The Spitzer Legacy Survey of the HST-ACS 2 sq. deg. COSMOS Field: survey strategy and first analysis

Abstract

The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0, 24.0, 70.0, 160.0 u). This paper describes the survey parameters, mapping strategy, data reduction procedures, achieved sensitivities to date, and the complete data set for future reference. We show that the observed infrared backgrounds in the S-COSMOS field are within 10% of the predicted background levels. The fluctuations in the background at 24u have been measured and do not show any significant contribution from cirrus, as expected. In addition, we report on the number of asteroid detections in the low galactic latitude COSMOS field. We use the Cycle 2 S-COSMOS data to determine preliminary number counts, and compare our results with those from previous Spitzer Legacy surveys (e.g. SWIRE, GOODS). The results from this "first analysis" confirm that the S-COSMOS survey will have sufficient sensitivity with IRAC to detect ~ L* disks and spheroids out to z ~ 3, and with MIPS to detect ultraluminous starbursts and AGN out to z ~3 at 24u and out to z ~1.5-2 at 70u and 160u.

21 pages including 4 tables and 9 figures. Accepted for Publication on ApJS COSMOS special Issue

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• The main sequence of star forming galaxies II. A non evolving slope at the high mass end
• A reassessment of the redshift distribution and physical properties of luminous (sub-)millimetre galaxies
• A${}^3$COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time
• The VIMOS Ultra Deep Survey: Ly$\alpha$ Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5
• A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
• The Evolution of Dusty Star formation in Galaxy Clusters to z = 1: Spitzer IR Observations of the First Red-Sequence Cluster Survey
• The redshift and nature of AzTEC/COSMOS 1: A starburst galaxy at z=4.6
• Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
• Decomposing Star Formation and Active Galactic Nucleus with Spitzer Mid-Infrared Spectra: Luminosity Functions and Co-Evolution
• Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)
• The ALPINE-ALMA [CII] survey: Small Lya-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6
• HST imaging of the brightest z~8-9 galaxies from UltraVISTA: the extreme bright end of the UV luminosity function
• A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population
• Fe K emission from active galaxies in the COSMOS field
• A spectroscopic follow-up program of very massive galaxies at 3<z<4: confirmation of spectroscopic redshifts, and a high fraction of powerful AGN
• GAMA/DEVILS: Constraining the cosmic star-formation history from improved measurements of the 0.3-2.2 micron Extragalactic Background Light
• Photometric redshifts for galaxies in the Subaru Hyper Suprime-Cam and unWISE and a catalogue of identified clusters of galaxies
• G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR
• Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation
• Star Formation Activity in CLASH Brightest Cluster Galaxies
• The AGN-Star Formation Connection: Future Prospects with JWST
• Galaxy clusters at high redshift and evolution of brightest cluster galaxies
• The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at $2<z<6$ with two bright clump
• Properties of the molecular gas in a starbursting QSO at z=1.83 in the COSMOS field
• Connecting the metallicity dependence and redshift evolution of high-mass X-ray binaries
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - I. Multiwavelength identifications and redshift distribution
• Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25
• No Redshift Evolution of Dust Temperatures from $0<z<2$
• The multiplicity of 250-$\mu$m Herschel sources in the COSMOS field
• Type 2 AGN host galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
• The Chandra COSMOS Legacy survey: the z>3 sample
• Old age and super-solar metallicity in a massive z~1.4 early-type galaxy from VLT/X-Shooter spectroscopy
• The physical scale of the far-infrared emission in the most luminous submillimetre galaxies II: evidence for merger-driven star formation
• Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• The optical spectra of 24 micron galaxies in the COSMOS field: I. Spitzer/MIPS bright sources in the zCOSMOS-bright 10k catalogue
• On the evolution of environmental and mass properties of strong lens galaxies in COSMOS
• Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate
• SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-$\mu$m-selected galaxies
• A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time
• Confirming the Quiescent Galaxy Population out to $z=3$: A Stacking Analysis of Mid-, Far-Infrared and Radio Data
• Mergers and Star Formation: The environment and Stellar Mass Growth of the Progenitors of Ultra-Massive Galaxies since z = 2
• Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0
• Extreme emission-line galaxies out to z$\sim$1 in zCOSMOS. I. Sample and characterization of global properties
• Cluster candidates around low power radio-galaxies at z~1-2 in COSMOS
• Morphologies of Radio, X-Ray, and Mid-Infrared Selected AGN
• Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
• Investigating evidence for different black hole accretion modes since redshift z~1
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• Radio-AGN Feedback: When the Little Ones were Monsters
• The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe
• HerMES: Spectral Energy Distributions of Submillimeter Galaxies at z >4
• The lack of star formation gradients in galaxy groups up to z~1.6
• Cosmic Evolution of Star-Formation Enhancement in Close Major-Merger Galaxy Pairs Since z = 1
• Comparison of star formation rates from Halpha and infrared luminosities as seen by Herschel
• The relationship between dust and [CI] at z=1 and beyond
• zCOSMOS 10k-bright spectroscopic sample: exploring mass and environment dependence in early-type galaxies
• Radio and Far-IR Emission Associated with a Massive Star-forming Galaxy Candidate at z$\simeq$6.8: A Radio-Loud AGN in the Reionization Era?
• CWISEP J193518.59$-$154620.3: An Extremely Cold Brown Dwarf in the Solar Neighborhood Discovered with CatWISE
• Simulating JWST deep extragalactic imaging surveys and physical parameter recovery
• An high definition view of the COSMOS Wall at z~0.73
• The VLA-COSMOS Survey: V. 324 MHz continuum observations
• Properties and environment of Radio Emitting Galaxies in the VLA-zCOSMOS survey
• The role of massive halos in the Star Formation History of the Universe
• Pan-STARRS1 variability of XMM-COSMOS AGN. I. Impact on photometric redshifts
• The demographics of obscured AGN from X-ray spectroscopy guided by multiwavelength information
• Classification of Extremely Red Objects in the COSMOS Field
• The SPLASH survey: Quiescent galaxies are more strongly clustered but are not necessarily located in high-density environments
• Compact, bulge dominated structures of spectroscopically confirmed quiescent galaxies at z~3
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• Possible identification of massive and evolved galaxies At z > 5
• The KMOS Galaxy Evolution Survey (KGES): the angular momentum of star-forming galaxies over the last ~10 Gyr
• A Method to Distinguish Quiescent and Dusty Star-forming Galaxies with Machine Learning
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47
• On R-W1 as A Diagnostic to Discover Obscured Active Galactic Nuclei in Wide-Area X-ray Surveys
• Dependence of the IRX-$\beta$ dust attenuation relation on metallicity and environment
• The QUEST-La Silla AGN Variability Survey
• Galactic winds and stellar populations in Lyman $\alpha$ emitting galaxies at z ~ 3.1
• Active Galactic Nuclei as seen by the Spitzer Space Telescope
• The stellar content of the COSMOS field as derived from morphological and SED based gtar/galaxy Separation
• Green galaxies in the COSMOS field
• Spitzer Observations of the North Ecliptic Pole
• The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies
• Blue Compact Dwarf Galaxies with Spitzer: The Infrared/Radio Properties
• Infrared-Faint Radio Sources: A Cosmological View - AGN Number Counts, the Cosmic X-Ray Background and SMBH Formation
• Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9
• Low-power Radio Galaxies in the Distant Universe: A search for FRI at 1<z<2 in the COSMOS field
• Quest for COSMOS submillimeter galaxy counterparts using CARMA and VLA: Identifying three high-redshift starburst galaxies
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• Obscured star-formation and environment in the COSMOS field
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• A Far-IR Characterization of 24 micron Selected Galaxies at 0<z<2.5 using Stacking at 70 microns and 160 microns in the COSMOS Field
• The evolution of galaxy star formation activity in massive halos
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): the Evolution of Dusty and Non-Dusty Galaxies with Stellar Mass at z=2-6
• Linear radio size evolution of $\mu$Jy populations
• Deep ALMA photometry of distant X-ray AGN: improvements in star formation rate constraints, and AGN identification
• CHILES VERDES: Radio variability at an unprecedented depth and cadence in the COSMOS field
• Revisiting the role of the Thermally-Pulsating Asymptotic Giant Branch phase in high-redshift galaxies
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• Ly-alpha emitters: blue dwarfs or supermassive ULIRGs? Evidence for a transition with redshift
• A Comparison of Photometric Redshift Techniques for Large Radio Surveys
• Cosmic Galaxy-IGM HI Relation at $z\sim 2-3$ Probed in the COSMOS/UltraVISTA $1.6$ deg${}^2$ Field
• Euclid: The selection of quiescent and star-forming galaxies using observed colours
• The Asteroid Catalog Using AKARI IRC Slow-Scan Observations
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
• A Strongly-Lensed Massive Ultra-Compact Quiescent Galaxy at z ~ 2.4 in the COSMOS/UltraVISTA Field
• ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5
• The SPLASH and Chandra COSMOS Legacy Survey: the Cross Power Between Near-Infrared and X-Ray Background Fluctuations
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• The composite nature of Dust-Obscured Galaxies (DOGs) at z~2-3 in the COSMOS field: I. A Far-Infrared View
• Galaxy And Mass Assembly: the evolution of the cosmic spectral energy distribution from z = 1 to z = 0
• Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates
• Molecular gas in radio galaxies in dense Mpc-scale environments at $z=0.4-2.6$
• Investigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0<z<1 using emission line diagnostic diagrams
• A GALEX/Spitzer survey of the Cl0016+16 supercluster at z=0.55: acceleration of the onset of star-formation in satellite groups
• Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$
• PRIMUS: Obscured Star Formation on the Red Sequence
• Concurrent starbursts in molecular gas disks within a pair of colliding galaxies at z = 1.52
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Far-IR Emission From Dust-Obscured Galaxies
• The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the ${\mathrm{L}}_{[\mathrm{CII}]}$-SFR relation
• The UV to FIR spectral energy distribution of star-forming galaxies in the redshift desert
• FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
• Spectral Energy Distributions of low-luminosity radio galaxies at z~1-3: a high-z view of the host/AGN connection
• AGN in dusty hosts: implications for galaxy evolution
• The COSMOS Density Field: A Reconstruction Using Both Weak Lensing and Galaxy Distributions
• The evolution of star formation activity in galaxy groups
• A closer look at the deep radio sky: Multi-component radio sources at 3-GHz VLA-COSMOS
• The S4G perspective on circumstellar dust extinction of AGB stars in M100
• The structure of massive quiescent galaxies at z~3 in the CANDELS-COSMOS field
• Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• Radio and millimeter properties of $z\sim 5.7$ Ly$\alpha$ emitters in the COSMOS field: limits on radio AGN, submm galaxies, and dust obscuration
• The close environment of 24 micron galaxies at 0.6<z<1.0 in the COSMOS field
• Spitzer MIPS 24 and 70 micron Imaging near the South Ecliptic Pole: Maps and Source Catalogs
• Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections
• Host galaxy properties and environment of obscured and unobscured X-ray selected Active Galactic Nuclei in the COSMOS survey
• Discovery of Massive, Mostly Star-formation Quenched Galaxies with Extremely Large Lyman-alpha Equivalent Widths at z ~ 3
• The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6
• Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2
• Of Genes and Machines: application of a combination of machine learning tools to astronomy datasets
• The missing FeII bump in faint JWST AGN: possible evidence for metal-poor broad-line regions at early cosmic times
• Complete IRAC mapping of the CFHTLS-DEEP, MUSYC AND NMBS-II FIELDS
• FIR measurements of Ly-$\alpha$ emitters at z$\lesssim$1.0: dust attenuation from PACS-\emph{Herschel}
• Submm/mm Galaxy Counterpart Identification Using a Characteristic Density Distribution
• The Rest-frame $H$-band Luminosity Function of Red Sequence Galaxies in Clusters at $1.0<z<1.3$
• Physical properties of Lyman-alpha emitters at $z\sim 0.3$ from UV-to-FIR measurements
• Morphological Evolution of the Hosts of Far-Infrared/Submillimeter Galaxies
• The optical spectra of Spitzer 24 micron galaxies in the COSMOS field: II. Faint infrared sources in the zCOSMOS-bright 10k catalogue
• The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting
• Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope
• Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Colour Properties, and the Existence of Powerful AGN
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
• Cold Dust Emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: Dependence on Luminosity, Obscuration & AGN Activity
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• The Opacity of Galactic Disks at z~0.7
• Revisiting the Color-Color Selection: Submillimeter and AGN Properties of NUV-r-J Selected Quiescent Galaxies
• Searching for Super-Eddington Quasars using a Photon Trapping Accretion Disc Model
• COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS
• MAGAZ3NE: Massive, Extremely Dusty Galaxies at $z\sim 2$ Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at $3<z<4$
• Near-infrared spectroscopy of 5 ultra-massive galaxies at 1.7 < z < 2.7
• The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ) I: IRAC mosaics
• Have we seen all the galaxies that comprise the cosmic infrared background at 250\,$\mu$m $\le \lambda \le$ 500\,$\mu$m?
• Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues I. Methodology and first application in the COSMOS field
• Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population
• On the nature of infrared-faint radio sources in the SXDF and VLA-VVDS fields
• Physical and Morphological Properties of [O II] Emitting Galaxies in the HETDEX Pilot Survey
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagrams
• X-ray properties of K-selected galaxies at 0.5<z<2.0: Investigating trends with stellar mass, redshift and spectral type
• Environments of a sample of AzTEC submillimetre galaxies in the COSMOS field
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• The Type Ia Supernova Rate in Radio and Infrared Galaxies from the CFHT Supernova Legacy Survey
• A Morphological Study on Galaxies Hosting Optical Variability-Selected AGNs in the COSMOS Field
• Investigating the Lyman photon escape in local starburst galaxies with the Cosmic Origins Spectrograph
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• Extinction law in ultraluminous infrared galaxies at z ~ 1
• Obscured AGNs in Bulgeless Hosts discovered by WISE: The Case Study of SDSS J1224+5555
• The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of active galactic nuclei
• MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at $z>0.25$
• Infrared spectroscopic confirmation of z~2 photometrically-selected obscured quasars
• Cosmic happenstance: 24-$\mu$m selected, multi-component Herschel sources are line-of-sight projections
• Radio stacking reveals evidence for star formation in the host galaxies of X-ray selected active galactic nuclei at z<1
• Stellar Mass and 3.4 $\mu$m M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ~ 1.0
• Simulations of the cosmic infrared and submillimeter background for future large surveys: II. Removing the low-redshift contribution to the anisotropies using stacking
• The Compilation and Validation of the Spectroscopic Redshift Catalogs for the DESI-COSMOS and DESI-XMMLSS Fields
• X-ray Selected Narrow-Line Active Galactic Nuclei in the COSMOS Field: Nature of Optically Dull Active Galactic Nuclei
• The optical luminosity function of LOFAR radio-selected quasars at $1.4\le z\le 5.0$ in the NDWFS-Boötes field
• The radio-loud AGN population at z>~1 in the COSMOS field. I. Selection and Spectral Energy Distributions
• Properties of IR selected Active Galactic Nuclei
• Gas properties as a function of environment in the proto-supercluster Hyperion at z ~ 2.45
• What is the origin of the stacked radio emission in radio-undetected quasars?: Insights from a radio-infrared image stacking analysis
• Role of AGNs in the Luminous Infrared Galaxy phase since z ~ 3
• A Large Massive Quiescent Galaxy Sample at z~1.2
• A new approach to constraining properties of AGN host galaxies by combining image and SED decomposition: testing upon the MBH-M* relation
• CONCERTO at APEX -- On-sky performance in continuum
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS Field
• Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z~3.3
• The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z $\sim$ 4.4-5.9
• Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field
• Detection of CO(J=1-0) Emission from Barred Spiral Galaxies at z~0.1
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• A candidate giant planet companion to the massive, young white dwarf GALEX J071816.4+373139 informs the occurrence of giant planets orbiting B stars
• A Ly-alpha nebula at z~3.3
• Counterparts of Candidate Dusty Starbursts at z > 6
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• Zangetsu: A Candidate of Isolated, Quiescent, and Backsplash Ultra-Diffuse Galaxy in the COSMOS Field
• ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• Simulating infrared spectro-photometric surveys with a SPRITZ
• Host galaxy and nuclear properties of IR-selected AGNs with and without outflow signatures
• Nature of hard X-ray (3-24 keV) detected luminous infrared galaxies in the COSMOS field
• The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z=1
• The major merger-active galactic nucleus connection up to the cosmic noon
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• CHILES X: Molecular and atomic gas at intermediate redshift
• The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection
• The Compact Star-Forming Galaxies at $2<z<3$ in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6
• Spitzer Publication Statistics
• Spectral energy distribution similarity of the local galaxies and the 3.6um selected galaxies from the Spitzer Extended Deep Survey
• Euclid: Discovery of bright $z\simeq 7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
• Physical properties of distant red galaxies in the COSMOS/UltraVISTA field