Sister blog of Physicists of the Caribbean. Shorter, more focused posts specialising in astronomy and data visualisation.

Friday, 6 October 2017

M31 seen at multiple wavelengths


I'm preparing short 6-hour lecture course on galaxy evolution. I thought it would be more interesting to show the popular multi-wavelength M31 data image as an animation, so here's a little gif. The positional matching of the data sets is just done by eye so it isn't very precise, but it's good enough.

I'll be making the course available online if and when time permits.

Thursday, 5 October 2017

Statistics is hard

I know nothing of forensics, though I will add a few related points.

The first is that in my own field I see people making extremely strong statistical claims based on somewhat dodgy data. For example there's this claim that satellite galaxies orbit their hosts in thin planes, which is not predicted by the standard model. Based on analysis of conventional models, claims have been made that the odds of the observations (especially of the Milky Way and our neighbour Andromeda) matching reality are something like 1 in 10,000. And I'm sure this is correct if you take it at face value and don't dig any deeper.

The problem is that there are huge uncertainties here at every level : the simulations don't take into account the gas physics, the observational uncertainties in distances (which strongly affects the narrowness of the planes), or the likelihood of galaxies interacting which has been shown can cause planes of satellites to narrow significantly. Not to mention that 1 in 10,000 isn't very impressive when you've got billions of galaxies. Or that galaxies in close proximity to each other are likely to be born in similar environments, and if these are (for whatever reason) more susceptible to forming planes, then the statistical probability that they're similar is based on a faulty assumption that they're drawn from a random population. And rather than saying, "let's see if there's some physical mechanism within the existing model that can explain the data", of which many have already been published, authors sometimes say, "the whole model must be fundamentally flawed".

This is fine in extragalactic astronomy where the worst that can happen is that one author will argue with another. Obviously if this happens in forensics then the consequences are very much worse. But I can easily believe that it could happen and I would understand why.

The second point is that I've come to the opinion that the formal error equation is bollocks. As an observer, I simply don't believe error bars that are smaller than the plotted data points - or worse, error bars that are smaller than the observed scatter when there's a clear underlying trend. In my experience, systematic effects always dominate. This doesn't mean that the results are wrong or the claims are wrong, just that I'd be automatically wary of claims of extremely high confidence in the results (with many caveats, depending on the particular data and claims being made). Not only do observers make mistakes, but sometimes the intrinsic scatter is high anyway.

The third point, which is understandable that Oliver doesn't mention, is that probability is hard. Intuitively, a test with a 99% success rate which produces a match implies there's a 1% chance that the match was false (because of the test limitations). But in reality, this simply isn't the case. : test limitations are not the only factor ! The test isn't meaningless, it's just nowhere near as good as you might think (honestly, I still have a hard time getting my head around this one) :
http://www.patheos.com/blogs/daylightatheism/2008/02/how-to-think-critically-vi/

So for all these reasons, I'm inclined to find this report credible. The chance that a test is correct is much more complicated than whether the test works. The test could function just fine and still get the wrong result, both because of the nature of statistical probability and because of not properly considering alternatives. You don't have to throw out the forensics, but you probably want to bring in a statistician too. And perhaps it would be worth considering (if this isn't done already, perhaps it is but the end section of the report suggests otherwise) giving independent forensic data to independent labs and not telling them the context of what they're dealing with. Don't tell them to identify the killer, just tell them to establish if two samples match with no other information at all. And give them also "decoy" samples so they have absolutely no preconceptions about whether a match is good or bad at all.

That's my two cents. But in keeping with the "I'm not a scientist, but..." fallacy, since I know nothing of forensics I may be talking out of my backside here. Perhaps this report is overly-selective and I'm misapplying my own experiences. The only correct way to finish the sentence, "I'm not an expert in..." is, "so therefore you shouldn't weight my opinion as seriously as an expert." Which in this case might not be a forensic scientist, but someone who's conducted large, long-term studies of the judicial system.
https://www.youtube.com/watch?v=ScmJvmzDcG0

Wednesday, 4 October 2017

Fancy-schmancy award ceremony !

From the CAS :

The Czech Academy of Sciences grants awards for achieved results which contribute to the prestige of Czech science in international comparison and from whose first publication or implementation no more than five years have passed. The awards are presented for completed scientific results of excellent and high-quality research strategically orientated on social priorities.

Awards of the CAS for young scientists [2017] for outstanding scientific achievements were presented to:

Dr. Rhys Taylor, PhD, from the Astronomical Institute of the CAS, for the outstanding scientific outcome Understanding the origin of optically dark hydrogen clouds: dark galaxies or tidal debris?





Wednesday, 27 September 2017

ALMA All-Hands 2017

Last year's ALMA all-hands meeting was in Lisbon and the conference freebie was a USB fan. This year it's in the Netherlands and we get an umbrella, a coaster and some waffles. Plus I won a free drink by getting all the quiz answers deliberately wrong :

Expand the following acronyms :
AQUA : ALMA QUality Alcohol (actually ALMA QUality Assurance)
APA : Annoyingly Precise Acronym (actually AQUA Pipeline Agent)
DRM : Dangerous Robotic Monkey (actually Data Reduction Manager)
OSF : Observatory Supports Farmyards (I would have gone for "fornication" but wasn't sure how the crowd would react; actually Observing Support Facility)
DARED : Deadly ALMA Really Extreme Database (actually... nope, I've already forgotten)
DPTT : Don't Produce This Tool (see above).


Friday, 8 September 2017

Dramatic instructions

I'm reviewing a paper for the first time. One of the instructions is a tad dramatic for my liking :

7. If qualified historians wish to use your report, we will ask you or your heirs. If you wish us to destroy your report, then please inform us.

Wednesday, 30 August 2017

Space Nazi Paper I

The author (my former housemate) is an expert on X-ray polarimetry and AGN, so why he's decided to do this I have no idea. It's quite fun though. I had a not inconsiderable hand in correcting the text prior to submission.

Basically he's written a code to try and estimate whether a population could survive in isolation given the effects of inbreeding and overpopulation, here applied to a multi-generational interstellar mission. The clever bit, as I understand it, is tracking the histories of each individual to calculate the degree of inbreeding. The deleterious effects of inbreeding are applied quite crudely, reducing lifespan by some value if above some threshold (neither of which are well-known, but can be adjusted). It can also apply an artificial breeding programme, in the sense of forbidding breeding between individuals who are too closely related.

Here he investigates three possibilities : 1) A small population (150) who are insanely horny and don't care a jot about food supplies, incest, or have any common sense - unsurprisingly, this doesn't work very well; 2) A small population where the number of births is tightly controlled but no other regulations are applied - this works much better but it's not great; 3) A large population (14,000) with the same simple population controls, which succeeds.

Oddly, he doesn't actually use the code's capability of limiting inbreeding. He mentioned something about that needing improvements, but I never found out what exactly. Also the populations of both the small and large (controlled) populations show an initial increase followed by a slow, prolonged decrease of a very similar pattern over time. I'm not sure why that should be, but it's worrying. I also never really understood why the populations are given such restricted initial age ranges (a crew entirely of twentysomethings running a starship ? hmmm...) - that just leaves it more vulnerable to disasters.

What I hope will be tackled with the second paper would be an attempt to find the smallest number that could survive the mission given sensible population controls and natural breeding restrictions (e.g. Jamie and Cersei aside, hardly anyone is going to fool around with their siblings). Of course in a real interstellar mission you'd just take along frozen genetic material and eliminate inbreeding with arbitrarily small populations, but it would be interesting to find the point at which that's not necessary.

I believe the intention is to make the code public (surely this could be applied to the Sims ?) but this isn't the case yet. My guess would be it's not quite in a sufficiently clean state for public distribution.
https://arxiv.org/abs/1708.08649

Wednesday, 9 August 2017

Astronomy is too big to fail

Alas the title, "A new astrophysical solution to the Too Big To Fail problem" does not refer to astronomers finding a way to support the banking sector, which would have been more unexpected...

The "Too Big To Fail Problem" is a variant of the "missing dwarf galaxy" problem, where there aren't as many dwarf galaxies detected as expected from simulations. Specifically, the most massive dwarf galaxies should be so large that there's no way - according to the simulations - that their dark matter "halos" can avoid attracting enough gas to start forming stars. It's not just that we're not finding many of the really small dwarfs (that's a problem too), it's that this is a problem even for the bigger guys. It only stops when you get to really massive galaxies.

Supernovae explosions and other processes might be able to explain why the littlest galaxies don't form any stars - a few big blasts could send the remaining gas off into the void, never to be seen again. So they form just a few stars, which eventually die off and thus we can't detect the smallest dwarfs any more. But this explanation shouldn't be possible for the largest dwarfs, which are so massive they ought to be able to hold on to their gas more strongly.

This latest paper uses a bunch of more advanced simulations with better resolution and (they think) treatment of the various processes at work. They make "synthetic observations" of their simulations so they can directly compare their results to real observations. They find that the observations would be underestimating the mass of the dark matter present. Although supernovae can't blast the gas out of the largest dwarfs, it can still cause disruption - the nice thin disc that we see in larger galaxies, and we assume is present in dwarves, gets "puffed up" and becomes substantially thicker. The gas is prevented from collapsing into stars both by its rotation and by this pressure support provided by the various feedback processes from the stars.

This means that the gas discs in the largest dwarves don't extend as far as we expect them to, so their rotation underestimates their true mass. So the dwarf galaxies we detect are actually quite a bit more massive than we've been estimating, if this scenario is correct. They haven't failed, they just aren't quite what we expected from a simpler assumption.

It's a rather technical paper, and personally I think they could have explained their results in a simpler way. I don't think they explain their various scaling relations in a very clear way, making it hard to check if their interpretation of their simulations is sensible. Also (although this isn't crucial), their sample is currently rather small. It would be useful to include more galaxies at different masses to see how well the gas traces the true rotation for other objects.
http://adsabs.harvard.edu/abs/2017arXiv170303810V

Friday, 4 August 2017

I won a thing !!!

I have an email, so I guess it's official now...

Dear Rhys,
We have received an information from the Head Office of the Czech Academy of Sciences saying that you are selected for the prize for young researchers, which our Institute proposed some time ago.
There will be a ceremony in Villa Lanna on 4th October 2017. Please save the date!
An official letter will follow.
Congratulations,

It comes with the glamorous title : "The Award of the CAS for young scientific employees for outstanding results of scientific work, achieved with the financial support of the CAS before reaching the age of 35."
I should get that on a badge. This is a general CAS award, not even limited to astronomy...

As far as I can tell, I think I might be the first non-Czech/Slovak winner...
http://www.avcr.cz/en/about-us/awards/prizes-of-the-cas/

Villa Lana is also super-shiny :
http://www.vila-lanna.cz/

Excuse me, I'm off to drink enough tea to shrink my head back down to its usual size...
http://www.avcr.cz/en/about-us/awards/prizes-of-the-cas/

A lot of knowledge is a dangerous thing


Yesterday I removed from a certain community's spam folder a post consisting of 94 slides about some sterotypical pseudoscience theory. The usual stuff : "Let us begin with E = mc^2..."
No. Let's not do that, because it's obvious that you haven't got a clue what you're talking about. Lo and behold, it got rapidly worse, with some boiler-plate text praising God at the top of each slide. Aaaarrgggh. If you want to praise God, then fine, but do it in your own time, mate. Not in an internet-based slideshow you apparently expect people to read.

Total ignorance is indeed never damaging, providing one understands that one is totally ignorant and not put in a position where expertise might be required. A little knowledge is a dangerous thing as well. But a lot of knowledge without proper understanding is much, much worse.

Thursday, 3 August 2017

The most useless law in nature ?

In which I summarise the current debate over whether this apparent "new law of nature" means anything or not, and conclude (spoiler !) that it probably doesn't.

It's been known for many years that there's a correlation between how fast matter in a galaxy rotates and how much gas and stars it contains. The problem is that there shouldn't be a nice relation, because galaxies seem to be dominated by dark matter. This strange relationship between normal and dark matter, which should be independent of each other, has been shown in different ways over the years. Recently it was claimed that all of these are just manifestations of a deeper underlying "law" : the Mass Discrepancy Acceleration Relation (or technically the Radial Acceleration Relation, but whatever).

The problem is that the expected acceleration of matter (based on its mass and standard Newtonian gravity) correlates very, very well with its actual acceleration. If there is, as we think for many other reasons, actually a huge amount of unseen "dark matter" present, then it shouldn't do that. Could it be that the dark matter theory is wrong ?

YES ! But it probably isn't. Although modified theories of gravity do predict this relation - indeed, did predict it 30 years ago - it seems that it also occurs in standard dark matter simulations without any difficulties. You can see a comparison of observations (left) and the simulations (right) in the example image below. Since both modifying gravity and using dark matter give the same result, this discovery is probably useless. Weird, but useless.

Read on for tales of academics behaving badly, pretty pictures of galaxies, lots of and lots of graphs, and a surprised dog...

Placeholder post intended to be replaced with a slightly better summary.

Making Shit Up

Today's paper is one that fits into a very rare category where I'm prepared to say : this should not have been accepted by the refe...