T-PHOT version 2.0: improved algorithms for background subtraction, local convolution, kernel registration, and new options
- Evidence for GN-z11 as a luminous galaxy at redshift 10.957
- The ALMA Frontier Fields survey I: 1.1 mm continuum detections in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
- Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
- ALMA twenty-six arcmin survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources
- ALMA Lensing Cluster Survey: Bright [CII] 158 m Lines from a Multiply Imaged Sub- Galaxy at
- Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
- Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
- The Evolving Interstellar Medium of Star-Forming Galaxies, as traced by
- ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-Forming Galaxies across
- ALMA Deep Field in SSA22: A near-infrared-dark submillimeter galaxy at z=4.0
- The ASTRODEEP Frontier Fields Catalogues III. Multiwavelength photometry and rest frame properties of MACS-J0717 and MACS-J1149
- A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
- Measuring the Stellar Masses of z~7 Galaxies with Spitzer Ultrafaint Survey Program (SURFS UP)
Cited by in corpus (32)
- An Atlas of Color-selected Quiescent Galaxies at in Public Fields
- JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy
- CEERS Key Paper V: A triality on the nature of HST-dark galaxies
- JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
- Templates for Fitting Photometry of Ultra-High-Redshift Galaxies
- The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
- COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method
- The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies
- Sub-Millimetre Galaxies with Webb: Near-Infrared Counterparts and Multi-wavelength Morphology
- The GLASS-JWST Early Release Science Program. II. Stage I release of NIRCam imaging and catalogs in the Abell 2744 region
- JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
- JWST UNCOVER: The Overabundance of Ultraviolet-luminous Galaxies at
- Insight Into a Lensed -dark Galaxy and its Quiescent Companion at
- MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field
- A spatially resolved analysis of star-formation burstiness by comparing UV and H in galaxies at z1 with UVCANDELS
- The Lyman Continuum Escape Fraction of Star-forming Galaxies at from UVCANDELS
- The cold interstellar medium of a normal sub- galaxy at the end of reionization
- Feedback and dynamical masses in high- galaxies: the advent of high-resolution NIRSpec spectroscopy
- MIDIS. Near-infrared rest-frame morphology of massive galaxies at in the Hubble eXtreme Deep Field
- The ALMA Frontier Fields Survey. VI. Lensing-corrected 1.1mm number counts in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370 and Abell S1063
- Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
- ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-ray Detected Active Galactic Nuclei
- "Dust Giant": Extended and Clumpy Star-Formation in a Massive Dusty Galaxy at
- Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
- Compact dust-obscured star-formation and the origin of the galaxy bimodality
- Unveiling the Dark Side of UV/Optical Bright Galaxies: Optically Thick Dust Absorption
- ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
- Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
- ALMA Lensing Cluster Survey: average dust, gas, and star formation properties of cluster and field galaxies from stacking analysis
- Uncovering the MIR emission of quiescent galaxies with
- Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
- VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova