==========================================================================
J/other/AstBu/70.24 Updated 2MFGC catalog (Mitronova+, 2015)
The following files can be converted to FITS (extension .fit or fit.gz)
2mfgc.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/AstBu/70.24
==========================================================================
drwxr-xr-x 42 cats archive 4096 Feb 2 13:09 [Up]
drwxr-xr-x 4 cats archive 315 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 473 Dec 19 2022 .message
-r--r--r-- 1 cats archive 5867 Mar 27 2015 ReadMe
-r--r--r-- 1 cats archive 576584 Mar 27 2015 2mfgc.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-rw-r--r-- 1 cats archive 1702 Mar 27 2015 +footg5.gif
-rw-r--r-- 1 cats archive 29200 Mar 27 2015 +footg8.gif Beginning of ReadMe :J/other/AstBu/70.24 Updated 2MFGC catalog (Mitronova+, 2015)
================================================================================
Visual survey of 18020 objects from the 2MFGC catalog.
Mitronova S.N., Korotkova G.G.
<Astrophys. Bull., 70, 24 (2015)>
=2015AstBu..70...24M
================================================================================
ADC_Keywords: Galaxies, IR ; Galaxy catalogs ; Infrared sources ;
Photometry, infrared ; Morphology
Keywords: galaxies: spiral - catalogs - surveys
Abstract:
We spent a solid overview of the infrared and visual images 18020
2MFGC galaxies selected in the automatic mode of 1.64 million.
Extended objects XSC-2MASS catalog with respect infrared axes, a/b>=3.
This work is aimed at excluding "spurious" objects from the list of
flattened galaxies. Browse more than 80000 images in different filters
were able to identify 1512 (8.4% of the total) of such objects. Found
duplicate in 2MASS measurements of 23 galaxies with, respectively, two
rooms 2MFGC, and 3 flat galaxy, not accounted for in other directories
and in close proximity with the three "spurious" galaxies. The main
part of the excluded facilities accounted for magnitudes less
Ks=13mag. They are characterized by small angular size, low surface
brightness and the concentration index. Exception objects identified
significantly reduced the spread of values in the two-dimensional
distribution. Results of work in the form of notes will be placed in
the astronomical database VizieR, NED, HYPERLEDA.