SUBJECT: Bright Star Monitor member participation
The AAVSO operates a global network of five, small robotically controlled, CCD equipped, telescopes. These scopes support a full complement of filters and are capable of precision photometry in the range of 3 to 13 magnitudes in the V filter. The network has been in operation for several years performing several major photometric surveys. Recently a decision has been made to promote an increase member use of the network. All members, including the visual observer, are welcome to participate in an initial roll-out of this program this fall without going through the normal proposal approval process. There is no cost to participate for members. We are looking for an intial group of six. Each participant can provide their own targets of interest. Mentors are available to assist the observer in plan preparation, image analysis using the AAVSO VPHOT analysis software and in the data submittal. Please respond to this post if you have an interest in participating and I will answer questions and fill in additional details.
Clear Skies,
Mike
Hi Mike,
I am interested in observing YSOs in the southern hemisphere.
Thanks
Hi VAastro,
Thank you for expressing your interest. I'd like to answer any questions you may have. I noticed you have a Observer code, are you an AAVSO member?
Mike
Yes, very interested in the program. Specifically, in observing RR Lyrae stars. I am a memeber of AAVSO. My observer code is PMAN. Thank you for posting the information about this exciting opportunity!
Hi PMAN,
Thanks for expressing your interest. Do you have a target in mind? If so, please start by providing the following info I will need to process your request.
Target: Name
Filter(s) for observations - Typically the V filter is included. You may want to include additional filter(s)
VPHOT: Do you want the images sent to AAVSO's VPHOT photometry application for analysis (and do you need help using it?)
Start and Finish Date: How long do you want to recive images for analysis
Once I have this info we can talk about the next step.
Thanks
Mike
Matt,
The TAC has approved your proposal. Depending on weather you should expect to see images available in VPHOT soon. Let me know when you get the analysis completed and whether we need to adjust the exposures. Also, let me know if you have any other questions.
Mike
Great, thank you. I will keep an eye on my VPHOT account.
Matt,
You should have seen a VPHOT notification for GK Per. There is a V filter image available. Check to see if we need to increase the exposure.
Mike
Thanks Matt,
I've seen your proposal request and we will get back to you ASAP.
Mike
Hi Mike,
Yes, I am a AAVSO member with Observer Code SDM.
Thanks
Erik
I'm interested in participating the the BSM program. I'm and member, and I use VPhot.
Phil Sullivan SPP
Hi Phil,
Do your have a target, do you have its RA and Dec coordinates found in VSX? You might want to view the https://www.aavso.org/how-write-aavsonet-proposal and https://www.aavso.org/apps/aavsonet/proposal/ to get a heads up on the next step.
Mike
Mike,
I'll send you a description of my proposed project by email.
Phil
Hi Mike,
I replied a few minutes ago but it didn't seem to get to th forum, so please excuse me if you've already seen my earlier post.
I'd like to participate in this initiative. Variable Stars South has a number of projects that would benefit greatly from the global coverage of BSM telescopes. Is the BSM-ARG system hosted by Jaime Garcia up and running? If so it would plug a gap in the longitude coverage in the southern hemisphere. Any plans for an African BSM system?
I am a member of AAVSO and have experience with using VPhot.
The first target I am keen to observe is V777 Sgr ( 17 46 25.39, -26 12 01.1 ) a long period eclipsing binary that is due to start ingress in a couple of weeks. We need to monitor with all southern hemisphere BSM systems in B and V (and U if possible?) a couple of times per night from before first contact until after second contact, a period of a few weeks.
Cheers,
Mark
Hi Mark,
Thanks for the interest. The South American site is unfortunately not up and running at this time, please stay tuned. V0777 Sgr is good target being in the range 8.59 - 8.72 V and at a resonable declination for the southern sites. Would you provide the data requested here, https://www.aavso.org/apps/aavsonet/proposal/ Please include in the Proposal Text box your name, membership status, method of communication such as email. Also, add your description of the target, and scientific purpose or educational context. At the top of the Text box please add that this is a request for the trial BSM roll-out period. Don't forget to hit the submit button. We will get back to you soon about setup of the observing plan. Again, thanks,
Mike
Hi Mike,
I've just submitted a proposal to observe V777 Sgr during the ingress phase of its upcoming eclipse. Let me know if further info or clarification is required. Cheers,
Mark
Mark,
It looks like your proposal will be approved, check back to your request to see when it's status changes from "New" to "Approved"
Mike
Thanks Mike, I'll check periodically. Cheers,
Mark
I would also like to participate if possible.
I'm a member also.
I would like to look at an EB star alp Oct. It is listed as EB with very little data at 2.877d but in the spectroscopic binary DB at 9.073d.
It is catalogued as measurung 5.22-5.26 so only a small dip. It is too bright for me to measure using my scope.
My spectra confirm the 2.87 d but it would be good to have a time series to add confirmation.
Terry
BHQ
Hi Terry,
Thanks for participating. I share your concern that the dip may not rise above the noise. The good news is that it is a fairly bright star. I checked the field around the target for comparision stars (2 degree field) but I didn't find any. There are two stars HIP 102162 (5.99 mag) and HIP 104365 (6.57 mag) which might be usable in this case. I think the thing I fear the most is the airmass at the declination (-77 01 25.6) which would also affect the uncertainty. The scope visible horizon just looks doable. Maybe you might have a better target? Let me know.
Mike
I would love to participate.
My interest is observing bright stars (brighter than 6. magnitude on the northern hemisphere) that can be used as comparisonstars.
That is making a list of bright stars with an accuracy of 0.002 mag if possible.
The current accuracy of bright stars is 0.141 mag . Is this realy the best observations today?
I am a member of AAVSO, and I am taking a course with Mark Blackfort this month (DSLR photometry)
Yours
Søren Toft
Denmark
Hi Søren,
I believe you are interested bright comparision stars that can be used for measuring other bright variables. If I got that right then I would recommend you request comparion stars from here: https://www.aavso.org/request-comparison-stars-variable-star-charts
Note: If your variable star has an existing sequence, even if it is only one comparison star, please request assistance via CHET. The above page is only for variables that have NO comparison stars.
In any case, if you have a need for observing with the BSM, let's continue our discusion.
Mike
I am intersted in using these 'scopes in conjunction with Alert notice 645 ( Maser Study)
I have been an AAVSO member for 8years plus.
I hold a degree in Mechanical Engineering Engineering, a 3 year university certificate in Astronomy and Astrophysics of Galaxies and I use a remote telescope with SSON as the winter nights here in Canada are very cold and not conducive to outdoor obdserving inthose log winter months.
Cheers
Dave DDJ
Dave,
Me too, I mean I have a Mechanical Engineering degree. The are many reasons we in the membership would find the BSM useful!. The next steps for you to follow are summarized below:
Important Input from the User captured here https://www.aavso.org/apps/aavsonet/proposal/
If you have any questiosn we could take them to e-mail.
Mike
Yes, it looks like the exposure time needs to be increased. As I understand it, that will increase the target size. As you can see from my attachment, GK Per looks very small and faint.
FYI: I will be unavailable the rest of tonight, as I am leaving for work soon. Thanks.
Matt,
Changes have been made, let me know if I can help with VPHOT.
Mike
Update:
Since the orginal post, four members proposed observation plans and they have been accepted. There is room for more participation. Please let me know if you are interested.
Mike
Hi Mike,
I've received several nights of V777 Sgr BVRI observations from BSM-S and BSM-Berry and I'm grateful for those. However, for our specific project the R and I observations are not useful because the eclipse depth in those bands is very shallow.
Currently there are 3 images in each of the BVRI filters, and only one set is recorded each night.
I would like to have the schedule changed to so that a set contains 5 images in each of B and V, and have two sets of images recorded at each telescope each clear night. The first set as early in the evening as possible (but not in twilight) and the second set when V777 Sgr reaches 40 degrees elevation.
The current exposure times (40sec in V, 80sec in B) are fine.
Finally, can the images be added to David Benn's ( BDJB ) VPhot account as well as my own?
Cheers,
Mark
OK, I'll get on it.
Please, give us a day or so to get this worked out
Thanks
Mike