VizieR

Distance ρ
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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/A+A/666/A140	-1		Titan's atmosphere analysis (Rannou+, 2022) ReadMe+ftp 2022A&A...666A.140R Similar Catalogs
	J/A+A/666/A140/et10e		Haze extinction at three wavelengths retrieved with occultation T10E (Figure 9 and 18) (kext_T10E.dat) (23 rows)
	J/A+A/666/A140/et10elw		Haze extinction at wavelength 4898nm retrieved with occultation T10E (Figure 18) (kext_T10ELW.dat) (12 rows)
	J/A+A/666/A140/et53e		Haze extinction at three wavelengths retrieved with occultation T53E (Figure 9 and 18) (kext_T53E.dat) (46 rows)
	J/A+A/666/A140/et53elw		Haze extinction at wavelength 4898nm retrieved with occultation T53E (Figure 18) (kext_T53ELW.dat) (32 rows)
	J/A+A/666/A140/et78e		Haze extinction at three wavelengths retrieved with occultation T78E (Figure 9 and 18) (kext_T78E.dat) (30 rows)
	J/A+A/666/A140/et78elw		Haze extinction at wavelength 4898nm retrieved with occultation T78E (Figure 18) (kext_T78ELW.dat) (13 rows)
	J/A+A/666/A140/et78i		Haze extinction at three wavelengths retrieved with occultation T78I (Figure 9 and 18) (kext_T78I.dat) (30 rows)
	J/A+A/666/A140/et78ilw		Haze extinction at wavelength 4898nm retrieved with occultation T78I (Figure 18) (kext_T78ILW.dat) (14 rows)
	J/A+A/666/A140/eslt10e		Haze spectral slope dLn(kext)/dLn(wavelength) relative to alpha_0 = -2.18 retrieved with occultation T10E (Figure 10) (kext_slopeT10E.dat) (23 rows)
	J/A+A/666/A140/eslt53e		Haze spectral slope dLn(kext)/dLn(wavelength) relative to alpha_0 = -2.18 retrieved with occultation T53E (Figure 10) (kext_slopeT53E.dat) (46 rows)
	J/A+A/666/A140/eslt78e		Haze spectral slope dLn(kext)/dLn(wavelength) relative to alpha_0 = -2.18 retrieved with occultation T78E (Figure 10) (kext_slopeT78E.dat) (30 rows)
	J/A+A/666/A140/eslt78i		Haze spectral slope dLn(kext)/dLn(wavelength) relative to alpha_0 = -2.18 retrieved with occultation T78I (Figure 10) (kext_slopeT78I.dat) (30 rows)
	J/A+A/666/A140/xch4t10e		Methane mixing ratio retrieved with occultation T10E (Figure 11 - top) (xch4_T10E.dat) (23 rows)
	J/A+A/666/A140/xch4t53e		Methane mixing ratio retrieved with occultation T53E (Figure 11 - top) (xch4_T53E.dat) (46 rows)
	J/A+A/666/A140/xch4t78e		Methane mixing ratio retrieved with occultation T78E (Figure 11 - top) (xch4_T78E.dat) (30 rows)
	J/A+A/666/A140/xch4t78i		Methane mixing ratio retrieved with occultation T78I (Figure 11 - top) (xch4_T78I.dat) (30 rows)
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