VizieR

Distance ρ
Position angle θ
Distance (x,y)
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J2000
B1950
Ecl. J2000

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If the access to catalogues with VizieR was helpful for your research work,the following acknowledgment would be appreciated: This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23

	J/MNRAS/480/1507	3444		1.87 and 2.07um observations of 3 GC clusters (Tanaka+, 2018) ReadMe+ftp 2018MNRAS.480.1507T Similar Catalogs
	J/MNRAS/480/1507/table4		^(c)Our detection of known WR stars in the Galactic Centre cluster area (17 rows)
	J/MNRAS/480/1507/table5		^(c)Our detection of known WR stars/LBVs in the Quintuplet cluster area (24 rows)
	J/MNRAS/480/1507/table6		^(c)Our detection of known WR stars in the Arches cluster area (19 rows)
	J/MNRAS/480/1507/table7		^(c)Correspondence of FN1875 detection with Dong et al. (2011MNRAS.417..114D) for the sources of the Galactic Centre cluster area (28 rows)
	J/MNRAS/480/1507/table8		^(c)Correspondence of FN1875 detection with Dong et al. (2011MNRAS.417..114D) for the sources of the Quintuplet cluster area (31 rows)
	J/MNRAS/480/1507/table9		^(c)Correspondence of FN1875 detection with Dong et al. (2011MNRAS.417..114D) for the sources of the Arches cluster area (26 rows)
	J/MNRAS/480/1507/table11		^(c)Extremely red sources (non-Miras) with T<1000K in the Galactic Centre cluster area (41 rows)
	J/MNRAS/480/1507/table12		^(c)Extremely red sources (non-Miras) with T<1000K in the Quintuplet cluster area (15 rows)
	J/MNRAS/480/1507/table13		^(c)Extremely red sources (non-Miras) with T<1000K in the Arches cluster area (9 rows)
ALL
			^(c) indicates tables which contain celestial coordinates

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