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
-5.6
Oct 20th
-6.3
Oct 18th
-0.086
Oct 14th
215.303-62.69842.120
--1
Oct 10th
-0.6
Oct 17th
-0.058
Oct 13th
19.63363.7424.30
-10.1
Sep 28th
--9.1
Oct 18th
-0.055
Oct 12th
84.72726.316111.10
--3.9
Oct 20th
--20.1
Oct 17th
-0.024
Oct 14th
324.87856.98623.850
100%34.5
Oct 19th
-5.3
Oct 18th
-0.16
Oct 14th
152.442-58.292249.4816.67
-0.2
Oct 18th
-0.049
Oct 14th
128.979-43.185105.80
-10.5
Oct 19th
--0.9
Oct 18th
-0.309
Oct 13th
195.321-61.602132.1890
195.498-63.9680
-2.8
Oct 19th
--2.1
Oct 17th
-0.098
Oct 15th
297.39830.20940.40
-10.7
Oct 17th
-0.099
Oct 14th
70.24744.531550
-12.7
Oct 18th
-0.294
Oct 13th
212.011-61.9830
-3.8
Oct 17th
-0.078
Oct 14th
315.89945.75212.70
--7.1
Oct 18th
280.899-3.730
-40.4
Oct 4th
--3.9
Oct 17th
-0.074
Oct 14th
53.7553.17334.250
--6.1
Oct 18th
-0.092
Oct 14th
284.6883.4320
-0.6
Oct 17th
-0.067
Oct 14th
296.41727.356169.20
-7.3
Oct 18th
246.65-51.941132.90
--1.1
Oct 18th
-0.086
Oct 14th
104.6-7.20
-3.6
Oct 19th
-12.5
Oct 17th
-0.065
Oct 14th
308.06437.63746.030
52.4%23.7
Oct 4th
-17.3
Oct 18th
58.84631.046250.31.54
-15.6
Oct 18th
72.778-69.8010
-2.1
Oct 17th
300.09132.18980
3.4%19.2
Oct 17th
26.75161.3570.97
--5.5
Oct 18th
-0.077
Oct 15th
267.291-26.63729.820
-9.7
Oct 20th
--9
Oct 18th
-0.069
Oct 14th
239.454-54.41529.560
-6.5
Oct 18th
-0.057
Oct 14th
284.7758.250
-16.8
Oct 19th
--1.3
Oct 18th
177-62.207187.50
-20.5
Oct 20th
--8.8
Oct 18th
282.074-2.42242.180
--2.8
Oct 20th
-12.1
Oct 18th
13.6508-73.6760
--5.1
Oct 18th
159.405-56.8220
--3.4
Oct 17th
295.5525.9312166.50
--3.4
Oct 20th
-1.6
Oct 18th
13.0235-72.434544.80
--6.9
Oct 18th
-0.349
Oct 14th
170.238-61.9167240
-3.7
Oct 18th
274.178-16.2232151.40
100%2123.9
Oct 17th
100%3.975
Oct 14th
40.918661.432342.86

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 06:16:19 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