| 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 | ||||||
| - | 1.1 | May 25th | - | -8 | May 24th | - | 0.089 | May 21st | 215.303 | -62.698 | 42.12 | 0 | ||
| - | -12.3 | May 12th | - | -14.4 | May 23rd | - | 0.07 | May 21st | 19.633 | 63.74 | 24.3 | 0 | ||
| - | 0.7 | May 25th | - | 45.1 | May 24th | - | 0.052 | May 21st | 84.727 | 26.316 | 111.1 | 0 | ||
| - | 3.5 | May 21st | - | 0.2 | May 23rd | - | 0.014 | May 20th | 324.878 | 56.986 | 23.85 | 0 | ||
| 100% | 248.1 | May 25th | 100% | 592.7 | May 24th | 100% | 1.417 | May 20th | 152.442 | -58.292 | 249.48 | 183.33 | ||
| - | 1.4 | May 23rd | - | 2.4 | May 24th | - | 0.05 | May 21st | 128.979 | -43.185 | 105.8 | 0 | ||
| - | 0.7 | May 25th | - | 2 | May 24th | - | 0.124 | May 21st | 195.321 | -61.602 | 132.189 | 0 | ||
| - | 15.3 | May 14th | 195.498 | -63.968 | 0 | |||||||||
| - | -0.1 | May 25th | - | -5.3 | May 23rd | - | 0.088 | May 20th | 297.398 | 30.209 | 40.4 | 0 | ||
| - | 6.9 | Apr 28th | - | -14.1 | May 20th | - | 0.048 | May 21st | 70.247 | 44.53 | 155 | 0 | ||
| - | 1.9 | May 23rd | - | -8.7 | May 24th | - | 0.191 | May 21st | 212.011 | -61.983 | 0 | |||
| - | -2.2 | May 21st | - | 2.6 | May 23rd | - | 0.058 | May 20th | 315.899 | 45.752 | 12.7 | 0 | ||
| - | 5 | May 23rd | - | 7.6 | May 24th | 280.899 | -3.73 | 0 | ||||||
| - | -12.4 | May 2nd | - | -20.7 | May 23rd | - | 0.058 | May 20th | 53.75 | 53.173 | 34.25 | 0 | ||
| - | 2.2 | May 23rd | - | -9.7 | May 24th | - | 0.123 | May 21st | 284.688 | 3.432 | 0 | |||
| - | -2.7 | May 23rd | - | 15 | May 23rd | - | 0.092 | May 21st | 296.417 | 27.356 | 169.2 | 0 | ||
| - | -6 | May 24th | 246.65 | -51.941 | 132.9 | 0 | ||||||||
| - | 0.8 | May 23rd | - | 1.2 | May 24th | - | 0.032 | May 19th | 104.6 | -7.2 | 0 | |||
| - | 16.8 | May 24th | - | -5.3 | May 23rd | - | 0.059 | May 20th | 308.064 | 37.637 | 46.03 | 0 | ||
| 88.6% | 34 | Apr 25th | 0.5% | 22.5 | May 9th | 58.846 | 31.046 | 250.3 | 2.89 | |||||
| - | 3.3 | May 24th | 72.778 | -69.801 | 0 | |||||||||
| - | -0.8 | May 23rd | 300.091 | 32.1898 | 0 | |||||||||
| - | -1.9 | May 23rd | 26.751 | 61.357 | 0 | |||||||||
| - | 9.1 | May 24th | - | 0.054 | May 20th | 267.291 | -26.637 | 29.82 | 0 | |||||
| - | 0.2 | May 25th | - | -1.5 | May 24th | - | 0.052 | May 20th | 239.454 | -54.415 | 29.56 | 0 | ||
| - | 3.8 | May 24th | - | 0.075 | May 20th | 284.775 | 8.25 | 0 | ||||||
| 29.6% | 11.3 | May 25th | - | 3 | May 24th | 177 | -62.207 | 187.5 | 14.8 | |||||
| - | 5.2 | May 25th | - | 0.9 | May 24th | 282.074 | -2.42 | 242.18 | 0 | |||||
| 8.2% | 11.2 | May 25th | - | -5.9 | May 24th | 13.6508 | -73.676 | 4.1 | ||||||
| - | 1.4 | May 24th | 159.405 | -56.822 | 0 | |||||||||
| - | -2 | May 23rd | 295.55 | 25.9312 | 166.5 | 0 | ||||||||
| - | -1.1 | May 25th | - | 4.9 | May 24th | 13.0235 | -72.4345 | 44.8 | 0 | |||||
| - | -9.5 | May 24th | - | 0.167 | May 20th | 170.238 | -61.9167 | 24 | 0 | |||||
| - | -10.6 | May 24th | 274.178 | -16.2232 | 151.4 | 0 | ||||||||
| - | 4.9 | May 4th | - | -11.2 | May 23rd | - | 0.074 | May 20th | 40.9186 | 61.4323 | 27.665 | 0 | ||
| - | 9.6 | May 25th | - | 14.9 | May 24th | - | 0.07 | May 20th | 292.483 | 18.3106 | 117 | 0 | ||
| - | 0 | May 23rd | - | -1.3 | May 24th | - | 0.102 | May 21st | 285.905 | 3.1919 | 22.5348 | 0 | ||
| - | 2.2 | May 22nd | - | 3.4 | May 23rd | - | 0.083 | May 21st | 314.698 | 41.777 | 0 | |||
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 18:16:49 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.
