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[vsnet-chat 4592] Name List 76
- Date: Wed, 11 Jul 2001 18:49:53 +0100 (BST)
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: crawl@zoom.co.uk
- Subject: [vsnet-chat 4592] Name List 76
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
- User-Agent: IMP/PHP IMAP webmail program 2.2.4-cvs
Seiichi Yoshida has kindly informed me that Name List 76
has just been released by the GCVS group, currently
available as IBVS 5135... ...www.konkoly.hu then follow
appropriate links to either an html version or the three
tables as ascii txt files.
I extend personal congratulations to Seiichi and his
observing team with regards to the plethora of MISAO
variables included in this Name List.
Other significant numbers of new variables also included
come from Takamizawa, with also a handful or so from
Haseda, a smattering from Bernhard and the odd TAV star.
It is also worthy of note that a significant number of
primary references for objects named within this new Name
List are actually references to vsnet!!!
Checking the GCVS Group's webpages I find no mention of
Name List 76 as yet... ...this will probably appear in a
few days, as well as an ftp availability of the Name List.
Ideally their online GCVS data file will have this new name
list immediately subsumed into it.
I will wait a few days for this to happen... ...if it does
not I will provide a TDF for Guide users so as to enable
them to use the data directly from table 1 of the ascii
files provided with the Name List.
I'll leave this a couple of days because i) the online GCVS
file may well include this data very soon, so simply
downloading this and using it with my previously vsnet-caht
posted GCVS TDF will suffice as update, ii) I'm tired and
I'm going down the pub.
Finally, the ability of the GCVS group to so easily include
new variables so quickly nowadays is as much a testament to
the quality, "depth" and availability of modern astrometric
reference catalogues as anything else.
Indeed, most of these objects are more readily recoverable
than are some GCVS objects that have been included in the
GCVS since its inception. This should be no great
surprise, the former use at least GSC 1.x and modern
computer algorithms for their positional reference and
calculation, whereas the latter had naught but a graduated
rule and a copy of a Durchmusterung or other from which to
obtain a position.
Cheers
John
John Greaves
UK
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