| Name | Plot | Ra | Dec | Orbital Period [d] | Ranking | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Activity Prob | Average flux [mCrab] | Data | Activity Prob | Average flux [mCrab] | Data | Activity Prob | Average pulsed flux [keV·cm-2·s-1] | Data | ||||||
| - | -0.4 | Jun 18th | - | 0.3 | Jun 17th | - | 0.075 | Jun 12th | 215.303 | -62.698 | 42.12 | 0 | ||
| - | 3.1 | Jun 19th | - | 1.1 | Jun 17th | - | 0.047 | Jun 11th | 19.633 | 63.74 | 24.3 | 0 | ||
| - | -6.6 | Jun 9th | - | 26.2 | Jun 3rd | - | 0.079 | Jun 12th | 84.727 | 26.316 | 111.1 | 0 | ||
| - | 3.5 | May 24th | - | -4.5 | Jun 17th | - | 0.018 | Jun 12th | 324.878 | 56.986 | 23.85 | 0 | ||
| 100% | 70.6 | Jun 19th | 100% | 133.1 | Jun 17th | 1.7% | 0.184 | Jun 12th | 152.442 | -58.292 | 249.48 | 140.21 | ||
| - | 5.5 | Apr 21st | - | 1.5 | Jun 17th | - | 0.06 | Jun 12th | 128.979 | -43.185 | 105.8 | 0 | ||
| - | 3 | Jun 18th | - | 10.1 | Jun 17th | - | 0.096 | Jun 11th | 195.321 | -61.602 | 132.189 | 0 | ||
| - | -10.9 | Apr 21st | 195.498 | -63.968 | 0 | |||||||||
| - | 3.9 | May 29th | - | -3.2 | Jun 17th | - | 0.093 | Jun 11th | 297.398 | 30.209 | 40.4 | 0 | ||
| - | 2 | Apr 21st | - | 17.9 | Jun 17th | - | 0.057 | Jun 12th | 70.247 | 44.53 | 155 | 0 | ||
| - | -43.4 | Apr 21st | - | 10.5 | Jun 17th | - | 0.173 | Jun 12th | 212.011 | -61.983 | 0 | |||
| 100% | 47.9 | May 24th | - | 0.8 | Jun 17th | - | 0.047 | Jun 9th | 315.899 | 45.752 | 12.7 | 1.23 | ||
| - | 14.9 | Apr 21st | - | -20.6 | Jun 16th | 280.899 | -3.73 | 0 | ||||||
| 27.4% | 16.2 | Jun 18th | 100% | 60.4 | Jun 17th | - | 0.035 | Jun 12th | 53.75 | 53.173 | 34.25 | 35.8 | ||
| 76.6% | 42.2 | Apr 21st | - | 1.1 | Jun 17th | - | 0.095 | Jun 11th | 284.688 | 3.432 | 0.43 | |||
| - | -2.1 | Apr 21st | - | 1 | Jun 17th | - | 0.088 | Jun 12th | 296.417 | 27.356 | 169.2 | 0 | ||
| - | -2.2 | Jun 17th | 246.65 | -51.941 | 132.9 | 0 | ||||||||
| - | -5.1 | Apr 21st | - | -7 | Jun 17th | - | 0.048 | Jun 11th | 104.6 | -7.2 | 0 | |||
| - | 2.3 | May 26th | 78.1% | 82.9 | Jun 17th | 3.1% | 0.235 | Jun 12th | 308.064 | 37.637 | 46.03 | 21.09 | ||
| 67.7% | 27.8 | Jun 19th | - | 41.5 | Jun 17th | 58.846 | 31.046 | 250.3 | 33.85 | |||||
| - | -5.9 | Jun 17th | 72.778 | -69.801 | 0 | |||||||||
| - | 1.7 | Jun 17th | 300.091 | 32.1898 | 0 | |||||||||
| - | 13.7 | Jun 17th | 26.751 | 61.357 | 0 | |||||||||
| - | -8.2 | Jun 16th | - | 0.253 | Jun 12th | 267.291 | -26.637 | 29.82 | 0 | |||||
| - | 1.5 | Jun 19th | - | 0.3 | Jun 17th | - | 0.055 | Jun 12th | 239.454 | -54.415 | 29.56 | 0 | ||
| - | 7.5 | Jun 17th | - | 0.056 | Jun 11th | 284.775 | 8.25 | 0 | ||||||
| - | 10 | Apr 21st | - | 3.1 | Jun 17th | 177 | -62.207 | 187.5 | 0 | |||||
| - | 13.6 | Jun 8th | - | 9.6 | Jun 16th | 282.074 | -2.42 | 242.18 | 0 | |||||
| 1% | 3.3 | Apr 21st | - | -3.4 | Jun 17th | 13.6508 | -73.676 | 0.01 | ||||||
| - | -12.4 | Jun 17th | 159.405 | -56.822 | 0 | |||||||||
| - | 0.4 | Jun 17th | 295.55 | 25.9312 | 166.5 | 0 | ||||||||
| - | 7.8 | Jun 18th | - | -0.1 | Jun 17th | 13.0235 | -72.4345 | 44.8 | 0 | |||||
| - | -0.2 | Jun 17th | - | 0.114 | Jun 11th | 170.238 | -61.9167 | 24 | 0 | |||||
| - | -2.8 | Jun 16th | 274.178 | -16.2232 | 151.4 | 0 | ||||||||
| - | -6.1 | Apr 21st | - | 20.8 | Jun 17th | - | 0.069 | Jun 12th | 40.9186 | 61.4323 | 27.665 | 0 | ||
| - | -4.1 | Apr 21st | - | 37.5 | Jun 17th | - | 0.101 | Jun 12th | 292.483 | 18.3106 | 117 | 0 | ||
| 100% | 110.1 | Apr 21st | 100% | 53.8 | Jun 17th | 3.9% | 0.175 | Jun 12th | 285.905 | 3.1919 | 22.5348 | 42.15 | ||
| 100% | 32.6 | Apr 21st | - | -16.9 | Jun 17th | - | 0.091 | Jun 12th | 314.698 | 41.777 | 0.56 | |||
About
Description
This is a monitor using data from Swift/BAT, MAXI and Fermi/GBM instruments.
Click on the table header to change the sorting behavior.
Color code for the probability: (rising flux , no change, decreasing flux)
The average flux is calculated as the average of the last 3 days of data, without taking the errors into account. The Fermi flux is not given in mCrab.
Please note that the accuracy of the probabilities is limited by the accuracy of the data used.
Release of Wednesday, the 30th of September 2015
Last updated at 14:16:47 UT
Created as an ESAC trainee project by Eva Laplace.
Supervisors: Peter Kretschmar, Emilio Salazar and Miguel Arregui.
See also the Black Hole X-ray Binaries Monitor .
Contact: peter.kretschmar@esa.int
Analysis method description
The analysis is an algorithm computing a flux change parameter by calculating a "relative distance" of two measurements and weighting it according to the instrument used and the given error.
