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Gary Poyner reports that HR Lyr was very faint last night (Dec 13.799, V = 16.63). He notes this is the faintest in V since 2016 Sep.
The light curve shows that HR Lyr has faded rapidly since the beginning of the month: just over 1 mag in 6 days.
How faint will it get? Let’s keep watching to find out…..
Jeremy
Thanks to everybody for arranging a superb meeting yesterday. Three brilliant talks; really good Sky Notes, Nick!
Really interesting, Robin.
Congratulations on receiving your gong at yesterday’s BAA meeting in London. Well deserved!
Hello Kevin,
I generally eyeball my data to see if there are any strange data points. Looking at the measured errors can also give a clue as to what might be happening- as can having a look at what is happening to the Check star at the same time. I’d be vary wary of any automated process for cleaning data.
But be careful about being too enthusiastic about deleting data as the results might be real!
Jeremy
I enjoyed seeing your light curve, Kevin.
You can submit the data as “Clear” filter (abbreviated to C).
For some purposes (like time series photometry of cataclysmic variables), C is perfectly acceptable (when you use a filter, you lose some of the light, so your signal to noise deteriorates). However, for many applications a filter is much preferred as it’s easier to compare data from different observers.
Many thanks everyone for your replies – also some I received offline.
I’ve ordered the Celestron NexYZ
Go well!
Jeremy
Thanks Paul. The behaviour looks different on the two nights (I realise the second run was quite a bit longer than the first)
An updated light curve covering the campaign up to Aug 9 is shown on the VSS website.
In the last month it’s faded by about a magnitude. Please do keep up nightly observations of the star and if anyone is able to do long CCD photometry runs (a few hours), it would be greatly appreciated.
There will be a more detailed update on the campaign in the next Variable Star Section Circular which is due to appear on Sept 1.
The Circular is emailed free to anyone that requests it – if you are not already on the distribution list please contact me using the “Send Email” button to the left of this message.
The NAM session was an excellent opportunity to meet up with some of the professionals we work with. Many thanks to Callum and Dirk Froebrich for proposing to the RAS that a pro-am session be held and for subsequently organising it.
A report will appear in a future Journal.
Very interesting results, Bill. Certainly an impressively faint detection limit.
I realise that you are mainly doing this for spectroscopy, but are you able to analyse the videos by UFO Analyser?
I hope you have some clear skies for the Perseids!
We are now 3 months into the HR Lyr campaign and we have a nice light curve of this old nova developing. This can be seen on the VSS website. It has been brightening steadily over the last 3 weeks and is now as bright has it has been for a very long while. It will be interesting to see just how bright it becomes.
Time-resolved photometry continues to show various humps and bumps in the light curve with an amplitude of ~0.15 mag. These appear to be fairly regular for a few cycles (~1.5 h), but they do not appear to be consistent. Moreover the shape of the bumps is quite variable.
A couple of requests:
1. Please keep the once-or twice per night snapshot photometry going. New observers are always welcome, of course.
2. Some really long photometry runs (several hours) over a few nights would help us to understand the short term variations and see whether a coherent signal emerges. Late July onwards would be a good time for this as the nights are becoming longer.
Many thanks to all the observers who have supply visual and CCD photometry:
David Boyd, Walter Cooney, Pavol Dubovsky, Sjoerd Dufoer, Carlo Gualdoni, Kevin Hills, Steve Johnston, Mel Joslin, Paul Leyland, JH Mallett, Ian Miller, Ken Menzies, Martin Mobberley, Roger Pickard, Gary Poyner, Jeremy Shears, Dave Smith, Richard Sabo, Tonny Vanmunster, Ivan Walton
Jeremy Shears
Good to hear you might be able to attend, Eric.
I’m staying in the conference hotel in Grimbergen the Friday and Saturday nights. Which is probably just as well since Grimbergen is well-known for its Trappist beers.
I wonder if anyone else is going from the UK.
Several hours, Grant, probably > 3 (there is a proposed period of 0.1 day, which could set the lower limit for t/series, but I’m doubtful about that). However, such long runs are not possible at these latitudes atm.
We are now one month into the campaign and, whilst it’s still early days, it’s good to see the first data coming in. Many thanks to: David Boyd, Walter Cooney, Sjoerd Dufoer, Ian Miller, Ken Menzies, Martin Mobberley, Roger Pickard and Gary Poyner.
The star has varied between mag 15.4 and 16.2. Time series photometry by Roger Pickard and Ken Menzies has shown various humps and bumps in the light curve, but it’s too early to determine if they are periodic.
With Lyra becoming more accessible in the evening sky, I hope that further observations will begin to flow in. Do feel to join in the campaign. We are looking for nightly snapshot photometry to determine the overall shape of the light curve and well as some multi-hour photometry runs to look for short-term periodicities.
Further details about the campaign can be found here.
Yes, I’m following it from my home observatory, Mike. I had it at mag 14.2 in an unfiltered CCD image last night (Apr 25 at 21.04 UT).
Looks like I’m in for a few cloudy nights, so I hope you are able to be more successful from Arizona
Glad to hear Alan’s talk went down well and to see him looking so well. Wonderful to hear his experiences of a lifetime in astronomy – I’m looking forward to the video.
Thanks Bill. David Portree tells me we can expect some more images of the crater:
“Stand by on that new Blagg crater image – tentative date is 4/25. We have the low-Sun image mosaic I used in the post and some high-Sun images that show mainly brightness variations – if all goes well, the new image (actually a pair taken on successive orbits) will be intermediate between the two, so we’ll see more of the Blagg crater floor and more secondary crater wall slump action (if it exists).”
If I hear more, I’ll let you know.
