Fetching the paper…
Reading the bibliography…
We present a simplified method for the extraction of meaningful signals from Hanford and Livingstone 32 seconds data for the GW150914 event made publicly available by the LIGO collaboration and demonstrate its ability to reproduce the LIGO collaboration's own results quantitatively given the assumption that all narrow peaks in the power spectrum are a consequence of physically uninteresting signals and can be removed.
Whelan, J. T., Sundaresan, S., Zhang, Y., & Peiris, P. 2015, Phys. Rev. D, 91, 102005
2015
Earlier work this paper cites.
Abbott, B. P., Abbott, R., Abbott, T. D., et al. 2016, Physical Review Letters, 116, 061102
2016
Earlier work this paper cites.
Abbott, B. P., Abbott, R., Abbott, T. D., et al. 2016, Physical Review Letters, 116, 241103
2016
Earlier work this paper cites.
The LIGO Scientific Collaboration, Martynov, D. V., Hall, E. D., et al. 2016, arXiv:1604.00439
2016
Cited alongside, same era.
The LIGO Scientific Collaboration, & the Virgo Collaboration 2016, arXiv:1602.03843
2016
Cited alongside, same era.
The LIGO data are publicly available at https://losc.ligo.org/events/GW150914/ . In this work, we use the strain time series centered at GPS 1126259462 with a 16384 Hz sampling rate and 32 and 4096 second length. An official tutorial about how to use the data is available at https://losc.ligo.org/s/events/GW150914/GW150914_tutorial.html
2016
Cited alongside, same era.
https://losc.ligo.org/events/GW151226/
2016
Closest in time.
LIGO Scientific Collaboration, “LIGO Open Science Center release of GW150914”, 2016, DOI 10.7935/K5MW2F23
2016
Closest in time.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…