VizieR

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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/ApJ/899/15	-1		Parameters for the 58 τHI(v) sightlines (Murray+, 2020) ReadMe+ftp 2020ApJ...899...15M Similar Catalogs
	J/ApJ/899/15/tabled1		^(c)Parameters for the 58 τHI(v) sightlines used for verifying the CNN model (58 rows)
	J/MNRAS/505/4048	-1		WISDOM Project IX study of GMCs in NGC 4429 (Liu+, 2021) ReadMe+ftp 2021MNRAS.505.4048L Similar Catalogs
	J/MNRAS/505/4048/table1		^(c)Observed properties of the clouds in NGC 4429 (Note)* (217 rows)
	J/MNRAS/505/4048/table3		Derived properties of the clouds in NGC 4429 (Note)* (217 rows)
	J/MNRAS/512/86	-1		ISM study with nearby AGNs and galaxies (Bernhard+, 2022) ReadMe+ftp 2022MNRAS.512...86B Similar Catalogs
	J/MNRAS/512/86/2jytab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the 2Jy sample (Note)* (46 rows)
	J/MNRAS/512/86/3crtab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the 3CR sample (Note)* (45 rows)
	J/MNRAS/512/86/atlatab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the Atlas3D sample (Note)* (6 rows)
	J/MNRAS/512/86/hrstab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the HRS sample (Note)* (8 rows)
	J/MNRAS/512/86/pgqtab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the PG QSO sample (Note)* (70 rows)
	J/MNRAS/512/86/t2qstab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of Type-II QSO sample (Note)* (86 rows)
	J/MNRAS/512/86/ulirtab1		^(c)Properties and dust masses derived with 100/160 microns flux ratios method of the ULIRG sample (Note)* (41 rows)
	J/MNRAS/512/86/2jytab2		Properties and dust masses derived with IR SED fits method of the 2Jy sample (Note)* (8 rows)
	J/MNRAS/512/86/3crtab2		Properties and dust masses derived with IR SED fits method of the 3CR sample (Note)* (4 rows)
	J/MNRAS/512/86/atlatab2		Properties and dust masses derived with IR SED fits method of the Atlas3D sample (Note)* (3 rows)
	J/MNRAS/512/86/pgqtab2		Properties and dust masses derived with IR SED fits method of the PG QSO sample (Note)* (9 rows)
	J/MNRAS/512/86/t2qstab2		Properties and dust masses derived with IR SED fits method of the Type-II QSO sample (Note)* (12 rows)
	J/MNRAS/512/86/ulirtab2		Properties and dust masses derived with IR SED fits method of the ULIRG sample (Note)* (14 rows)
	J/MNRAS/512/86/2jytab3		K-band stellar mass and SFRs for the 2Jy sample (Note)* (46 rows)
	J/MNRAS/512/86/3crtab3		K-band stellar mass and SFRs for the 3CR sample (Note)* (45 rows)
	J/MNRAS/512/86/atlatab3		K-band stellar mass and SFRs for Atlas3D sample (Note)* (6 rows)
	J/MNRAS/512/86/hrstab3		K-band stellar mass and SFRs for the HRS sample (Note)* (8 rows)
	J/MNRAS/512/86/pgqtab3		K-band stellar mass and SFRs for PG QSO sample (Note)* (70 rows)
	J/MNRAS/512/86/t2qstab3		K-band stellar mass and SFRs for Type-II QSO sample (Note)* (86 rows)
	J/MNRAS/512/86/ulirtab3		K-band stellar mass and SFRs for ULIRG sample (Note)* (41 rows)
ALL
			^(c) indicates tables which contain celestial coordinates

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