z~7 galaxy candidates from NICMOS observations over the HDF South and the CDF-S and HDF-N GOODS fields
arXiv:1003.1706 · doi:10.1088/0004-637X/725/2/1587
Abstract
We use ~88 arcmin**2 of deep (>~26.5 mag at 5 sigma) NICMOS data over the two GOODS fields and the HDF South to conduct a search for bright z>~7 galaxy candidates. This search takes advantage of an efficient preselection over 58 arcmin**2 of NICMOS H-band data where only plausible z>~7 candidates are followed up with NICMOS J-band observations. ~248 arcmin**2 of deep ground-based near-infrared data (>~25.5 mag, 5 sigma) is also considered in the search. In total, we report 15 z-dropout candidates over this area -- 7 of which are new to these search fields. Two possible z~9 J-dropout candidates are also found, but seem unlikely to correspond to z~9 galaxies. The present z~9 search is used to set upper limits on the prevalence of such sources. Rigorous testing is undertaken to establish the level of contamination of our selections by photometric scatter, low mass stars, supernovae (SNe), and spurious sources. The estimated contamination rate of our z~7 selection is ~24%. Through careful simulations, the effective volume available to our z>~7 selections is estimated and used to establish constraints on the volume density of luminous (L*(z=3), or -21 mag) galaxies from these searches. We find that the volume density of luminous star-forming galaxies at z~7 is 13_{-5}^{+8}x lower than at z~4 and >25x lower (1 sigma) at z~9 than at z~4. This is the most stringent constraint yet available on the volume density of >~L* galaxies at z~9. The present wide-area, multi-field search limits cosmic variance to <20%. The evolution we find at the bright end of the UV LF is similar to that found from recent Subaru Suprime-Cam, HAWK-I or ERS WFC3/IR searches. The present paper also includes a complete summary of our final z~7 z-dropout sample (18 candidates) identified from all NICMOS observations to date (over the two GOODS fields, the HUDF, galaxy clusters).
13 pages, 6 figures, 6 tables, accepted for publication in the Astrophysical Journal, replaced to match accepted version, see http://firstgalaxies.org/astronomers-area/ for a link to a complete reduction of the NICMOS observations over the two GOODS fields
References in corpus (36)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- The Hubble Ultra Deep Field
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- Galaxies in the Hubble Ultra Deep Field: I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
- UV Continuum Slope and Dust Obscuration from z~6 to z~2: The Star Formation Rate Density at High Redshift
- Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR Observations
- Large Area Survey for z=7 Galaxies in SDF and GOODS-N: Implications for Galaxy Formation and Cosmic Reionization
- z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
- The Stellar Mass Density and Specific Star Formation Rate of the Universe at z~7
- z~7 Galaxies in the HUDF: First Epoch WFC3/IR Results
- Structure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imaging of the HUDF
- Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?
- Galaxies at z = 6 - 9 from the WFC3/IR imaging of the HUDF
- On the Stellar Populations and Evolution of Star-Forming Galaxies at 6.3 < z < 8.6
- NICMOS Imaging of DRGs in the HDF-S: A Relation Between Star-Formation and Size at z ~ 2.5
- Star formation rates and stellar masses of z=7-8 galaxies from IRAC observations of the WFC3/IR ERS and the HUDF field
- New Constraints on the Lyman Continuum Escape Fraction at z~1.3
- A Deep HST Search for Escaping Lyman Continuum Flux at z~1.3: Evidence for an Evolving Ionizing Emissivity
- Ultradeep Infrared Array Camera Observations of sub-L* z~7 and z~8 Galaxies in the Hubble Ultra Deep Field: the Contribution of Low-Luminosity Galaxies to the Stellar Mass Density and Reionization
- The Great Observatories Origins Deep Survey - VLT/ISAAC Near-Infrared Imaging of the GOODS-South Field
- Discovery of a Very Bright Strongly-Lensed Galaxy Candidate at z ~ 7.6
- A Hubble & Spitzer Space Telescope Survey for Gravitationally-Lensed Galaxies: Further Evidence for a Significant Population of Low Luminosity Galaxies beyond Redshift Seven
- The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5
- The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3
- The UDF05 Follow-up of the HUDF: II. Constraints on Reionization from z-dropout Galaxies
- Rapid Evolution in the Most Luminous Galaxies During the First 900 Million Years
- z~7-10 Galaxies behind Lensing Clusters: Contrast with Field Search Results
- Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field
- Probing Lyman-break Galaxies at in GOODS-South with WFC3 on HST
- New Star Forming Galaxies at z\approx 7 from WFC3 Imaging
- Evidence for strong evolution of the cosmic star formation density at high redshift
- Galaxy Formation In The Reionization Epoch As Hinted By Wide Field Camera 3 Observations Of The Hubble Ultra Deep Field
- A Limit on the Number Density of Bright z~7 Galaxies
- Constraints on Star Forming Galaxies at z> 6.5 from HAWK-I Y-band Imaging of GOODS-South
- Light-Cone Distortion of the Clustering and Abundance of Massive Galaxies at High-Redshifts
Cited by in corpus (69)
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- The Dark Energy Survey: more than dark energy - an overview
- The Frontier Fields: Survey Design
- UV Luminosity Functions from 132 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR Observations
- The First Galaxies
- New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency
- JADES NIRSpec Spectroscopy of GN-z11: Lyman- emission and possible enhanced nitrogen abundance in a luminous galaxy
- The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
- 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
- JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr After the Big Bang
- Essential physics of early galaxy formation
- Observational Searches for Galaxies at z > 6
- The Bright End of the z~9 and z~10 UV Luminosity Functions using all five CANDELS Fields
- The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
- NIR Spectroscopy of Star-Forming Galaxies at z~1.4 with Subaru/FMOS: The Mass-Metallicity Relation
- Probability Distribution Functions of Cosmological Lensing: Convergence, Shear, and Magnification
- The size-luminosity relation at z=7 in CANDELS and its implication on reionization
- The escape fraction of ionizing photons from high redshift galaxies from data-constrained reionization models
- The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3
- Constraints on the star-formation rate of z~3 LBGs with measured metallicity in the CANDELS GOODS-South field
- JWST-JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11
- Gas Accretion as a Dominant Formation Mode in Massive Galaxies from the GOODS NICMOS Survey
- A Survey of MgII Absorption at 2 < z < 6 with Magellan / FIRE: I: Sample and Evolution of the MgII Frequency
- Precious Metals in SDSS Quasar Spectra I: Tracking the Evolution of Strong, 1.5 < z < 4.5 CIV Absorbers with Thousands of Systems
- Simulating the assembly of galaxies at redshifts z = 6 - 12
- The Physical Conditions of a Lensed Star-forming Galaxy at z=1.7
- Reionization and Galaxy Formation in Warm Dark Matter Cosmologies
- Early galaxy formation in warm dark matter cosmologies
- Bright galaxies at Hubble's redshift detection frontier: Preliminary results and design from the redshift z~9-10 BoRG pure-parallel HST survey
- A critical analysis of the UV Luminosity Function at redshift~7 from deep WFC3 data
- Young Galaxy Candidates in the Hubble Frontier Fields - III. MACSJ0717.5+3745
- Star Formation from DLA Gas in the Outskirts of Lyman Break Galaxies at z~3
- Keck/MOSFIRE Spectroscopy of z=7-8 Galaxies: Ly Emission from a Galaxy at z=7.66
- Galaxy properties in different environments up to z ~ 3 in the GOODS NICMOS Survey
- Searching for z~7.7 Lyman Alpha Emitters in the COSMOS Field with NEWFIRM
- Observing the first galaxies
- High-redshift galaxies and low-mass stars
- Precious Metals in SDSS Quasar Spectra II: Tracking the Evolution of Strong, 0.4 < z < 2.3 MgII Absorbers with Thousands of Systems
- Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
- Ultra-faint high-redshift galaxies in the Frontier Fields
- Mapping Compound Cosmic Telescopes Containing Multiple, Projected Cluster-Scale Halos
- Lyman-Break Galaxies at in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
- MgII Absorption at 2 < z < 6 with Magellan / FIRE. II: A Longitudinal Study of HI, Metals, and Ionization in Galactic Haloes
- MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field
- A model for GN-z11: top-heavy stellar initial mass functions in forming galactic nuclei and ultra-compact dwarfs
- Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
- Near-Infrared Survey of the GOODS-North Field: Search for Luminous Galaxy Candidates at z=>6.5
- Rapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
- MOS spectroscopy of protocluster candidate galaxies at z=6.5
- AGN Unification at z ~ 1: u - R Colors and Gradients in X-ray AGN Hosts
- Reionization and feedback in overdense regions at high redshift
- Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
- Far infrared constraints on the contamination by dust obscured galaxies of high-z dropout searches
- Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
- The Taiwan ECDFS Near-Infrared Survey: Very Bright End of the Luminosity Function at z>7
- Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North field
- Is GN-z11 powered by a super-Eddington massive black hole?
- Probing the nature of Dark Matter through the metal enrichment of the intergalactic medium
- X-ray stacking of Lyman break galaxies in the 4\,Ms CDF-S - X-ray luminosities and star formation rates across cosmic time
- Extragalactic Fields Optimized for Adaptive Optics
- Detecting Massive Galaxies at High Redshift using the Dark Energy Survey
- Modelling the escape of Lyman Continuum photons from galaxies in the Epoch of Reionization
- An ionised bubble powered by a proto-cluster at z = 6.5
- The effects of convection criteria on the evolution of population III stars and the detectability of their supernovae
- Is the Bremer Deep Field ionised, at z~7?
- CLUES to the past: Local Group progenitors amongst high-redshift Lyman Break Galaxies
- MIRI spectrophotometry of GN-z11: Detection and nature of an optical red continuum component
- Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope
- Direct N-body simulations of rotating and extremely massive Population III star clusters