Constraints on z~10 Galaxies from the Deepest HST NICMOS Fields
arXiv:astro-ph/0503116 · doi:10.1086/430302
Abstract
We use all available fields with deep NICMOS imaging to search for J dropouts (H<28) at z~10. Our primary data set for this search were the two J+H NICMOS parallel fields taken with the ACS HUDF. The 5 sigma limiting mags were 28.6 in J and 28.5 in H. Several shallower fields were also used: J+H NICMOS frames available over the HDF North, the HDF South NICMOS parallel, and the ACS HUDF. The primary selection criterion was (J-H)>1.8. 11 such sources were found in all search fields using this criterion. 8 of these were clearly ruled out as credible z~10 sources, either as a result of detections (>2 sigma) blueward of J or their colors redward of the break (H-K~1.5). The nature of the 3 remaining sources could not be determined from the data. The number appears consistent with the expected contamination from low-z interlopers. Analysis of the stacked images for the 3 candidates also suggests contamination. Regardless of their true redshifts, the actual number of z~10 sources must be <=3. To assess the significance of these results, two lower redshift samples (a z~3.8 B-dropout and z~6 i-dropout sample) were projected to z~8-12 using a (1+z)^{-1} size scaling. They were added to the image frames, and the selection repeated, giving 15.6 and 4.8 J-dropouts, respectively. This suggests that to the limit of this probe (0.3 L*) there has been evolution from z~3.8 and possibly from z~6. This is consistent with the strong evolution already noted at z~6 and z~7.5 relative to z~3-4. Even assuming that 3 sources from this probe are at z~10, the rest-frame continuum UV (~1500 A) luminosity density at z~10 (integrated down to 0.3 L*) is just 0.19_{-0.09}^{+0.13}x that at z~3.8 (or 0.19_{-0.10}^{+0.15}x including cosmic variance). However, if none of our sources is at z~10, this ratio has a 1 sigma upper limit of 0.07. (abridged)
13 pages, 3 figures, 2 tables, accepted for publication in the Astrophysical Journal Letters
Cited by in corpus (67)
- The James Webb Space Telescope
- On the normalisation of the cosmic star formation history
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Observational constraints on Cosmic Reionization
- UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
- Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
- The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >5: Evidence for a photon starved and extended epoch of reionization
- Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts
- Formation of z ~ 6 quasars from hierarchical galaxy mergers
- A galaxy at a redshift z = 6.96
- z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
- The First Appearance of the Red Sequence of Galaxies in Proto-Clusters at 2<~z<~3
- A Keck Survey for Gravitationally-Lensed Lyman-alpha Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low Luminosity Sources to Cosmic Reionization
- The redshift distribution of SWIFT Gamma-Ray Bursts: evidence for evolution
- Spitzer Imaging of i'-drop Galaxies: Old Stars at z~6
- The Stellar Masses and Star Formation Histories of Galaxies at z ~ 6: Constraints from Spitzer Observations in the Great Observatories Origins Deep Survey
- The Stellar Mass Density at z~6 from Spitzer Imaging of i-drop Galaxies
- The Epoch of Reionization
- Focusing Cosmic Telescopes: Exploring Redshift z~5-6 Galaxies with the Bullet Cluster 1E0657-56
- A Hubble & Spitzer Space Telescope Survey for Gravitationally-Lensed Galaxies: Further Evidence for a Significant Population of Low Luminosity Galaxies beyond Redshift Seven
- Expanded Search for z~10 Galaxies from HUDF09, ERS, and CANDELS Data: Evidence for Accelerated Evolution at z>8?
- Constraints on the IMF of the first stars
- The Role of the Dust in Primeval Galaxies: A Simple Physical Model for Lyman Break Galaxies and Lyman Alpha Emitters
- A New Measurement of the Stellar Mass Density at z~5: Implications for the Sources of Cosmic Reionization
- Lyman Alpha Emitters at z=7 in the Subaru/XMM-Newton Deep Survey Field: Photometric Candidates and Luminosity Function
- Star Formation Feedback and Metal Enrichment History Of The Intergalactic Medium
- The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form?
- Updating reionization scenarios after recent data
- Constraining the population of 6 < z < 10 star-forming galaxies with deep near-IR images of lensing clusters
- Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies using X-ray Emission: Results from the Chandra Deep Fields
- SPACE: the SPectroscopic All-sky Cosmic Explorer
- Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field
- Searching for the reionization sources
- Faint InfraRed Extragalactic Survey: Data and Source Catalogue of the MS1054-03 field
- Constraints on the Cosmic Near Infrared Background Excess from NICMOS Deep Field Observations
- Star-Forming or Starbursting? The Ultraviolet Conundrum
- An Empirically-Calibrated Model For Interpreting the Evolution of Galaxies During the Reionization Era
- Evidence for strong evolution of the cosmic star formation density at high redshift
- A Brighter Past: Galaxy Luminosity Function At High Redshifts
- Probing the star formation history using the redshift evolution of luminosity functions
- Constraining reionization using 21 cm observations in combination with CMB and Lyman-alpha forest data
- Constrained semi-analytical models of Galactic outflows
- The effect of peculiar velocities on the epoch of reionization (EoR) 21-cm signal
- On the nature of the sources of the cosmic infrared background
- Observing the first galaxies
- Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
- Where are the sources of the Near Infrared Background?
- Supernova progenitors and iron density evolution from SN rate evolution measurements
- Lyman Break Galaxies at z~5: Rest-frame UV Spectra II
- Expanding the search for galaxies at z ~7-10 with new NICMOS Parallel Fields
- Scenario Machine: fast radio bursts, short gamma-ray burst, dark energy and Laser Interferometer Gravitational-wave Observatory silence
- Constraints on Star Forming Galaxies at z> 6.5 from HAWK-I Y-band Imaging of GOODS-South
- A Lyman Break Galaxy Candidate at z~9
- Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
- SuperNova Acceleration Probe (SNAP): Investigating Photometric Redshift Optimization
- Detectable Signatures of Cosmic Radiative Feedback
- The Infrared Glow of First Stars
- A search for Lyman Break Galaxies at z>8 in the NICMOS Parallel Imaging Survey
- Searching for the Sources Responsible for Cosmic Reionization: Probing 7 < z < 10 and Beyond
- Star Formation Rate and Extinction in Faint z~4 Lyman-Break Galaxies
- Large Scale Structure traced by Molecular Gas at High Redshift
- First Light and Reionization: A Conference Summary
- Negative feedback effects on star formation history and cosmic reionization
- Modelling the evolution of dusty starburst galaxies in multi-band deep surveys
- A survey of NB921 dropouts in the Subaru Deep Field
- Simulations of Early Galaxy Formation
- Star Forming Galaxies at z > 5