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
-4.5
Aug 17th
-4.9
Aug 16th
-0.099
Aug 13th
215.303-62.69842.120
100%86
Jul 30th
100%215.2
Aug 16th
3.9%0.517
Aug 12th
19.63363.7424.372.58
-0.5
Aug 17th
-2.7
Aug 16th
-0.063
Aug 12th
84.72726.316111.10
--1.6
Aug 10th
--7.4
Aug 15th
-0.023
Aug 12th
324.87856.98623.850
100%198.6
Aug 17th
100%449.7
Aug 16th
100%1.925
Aug 12th
152.442-58.292249.48184.85
-8.6
Aug 16th
-0.052
Aug 12th
128.979-43.185105.80
--4.9
Aug 17th
--1.8
Aug 16th
-0.276
Aug 11th
195.321-61.602132.1890
195.498-63.9680
-1.5
Aug 17th
-4.9
Aug 16th
-0.113
Aug 12th
297.39830.20940.40
--4.2
Aug 16th
-0.069
Aug 13th
70.24744.531550
-3.9
Aug 16th
-0.288
Aug 12th
212.011-61.9830
--5.2
Aug 15th
-0.14
Aug 11th
315.89945.75212.70
--3.7
Aug 16th
280.899-3.730
-2.9
Jul 29th
-5.4
Aug 16th
-0.043
Aug 12th
53.7553.17334.250
--15.8
Aug 16th
-0.246
Aug 12th
284.6883.4320
--17.4
Aug 16th
-0.095
Aug 13th
296.41727.356169.20
--5
Aug 16th
246.65-51.941132.90
-2.2
Aug 16th
-0.054
Aug 11th
104.6-7.20
-1.2
Aug 14th
--10.4
Aug 16th
-0.074
Aug 12th
308.06437.63746.030
33.4%24.1
Jul 29th
-19.3
Aug 16th
58.84631.046250.30.84
--1.8
Aug 16th
72.778-69.8010
-2.8
Aug 16th
300.09132.18980
-1.8
Aug 16th
26.75161.3570
--8
Aug 16th
-0.096
Aug 13th
267.291-26.63729.820
-4.8
Aug 17th
-1
Aug 16th
-0.072
Aug 13th
239.454-54.41529.560
--2.4
Aug 16th
-0.055
Aug 11th
284.7758.250
30.7%12.4
Aug 17th
-0.9
Aug 16th
177-62.207187.515.35
30.9%10.3
Aug 17th
-5.4
Aug 16th
282.074-2.42242.1815.45
9.1%5.1
Aug 17th
--2.9
Aug 16th
13.6508-73.6764.55
-14.2
Aug 16th
159.405-56.8220
--15.2
Aug 16th
295.5525.9312166.50
--0.1
Aug 17th
-1.7
Aug 16th
13.0235-72.434544.80
-0.7
Aug 16th
-0.208
Aug 11th
170.238-61.9167240
--3.8
Aug 16th
274.178-16.2232151.40

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 20:16:29 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