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[vsnet-chat 3182] Re: IRAS18314+0134



     There are five blue plate scans available for this field, and 
sequencing through them indicates no obvious variability:  it is always
lsightly brighter than the star northwest shown on these cutouts:

Field Name: iras
RA, Dec   = 18:33:58.7, +01:36:25.2

The information file (with links to all the images) is:
  http://vsnet.nofs.navy.mil/tmp/fchaaiffa_fch.html

The image files containing the data can be found at:

Merged Images:
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_se0631.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_so0631.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sj0878.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sf0878.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sn0878.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sj0879.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sf0879.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sn0879.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sb0878.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sb0879.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sr0878.000.jpg
  jpg file: http://vsnet.nofs.navy.mil/tmp/fchaaiffa_sr0879.000.jpg

Very bright of course on the red and far-red plates, but the variations
should be most evident (and largest amplitude) on the blue plates.

\Brian

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