(fwd) Checking New Variables (Greaves) Date: Mon, 17 Apr 2000 08:36:49 +0000 From: JG <jgts@jgws.totalserve.co.uk> Subject: Checking New Variables [This file contains links to suspected variable data sources] The fact that there are now nearly as many 'known' variable stars unlisted in official repositories as there are listed ones is becoming a problem for the more well equipped and/or interested observer. Whilst searching for some lists myself via the VSNET website's excellent internal search device [especially excellent compared to the usual fare of web search engines] I noted that data on new variables were dotted about many disparate listings throughout the site. I also noticed that debates have arisen from time to time re correcting this situation, with professionals noting that the IBVS is the proper place for things to be published [which it is], whilst amateurs have noted how difficult that is, especially when the character of the object has not yet been fully ascertained. The publishing system of TeX is also one of those difficult, somewhat arcane, esoteric systems that can only defended by those that know it intimately, ie the cognoscenti. The Sternberg Astronomical Institute of late has put great expertise and effort into correcting such situations, with an increased output and higher rate of relevant catalogues which are often accessible via the CDS for download or for interrogation via SIMBAD and/or VIZIER. SIMBAD and VIZIER are on the whole not strictly relevant here, however, because the preliminary level that the data for these sort of objects is often at, is not within their remit. VSNET itself tries to resolve some of these problems with postings and links. Yet the case remains that the problem is still more or less intransigent for the _barely_ suspected variables. A case in point has arisen very recently. After reading VSNET-CHAT 02818 I happened to follow the link to G. Masi's [impressive] website. There I noted some interesting pages showing images of a probable variable lying near the planetary nebula M27 that were taken in 1996,7. Checking this against my datafiles I find that this variable is exactly coincident with the independently discovered MisV0719, and on checking their webiste I found MisV0719 was logged as a late 1999 discovery. Given its position near a photogenic object, and its magnitude range, I would not be surprised if it had been noted on many separate occasions. Of late I have proffered TDF files to anybody interested listing as many suspect variables as I could easily obtain data for. People need the Guide 7 planetarium program to use these files effectively, but I know that many Australian, German, Japanese, UK and US observers use this software, and the number of other languages it is available in suggests that other Europeans also make strong use of it [eg Holland, Italy: nearly all non-English language versions are apparently translated by users]. A handful of direct and indirect indications have revealed that some of these files have been of great practical use to some variable star observers. I therefore repeat here links to all the added datasets I have made TDF files for over the past year or so, some of which have been posted at www.projectpluto.com/extras and some at www.kusastro.kyoto-u.ac.jp/vsnet. By placing them together I hope to provide one easily referred to link, and have hopefully named this message appropriately re search engines. The links contain full details of the data and how to freely access/download the relevant files, plus details of how to use these files via the included TDF [and occasional ETB] files. Relevant references re the source data are also given at these links. ETHOS Basically, if someone feels they have discovered a new variable, they should turn on every one of these user datasets and check the position of the object in question to see if it is already known. It would also be wise to turn on every internal dataset that comes with Guide, which includes ones for the GCVS & NSV & Downes&Shara and for objects like AGNs, BLLACs and QSOs. To some extent this can also be used as a test for cross identifications for already known objects, although only on a one at a time basis: there is no facility to match entire lists, that is a database management package function. An example would be CGCS 1960 = TmzV386 = HS 434 = GSC 4833 0939. [Of course, normal checks re asteroids must also be made, and things like past images checked when near galaxies fields: ie for suspected supernovae]. Remember also, that there are still several small datasets not included here, and also some other objects [eg Dahlmark variables] for which I have not been able to find a suitable ascii dataset. These files are freely available for anybody to use whenever, the only constraint is that any results based on these works _must_ take the usual proper route via academic references re the _original_ source data [references are noted in the links]. There is, on the other hand, no need whatsoever to refer to the TDFs etc having been used, nor to myself. Any truly interesting results so gleaned ought to also be checked via the more traditional routes. Once we are on the internet we sometimes forget that not every other astronomer going who has a computer is also on the internet, or if so, is not necessarily a subscriber to or browser of VSNET. Therefore folk should feel free to distribute these files freely to whomever they feel would benefit, whether to friends or to observing groups, via floppy disk. [No charge must be made except possibly to recoup the cost of the floppies: also adhere to the restrictions stated with the source data re distribution, usually included in a readme file accompanying the data at the relevant website]. Others will use another planetarium program instead of Guide. I have exclusively used Guide since version 2 in 1993 and have never used any other suite of its ilk, so if users of other software packages are interested in this sort of idea, they will have to do their own relevant conversions. In these instances the following links will at least point them towards the data sources. [I am not a VSNET subscriber, so general points re this posting should be directed to me rather than waste VSNET bandwidth. Unless, of course, the point being made is relevant to VSNET and/or the problem of new variables as a whole. Guide by ProjectPluto has its own egroup with a link via www.projectpluto.com, so kindly don't flood VSNET with questions re Guide usage]. John John Greaves, UK jgts@jgws.totalserve.co.uk Takamizawa Variables:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02733.html with the Takamizawa files available via:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02735.html MISAO variables TDF & ETB, & ETB for some TA var's:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02764.html FASTT stars:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02819.html Haseda Variables & MISAO variables update:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02820.html New Suspected Variable Supplement data:- http://vsnet.projectpluto.com/extras.htm#NSVS New Suspected Variable Supplement notes & cross IDs:- http://vsnet.projectpluto.com/extras.htm#NSVS_notes Catalogue of Cool Galactic Carbon Stars (CGCS):- http://vsnet.projectpluto.com/extras.htm#cgcs Name List 75 details, TDF and errata:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02811.html http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02812.html NameList 75: inclusion of cross identification data:- http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02814.html