Z 176-40 , the SIMBAD biblio

Z 176-40 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST21:36:02


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Bibcode/DOI Score in Title|Abstract|
Keywords
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Title First 3 Authors
1987AJ.....93.1326B 133 22 A study of the large-scale structure in the distribution of galaxies in a region centered about the Cancer cluster. III. Further observational results. BICAY M.D. and GIOVANELLI R.
1996A&AS..117..467G viz 22339 19 An image database. II. Catalogue between δ=-0deg and δ=70deg. GARNIER R., PATUREL G., PETIT C., et al.
1996AJ....112.1803M viz 1940 39 Large-scale structure at low galactic latitude. MARZKE R.O., HUCHRA J.P. and GELLER M.J.
1999ApJS..125..409C viz 13439 54 Arcsecond positions of UGC galaxies. COTTON W.D., CONDON J.J. and ARBIZZANI E.
1999PASP..111..438F viz 14       D               1 19407 418 The updated Zwicky catalog (UZC). FALCO E.E., KURTZ M.J., GELLER M.J., et al.
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2011A&A...532A..74B viz 15       D               1 4469 118 The EFIGI catalogue of 4458 nearby galaxies with detailed morphology. BAILLARD A., BERTIN E., DE LAPPARENT V., et al.
2017ApJ...837..120G viz 16       D               1 14404 66 LOSS revisited. I. Unraveling correlations between supernova rates and galaxy properties, as measured in a reanalysis of the Lick Observatory Supernova Search. GRAUR O., BIANCO F.B., HUANG S., et al.
2019MNRAS.488..590B viz 16       D               1 4467 ~ The systematics of galaxy morphology in the comprehensive de Vaucouleurs revised Hubble-Sandage classification system: application to the EFIGI sample. BUTA R.J.
2022ApJ...935..170A viz 17       D               1 44067 26 Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory. ABREU P., AGLIETTA M., ALBURY J.M., et al.
2023ApJS..269....3M viz 17       D               1 356397 ~ Siena Galaxy Atlas 2020. MOUSTAKAS J., LANG D., DEY A., et al.

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