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Round 1 - Data Sets
These are the original datasets for MLDC Round 1 which was completed on Dec 4, 2006. The key files with information about the sources included in the blind challenge data set are now available here.
Complete information on the Round 1 challenges, including the LISA model, the source models, and the parameter range specifications are discussed in Sixth LISA Symposium (Overview,HOW-TO) and in the Round 1 challenge specification document.
Challenge 1.1 - Galactic White Dwarf Binaries
Challenge 1.1.1 - Single Galactic Binaries
- a) 1 year of Gaussian stationary instrument noise + 1 exactly monochromatic WD with SNR ~10 ->20 over 1 year (for single IFO) at frequency 1.0+/-.1 mHz
- b) 1 year of Gaussian stationary instrument noise + 1 exactly monochromatic WD with SNR ~10 -> 20 over 1 year (for single IFO) at frequency a 3.0+/-.1 mHz
- c) 1 year of Gaussian stationary instrument noise + 1 exactly monochromatic WD with SNR ~10 -> 20 over 1 year (for single IFO) at frequency a 10+/-1 mHz
Challenge 1.1.2 - Verification Binaries
1 year of Gaussian stationary instrument noise with 5 true verification binaries (parameters chosen according to our current best guess) + 15 mock verification binaries in the frequency range 0.5 mHz - 12 mHz. All the signals will be monochromatic (no fdot). Since these are verification binaries, the sky locations and orbital frequencies will be given. The orientation parameters and distances will be considered unknown.
Challenge 1.1.3 - Resolvable Binaries* (LISA Simulator Training data were corrected 26 Oct 2006.)
1 year of Gaussian stationary instrument noise with 20 resolvable binaries (parameters chosen from the BLT population synthesis code) with frequencies spread over the LISA band. All the signals will be monochromatic (no fdot).
*The LISA Simulator Training Data sets for Challenge 1.1.3 had been created with the wrong simulator version, giving an inconsistent noise relaization. The blind challenge, and synthetic LISA data sets were not affected. Corrected data were uploaded 26 Oct 2006.
Challenge 1.1.4 - Source Confusion* (LISA Simulator Training data were corrected 26 Oct 2006.)
1 year of Gaussian stationary instrument noise with 40 < N < 60 WD binaries chosen with frequencies f in a narrow band ( 3.000 mHz < f < 3.015 mHz ) and with SNR > 5. Sources are drawn from the BLT population synthesis code. All the signals will be monochromatic (no fdot). The number of sources will not be given.
*The LISA Simulator Training Data sets for Challenge 1.1.4 had been created with the wrong simulator version, giving an inconsistent noise relaization. The blind challenge, and synthetic LISA data sets were not affected. Corrected data were uploaded 26 Oct 2006.
Challenge 1.1.5 - Strong Source Confusion
1 year of Gaussian stationary instrument noise with 30 < N < 50 WD binaries chosen with frequencies f in a very narrow band ( 2.9985 mHz < f < 3.0015 mHz ) and with SNR > 5. Sources are drawn from the BLT population synthesis code. All the signals will be monochromatic (no fdot). The number of sources will not be given.
Challenge 1.2 - MBH Binaries * (These data were corrected 18 Sep 2006)
Challenge 1.2.1*
1 year of Gaussian stationary instrument noise + 1 Schwarzschild SMBH binary with time to coalescence 6(+/-1) months and masses m1 1-5 million solar masses and m2 = m1/x, where 1 < x < 4 . The signals have SNR for one IFO in the range 450 < SNR < 500 . The waveform model for the inspiral is restricted to the 2PN approximation with no spin-orbit nor spin-spin modultations.
Challenge 1.2.2*
1 year of Gaussian stationary instrument noise + 1 Schwarzschild SMBH binary with time to coalescence 400+/-40 days and masses m1 1-5 million solar masses and m2 = m1/x, where 1 < x < 4 . The signals have SNR for one IFO in the range 20 < SNR < 100 . The waveform model for the inspiral is restricted to the 2PN approximation with no spin-orbit nor spin-spin modultations.
*If you have downloaded BBH merger data before 18 Sep 2006, please update your data. A correction was made to the key files on 28 Sep 2006.
Challenge 1.3 - EMRIs
Challenge 1.3 is on a different timescale from the other Round 1 challenges and is now being administered in coordination with Round 2.
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