Dictionary of Nomenclature of Celestial Objects
(Last update: 29-Nov-2021)

Result of query: info cati BIG NNNa$



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Details on Acronym:   BIG
   BIG (Byurakan, IR Galaxy) Write:<<BIG NNNa>> N: ? Object:G  (SIMBAD class: Galaxy) Note:FBS IRAS galaxies.
Stars and galaxies are simultaneously included in the four first refs, and a general numbering was made.
See [M97c], BIS.
2000Ap.....43..309M:
"179 IR sources were identified with extragalactic objects in the first refs, the numbering continues from the number 180. The galaxies published earlier will be designated BIG 1 to 179 in the order of publication". Ref:=1997Ap.....40....1M byMICKAELIAN A.M. Astrophysics, 40, 1-9 (1997) Optical identification of 100 IRAS point sources at high galactic latitude. oGalaxies 'BIG NN' and stars 'BIS NN' are not numbered here, they are respectively the galaxies and the stars included in [M97c] NNN objects. oTable 1: <[M97c] NNN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)? Ref:=1997Ap.....40..379M byMICKAELIAN A.M. , GIGOYAN K.S., RUSSEIL D. Astrophysics, 40, 379-389 (1997) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. II. oGalaxies 'BIG NN' are not numbered here, they are added to the galaxies in the first '[M97c]' reference: 1997Ap.....40....1M. oTable 1: <[M97c] NNNa> (Nos 101-158) N=68. Table 1: <BIG NNN> N=? Ref:=1998Ap.....41..161M byMICKAELIAN A.M. , GIGOYAN K.S. Astrophysics, 41, 161-169 (1998) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. III. oGalaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. oTable 1: <[M97c] NNNa> (Nos 159-206) N=62. Table 1: <BIG NNN> N=? Ref:=1998Ap.....41..232M byMICKAELIAN A.M. , GIGOYAN K.S. Astrophysics, 41, 232-238 (1998) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. IV. oGalaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. oTable 1: <[M97c] NNNa> (Nos 207-240) N=51. Table 1: <BIG NNN> N=? Ref:=2000Ap.....43..309M byMICKAELIAN A.M. Astrophysics, 43, 309-321 (2000) Optical identification of IRAS point sources. Galaxies. V. oBIG numbering (Nos 1-179) are the galaxies in 1997Ap.....40....1M, 1997Ap.....40..379M, 1998Ap.....41..161M, 1998Ap.....41..232M. oTable 1: <BIG NNNa> (Nos 180-238) N=89. Ref:=2001Ap.....44...33M byMICKAELIAN A.M. Astrophysics, 44, 33-45 (2001) Optical identifications of IRAS point sources. Galaxies. VI. oTable 1: <BIG NNNa> (Nos 239-298) N=87. Ref:=2001Ap.....44..185M byMICKAELIAN A.M. Astrophysics, 44, 185-198 (2001) Optical identifications of IRAS Point Sources. Galaxies. VII. oTable 1: <BIG NNNa> (Nos 299-361) N=95. Ref:=2002Ap.....45..288M byMICKAELIAN A.M. Astrophysics, 45, 288-301 (2002) Optical identifications of IRAS Point Sources. Galaxies. VIII. oTable 1: <BIG NNNa> (Nos 362-416) N=89. Ref:=2004Ap.....47...91M byMICKAELIAN A.M. , SARGSYAN L.A. Astrophysics, 47, 91-103 (2004) Optical identification of IRAS Point Sources Galaxies IX. oTable 1: <BIG NNNa> (Nos 417-476) N=87. Ref:=2004Ap.....47..213M byMICKAELIAN A.M. , SARGSYAN L.A. Astrophysics, 47, 213-228 (2004) Optical identification of IRAS point sources. Galaxies. X. oTable 1: <BIG NNNa> (Nos 476-536) N=104. Originof the Acronym: A = Assigned by the author(s)

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