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Re: (cba:news) (cba:chat) March stars (Joe Patterson) [2018-03-16T22:22:32Z]


Yes, I strongly recommend intense coverage of AT Cnc, for as many hours as you can get it. Best *morning* target for the next 1-2 weeks is AM CVn - also intensive.

Duplicating coverage on AM CVn isn't bad - in fact, it's highly desirable.  AM CVn has three periodicities: at 525 s, 1051 s, and 1028 s.  The first two are generally the strongest; but because they're superhumps - not stable on long timescales - they have to be removed in order to track the orbital 1028 s signal.  Somewhat tricky, but can always be done if the data are DENSELY distributed.  That's the key - dense coverage.  This is true for most CBA programs, to some degree - but never as much as AM CVn, because separating these closely spaced frequencies is critical.


joe

On 3/16/2018 5:03 PM, Shawn Dvorak wrote:

As an extra incentive, AT Cnc is currently in a Z Cam standstill. The AAVSO data shows it "got stuck" around mag 13.6 near the end of January. Although the data is a bit sparse, it seems to be showing a 0.4 mag amplitude variation with a ~6.5 day period. Interesting, but possibly just a coincidence. It looks like I'll have mostly clear skies tonight so I'll get a longish run on it from 0:30 - 06:30 UT

Shawn


On 03/04/2018 07:34 PM, Joe Patterson wrote:
Dear CBAers,

Muchas gracias for all the great data you've been sending, especially re the DQ Her stars which you've been covering so faithfully.  It's been a winter of ice and mishap and hard work - nothing really serious but maybe I got kind of soft after a semester off from work.

The DQs are relatively sparse in the (northern) springtime sky, so that program can rest - a little.  Here are my recommendations for northern observers:

1. AT Cnc.  Probably a very ancient nova, and our last campaign showed a credible signal around 28 minutes.  Very desirable to get long runs now, the more the better.

2. NY Ser.  Reputed to be in a standstill state now around 15.5 - I think the first such event observed in this star's sparse history. Excellent morning target.

3. AM CVn.  Perhaps the least exciting star to observe (always within 0.15 mag of 14.2), but very important since it is the prototype of one of the most important classes - the mass-transferring double white dwarfs.  We have a TENTATIVE detection of period change through 2016, but a good 2018 season should nail it down.  This calls for steady coverage through April (especially) and March.

4. HT Cam.  A DQ Her star for which we'd like to get a particularly accurate estimate of period change.

5. BK Lyn.  What's it doing this year?  Pretty steady, or cycling like the ER UMa stars.  Spot checks will be fine, not necessarily time series.

And for southern observers:

1. V598 Pup.  Lots of activity in this fascinating recent nova. Except for Berto, who always seems to spot the most interesting jewels, we've never observed it before.

2. IM Nor.  Back in the sky now.  At 18.5, maybe only Gordon can work on it.  But some eclipse timings in the new season - i.e. maybe 20-25 hours of coverage - would be great to add to our >95% completed paper on this star.

3. V959 Mon.  Another recent nona for which we need the 2018 orbital light curve.  It's a long period, so your runs need to be at least 4 hours.

4. WX Pyx.  Keep going on this one, the Pdot is still kinda insecure.
(I think; Enrique would know for sure).

And both hemispheres: SW Sex.  We've never done a good job on it, and there's no excuse for it.  ALL the SW Sexers have been good to us... so let's give the prototype a chance!

Those are my recs.  Enrique may send his, of course.

joe

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