A dataset provided by the European Space Agency

Name 12444
Title Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- GOODS-North Field, Middle Visits of SNe Search
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12444;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-hnusxjb
Author Faber, Sandra M.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12444&mission=hst
Publication
  • 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
  • A Calibration of NICMOS Camera 2 for Low Count Rates
  • A CANDELS-3D-HST synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5
  • A catalog of polychromatic bulge-disc decompositions of ~17.600 galaxies in CANDELS
  • Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI
  • A deeper look at the dust attenuation law of star-forming galaxies at high redshift
  • A Duality in the Origin of Bulges and Spheroidal Galaxies
  • A dusty compact object bridging galaxies and quasars at cosmic dawn
  • A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
  • A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with M BH 106-108 M and Their Host Galaxy Properties
  • A Lyman Break Galaxy in the Epoch of Reionization from Hubble Space Telescope Grism Spectroscopy
  • A Molecular Line Scan in the Hubble Deep Field North
  • A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density
  • An enhanced merger fraction within the galaxy population of the SSA22 protocluster at z = 3.1
  • A new derivation of the Hubble constant from g-ray attenuation using improved optical depths for the Fermi and CTA era
  • An insight into the extragalactic transient and variable microJy radio sky across multiple decades
  • An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
  • A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
  • A Simulation-driven Deep Learning Approach for Separating Mergers and Star-forming Galaxies: The Formation Histories of Clumpy Galaxies in All of the CANDELS Fields
  • A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
  • A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
  • A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
  • Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
  • Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
  • Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2 <= z <= 1.5
  • Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope Observations, Imaging Data Products, and Mosaics
  • Can Minor Merging Account for the Size Growth of Quiescent Galaxies? New Results from the CANDELS Survey
  • Comparison of Observed Galaxy Properties with Semianalytic Model Predictions Using Machine Learning
  • Conditions for galaxy quenching at 0.5 < z < 2.5 from CANDELS: compact cores and environment
  • Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
  • Contamination of Broadband Photometry by Nebular Emission in High-redshift Galaxies: Investigations with Kecks MOSFIRE Near-infrared Spectrograph
  • Deep JVLA Imaging of GOODS-N at 20 cm
  • Definitive upper bound on the negligible contribution of quasars to cosmic reionization
  • Delay Time Distributions of Type Ia Supernovae from Galaxy and Cosmic Star Formation Histories
  • Delving deep: A population of extremely dusty dwarfs observed by JWST
  • Density perturbations for running vacuum: a successful approach to structure formation and to the s8-tension
  • Dependence of galaxy clustering on UV luminosity and stellar mass at z ~ 4-7
  • Detecting outliers in astronomical images with deep generative networks
  • Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
  • Distinguishing Mergers and Disks in High-redshift Observations of Galaxy Kinematics
  • Does black hole growth depend fundamentally on host-galaxy compactness?
  • Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ~ 2
  • Dust attenuation, dust content, and geometry of star-forming galaxies
  • Episodic star formation in a group of LAEs at z = 5.07.
  • Evidence for GN-z11 as a luminous galaxy at redshift 10.957
  • Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
  • Evidence of Environmental Quenching at Redshift z 2
  • Evident black hole-bulge coevolution in the distant universe
  • Evolution of Stellar-to-Halo Mass Ratio at z = 0 - 7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
  • Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
  • Extending the evolution of the stellar mass-size relation at z <= 2 to low stellar mass galaxies from HFF and CANDELS
  • Extremely Red Galaxies at z = 5-9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?
  • Fraction of Clumpy Star-forming Galaxies at 0.5 <= z <= 3 in UVCANDELS: Dependence on Stellar Mass and Environment
  • FUV and NIR size of the HI selected low surface brightness galaxies
  • Galaxy clustering measurements out to redshift z ~ 8 from Hubble Legacy Fields
  • Galaxy Ellipticity Measurements in the Near-infrared for Weak Lensing
  • Galaxy Evolution in All Five CANDELS Fields and IllustrisTNG: Morphological, Structural, and the Major Merger Evolution to z 3
  • Galaxy Inclination and the IRX-b Relation: Effects on UV Star Formation Rate Measurements at Intermediate to High Redshifts
  • Galaxy luminosity function pipeline for cosmology and astrophysics
  • Galaxy Merger Rates up to z ~ 3 Using a Bayesian Deep Learning Model: A Major-merger Classifier Using IllustrisTNG Simulation Data
  • Galaxy Mergers up to z < 2.5. II. AGN Incidence in Merging Galaxies at Separations of 3-15 kpc
  • Galaxy Mergers up to Z < 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3-15 kpc
  • Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
  • Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
  • GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
  • Half-mass Radii of Quiescent and Star-forming Galaxies Evolve Slowly from 0 z <= 2.5: Implications for Galaxy Assembly Histories
  • Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
  • HDUV: The Hubble Deep UV Legacy Survey
  • High Equivalent Width of Ha+N II Emission in z 8 Lyman-break Galaxies from IRAC 5.8 mm Observations: Evidence for Efficient Lyman-continuum Photon Production in the Epoch of Reionization
  • Improved photometric redshifts with colour-constrained galaxy templates for future wide-area surveys
  • Inference of the cosmic rest-frame from supernovae Ia
  • Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 < z < 3.0
  • Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
  • JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z 9 - 15
  • JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon
  • Late-time acceleration due to a generic modification of gravity and the Hubble tension
  • Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
  • Local Analogs to High-redshift Galaxies. I. Characterization of Dust Emission and Star Formation History
  • Lyman continuum leaker candidates at z ~ 3-4 in the HDUV based on a spectroscopic sample of MUSE LAEs
  • Mass assembly history of dark matter haloes in the light of H0 tension
  • MCSED: A Flexible Spectral Energy Distribution Fitting Code and Its Application to z ~ 2 Emission-line Galaxies
  • Millimeter Mapping at z ~ 1: Dust-obscured Bulge Building and Disk Growth
  • Mock light-cones and theory friendly catalogues for the CANDELS survey
  • Model-independent test of the running Hubble constant from the Type Ia supernovae and the Hubble parameter data
  • Morpheus: A Deep Learning Framework for the Pixel-level Analysis of Astronomical Image Data
  • Morphologies of ~190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lya Emitters
  • Nature versus nurture: what regulates star formation in satellite galaxies?
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • New Determinations of the UV Luminosity Functions from z 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency
  • New technique to select recent fast-quenching galaxies at z 2 using the optical colours
  • NIHAO-UHD: the properties of MW-like stellar discs in high-resolution cosmological simulations
  • Nonparametric reconstruction of interaction in the cosmic dark sector
  • Nonparametric Star Formation History Reconstruction with Gaussian Processes. I. Counting Major Episodes of Star Formation
  • Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
  • Observational constraints on the deceleration parameter in a tilted universe
  • Observational Constraints on the Merger History of Galaxies since z 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields
  • Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
  • Observations contradict galaxy size and surface brightness predictions that are based on the expanding universe hypothesis
  • Observations of Environmental Quenching in Groups in the 11 GYR since z = 2.5: Different Quenching for Central and Satellite Galaxies
  • On the AGN Nature of Two UV-bright Sources at zspec ~ 5.5 in the CANDELS Fields: An Update on the AGN Space Density at M1450 ~ -22.5
  • Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-luminous Infrared Galaxies at z > 1 and the Effect of Source Blending
  • Phantom dark energy as a natural selection of evolutionary processes a ^ la genetic algorithm and cosmological tensions
  • Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
  • Photometry of high-redshift blended galaxies using deep learning
  • Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-triggered AGN-Galaxy Coevolution Models?
  • Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
  • Probabilistic model for dynamic galaxy decomposition
  • Probing cosmic dawn: modelling the assembly history, SEDs, and dust content of selected z ~ 9 galaxies
  • Probing the Star Formation Main Sequence Down to 108 M at 1.0 < z < 3.0
  • Quantifying Non-parametric Structure of High-redshift Galaxies with Deep Learning
  • Quenching as a Contest between Galaxy Halos and Their Central Black Holes
  • Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon
  • Red and dead CANDELS: massive passive galaxies at the dawn of the Universe
  • Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
  • Revealing the formation histories of the first stars with the cosmic near-infrared background
  • Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
  • Selection of Massive Evolved Galaxies at 3 <= z <= 4.5 in the CANDELS Fields
  • Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
  • SMA Observations on Faint Submillimeter Galaxies with S 850 < 2 mJy: Ultra Dusty Low-luminosity Galaxies at High Redshift
  • Space Densities and Emissivities of Active Galactic Nuclei at z > 4
  • Spatially Resolved Properties of Galaxies from CANDELS+MUSE: Radial Extinction Profile and Insights on Quenching
  • Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
  • Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lya Emitters in COSMOS and GOODS-N
  • Spectroscopic Confirmation of the Rich z = 1.80 Galaxy Cluster JKCS 041 using the WFC3 Grism: Environmental Trends in the Ages and Structure of Quiescent Galaxies
  • Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
  • Stellar Populations of Lya-emitting Galaxies in the HETDEX Survey. I. An Analysis of LAEs in the GOODS-N Field
  • Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ~ 1 and z ~ 2 in the Absence of Infrared Data
  • Structural analysis of massive galaxies using HST deep imaging at z < 0.5
  • Studying the physical properties of tidal features - I. Extracting morphological substructure in CANDELS observations and VELA simulations
  • Subaru narrow-band imaging search for Lyman continuum from galaxies at z > 3 in the GOODS-N field
  • Texas Spectroscopic Search for Lya Emission at the End of Reionization I. Constraining the Lya Equivalent-width Distribution at 6.0 < z < 7.0
  • Texas Spectroscopic Search for Lya Emission at the End of Reionization. III. The Lya Equivalent-width Distribution and Ionized Structures at z > 7
  • The abundance of massive compact galaxies at 1.0 < z < 3.0 in 3D-HST/CANDELS
  • The Accretion History of AGN: The Spectral Energy Distributions of X-Ray-luminous Active Galactic Nuclei
  • The ALPINE-ALMA CII survey. Dust mass budget in the early Universe
  • The ALPINE-ALMA C II survey. Luminosity function of serendipitous C II line emitters at z ~ 5
  • The ALPINE-ALMA CII survey. The contribution of major mergers to the galaxy mass assembly at z ~ 5
  • The Assembly of Milky-Way-like Galaxies Since z ~ 2.5
  • The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field
  • The AstroSat UV deep field north: direct determination of the UV luminosity function and its evolution from z 0.8-0.4
  • The Carnegie-Irvine Galaxy Survey. VI. Quantifying Spiral Structure
  • The clustering properties of high-redshift passive galaxies
  • The connection between mergers and AGN activity in simulated and observed massive galaxies
  • The cosmic epoch dependence of environmental effects on size evolution of red-sequence early-type galaxies
  • The Dearth of z ~ 10 Galaxies in All HST Legacy Fields--The Rapid Evolution of the Galaxy Population in the First 500 Myr
  • The Effect of the Morphological Quenching Mechanism on Star Formation Activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
  • The emergence of passive galaxies in the early Universe
  • The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description
  • The Evolution of Galaxy Size and Morphology at z ~ 0.5-3.0 in the GOODS-N Region with Hubble Space Telescope/WFC3 Data
  • The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys
  • The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z~ 5
  • The GOGREEN survey: constraining the satellite quenching time-scale in massive clusters at z 1
  • The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0
  • The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections
  • The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
  • The Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: The Brightest Lyman-break Galaxies at z ~ 6
  • The MAGPI survey: evolution of radial trends in star formation activity across cosmic time
  • The Mass Dependence of Structure, Star Formation Rate, and Mass Assembly Mode at 0.5 < z < 2.5
  • The Mass-Metallicity Relation at z 1-2 and Its Dependence on the Star Formation Rate
  • The mass-metallicity-star formation rate relation at z 2 with 3D Hubble Space Telescope
  • The missing light of the Hubble Ultra Deep Field
  • The Morphology-Density Relationship in 1 < z < 2 Clusters
  • The MOSDEF survey: a comprehensive analysis of the rest-optical emission-line properties of z ~ 2.3 star-forming galaxies
  • The MOSDEF Survey: AGN Multi-wavelength Identification, Selection Biases, and Host Galaxy Properties
  • The MOSDEF survey: an improved Voronoi binning technique on spatially resolved stellar populations at z ~ 2
  • The MOSDEF Survey: Dissecting the Star Formation Rate versus Stellar Mass Relation Using Ha and Hb Emission Lines at z ~ 2
  • The MOSDEF Survey: Electron Density and Ionization Parameter at z ~ 2.3
  • The MOSDEF survey: probing resolved stellar populations at z 2 Using a new bayesian-defined morphology metric called patchiness
  • The MOSDEF survey: the dependence of H a-to-UV SFR ratios on SFR and size at z 2
  • The MOSDEF survey: towards a complete census of the z 2.3 star-forming galaxy population
  • The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 < z < 3.8
  • The Most Luminous z ~ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 Myr
  • The O IIIl5007 equivalent width distribution at z 2: the redshift evolution of the extreme emission line galaxies
  • The Pantheon+ Analysis: Cosmological Constraints
  • The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
  • The Pantheon+ Analysis: The Full Data Set and Light-curve Release
  • The Physical Properties of Massive Green Valley Galaxies as a Function of Environments at 0.5 < z < 2.5 in 3D-HST/Candels Fields
  • The Star Formation Rate-Radius Connection: Data and Implications for Wind Strength and Halo Concentration
  • The stellar host in star-forming low-mass galaxies: Evidence for two classes
  • The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
  • The structural properties of classical bulges and discs from z ~ 2
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  • The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4
  • The UV spectral slope b and stellar population of most active star-forming galaxies at z ~ 4
  • The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
  • Tracing the rise of supermassive black holes. A panchromatic search for faint, unobscured quasars at z 6 with COSMOS-Web and other surveys
  • TRINITY I: self-consistently modelling the dark matter halo-galaxy-supermassive black hole connection from z = 0-10
  • Two Massive, Compact, and Dust-obscured Candidate z 8 Galaxies Discovered by JWST
  • Two SNe Ia at Redshift ~2: Improved Classification and Redshift Determination with Medium-band Infrared Imaging
  • Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
  • Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS: Searching for Prompt Explosions in the Early Universe
  • Unbiased Differential Size Evolution and the Inside-out Growth of Galaxies in the Deep CANDELS GOODS Fields at 1 <= z <= 7
  • UV and NIR size of the low-mass field galaxies: the UV compact galaxies
Instrument ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2012-09-10T01:44:44Z/2013-01-06T00:14:48Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2013-01-07T19:56:02Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Faber comma Sandra M., 2013, 'Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- GOODS-North Field, Middle Visits of SNe Search', 1.0, European Space Agency, https://doi.org/10.5270/esa-hnusxjb