Hermes files made by Pieter Vuylsteke on 10 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 65583 | 14.886 | 30 | 2461110.342498 | -23.431169 | 120.13375 | 29.21236 | 0.00 | ||||
| HRF | HD42818 | 14.886 | 480 | 2461110.3474686 | -20.292194 | 94.71157 | 69.31979 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 30 | 2461110.3522436 | -11.980762 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TIC 354388980 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 1250 | 2461110.3620582 | -28.27831 | 88.99254 | 40.4682 | 0.00 | ||||
| | HRF | TIC 264594193 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 320 | 2461110.3725886 | -27.946719 | 80.77304 | 1.05692 | 0.00 | |||
| | HRF | TIC 431800989 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 1001 | 2461110.3809326 | -26.686613 | 53.80925 | 42.59079 | 0.00 | |||
| | HRF | TIC 2778177 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 3000 | 2461110.4080246 | -29.63186 | 80.5825 | 33.78623 | 0.00 | |||
| HRF | HD57060 | One observation every run is sufficient, the S/N must be higher than 120 (it is important) | 120 | 2461110.4303281 | -16.630455 | 109.66824 | -24.5587 | 0.00 | ||||
| | HRF | Gaia DR3 3032784851342772608 | One observation every run is sufficient, the S/N must be higher than 120 (it is important) | 2600 | 2461110.4481298 | -20.175909 | 110.28484 | -13.37213 | 0.00 | |||
| HRF | V*VYPyx | One observation every run is sufficient, the S/N must be higher than 120 (it is important) | 400 | 2461110.4691525 | -9.715321 | 133.62346 | -23.52182 | 0.00 | ||||
| | HRF | TYC1941-1035-1 | One observation every run is sufficient, the S/N must be higher than 120 (it is important) | 1800 | 2461110.4840534 | -21.572953 | 126.54231 | 22.95492 | 0.00 | |||
| | HRF | Gaia DR3 808086453088065280 | long period variable: observe once per run | 1000 | 2461110.5027028 | -14.230761 | 150.30613 | 43.66706 | 0.00 | |||
| | HRF | Gaia DR3 828300630766393344 | long period variable: observe once per run | 1200 | 2461110.5190327 | -14.43906 | 150.5103 | 52.8775 | 0.00 | |||
| | HRF | HR4049 | sparsly sampled spectra | 240 | 2461110.5322067 | -0.090834 | 154.53162 | -28.99222 | 0.00 | |||
| | HRF | HR4049 | sparsly sampled spectra | 240 | 2461110.5378802 | -0.105853 | 154.53162 | -28.99222 | 0.00 | |||
| | HRF | V*RUMa | High priority: first Mira SB !! | 366 | 2461110.5415247 | -12.166296 | 161.1603 | 68.77575 | 0.00 | |||
| | HRF | Gaia DR3 722395361541004416 | long period variable: observe once per run | 720 | 2461110.5530014 | -9.478819 | 157.3401 | 23.06213 | 0.00 | |||
| | HRF | LoTr5 | long period variable: observe once per run | 550 | 2461110.5624878 | 5.750187 | 193.8906 | 25.89183 | 0.00 | |||
| | HRF | LoTr5 | long period variable: observe once per run | 550 | 2461110.5694384 | 5.73211 | 193.8906 | 25.89183 | 0.00 | |||
| | HRF | Gaia DR3 628305547347284608 | long period variable: observe once per run | 700 | 2461110.5793204 | -11.419924 | 152.08312 | 20.00371 | 0.00 | |||
| | HRF | V* TX CVn | long period variable: observe once per run | 1000 | 2461110.5908412 | 1.625495 | 191.17525 | 36.76406 | 0.00 | |||
| | HRF | HD105262 | long period variable: observe once per run | 480 | 2461110.6028207 | 3.597504 | 181.79511 | 12.98547 | 0.00 | |||
| | HRF | HD95241 | long period variable: observe once per run | 240 | 2461110.6081123 | -9.243577 | 165.08615 | 42.91172 | 0.00 | |||
| | HRF | R_Hya | ATOMIUM object. Pulsator | 600 | 2461110.6156035 | 18.909254 | 202.42825 | -23.28132 | 0.00 | |||
| | HRF | V*ALVir | ATOMIUM object. Pulsator | 800 | 2461110.6252942 | 21.62039 | 212.78771 | -13.31067 | 0.00 | |||
| | HRF | BD+16_3061 | Binary. Halo star discovered by Bond. similar to post-AGB binaries | 3600 | 2461110.6499723 | 23.643345 | 247.45246 | 14.26198 | 0.00 | |||
| | HRF | TYC 6190-434-1 | sparse sampling | 2000 | 2461110.688712 | 28.175947 | 237.07438 | -17.73769 | 0.00 | |||
| | HRF | BD+32_2754 | Possible pagb star | 549 | 2461110.7055927 | 16.811315 | 249.04871 | 32.48927 | 0.00 |
Hermes files made by Pieter Vuylsteke on 11 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 82106 | 29.913 | 35 | 2461111.4613552 | -13.477941 | 142.47833 | 5.65514 | 0.00 | ||||
| HRF | HD46300 | 29.913 | 360 | 2461111.4625094 | -27.624269 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 30 | 2461111.4655342 | -12.016153 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TIC237629152 | Observe at random times, but not more often than once per same run for same target | 3000 | 2461111.4871306 | -25.989745 | 103.44549 | 2.82949 | 0.00 |
Hermes files made by Pieter Vuylsteke on 12 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 65583 | 14.886 | 30 | 2461112.3679684 | -24.102469 | 120.13375 | 29.21236 | 0.00 | ||||
| HRF | HD46300 | 14.886 | 360 | 2461112.371173 | -27.554172 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 30 | 2461112.3746993 | -12.04033 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TIC 2010901 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 1250 | 2461112.3839464 | -29.464911 | 79.27525 | 35.32126 | 0.00 | ||||
| HRF | TIC122104755 | Observe at random times, but not more often than once per same run for same target | 2600 | 2461112.4078805 | -28.645453 | 76.28945 | 41.24089 | 0.00 | ||||
| HRF | Gaia DR3 3032784851342772608 | Observe at random times, but not more often than once per same run for same target | 1800 | 2461112.4384535 | -20.634413 | 110.28484 | -13.37213 | 0.00 | ||||
| HRF | TIC 234259427 | Binary, Orbital period 1.51 days. Please observe in consecutive nights for best phase coverage. | 3200 | 2461112.4686151 | -26.613602 | 102.04083 | 3.96144 | 0.00 | ||||
| HRF | TIC 440775832 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 50-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 3600 | 2461112.510774 | -26.477918 | 108.84775 | 12.34468 | 0.00 | ||||
| HRF | V*VHya | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 50-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 900 | 2461112.5416862 | 0.888883 | 162.90523 | -21.25009 | 0.00 | ||||
| | HRF | IRAS09371+1212 | Frosty Leo PPNe | 3000 | 2461112.5688152 | -14.246288 | 144.97483 | 11.98128 | 0.00 | |||
| | HRF | V* T CrB | Frosty Leo PPNe | 1000 | 2461112.5917138 | 18.349542 | 239.87567 | 25.92017 | 0.00 | |||
| | HRF | HD146116 | SB? | 60 | 2461112.6024942 | 26.626752 | 243.65998 | -0.39875 | 0.00 | |||
| | HRF | V* V934 Her | SB? | 70 | 2461112.6041314 | 20.67863 | 256.64379 | 23.97185 | 0.00 | |||
| HRF | HD 128165 | 11.392 | 72 | 2461112.6099341 | 3.038045 | 218.37042 | 52.90878 | 0.00 | ||||
| HRF | HD118098 | 11.392 | 280 | 2461112.6169113 | 15.027604 | 203.6733 | -0.59582 | 0.00 | ||||
| HRF | V*TDra | SB, Mira Variable V from 7 to13 | 60 | 2461112.6169342 | 4.54169 | 269.09708 | 58.21849 | 0.00 | ||||
| | HRF | BT_Lib | SB, Mira Variable V from 7 to13 | 3200 | 2461112.641349 | 27.254751 | 232.81615 | -23.36006 | 0.00 | |||
| | HRF | EM* StHA 149 | SB, Mira Variable V from 7 to13 | 3600 | 2461112.679818 | 18.585951 | 274.73279 | 27.44103 | 0.00 | |||
| | HRF | V*AC_Her | sparsly sampled spectra | 104 | 2461112.7028802 | 20.36685 | 277.56763 | 21.86683 | 0.00 | |||
| | HRF | CC_Lyr | very depleted (low Fe abundance) star so higher S/N because of the lack of lines | 3600 | 2461112.7265188 | 16.386537 | 278.48921 | 31.64005 | 0.00 |
Hermes files made by Pieter Vuylsteke on 13 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 62613 | -7.752 | 60 | 2461113.3461003 | -15.288158 | 119.07167 | 80.26556 | 0.00 | ||||
| HRF | HD46300 | -7.752 | 700 | 2461113.3537345 | -27.655136 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 70 | 2461113.3598691 | -12.063513 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | HD35652 | All the observations can be done during one or two (non-consecutive) runs to follow the triple (outer) stars. | 1300 | 2461113.3698373 | -29.491957 | 81.96833 | 34.78285 | 0.00 | ||||
| HRF | TIC 234259427 | Binary, Orbital period 1.51 days. Please observe in consecutive nights for best phase coverage. | 3600 | 2461113.4023083 | -26.629908 | 102.04083 | 3.96144 | 0.00 | ||||
| HRF | TIC 264594193 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 640 | 2461113.4268693 | -28.048539 | 80.77304 | 1.05692 | 0.00 | ||||
| HRF | TIC2943965 | Observe at random times, but not more often than once per same run for same target | 5000 | 2461113.4638864 | -29.742599 | 82.02828 | 33.78579 | 0.00 | ||||
| HRF | V*RCrt | Get orbit (Jets + rapid rotation) | 1200 | 2461113.5486834 | 0.783947 | 165.14105 | -18.32488 | 0.00 | ||||
| | HRF | V*VHya | Get orbit (Jets + rapid rotation) | 1202 | 2461113.5641059 | 0.352625 | 162.90523 | -21.25009 | 0.00 | |||
| | HRF | HD98839 | Get orbit (Jets + rapid rotation) | 90 | 2461113.5734092 | -8.456963 | 170.70658 | 43.48269 | 0.00 | |||
| | HRF | Gaia DR3 1020598239437675776 | long period variable: observe once per run | 120 | 2461113.5752702 | -16.669214 | 146.03273 | 53.76674 | 0.00 | |||
| | HRF | Gaia DR3 1046469816758286336 | long period variable: observe once per run | 720 | 2461113.5815526 | -15.609911 | 149.44973 | 58.24428 | 0.00 | |||
| | HRF | HD123949 | forthcoming periastron passage of a very eccentric system | 600 | 2461113.5931755 | 21.179959 | 212.74715 | -19.14395 | 0.00 | |||
| | HRF | V* T CrB | forthcoming periastron passage of a very eccentric system | 1200 | 2461113.6038721 | 18.13079 | 239.87567 | 25.92017 | 0.00 | |||
| | HRF | Gaia DR3 1165299020534791552 | long period variable: observe once per run | 1200 | 2461113.6204257 | 22.246118 | 234.79255 | 10.5785 | 0.00 | |||
| | HRF | Gaia DR3 1222377898949342208 | long period variable: observe once per run | 720 | 2461113.6332716 | 17.029647 | 233.90235 | 25.75276 | 0.00 | |||
| | HRF | Gaia DR3 1226842362832655488 | long period variable: observe once per run | 720 | 2461113.6454485 | 15.632419 | 214.52019 | 13.1677 | 0.00 | |||
| | HRF | Gaia DR3 1285985917926276736 | long period variable: observe once per run | 160 | 2461113.652704 | 11.514042 | 220.30566 | 31.57217 | 0.00 | |||
| | HRF | Gaia DR3 1369659543073383680 | long period variable: observe once per run | 450 | 2461113.6582232 | 15.459615 | 237.74478 | 31.50096 | 0.00 | |||
| | HRF | Gaia DR3 1372316959598411520 | long period variable: observe once per run | 240 | 2461113.6654091 | 13.852622 | 239.6279 | 36.02215 | 0.00 | |||
| | HRF | V*TDra | SB, Mira Variable V from 7 to13 | 67 | 2461113.6700789 | 4.514585 | 269.09708 | 58.21849 | 0.00 | |||
| | HRF | Gaia DR3 1475404077441813632 | long period variable: observe once per run | 240 | 2461113.6783195 | 3.907827 | 202.68315 | 37.77466 | 0.00 | |||
| | HRF | V*TDra | SB, Mira Variable V from 7 to13 | 120 | 2461113.6784875 | 4.507695 | 269.09708 | 58.21849 | 0.00 | |||
| | HRF | Gaia DR3 1503941145827097984 | long period variable: observe once per run | 450 | 2461113.6876832 | 2.104508 | 205.7374 | 46.13524 | 0.00 | |||
| | HRF | V*TDra | SB, Mira Variable V from 7 to13 | 600 | 2461113.6922424 | 4.495423 | 269.09708 | 58.21849 | 0.00 | |||
| | HRF | Gaia DR3 1589555924392273024 | long period variable: observe once per run | 180 | 2461113.701097 | 5.716932 | 227.89573 | 49.90301 | 0.00 | |||
| | HRF | V*AC_Her | sparsly sampled spectra | 80 | 2461113.702056 | 20.474089 | 277.56763 | 21.86683 | 0.00 | |||
| HRF | TIC271960811 | Observe at random times, but not more often than once per same run for same target | 3600 | 2461113.7243963 | 9.194584 | 295.67877 | 42.32081 | 0.00 |
Hermes files made by Pieter Vuylsteke on 14 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 42807 | 6.1 | 60 | 2461114.3502974 | -28.792579 | 93.30208 | 10.62714 | 0.00 | ||||
| HRF | HD46300 | 6.1 | 450 | 2461114.355672 | -27.799671 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 50 | 2461114.3600766 | -12.083557 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TIC 234259427 | Binary, Orbital period 1.51 days. Please observe in consecutive nights for best phase coverage. | 2400 | 2461114.3785147 | -26.737571 | 102.04083 | 3.96144 | 0.00 | ||||
| HRF | Gaia DR3 2924741405657605760 | Binary, Orbital period 1.51 days. Please observe in consecutive nights for best phase coverage. | 2200 | 2461114.4065635 | -19.657995 | 98.71591 | -23.48423 | 0.00 | ||||
| HRF | TIC2688362 | Observe at random times, but not more often than once per same run for same target | 1800 | 2461114.4304768 | -29.824992 | 80.44855 | 32.38538 | 0.00 | ||||
| HRF | TIC 2010901 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 3600 | 2461114.463433 | -29.555807 | 79.27525 | 35.32126 | 0.00 | ||||
| | HRF | TIC 2778177 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 4000 | 2461114.5093203 | -29.771997 | 80.5825 | 33.78623 | 0.00 | |||
| HRF | V*RCrt | Get orbit (Jets + rapid rotation) | 1200 | 2461114.5475264 | 0.30104 | 165.14105 | -18.32488 | 0.00 | ||||
| | HRF | Gaia DR3 628305547347284608 | long period variable: observe once per run | 720 | 2461114.5627672 | -13.267094 | 152.08312 | 20.00371 | 0.00 | |||
| | HRF | Gaia DR3 722395361541004416 | long period variable: observe once per run | 720 | 2461114.5727294 | -11.446543 | 157.3401 | 23.06213 | 0.00 | |||
| | HRF | Gaia DR3 808086453088065280 | long period variable: observe once per run | 1200 | 2461114.5847916 | -15.896374 | 150.30613 | 43.66706 | 0.00 | |||
| | HRF | Gaia DR3 828300630766393344 | long period variable: observe once per run | 1200 | 2461114.5997959 | -15.850072 | 150.5103 | 52.8775 | 0.00 | |||
| | HRF | Gaia DR3 836944681947087744 | long period variable: observe once per run | 720 | 2461114.6128546 | -13.026214 | 160.47168 | 51.63325 | 0.00 | |||
| | HRF | Gaia DR3 837969014467045888 | long period variable: observe once per run | 240 | 2461114.6209769 | -10.898175 | 166.89974 | 49.17703 | 0.00 | |||
| | HRF | HD123949 | forthcoming periastron passage of a very eccentric system | 900 | 2461114.6307745 | 20.699683 | 212.74715 | -19.14395 | 0.00 | |||
| | HRF | V* T CrB | forthcoming periastron passage of a very eccentric system | 1200 | 2461114.6438644 | 17.848488 | 239.87567 | 25.92017 | 0.00 | |||
| | HRF | CC_Lyr | very depleted (low Fe abundance) star so higher S/N because of the lack of lines | 4200 | 2461114.6742777 | 16.6447 | 278.48921 | 31.64005 | 0.00 | |||
| | HRF | V*AC_Her | sparsly sampled spectra | 110 | 2461114.7012188 | 20.575116 | 277.56763 | 21.86683 | 0.00 | |||
| | HRF | V*AC_Her | sparsly sampled spectra | 300 | 2461114.8026933 | 20.382937 | 277.56763 | 21.86683 | 0.00 |
Hermes files made by Pieter Vuylsteke on 15 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 42807 | 6.1 | 30 | 2461115.3467832 | -28.871187 | 93.30208 | 10.62714 | 0.00 | ||||
| HRF | HD46300 | 6.1 | 360 | 2461115.3512817 | -27.918668 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | TYC5917-726-1 | At most one epoch per run. S/N of 20-25 required in at least one of B or V bands. | 1200 | 2461115.3614276 | -23.128215 | 85.77154 | -16.4827 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 50 | 2461115.3732523 | -12.100159 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TYC5917-726-1 | At most one epoch per run. S/N of 20-25 required in at least one of B or V bands. | 1200 | 2461115.3832656 | -23.177533 | 85.77154 | -16.4827 | 0.00 | ||||
| HRF | Gaia DR3 2924741405657605760 | At most one epoch per run. S/N of 20-25 required in at least one of B or V bands. | 2000 | 2461115.4047719 | -19.766981 | 98.71591 | -23.48423 | 0.00 | ||||
| HRF | TIC 426415358 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 3400 | 2461115.437276 | -28.922906 | 86.41158 | 39.7847 | 0.00 | ||||
| HRF | Betelgeuse | Very bright!! Take care for saturation | 2 | 2461115.4585918 | -29.011196 | 88.79294 | 7.40706 | 0.00 | ||||
| HRF | TIC 354388980 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 2500 | 2461115.4752898 | -28.788038 | 88.99254 | 40.4682 | 0.00 | ||||
| HRF | V*RCrt | Get orbit (Jets + rapid rotation) | 900 | 2461115.5028448 | -0.055452 | 165.14105 | -18.32488 | 0.00 | ||||
| | HRF | Gaia DR3 3945026181200439424 | long period variable: observe once per run | 720 | 2461115.5140257 | 5.464293 | 196.97165 | 23.62477 | 0.00 | |||
| | HRF | Gaia DR3 846200199030154880 | long period variable: observe once per run | 1200 | 2461115.52621 | -9.245111 | 176.75627 | 58.23826 | 0.00 | |||
| | HRF | Gaia DR3 847599155778203776 | long period variable: observe once per run | 1200 | 2461115.5424353 | -14.47 | 156.20053 | 51.17802 | 0.00 | |||
| | HRF | Gaia DR3 1679548064908345600 | long period variable: observe once per run | 720 | 2461115.5543749 | -7.159164 | 195.51739 | 68.232 | 0.00 | |||
| HRF | HD87887 | long period variable: observe once per run | 360 | 2461115.5685114 | -10.433631 | 151.9845 | -0.37164 | 0.00 | ||||
| HRF | HD 128165 | 11.392 | 36 | 2461115.5707625 | 2.359901 | 218.37042 | 52.90878 | 0.00 | ||||
| HRF | V*BFSer | Pop II Cepheid with dust | 3600 | 2461115.5953995 | 18.611639 | 229.11871 | 16.44436 | 0.00 | ||||
| | HRF | V*ALVir | Pop II Cepheid with dust | 1000 | 2461115.6251967 | 19.67949 | 212.78771 | -13.31067 | 0.00 | |||
| | HRF | HD123949 | forthcoming periastron passage of a very eccentric system | 300 | 2461115.6344829 | 20.301911 | 212.74715 | -19.14395 | 0.00 | |||
| | HRF | V* T CrB | forthcoming periastron passage of a very eccentric system | 597 | 2461115.6400448 | 17.644742 | 239.87567 | 25.92017 | 0.00 | |||
| | HRF | HD134698 | SB1 very long orbit | 168 | 2461115.6477375 | 24.220212 | 227.92376 | -10.50766 | 0.00 | |||
| | HRF | HD137569 | SB1 very long orbit | 300 | 2461115.6523639 | 19.656252 | 231.58674 | 14.69342 | 0.00 | |||
| | HRF | BD-21 3873 | SB1 very long orbit | 1800 | 2461115.6678804 | 20.928228 | 214.14288 | -21.7639 | 0.00 | |||
| | HRF | CC_Lyr | very depleted (low Fe abundance) star so higher S/N because of the lack of lines | 2500 | 2461115.6897925 | 16.717665 | 278.48921 | 31.64005 | 0.00 | |||
| | HRF | BD-11_3853 | SB1 very long orbit | 1300 | 2461115.7188021 | 23.452277 | 225.12889 | -12.44907 | 0.00 | |||
| HRF | HD345431 | At most one epoch per run. S/N of 20-25 required in at least one of B or V bands. | 2000 | 2461115.7339911 | 16.004098 | 300.17956 | 23.2671 | 0.00 |
Hermes files made by Pieter Vuylsteke on 16 - 03 - 2026
| program | File | Fiber | Star | Simbad | Sp.Type | comment | Exp. time | BJD | BVCOR | RA | DEC | SNR65 |
| HRF | HD 42807 | 6.1 | 30 | 2461116.3404501 | -28.933504 | 93.30208 | 10.62714 | 0.00 | ||||
| HRF | HD46300 | 6.1 | 360 | 2461116.3451008 | -28.024199 | 98.22595 | 7.33296 | 0.00 | ||||
| HRF | alfUMi | tonight at z < 2 | 30 | 2461116.3488335 | -12.111878 | 37.9545 | 89.26411 | 0.00 | ||||
| HRF | TIC 234259427 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 4200 | 2461116.3774743 | -27.053203 | 102.03783 | 3.96144 | 0.00 | ||||
| HRF | Gaia DR3 3445116310345060096 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 2000 | 2461116.4140708 | -29.831122 | 87.24033 | 31.53244 | 0.00 | ||||
| HRF | TIC285419474 | Observe at random times, but not more often than once per same run for same target | 3100 | 2461116.4450942 | -28.348065 | 78.50671 | 42.95363 | 0.00 | ||||
| HRF | TIC 306112725 | Uniform coverage of the binary orbit required (8 epochs per binary period), SNR 80-100. Please consult the spreadsheet of P122 for instructions and needed times of observations for each target. Please search objects by name (TIC or KIC number) as the scheduler"s GOB numbers are reassigned from time to time | 6000 | 2461116.5003763 | -25.970666 | 87.72067 | 53.97322 | 0.00 | ||||
| HRF | TYC 807-636-1 | sparse sampling | 2400 | 2461116.5543977 | -23.46754 | 125.04017 | 13.47525 | 0.00 |
134 files made by Pieter Vuylsteke between Tuesday 10 March 2026 and Monday 16 March 2026