Time, Space, Choices, and an Online Chat about Purr

The Interplay of , , , and Online Chats about

Time, space, choices, and an about purr encompass a diverse range of intriguing subjects. Time, as a concept, captivates us with its enigmatic nature and the various ways it shapes our lives. Exploring the vast expanse of space unveils celestial wonders, from distant galaxies to the mysteries of black holes. Choices hold immense power, influencing our personal growth and shaping our destinies. Meanwhile, engaging in an online chat about purr brings together cat enthusiasts, fostering connections and sharing the joys of feline companionship virtually. These topics invite contemplation, wonder, and the exploration of both inner and outer worlds.

How my book Purr: The Science of Making Your Cat Happy can help shelter cats.

Zazie todd's tortoiseshell cat melina at the top of a cat tree with purr behind
Zazie Todd’s cat Melina was adopted from the BC SPCA. She’s pictured in front of the book she helped inspire, and in which she features. Photo: Zazie Todd.

By Zazie Todd PhD

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Time, space and choices: Article about Purr

There is a wonderful article about my book, Purr, in the current issue of BARKS from the Guild.

It’s called Time, Space and Choices: Improving Welfare for Shelter Cats with Dr. Zazie Todd’s Purr.

It is all about how the tips in Purr: The Science of Making Your Cat Happy can help cats in shelter and rescue, as well as once they move to their new home. As you might guess from the title, giving the cat time to settle in, setting up their space right, and giving them choices (including letting them make the choice to hide) are all important.

Online chat about Purr and shelter cats

I will also be chatting about Purr and shelter cats at the PPG’s online Shelter and Rescue Divisional Meetup on Tuesday March 28th at 10am Pacific/1pm Eastern.

This event is free for all members of The Pet Professional Guild. If you’re a cat guardian, membership of the PPG is free. For pet professionals, the PPG is committed to force-free methods only and a membership is very worthwhile.

I hope to see you on Tuesday!

Zazie Todd, PhD, is the award-winning author of Wag: The Science of Making Your Dog Happy and Purr: The Science of Making Your Cat Happy. She is the creator of the popular blog, Companion Animal Psychology, and also has a column at Psychology Today. Todd lives in Maple Ridge, BC, with her husband, one dog, and two cats.
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Humans Help Computers Spot Burst of Space Debris

Humans Help Computers Spot Burst of Space Debris

The ThunderKAT radio survey keeps constant tabs on objects, such as accreting black holes and magnetized neutron stars, that are known to exhibit big, sporadic changes in their radio flux. The survey also searches for new transient sources. Finding them is primarily done by computer algorithms, but given how good humans are at pattern recognition, the ThunderKAT team wondered if human volunteers could find new transients more effectively. The answer is yes. In a trial that lasted three months, 1000 volunteers discovered 142 new transients [1]. The effort could inform how future transient surveys should be conducted.

ThunderKAT Team Specialists

Astronomers have cataloged many types of transients, from bursters to cataclysmic variables. The variability of these objects arises from explosive, out-of-equilibrium processes under extreme conditions. To better understand these processes, the ThunderKAT team studies transient phenomena in the Southern Sky using MeerKAT, an array of 64 radio telescopes located at a remote site in South Africa’s arid interior. When MeerKAT points at a known transient, ThunderKAT’s algorithms search for other point sources in the array’s 1° × 1° field. If the algorithms find a new transient, the computer program then sifts through archive data to see if radio signals have been observed from the source location during previous MeerKAT observations. If so, the program assembles a light curve, which is a record of the radio flux over . Whether the new source is classified as a transient depends on how it scores with respect to two variability statistics: η𝜂, which sums over the flux variations with respect to mean, and V, which divides the standard deviation by the mean flux.

The meerkat radio telescope array in south africa

The algorithms have identified many new transients, but the team decided to have humans look through some of the data to check whether any objects might have been missed. The data used in the trial extended over two years and came from weekly observations of 11 known transient sources. Within a three-month window, human volunteers evaluated candidates on the citizen science platform Zooniverse. For each candidate, the volunteers faced two tasks. The first was to look at an image and determine if the source in the center was a point source. (Extended sources are outside ThunderKAT’s remit.) The second task was to look at the corresponding light curve and evaluate whether the variability it embodied was significant.

Volunteers Called into Action

The volunteers found the 168 sources that ThunderKAT’s algorithms had already flagged as transient. But they also found 142 more that the algorithms had missed. Those sources turned out to have values of η𝜂 and V that were insufficiently extreme to trigger selection by the algorithms. Humans, it seems, were better at recognizing the normal variability of faint sources.

Astronomer and citizen science proponent Lucy Fortson of the University of Minnesota, Twin Cities, points out that it’s not just pattern recognition that humans excel at. “Humans also need less training data for recognizing patterns,” she says. “They also generalize better and can recognize more readily patterns ‘out of class.’”

New Discoveries

Some of the newly discovered sources turned out to have counterparts that had been observed before by other facilities at other wavelengths. One of them is the red supergiant star OH 30.1–0.7, whose radio emission comes from radiationally pumped hydroxyl radicals in the star’s strong wind. The variability of the radio emission suggests that OH 30.1–0.7 could have a binary companion, but other explanations remain in play.

Observations by the 24-inch MeerLICHT optical telescope, which is co-located with MeerKAT, suggest that the majority of the citizen science identifications are active galactic nuclei. The observed variability of these objects on timescales of months to years is likely not intrinsic. Rather, it arises from a more prosaic effect: refractive interstellar scintillation—twinkling—caused by the passage of extragalactic radio waves through the Milky Way’s turbulent interstellar medium.

Even if only a fraction of the new sources are found to be genuine transients, the ThunderKAT team can use the citizen science findings to tweak their algorithms. In addition, one of MeerKAT’s original goals is to test technologies for the similar, but much larger, Square Kilometre Array (SKA), whose 1000 antennas are expected to start gathering data in 2027. The researchers conclude that the success of ThunderKAT’s citizen science project will improve not only MeerKAT’s data-crunching algorithms but also SKA’s.

By: Charles Day: Senior Editor for Physics Magazine.

References

  1. A. Andersson et al., “Bursts from : MeerKAT – The first citizen science project dedicated to commensal radio transients,” arXiv:2304.14157; Mon. Not. R. Astron. Soc. (to be published).

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