Archive for Hitomi

The 3.5 keV “Line” that (probably) wasn’t…

Posted in Bad Statistics, The Universe and Stuff with tags , , , , , , , on July 26, 2016 by telescoper

About a year ago I wrote a blog post about a mysterious “line” in the X-ray spectra of galaxy clusters corresponding to an energy of around 3.5 keV. The primary reference for the claim is a paper by Bulbul et al which is, of course, freely available on the arXiv.

The key graph from that paper is this:

XMMspectrum

The claimed feature – it stretches the imagination considerably to call it a “line” – is shown in red. No, I’m not particularly impressed either, but this is what passes for high-quality data in X-ray astronomy!

Anyway, there has just appeared on the arXiv a paper by the Hitomi Collaboration describing what are basically the only set of science results that the Hitomi satellite managed to obtain before it fell to bits earlier this year. These were observations of the Perseus Cluster.

Here is the abstract:

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of various massive systems, such as galaxies and clusters, including the Perseus cluster. We have analyzed the Hitomi first-light observation of the Perseus cluster. The emission line expected for Perseus based on the XMM-Newton signal from the large cluster sample under the dark matter decay scenario is too faint to be detectable in the Hitomi data. However, the previously reported 3.5 keV flux from Perseus was anomalously high compared to the sample-based prediction. We find no unidentified line at the reported flux level. The high flux derived with XMM MOS for the Perseus region covered by Hitomi is excluded at >3-sigma within the energy confidence interval of the most constraining previous study. If XMM measurement uncertainties for this region are included, the inconsistency with Hitomi is at a 99% significance for a broad dark-matter line and at 99.7% for a narrow line from the gas. We do find a hint of a broad excess near the energies of high-n transitions of Sxvi (E=3.44 keV rest-frame) – a possible signature of charge exchange in the molecular nebula and one of the proposed explanations for the 3.5 keV line. While its energy is consistent with XMM pn detections, it is unlikely to explain the MOS signal. A confirmation of this interesting feature has to wait for a more sensitive observation with a future calorimeter experiment.

And here is the killer plot:

Perseus_Hitomi

The spectrum looks amazingly detailed, which makes the demise of Hitomi all the more tragic, but the 3.5 keV is conspicuous by its absence. So there you are, yet another supposedly significant feature that excited a huge amount of interest turns out to be nothing of the sort. To be fair, as the abstract states, the anomalous line was only seen by stacking spectra of different clusters and might still be there but too faint to be seen in an individual cluster spectrum. Nevertheless I’d say the probability of there being any feature at 3.5 keV has decreased significantly after this observation.

P.S. rumours suggest that the 750 GeV diphoton “excess” found at the Large Hadron Collider may be about to meet a similar fate.

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The End of Hitomi..

Posted in The Universe and Stuff with tags , , , on April 4, 2016 by telescoper

Time for a gloomy Monday update to my recent post about the Japanese X-ray satellite Hitomi.

First here’s a new plot of the debris (via Jonathan McDowell):

Hitomi

This shows more pieces of debris than the one I showed previously, and also demonstrates that some of the pieces are in rapidly-decaying orbits. A rough estimate suggests that some of these – those in the lower right of the diagram- will burn up in the atmosphere within a week or so. This behaviour is consistent with them being rather light fragments, on which the effect of drag is greater, and consequently possibly rather small.  Their behaviour does not therefore necessarily imply anything too catastrophic about the main spacecraft.

However, there is now strong evidence that the main spacecraft actually did break up fairly completely rather than shedding a few pieces of casing or whatever. Two of the brightest pieces are of roughly equal size and, ominously, the original identification of one of them with the main part of the spacecraft has been shown to be wrong. Furthermore, no signals have been received from the onboard beacon for six days now. It all sounds very terminal to me.

2-hitomispacec

So what happened? Of course I don’t know for sure, but the above picture suggests the possibility of an explosion (possibly violent outgassing of cryogens needed for the instruments near the rear of the main body of the vehicle). The structure to the rear of the vehicle is a deployable optical bench used to increase the focal length of the telescope for hard X-ray work. This could well have broken off during such an explosion, as could all or part of the solar panels used to supply power to the satellite.

The Japanese Space Agency JAXA has not officially given up on Hitomi (formerly known as ASTRO-H) but I think the hopes of most commenters I’m aware of have now faded away.

It’s all very sad.

 

 

 

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The Trouble with Hitomi

Posted in The Universe and Stuff with tags , , on March 31, 2016 by telescoper

One of the stories I’ve been following a bit while taking a break from blogging has been that of the Japanese X-ray satellite Hitomi (formerly known as ASTRO-H), which was launched into a low-Earth orbit on February 17th 2016, experienced a “communication anomaly” on Saturday March 26th. It has now become clear that this was more than a simple communications glitch. Astronomer Jonathan McDowell posted this diagram on Twitter that showed a sudden decrease in the orbital period of the satellite:CekOyLxXEAAeNxF

Students of orbital dynamics will know that a decrease in orbital period corresponds to a decrease in the semi-major axis of the orbit, so Hitomi actually fell during this episode. It dropped only slightly – look at the % change on the graph – but by enough to be very worrying.

The plot thickened still further when radar detected five pieces of debris near the satellite and visual observations indicated the spacecraft to be tumbling rapidly. That suggested a very grim picture.

Putting the evidence together it seems that some kind of explosive event – possibly connected with out-gassing of cryogenic material from one of the on-board experiments – had damaged the satellite, changed its orbit and set it spinning uncontrollably.

Since then ground stations have picked up some signals from Hitomi, which is good news,  but these broadcasts are just from the on-board beacon. It has not yet proved possible to communicate with the attitude control system which is the only way to get it back into a stable state.

Obviously it’s touch and go as to whether the Japanese Space Agency JAXA will be able to regain control of Hitomi, but at least there’s more hope than on Saturday when many of us thought the vehicle had fallen apart. In fact the pieces of debris reported may be rather small (ten cm or so is detectable) and the main body of the telescoper may be intact. Maybe.

Update: April 1st. Tracking facilities are now reporting 11 pieces of debris, and also suggesting the object whose period is plotted in the above graph may not be the main part of the spacecraft. This does not sound good.

Update: April 2nd. The debris from Hitomi has now spread out due to different orbital speeds. The two largest pieces are both spinning out of control. I would say at this point that hope of a recovery has now disappeared. It’s very sad.

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