Authors: The Event Horizon Telescope Collaboration et al.
Date: March, 2024
Primary Reference: The Event Horizon Telescope Collaboration, et al. 2024, A&A, 681, A79
Data Product Code: 2024-D01-01
Brief Description:
We release a data set to accompany the M87 Event Horizon Telescope (EHT) Results from the April 2018 observing campaign (EHT Collaboration et al. 2024). The data set is derived from the Level 2 Version 1 (L2V1) of the calibrated data released internally within the collaboration. It is now made public simultaneously with four imaging pipelines used to produce the images in the paper, and one direct modeling pipeline.
This data set contains M87 data for all four bands (b1, b2, b3, and b4) for three of the observed days (April 21st, 22nd, 27th, 2018). Data from the 2018 observations were processed through two independent reduction pipelines (Blackburn et al. 2019, Janssen et al. 2019, Paper III). This release includes the fringe fitted, a-priori calibrated, and network calibrated data from both the EHT-HOPS and CASA rPICARD pipelines. Independent flux calibration is performed based on estimated station sensitivities during the campaign (Koay et al. 2023). A description of the data properties, their validation, and estimated systematic errors is given in Section 3 of the 2018 M87 paper (EHT Collaboration et al. 2024).
The data are time averaged to 10 seconds and frequency averaged over all 32 intermediate frequencies (IFs). All polarization information is explicitly removed. To make the resulting uvfits files compatible with popular very-long-baseline interferometry (VLBI) software packages, the circularly polarized cross-hand visibilities RL and LR are set to zero along with their errors, while parallel-hands RR and LL are both set to an estimated Stokes I value. Measurement errors for RR and LL are each set to sqrt(2) times the statistical errors for Stokes I.
All uvfits files are located in the "uvfits/" subdirectory. Easy-to-read csv and txt files are derived from the uvfits files and provided in "csv/" and "txt/", respectively. Finally, the run.sh script in the top directory will convert uvfits files into csv and txt files.
The three tgz files are gzipped tarballs that contains uvfits, txt, and csv files, respectively. They are included in this repository for convenience.
File Name Convention:
The data files are named in the following convention:
[Data-Release-Tag]_[Source]_[year]_[day-of-year]_[band]_[pipeline]_[stage]_StokesI.[format]
Station Code Table:
| UVFITS Code | Station Name | Location |
|---|---|---|
| AA | ALMA | Chile |
| AX | APEX | Chile |
| GL | Greenland Telescope | Greenland |
| LM | Large Millimeter Telescope | Mexico |
| MG | Submillimeter Telescope | Arizona |
| MM | James Clerk Maxwell Telescope | Hawai'i |
| PV | IRAM | Spain |
| SW | Submillimeter Array | Hawai'i |
References:
- EHT Collaboration Data Portal Website
- The Event Horizon Telescope Collaboration, et al. 2024, A&A, 681, A79
- Blackburn, L., Chan, C.-k., Crew, G., et al. 2019, ApJ, 822, 23
- Janssen, M., Goddi, C., van Bemmel, I., et al. 2019, A&A, 626, A75
- Koay, J. Y., Romero-Cañizales, C., Matthews, L., et al. 2023, EHT Memo 2023-L1-01