High-Frequency GW Sources. Bernard F Schutz Albert Einstein Institute – Max Planck Institute for Gravitational Physics, Golm, Germany and Cardiff University, Cardiff, UK http://www.aei.mpg.de [email protected] Ground-based GW Astronomy.
1s noise in
log(f/Hz)Upper limits on some known pulsars
What sources might live in this band (cf Ungarelli & Vecchio)?
Assume Sh = 10-44 Hz-1 between 0.1 and 10 Hz, observation
lasts up to one year, chirping binary at z = 1.
Binary chirp mass (solar)
log(SNR) intermediate band
Binary chirp mass (solar)Chirp sensitivity of LISA follow-on instrument in intermediate band. II