New 145-MHz Source Measurements by PAPER in the Southern Sky
arXiv:1105.1367 · doi:10.1088/2041-8205/734/2/L34
Abstract
We present observations from the Precision Array for Probing the Epoch of Reionization (PAPER) in South Africa, observed in May and September 2010. Using two nights of drift scanning with PAPER's 60\arcdeg\ FWHM beam we have made a map covering the entire sky below +10 degrees declination with an effective center frequency of 145 MHz, a 70-MHz bandwidth, and a resolution of 26\arcmin. A 4800 square-degree region of this large map with the lowest Galactic emission reaches an RMS of 0.7 Jy. We establish an absolute flux scale using sources from the 160-MHz Culgoora catalog. Using the 408-MHz Molonglo Reference Catalog (MRC) as a finding survey, we identify counterparts to 480 sources in our maps, and compare our fluxes to the MRC and to 332 sources in the Culgoora catalog. For both catalogs, the ratio of PAPER to catalog flux averages to 1, with a standard deviation of 50%. This measured variation is consistent with comparisons between independent catalogs observed at different bands. The PAPER data represent new 145-MHz flux measurements for a large number of sources in the band expected to encompass cosmic reionization, and represents a significant step toward establishing a model for removing foregrounds to the reionization signal.
arXiv comment3 figures, 2 tables, machine readable table. Accepted by ApJL
References in corpus (16)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Observational constraints on Cosmic Reionization
- A model of diffuse Galactic Radio Emission from 10 MHz to 100 GHz
- The Precision Array for Probing the Epoch of Reionization: 8 Station Results
- The VLA Low-frequency Sky Survey
- The Murchison Widefield Array: Design Overview
- The non-coplanar baselines effect in radio interferometry: The W-Projection algorithm
- The GMRT-EoR Experiment: A new upper limit on the neutral hydrogen power spectrum at z~8.6
- Advances in Calibration and Imaging Techniques in Radio Interferometry
- Calibration of Low-Frequency, Wide-Field Radio Interferometers Using Delay/Delay-Rate Filtering
- A Scalable Correlator Architecture Based on Modular FPGA Hardware, Reuseable Gateware, and Data Packetization
- The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory
- A search for steep spectrum radio relics and halos with the GMRT
- The Molonglo Southern 4 Jy sample (MS4). I. Definition
- Radio Frequency Spectra of 388 Bright 74 MHz Sources
Cited by in corpus (32)
- GLEAM: The GaLactic and Extragalactic All-sky MWA survey
- The Giant Radio Array for Neutrino Detection (GRAND): Science and Design
- New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7
- PAPER-64 Constraints on Reionization: The 21cm Power Spectrum at z=8.4
- The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts
- Initial deep LOFAR observations of Epoch of Reionization windows: I. The North Celestial Pole
- The Impact of Modeling Errors on Interferometer Calibration for 21 cm Power Spectra
- First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating
- A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype
- The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations
- Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421
- Multi-redshift limits on the 21cm power spectrum from PAPER
- Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWA
- The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology
- Discovery of HI gas in a young radio galaxy at using the Australian Square Kilometre Array Pathfinder
- A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz
- The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14,110 Compact Radio Sources over 6,100 Square Degrees
- DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra
- A Technique for Primary Beam Calibration of Drift-Scanning, Wide-Field Antenna Elements
- Radio Sources in the NCP Region Observed with the 21 Centimeter Array
- Low Frequency Imaging of Fields at High Galactic Latitude with the Murchison Widefield Array 32-Element Prototype
- Investigating the cause of the - relation
- A Flux Scale for Southern Hemisphere 21cm EoR Experiments
- Probing reionization with the cross power spectrum of 21 cm and near-infrared radiation backgrounds
- The brightness and spatial distributions of terrestrial radio sources
- ViCTORIA project: The LOFAR HBA Virgo Cluster Survey
- Imaging on PAPER: Centaurus A at 148 MHz
- The precision and accuracy of early Epoch of Reionization foreground models: comparing MWA and PAPER 32-antenna source catalogs
- A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field
- Pre-selection of the Candidate Fields for Deep Imaging of the Epoch of Reionization with SKA1-Low
- Influence of synchrotron self-absorption on the 21cm experiments
- A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies