(Re)discover new pulsars
With recent discoveries of pulsars in ULX and other extragalactic pulsars, it is interesting to reproduce these results right on this website.
NGC 5907 ULX — super-Eddington neutron star
Period 1.13 s, maximum X-ray luminosity 1e41 erg/s
- Do query:
cone('NGC 5907', '4 arcmin') AND is_ulx = True
to search for ULXs in NGC 5907 and choose the brightest source (with SC_EP_8_FLUX = 1.3e-12) in the results - On the source page choose its detection from e.g. Jul 2014 (direct link to the detection page)
- Click on the "Detection image and event list tools" link at the top to go to the region extraction page
- Adjust region to your liking and click Get data → Extract photons. Wait couple of minutes until photons are extracted and power density spectrum plot is generated.
- Voilà: you should see pulsations at 0.879 Hz
NGC 7793 P13 — super-Eddington neutron star
Period 0.42 s, maximum X-ray luminosity 5e39 erg/s
- Do query:
cone('NGC 7793', '4 arcmin')
and choose the brightest source (with SC_EP_8_FLUX = 9e-14) in the results - On the source page choose its detection from e.g. Jul 2014 (direct link to the detection page)
- Click on the "Detection image and event list tools" link at the top to go to the region extraction page
- Adjust region to your liking and click Get data → Extract photons. Wait couple of minutes until photons are extracted and power density spectrum plot is generated.
- Voilà: you should see pulsations at 2.39 Hz
M31 XB091D — the slowest spinning X-ray pulsar in a globular cluster
Period 1.2 s, maximum X-ray luminosity 1e38 erg/s
- Do query:
Bol D91
to search for pulsar's host globular cluster in M31 galaxy and choose the brightest source (with 30+ observations) in the results - On the source page choose e.g. its 60 ksec observation made on 2002-01-06 (direct link to the detection page)
- Click on the "Detection image and event list tools" link at the top to go to the region extraction page
- Adjust region to your liking and click Get data → Extract photons. Wait couple of minutes until photons are extracted and power density spectrum plot is generated.
- Voilà: you should see pulsations at 0.831 Hz