Technical details for Advanced LIGO event data releasesFor the 4096-second data release associated with advanced LIGO events, the data is expressed at a time series of strain values at 4 kHz or 16 kHz, accompanied by two bitfield integers at 1 Hz, for Data Quality and Injections. Thus for each second several quality flags are combined into an integer with binary bits, for example the flags PASS FAIL FAIL PASS PASS PASS would be encoded as binary 100111, or 39 in decimal.
Data quality for event data releaseData quality categories are used to characterize the quality of the data at a given time. Data quality categories for this data release are defined and described in the paper "Characterization of Transient Noise in Advanced LIGO Relevant to Gravitational Wave Signal GW150914" (available from LIGO DCC or arXiv).
The meaning of the bits for Data Quality are:
In particular, the DATA bit channel defines the seconds when LIGO data are available: if the DATA flag is not set, the strain data will have NaN values. For this data release, the data pass all data quality categories, so the data quality bitfield integer is 1111111 binary = 127 decimal, for each of the 4096 seconds. See the LOSC tutorials page for information about how to access these, or the tutorial on segment lists.For a full description of Advanced LIGO data quality, see arXiv:1602.03844 and the segments tutorial. Generally:
Injections for the event data releasersThe second bitfield integer is to show injection status, where a 1 indicates NO injection.
During the 4096-seconds of the data release, there were no transient hardware injections during this time, and therefore all these bits are also equal to 1. However, there were (non-transient) pulsar injections in both detectors. Therefore the injection bitfield integer is 10111 binary = 23 decimal, for each of the 4096 seconds. Note that the amplitudes of these pulsar injections are such that they are probably too small to detect over the noise during this 4096-second release. If you need more information, please contact us at firstname.lastname@example.org.
Spectral LinesThere are in addition a variety of instrumental spectral lines in the data. These include harmonics of the mirror suspension resonances at ~500 Hz; electrical power lines at 60 Hz and harmonics; and calibration lines throughout the spectrum. Such lines are not relevant to the detection or analysis of this event.
Advanced LIGO data are not calibrated under 10 HzAdvanced LIGO detector noise rises rapidly below 10 Hz; it is many orders of magnitude larger than any conceivable gravitational wave strain signal. Further, the data made available on LOSC are aggressively high-pass-filtered at 8 Hz in order to avoid downstream signal processing problems, so it doesn't properly represent either signal or noise at those low frequencies. In particular, any DC offsets have no significance. In the Initial LIGO (S5 and S6) datasets, data below 40 Hz is similarly uncalibrated and suppressed. The 8 Hz roll-off is visible in this example low frequency spectrum.
Version 2 filesFor events GW150914, LVT151012, and GW151226, the tables point to version 2 of the data files (v2). These v2 data files were posted in October of 2016. They differ from v1 in that they use an updated version of the LIGO calibration (C02 instead of C01). Also, the v1 4096 Hz files included a minor time-offset, roughly 1 ms, introduced during the down-sampling process. This has been corrected in the v2 files.
Other DetailsLOSC strain data have been decimated from 16384 Hz to 4096 Hz. This has been done with the decimate method in the scipy package, with the "fir" filter type option: please see the tutorial associated with GW150914 for information about this. Files of duration 32 sec and 4096 sec are computed independently, by decimation, from the 16 kHz data. There may be a slight difference between them, at the level of one part in 10^8. This is because the decimation filter used was an infinite impulse response filter."