The star formation history inferred from long gamma-ray bursts with high pseudo-redshifts

Abstract

By employing a simple semi-analytical star formation model where the formation rates of Population (Pop) I/II and III stars can be calculated, respectively, we account for the number distribution of gamma-ray bursts (GRBs) with high pseudo-redshifts that was derived from an empirical luminosity-indictor relationship. It is suggested that a considerable number of Pop III GRBs could exist in the present sample of Swift GRBs. By further combining the implication for the star formation history from the optical depth of the CMB photons, it is also suggested that only a very small fraction 0.6% of Pop III GRBs could have triggered the Swift BAT. These results could provide an useful basis for estimating future detectability of Pop III stars and their produced transient phenomena.

arXiv comment5 pages, 3 figures, 1 table, accepted for publication in New Astronomy

References in corpus (59)

• Large scale bias and the peak background split
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• On the normalisation of the cosmic star formation history
• The Nucleosynthetic Signature of Population III
• A very energetic supernova associated with the gamma-ray burst of 29 March 2003
• The Formation of the First Star in the Universe
• In the Beginning: The First Sources of Light and the Reionization of the Universe
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters
• Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
• The Formation of the First Stars. I. The Primordial Star Forming Cloud
• Massive Black Holes as Population III Remnants
• The history of star formation in a LCDM universe
• A Photometric Redshift of z ~ 9.4 for GRB 090429B
• The Formation of the First Low-Mass Stars From Gas With Low Carbon and Oxygen Abundances
• Protostellar Feedback Halts the Growth of the First Stars in the Universe
• The Radiative Feedback of the First Cosmological Objects
• Revealing the High-Redshift Star Formation Rate with Gamma-Ray Bursts
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Early star-forming galaxies and the reionization of the Universe
• On the Association of Gamma-ray Bursts with Massive Stars: Implications for Number Counts and Lensing Statistics
• The abundance and clustering of dark haloes in the standard Lambda CDM cosmogony
• The Star Formation Rate in the Reionization Era as Indicated by Gamma-ray Bursts
• Very low metallicity massive star models: Pre-SN evolution and primary nitrogen production
• Population III stars: hidden or disappeared ?
• The First Stars: Mass Growth Under Protostellar Feedback
• High-Redshift Gamma-Ray Bursts from Population III Progenitors
• Three Epochs of Star Formation in the High Redshift Universe
• Cosmological Gamma-Ray Bursts and Evolution of Galaxies
• Two populations of metal-free stars in the early Universe
• The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization Era
• Reheating of the Universe and Population III
• The redshift distribution of SWIFT Gamma-Ray Bursts: evidence for evolution
• An Unexpectedly Swift Rise in the Gamma-ray Burst Rate
• Population III.1 and III.2 gamma-Ray Bursts: Constraints on the event rate for future radio and X-ray surveys
• Population III Gamma Ray Bursts
• Can Gamma-Ray Burst Jets Break Out the First Stars?
• Metal Absorption Lines as Probes of the Intergalactic Medium Prior to the Reionization Epoch
• Do long-duration GRBs follow star formation?
• Is Double Reionization Physically Plausible?
• Spitzer Observations of Gamma-Ray Burst Host Galaxies: A Unique Window into High Redshift Chemical Evolution and Star-formation
• Evidence for Luminosity Evolution of Long Gamma-ray Bursts in Swift Data
• The high-redshift star formation rate derived from GRBs: possible origin and cosmic reionization
• Protostellar Feedback and Final Mass of the Second-Generation Primordial Stars
• Gravitational wave backgrounds and the cosmic transition from Population III to Population II stars
• Probing cosmic star formation up to z = 9.4 with GRBs
• High-redshift star formation rate up to z~8.3 derived from gamma-ray bursts and influence of background cosmology
• The Number and Observability of Population III Supernovae at High Redshifts
• An Evolving Stellar Initial Mass Function and the Gamma-Ray Burst Redshift Distribution
• The luminosity function of Swift long gamma-ray bursts
• The Role of Heating and Enrichment in Galaxy Formation
• The First Stars in the Universe and Cosmic Reionization
• Redshift distribution and luminosity function of long gamma-ray bursts from cosmological simulations
• High Redshift Gamma-Ray Bursts: Observational Signatures of Superconducting Cosmic Strings?
• The Lack of Gamma-Ray Bursts from Population III Binaries
• Determining the luminosity function of Swift long gamma-ray bursts with pseudo-redshifts
• Outflow or galactic wind: The fate of ionized gas in the halos of dwarf galaxies
• The Reionization History and Early Metal Enrichment inferred from the Gamma-Ray Burst Rate
• Cosmic histories of star formation and reionization: An analysis with a power-law approximation

Cited by in corpus (2)

• Compact Binary Mergers and The Event Rate of Fast Radio Bursts
• Research on the redshift evolution of luminosity function and selection effect of GRBs