Recent activity of selected Be X-ray binaries as detected by three X-ray monitors
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
-8.9
Dec 4th
--1
Dec 10th
-0.095
Dec 3rd
215.303-62.69842.120
-12.4
Dec 4th
-11.7
Dec 10th
-0.394
Dec 3rd
19.63363.7424.30
0.5%9
Dec 4th
-27
Dec 10th
-0.127
Dec 3rd
84.72726.316111.10.02
-4.5
Dec 4th
-7.8
Dec 10th
-0.024
Dec 2nd
324.87856.98623.850
-7.6
Dec 4th
-3.2
Dec 10th
-0.075
Dec 2nd
152.442-58.292249.480
--1.3
Dec 10th
-0.056
Dec 3rd
128.979-43.185105.80
--2.8
Dec 4th
-4.3
Dec 10th
-0.193
Dec 3rd
195.321-61.602132.1890
195.498-63.9680
-10.3
Dec 4th
-4.7
Dec 10th
-0.102
Dec 2nd
297.39830.20940.40
-5.5
Dec 10th
-0.147
Dec 3rd
70.24744.531550
-2.8
Dec 10th
-0.333
Dec 3rd
212.011-61.9830
-2.8
Dec 10th
-0.102
Dec 3rd
315.89945.75212.70
-1.2
Dec 9th
280.899-3.730
-4.9
Dec 4th
--1.9
Dec 10th
-0.428
Dec 2nd
53.7553.17334.250
--17.2
Dec 10th
-0.104
Dec 3rd
284.6883.4320
-7.3
Dec 10th
-0.081
Dec 3rd
296.41727.356169.20
-29.5
Dec 10th
246.65-51.941132.90
-18.4
Dec 10th
-0.047
Dec 2nd
104.6-7.20
-11.8
Dec 3rd
18.8%17.8
Dec 10th
-0.079
Dec 3rd
308.06437.63746.032.51
56.6%6.4
Dec 4th
-37.4
Dec 10th
58.84631.046250.33.14
-1.5
Dec 10th
72.778-69.8010
-4
Dec 10th
300.09132.18980
-26.1
Dec 10th
26.75161.3570
--20.3
Dec 8th
-0.059
Dec 2nd
267.291-26.63729.820
-1.1
Dec 3rd
-5
Dec 10th
-0.059
Dec 3rd
239.454-54.41529.560
--7.7
Dec 10th
-0.132
Dec 2nd
284.7758.250
1.9%7.3
Dec 4th
--1.7
Dec 10th
177-62.207187.50.11
-13.5
Dec 4th
41.2%36.1
Dec 9th
282.074-2.42242.185.89
10.3%19.7
Dec 4th
--4.1
Dec 10th
13.6508-73.6760.57
-5.8
Dec 10th
159.405-56.8220
--11.9
Dec 10th
295.5525.9312166.50
-4.9
Dec 4th
--9.7
Dec 10th
13.0235-72.434544.80
--4
Dec 10th
-0.179
Dec 2nd
170.238-61.9167240
-5.6
Dec 9th
274.178-16.2232151.40
-10.3
Dec 4th
100%2604.9
Dec 10th
100%8.16
Dec 3rd
40.918661.432333.33

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 07:16:04 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.

Be XRB monitor Be X-ray binary monitor transient outburst accreting pulsar BEXRB HMXB LMXB persistent light-curve x-rays ESAC binaries activity type folding probability variability variable bursting giant burst beXRB be xrb