This folder contains the following files selected for their peculiarities:
| Name | peculiarity |
|---|---|
2004-FKV1137.fits |
only 1 Nwave |
2008-Contest_Binary.oifits |
no particular, no OI_VIS table |
2009-11-eps_Aur-avg5.oifits |
a lot of tables for OI_ARRAY (26), OI_WAVELENGTH (26), OI_VIS2(26), OI_T3(26) |
2012-03-24_ALL_oiDataCalib.fits |
A lot of target (18) |
AMBER_070409.fits |
INSNAME = AMBER and 2 table for datas. |
GGTauA_H_MJD56269_CAL_HD28462_V990Tau7Holesb-copy.oifits |
no OI_ARRAY, no OI_VIS, 2 target and INSNAME = SAM |
GRAVITY.2016-01-09T05-37-06-singlesci_calibrated.fits |
V2 file, OI_FLUX, have VISDATA complex colunm |
GRAVI.2016-06-23T03:10:17.458_singlesciviscalibrated.fits |
More compliant oifits V2 60.A-9174(A) (Kraus et al. 2017) : Zooming in on the accretion processes in high-mass star formation SVT GRAVITY |
NGC5128_2005.oifits |
ARRNAME = VLTI and INSNAME = MIDI/PRISM |
PRODUCT_V838_Mon_1.90-2.53micron_2013-04-15T01_49_24.8034--------0.00000------------inf--------1--------2--------3.fits |
V2 file, new colunm on table. |
TEST_CreateOIFileV1.fits |
Your creating file for V1, no particularity (have header cards) |
T_PYX_oiDataCalib.fits |
INSNAME = PIONIER_Pnat, 2 OI_WAVELENGTH, 2 OI_VIS2, 3 OI_T3. |
bigtest2.fits |
V2 file, OI_CORR, OI_INSPOL. |
Mystery-Med_H-AmberVISPHI.oifits |
1 extra byte at the End of file + NaN in vis* data |
A-CLUSTER__2T3T__1-PHASEREF__SIMPLE_nsr0.05__20160812_193521_1.oifits |
sample synthetic oifits file from the gomes2016 public collection |
A-CLUSTER__2T3T__1-PHASEREF__SIMPLE_nsr0.05__20160812_193521_1.image-oi.oifits |
copy of previous file with an image and IMAGE-OI INPUT PARAM HDUs generated by OImaging software |
testdata_opt.fits |
full v2 file with all keyword and column for tests |