This tutorial is meant to show the general process followed to generate LDC data, including gravitational-wave (GW) signal and noise.
The objective is to:
- Display source parameter: get the first MBHB from spritz
- Compute h+,hx with the LDC
- Compute projected strain with gw-response and save to file
- Compute projected strain with the LDC
- Inject GW signal in lisa-instrument or in pyTDI
This tutorial shows how to use the fast waveform generators to match signals injected in LDC datasets.
The objective is to:
- Generate fast waveforms in the frequency domain for Galactic binaries (GB)
- Generate fast waveforms in the frequency domain for massive black hole binaries (MBHB)
- Generate fast waveforms for EMRI (if time permits)
- Plot the waveform against simulated data
This tutorial shows the general process to follow when analysing LDC data to detect and characterize gravitational-waves from Galactic compact binaries sources.
The objective is to:
1. Load and plot the TDI data in time and frequency domain
2. Compute a source SNR
3. Compute a likelihood
4. Compute the F-statistics
5. Detect sources using the F-statistics
6. Perform parameter estimation
This tutorial shows the general process to follow when analyzing LDC data to detect and characterize gravitational-waves from massive black hole binary sources.
The objective is to:
1. Load and plot the TDI data in time and frequency domain
2. Compute a source SNR
3. Compute a likelihood
4. Transformation to LISA frame and how it helps
6. Perform parameter estimation in the noiseless case
