Discovering the Sky at the Longest Wavelengths with Small Satellite Constellations
arXiv:1907.10853
Abstract
Due to ionosphere absorption and the interference by natural and artificial radio emissions, ground observation of the sky at the decameter or longer is very difficult. This unexplored part of electromagnetic spectrum has the potential of great discoveries, notably in the study of cosmic dark ages and dawn, but also in heliophysics and space weather, planets, cosmic ray and neutrinos, pulsar and interstellar medium, extragalactic radio sources, and even SETI. At a forum organized by the International Space Science Institute-Beijing (ISSI-BJ), we discussed the prospect of opening up this window for astronomical observations by using a constellation of small or micro-satellites. We discussed the past experiments and the current ones such as the low frequency payload on Chang'e-4 mission lander, relay satellite and the Longjiang satellite, and also the future DSL mission, which is a linear array on lunar orbit which can make synthesized map of the whole sky as well as measure the global spectrum. We also discuss the synergy with other experiments, including ground global experiments such as EDGES, SARAS, SCI-HI and High-z, PRIZM/Albatros, ground imaging facillities such as LOFAR and MWA, and space experiments such as SUNRISE, DARE/DAPPER and PRATUSH. We also discussed some technical aspects of the DSL concept.
arXiv commentThe report of the ISSI-BJ forum on "Discovering the Sky at the Longest Wavelengths with Small Satellite Constellations" held on January 23-25, 2019. 62 pages
References in corpus (29)
- LOFAR: The LOw-Frequency ARray
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- An absorption profile centred at 78 megahertz in the sky-averaged spectrum
- Upper limits on the 21-cm Epoch of Reionization power spectrum from one night with LOFAR
- Experimental Limit on the Cosmic Diffuse Ultra-high Energy Neutrino Flux
- A lower limit of dz > 0.06 for the duration of the reionization epoch
- Charting the Parameter Space of the Global 21-cm Signal
- Signature of Excess Radio Background in the 21-cm Global Signal and Power Spectrum
- Statistics of Giant Radio Halos from Electron Reacceleration Models
- Design and characterization of the Large-Aperture Experiment to Detect the Dark Age (LEDA) radiometer systems
- First results on the Epoch of Reionization from First Light with SARAS 2
- The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z=20-25 from LOFAR
- SARAS 2: A Spectral Radiometer for probing Cosmic Dawn and the Epoch of Reionization through detection of the global 21 cm signal
- LUNASKA experiments using the Australia Telescope Compact Array to search for ultra-high energy neutrinos and develop technology for the lunar Cherenkov technique
- Revised statistics of radio halos and the re-acceleration model
- Constraining High Redshift X-ray Sources with Next Generation 21 cm Power Spectrum Measurements
- First evidence of diffuse ultra-steep-spectrum radio emission surrounding the cool core of a cluster
- A Space-Based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21-cm Global Spectrum
- Charting the Parameter Space of the 21-cm Power Spectrum
- Low Frequency Observations of the Moon with the Murchison Widefield Array
- Quantifying Suppression of the Cosmological 21-cm Signal due to Direction Dependent Gain Calibration in Radio Interferometers
- Space VLBI: from first ideas to operational missions
- Wide-field LOFAR-LBA power-spectra analyses: Impact of calibration, polarization leakage and ionosphere
- Brute-Force Mapmaking with Compact Interferometers: A MITEoR Northern Sky Map from 128 MHz to 175 MHz
- Measuring the global 21-cm signal with the MWA-I: improved measurements of the Galactic synchrotron background using lunar occultation
- FIRST Explorer -- An innovative low-cost passive formation-flying system
- Radio Interferometers Larger than Earth: Lessons Learned and Forward Look of Space VLBI
- SETI surveys of the nearby and distant universe employing wide-field radio interferometry techniques
- Measuring the 21 cm Global Brightness Temperature Spectrum During the Dark Ages with the SCI-HI Experiment
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- The Electrical Design of a Membrane Antenna for Lunar-based Low-frequency Radio Telescope
- Confronting global 21-cm signal with symmetric dark matter models
- The Array of Long Baseline Antennas for Taking Radio Observations from the Sub-Antarctic
- On the accuracy of posterior recovery with neural network emulators
- Recovering 21cm Monopole Signals Without Smoothness
- An SBC-based controller and processor for the laboratory model of PRATUSH Digital Receiver