An Observational Pursuit for Population III Stars in a Ly_alpha Emitter at z=6.33 through HeII Emission
arXiv:astro-ph/0508443 · doi:10.1086/497135
Abstract
We present a very deep near-infrared spectroscopic observation of a strong Ly_alpha emitter at z=6.33, SDF J132440.6+273607, which we used to search for HeII 1640. This emission line is expected if the target hosts a significant number of population III stars. Even after 42 ksec of integration with the Subaru/OHS spectrograph, no emission-line features are detected in the JH band, which confirms that SDF J132440.6+273607 is neither an active galactic nucleus nor a low- emission-line object. We obtained a 2sigma upper-limit of 9.06e-18 ergs/s/cm^2 on the HeII 1640 emission line flux, which corresponds to a luminosity of 4.11e42 ergs/s. This upper-limit on the HeII 1640 luminosity implies that the upper limit on population III star-formation rate is in the range 4.9--41.2 M_sun/yr if population III stars suffer no mass loss, and in the range 1.8--13.2 M_sun/yr if strong mass loss is present. The non-detection of HeII in SDF J132440.6+273607 at z=6.33 may thus disfavor weak feedback models for population III stars.
13 pages, 3 figures, to appear in The Astrophysical Journal Letters
References in corpus (37)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- The Nucleosynthetic Signature of Population III
- The Formation of the First Star in the Universe
- The Formation of the First Stars. I. The Primordial Star Forming Cloud
- On the properties of massive Population III stars and metal-free stellar populations
- Forming the First Stars in the Universe: The Fragmentation of Primordial Gas
- The transition from Population III to normal galaxies: Ly-a and HeII 1640 emission and the ionising properties of high redshift starburst galaxies
- Generic Spectrum and Ionization Efficiency of a Heavy Initial Mass Function for the First Stars
- Formation of the First Stars by Accretion
- On the Initial Mass Function of Population III Stars
- A Redshift z = 6.56 Galaxy Behind the Cluster Abell 370
- Zero-Metallicity Stars and the Effects of the First Stars on Reionization
- Signatures of Stellar Reionization of the Universe
- The Subaru Deep Field Project: Lyman Emitters at Redshift of 6.6
- Early Reionization by the First Galaxies
- The Detectability of the First Stars and Their Cluster Enrichment Signatures
- The Discovery of Two Lyman Emitters Beyond Redshift 6 in the Subaru Deep Field
- IRTS observation of the near-infrared extragalactic background light
- The Contribution of the First Stars to the Cosmic Infrared Background
- The Subaru Deep Field: The Optical Imaging Data
- Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope
- The Detectability of High Redshift Lyman Alpha Emission Lines Prior to the Reionization of the Universe
- The Imprint of the Cosmic Dark Ages on the Near Infrared Background
- The Cosmic Infrared Background at 1.25 microns and 2.2 microns using DIRBE and 2MASS: a contribution not due to galaxies ?
- Spectroscopic Properties of the z=4.5 Lyman-alpha Emitters
- Detection of the Cosmic Infrared Background at 2.2 and 3.5 microns Using DIRBE Observations
- A Luminous Lyman-alpha Emitting Galaxy at Redshift z=6.535: Discovery and Spectroscopic Confirmation
- HeII Recombination Lines From the First Luminous Objects
- A Galaxy at z = 6.545 and Constraints on the Epoch of Reionization
- Cosmological Effects of the First Stars: Evolving Spectra of Population III
- CISCO: Cooled Infrared Spectrograph and Camera for OHS on the Subaru Telescope
- A deep, narrow J-band search for proto-galactic Lyman Alpha emission at redshifts z~9
- A Lyman alpha emitter at z = 6.5 found with slitless spectroscopy
- OHS: OH-airglow Suppressor for the Subaru Telescope
- A Strong Lyman-alpha Emitter at z=6.33 in the Subaru Deep Field Selected as an i' Dropout
- Early Enrichment of Quasars by First Stars
- The effects of population III stars on the chemical and photometrical evolution of ellipticals
Cited by in corpus (28)
- The First Galaxies
- The spectral evolution of the first galaxies. I. James Webb Space Telescope detection limits and color criteria for population III galaxies
- Population III stars: hidden or disappeared ?
- SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
- Metal-Free Gas Supply at the Edge of Reionization: Late-Epoch Population III Star Formation
- Significant primordial star formation at redshifts z ~ 3-4
- The First Galaxies: Signatures of the Initial Starburst
- HeII emitters in the VIMOS VLT Deep Survey: PopIII star formation or peculiar stellar populations in galaxies at 2<z<4.6?
- The physical properties of Lyalpha emitting galaxies: not just primeval galaxies?
- Spitzer Constraints on the z=6.56 Galaxy Lensed by Abell 370
- The Discovery of a Large Lyman-alpha+HeII Nebula at z~1.67: A Candidate Low Metallicity Region?
- A photometric survey for Lyalpha-HeII dual emitters: Searching for Population III stars in high-redshift galaxies
- A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
- A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
- Ly-alpha emitters in the GOODS-S field: a powerful pure nebular SED with N IV] emission at z=5.563
- Lyman alpha Luminosity Functions at Redshift z = 4.5
- Probing Population III Stars in Galaxy IOK-1 at z = 6.96 through He II Emission
- Ly Emitters with Very Large Ly Equivalent Widths, EW(Ly) Å, at
- Deep rest-frame far-UV spectroscopy of the giant Lyman-alpha emitter 'Himiko'
- First HETDEX Spectroscopic Determinations of Ly and UV Luminosity Functions at : Bridging a Gap Between Faint AGN and Bright Galaxies
- Population III Star Clusters in the Reionized Universe
- Spectroscopy of i-Dropout Galaxies with an NB921-Band Depression in the Subaru Deep Field
- High-redshift Ly alpha emitters with a large equivalent width: Properties of i-dropout galaxies with an NB921-band depression in the Subaru Deep Field
- CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview
- Constraining Very High Mass Population III Stars through He II Emission in Galaxy BDF-521 at z = 7.01
- The search for Population III stars
- Revealing the formation histories of the first stars with the cosmic near-infrared background
- Star Forming Galaxies at z > 5