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2SXPS J080107.1+073909

[Spectral/flux information | Temporal information | External catalogue matches | Detections | Non-detections ]

Total | Soft | Medium | Hard | Exposure

Postage stamp image of 2SXPS J080107.1+073909

This image is 160 pixels (=6.3′ to a side).
2SXPS J080107.1+073909 is indicated by the cross-hairs. What do the colours mean?The next nearest source is 88′′ away.

Detection flag:: Good
Total exposure:: 22 ks
RA (J2000):: 08^h 01^m 07.12^s=120.2797°
Dec (J2000):: +07° 39′ 09.2″=+7.6526°
Err₉₀:: 4.5′′(Star trackers)
l:: +213° 56′ 54.5″=213.9485°
b:: +18° 57′ 10.3″=+18.9529°
Mean count rate: 1.0 (±0.4) ×10^-3 ct s^-1
Galactic N_H: 3.0×10²⁰ cm^-2
HRs: HR1=0.2 (+0.5, -0.4)
HR2=0.26 (+0.33, -0.28)
Observed between:: 2016-04-17 04:26 and 2016-04-20 23:17
Present in:: 6 datasets (total)
3 datasets (with blind detections)
3 datasets (count-rate detections)
External catalogue matches:: 1
Search Vizier | Simbad.
2SXPS ID: 82090

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Spectral / Flux information

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Temporal Information

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Band	Total (0.3—10 keV)	Soft (0.3—1 keV)	Medium (1—2 keV)	Hard (2—10 keV)
Mean rate (ct s^-1)	1.0 (±0.4) ×10^-3	1.6 (+2.1, -1.6) ×10^-4	2.5 (±1.9) ×10^-4	4.5 (±2.3) ×10^-4
Peak rate (ct s^-1)	3.6 (+2.4, -1.7) ×10^-3	1.6 (+2.1, -1.6) ×10^-4	1.9 (+1.9, -1.1) ×10^-3	10 (+6, -4) ×10^-4
Detected?	Yes	Blind: No Retrospective: No	Yes	Yes
3 σ UL (ct s^-1)	N/A	< 8.18× 10^-4	N/A	N/A
Counts detected	29	8	8	12
BG counts	11.74	5.210	3.676	4.08
Corr fact	1.47	1.47	1.47	1.47
P_const,χ	2.42×10^-4 (obs) 0.25 (snapshot)	6.92×10^-2 (obs) 0.54 (snapshot)	6.92×10^-2 (obs) 0.10 (snapshot)	6.92×10^-2 (obs) 0.90 (snapshot)

One bin per observation

Total | Soft | Medium | Hard | HR1 | HR2

X-axis: Non-detections:

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Data file | Enlarge.

One bin per snapshot

Total | Soft | Medium | Hard | HR1 | HR2

X-axis: Non-detections:

Show bin markers? Include flagged bins?

Show plot axis controls or click to zoom [more].

Data file | Enlarge.

External Catalogue matches

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Detections

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Non-detections

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Data for your light curve

2SXPS J080107.1+073909 — , per- binning.