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J/ApJS/260/35

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	J/ApJS/260/35	4021		Classical Be stars from LAMOST MRS DR7 (Wang+, 2022) ReadMe+ftp 2022ApJS..260...35W Similar Catalogs
	J/ApJS/260/35/table2		^(c)Be candidate spectra selected for the training sample (1042 rows)
	J/ApJS/260/35/table3		^(c)Non-Be candidate spectra selected for the training sample (1042 rows)
	J/ApJS/260/35/table5		^(c)Oe stars found from the LAMOST MRS DR7 sample (8 rows)
	J/ApJS/260/35/table6		^(c)Known Be stars found from the MRS sample (151 rows)
	J/ApJS/260/35/table7		^(c)Newly identified classical Be (CBe) stars from the LAMOST MRS DR7 sample (183 rows)
	J/ApJS/260/35/table8		^(c)Open cluster memberships for identified CBe stars from the LAMOST MRS DR7 sample (41 rows)
	J/ApJS/260/35/table9		^(c)The peculiar velocities of the 16 runaway CBe stars identified from the LAMOST MRS DR7 sample (16 rows)
	J/ApJS/260/35/tablea1		^(c)Candidate Be stars displaying Ha emission profiles with absorption shell line identified from the LAMOST MRS DR7 sample (113 rows)
	J/ApJS/260/35/tablea2		^(c)Candidate Be stars displaying Ha absorption profiles with shell line identified from the LAMOST MRS DR7 sample (199 rows)
	J/ApJS/260/35/refs		References (85 rows)
ALL
			^(c) indicates tables which contain celestial coordinates

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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