D.R.E.A.M.
Database on Rare Earths At Mons University
1Astrophysique et Spectroscopie, Université de Mons-Hainaut, B-7000 Mons, Belgium.
2Institut de Physique Nucléaire, Atomique et de Spectroscopie
(IPNAS), Université de Liège, B-4000
Liege, Belgium.
Maintained by Pascal Quinet
(quinet@umh.ac.be)
1. General introduction and presentation of the tables
Despite their low cosmic abundance, the lanthanides (Z=57-71) become
increasingly important in astrophysics because they are observed on the
high resolution spectra of some stars now currently available via
ground-based or satellite observations. The main purpose of D.R.E.A.M.
(Database on Rare-Earths At Mons University) is to provide the
astrophysicists, but also the physicists, with an updated information
concerning the wavelengths, the oscillator strengths, the transition
probabilities and the radiative lifetimes of neutral, singly or
multiply ionized lanthanides.
In our compilation, the spectra are classified in order of increasing
Z-values and, for a given Z, according to the ionization degree.
For each line in a particular spectrum,
the tables show, respectively:
- the wavelength (in A) deduced from the experimental energy levels.
These wavelengths are given in air above 2000 A and in vacuum below that limit;
- the lower level of the transition represented by its experimental
value (in cm-1), its parity ((e) for even and (o) for odd)
and its J-value. Level energies are taken from the NIST compilation
(W.C. Martin, R. Zalubas and L. Hagan, Atomic Energy Levels - The
Rare-Earth Elements, NBS-NSRDS 60, 1978) except when otherwise
indicated;
- the upper level of the transition presented in the same way as for
the lower level;
- the calculated oscillator strength, log gf, where g=2J+1 is
the statistical weight of the lower level of the transition.
More details about the computational procedure are given in the
different publications listed below. Only transitions
for which log gf > -4.0 are reported in the tables.
For some ions, experimental oscillator strengths or normalized oscillator
strengths using measured lifetimes are given. In these
cases, "EXPT" or "NORM" appears in the last column of the tables;
- the calculated transition probability, gA in s-1, where
g=2J+1 is the statistical weight of the upper level of the transition.
For some ions, experimental gA-values or normalized gA-values using
measured lifetimes are given. In these cases, "EXPT" or "NORM"
appears in the last column of the tables;
- the cancellation factor, CF, as defined by Cowan (1981). Small values
of this factor (typically CF < 0.01) indicate transitions affected by
severe cancellation effects.
2. Publications related to rare-earth elements
- E. Biémont, J.-F. Dutrieux, I. Martin and P. Quinet,
"Lifetime calculations in Yb II",
J. Phys. B: At. Mol. Opt. Phys. 31, 3321-3333 (1998).
(Abstract)
- E. Biémont and P. Quinet,
"Theoretical study of the 4f146s 2S1/2-
4f136s2 2F7/2 E3 transition
in Yb II",
Phys. Rev. Lett. 81, 3345-3346 (1998).
(Abstract)
- P. Quinet, P. Palmeri and E. Biémont,
"On the use of the Cowan's code for atomic structure calculations in
singly ionized lanthanides",
J. Quant. Spectrosc. Rad. Transfer 62, 625-646 (1999).
(Abstract)
- E. Biémont, J.-F. Dutrieux, I. Martin and P. Quinet,
"Ion traps and lifetime calculations in Yb II",
Proc. of the 6th ASOS Conference, Victoria, Canada,
pp. 12--14 (1999).
- P. Quinet, P. Palmeri and E. Biémont,
"On the use of the Cowan code for atomic structure calculations in singly
ionized lanthanides",
Proc. of the 6th ASOS Conference, Victoria, Canada,
pp. 126--128 (1999).
- Z.S. Li, S. Svanberg, P. Quinet, X. Tordoir and E. Biémont,
"Lifetime measurements in Yb II with time-resolved laser spectroscopy",
J. Phys. B: At. Mol. Opt. Phys. 32, 1731-1737 (1999).
(Abstract)
- P. Quinet, P. Palmeri, E. Biémont, M.M. McCurdy, G. Rieger, E.H. Pinnington,
M.E. Wickliffe and J.E. Lawler,
"Experimental and theoretical radiative lifetimes, branching fractions and
oscillator strengths in Lu II",
Mon. Not. R. Astr. Soc. 307, 934-940 (1999).
(Abstract)
- E. Biémont, Z.S. Li, P. Palmeri and P. Quinet,
"Radiative lifetimes in La III and oscillator strengths in La III and Lu III",
J. Phys. B: At. Mol. Opt. Phys. 32, 3409-3419 (1999).
(Abstract)
- P. Palmeri, P. Quinet, J.-F. Wyart and E. Biémont,
"Theoretical lifetimes and oscillator strengths in Ce II. Application to the
chemical composition of the sun",
Phys. Scr. 61, 323-334 (2000).
(Abstract)
- P. Palmeri, P. Quinet, Y. Frémat, J.-F. Wyart and E. Biémont,
"Theoretical oscillator strengths in Pr III and application to some
CP stars",
Astrophys. J. Suppl. Ser. 129, 367-376 (2000).
(Abstract)
- E. Biémont, P. Palmeri and P. Quinet,
"A new database of astrophysical interest",
Proc. Conf. A New Millenium for Galaxy Morphology, South Africa,
Astrophys. Space Sci. 269-270, 635-637 (1999)
(Abstract)
- J.A. Fedchak, E.A. Den Hartog, J.E. Lawler, P. Palmeri, P. Quinet and
E. Biémont,
"Experimental and theoretical radiative lifetimes, branching fractions and
oscillator strengths for Lu I and experimental lifetimes for Lu II and
Lu III",
Astrophys. J. 542, 1109-1118 (2000).
(Abstract)
- E. Biémont, H.P. Garnir, T. Bastin, P. Palmeri, P. Quinet, Z.S. Li,
Z.G. Zhang, V. Lokhnygin and S. Svanberg,
"Radiative lifetime measurements and transition probabilities of astrophysical
interest in Er III",
Mon. Not. R. Astron. Soc. 321, 481-486 (2001).
(Abstract)
- J.F. Wyart, W.U.L. Tchang-Brillet, N. Spector, P. Palmeri, P. Quinet
and E. Biémont,
"Extended analysis of the spectrum of triply-ionized ytterbium (Yb IV)
and transition probabilities",
Phys. Scr. 63, 113-121 (2001).
(Abstract)
- Z.G. Zhang, S. Svanberg, Z. Jiang, P. Palmeri, P. Quinet and E. Biémont,
"Natural radiative lifetimes in Ce II",
Phys. Scr. 63, 122-127 (2001).
(Abstract)
- E. Biémont, H.P. Garnir, P. Palmeri, P. Quinet, Z.S. Li, Z.G. Zhang
and S. Svanberg,
"Core-polarization effects and radiative lifetime measurements in Pr III",
Phys. Rev. A 64, 022503 (2001).
- Z.S. Li, Z.G. Zhang, V. Lokhnygin, S. Svanberg, T. Bastin, E. Biémont,
H.P. Garnir, P. Palmeri and P. Quinet,
"Radiative lifetime measurements in Tm III with time-resolved laser
spectroscopy and comparisons with HFR calculations",
J. Phys. B: At. Mol. Opt. Phys. 34, 1349-1359 (2001).
- E. Biémont, H.P. Garnir, Z.S. Li, V. Lokhnygin, P. Palmeri, P. Quinet,
S. Svanberg, J.-F. Wyart and Z.G. Zhang,
"Experimental and theoretical energy levels, transition probabilities
and radiative lifetimes in Yb III",
J. Phys. B: At. Mol. Opt. Phys. 34, 1869-1876 (2001).
- E. Biémont, P. Palmeri, P. Quinet, G. Paquin, Z.G. Zhang, G. Somesfalean
and S. Svanberg,
"Measurement of radiative lifetimes and determination of transition
probabilities of astrophysical interest in Ho III",
Mon. Not. R. Astr. Soc. 328, 1085-1090 (2001).
- Z.G. Zhang, G. Somesfalean, S. Svanberg, P. Palmeri, P. Quinet and
E. Biémont,
"Radiative lifetime measurements and oscillator strengths of
astrophysical interest in Ho III",
Astron. Astrophys. 384, 364-370 (2002).
- Z.G. Zhang, S. Svanberg, P. Palmeri, P. Quinet and E. Biémont,
"Measurement of lifetimes by laser-induced fluorescence and determination
of transition probabilities of astrophysical interest in Nd III",
Astron. Astrophys. 385, 724-732 (2002).
- Z.G. Zhang, S. Svanberg, P. Quinet, P. Palmeri and E. Biémont,
"Time-resolved laser spectroscopy of multiply ionized atoms - Natural
radiative lifetimes in Ce IV",
Phys. Rev. Lett. 87, 273001 (2001).
- Z.G. Zhang, Z.S. Li, S. Svanberg, P. Palmeri, P. Quinet and E. Biémont,
"Experimental and theoretical lifetimes in Yb III",
Eur. Phys. J. D 15, 301-305 (2001).
- P. Quinet, P. Palmeri, E. Biémont, Z.S. Li, Z.G. Zhang and S. Svanberg,
"Radiative lifetime measurements and transition probability calculations
in lanthanide ions",
J. Alloys Comp. 344, 255-259 (2002).
- Z.G. Zhang, S. Svanberg, P. Palmeri, P. Quinet and E. Biémont,
"Experimental and theoretical studies of Dy III: radiative lifetimes and
oscillator strengths of astrophysical interest",
Mon. Not. R. Astron. Soc. 334, 1-10 (2002).
- E. Biémont, H.P. Garnir, P. Quinet, S. Svanberg and Z.G. Zhang,
"Time-resolved laser-induced fluorescence lifetime measurements and
theoretical transition probabilities in Tb III",
Phys. Rev. A 65, 052502 (2002).
- E. Biémont, P. Palmeri, P. Quinet, Z.G. Zhang and S. Svanberg,
"Doubly ionized thorium: laser lifetime measurements and transition
probability determination of interest in cosmochronology",
Astrophys. J. 567, 1276-1283 (2002).
- E. Biémont, P. Palmeri, P. Quinet, S. Svanberg and Z.G. Zhang,
"Lifetime measurements in doubly ionized uranium",
J. Phys. B: At. Mol. Opt. Phys. 35, 1701-1705 (2002).
- E. Biémont, P. Quinet and T.A. Ryabchikova,
"Core-polarization effects in doubly ionized cerium (Ce III) for
transitions of astrophysical interest",
Mon. Not. R. Astr. Soc. 336, 1155-1160 (2002).
- E. Biémont, G. Kohnen and P. Quinet,
"Transition probabilities in Gd III",
Astron. Astrophys. 393, 717-720 (2002).
- E. Biémont, P. Quinet, Z. Dai, Z. Jiang, Z.G. Zhang, H. Xu and
S. Svanberg,
"Lifetime measurements and calculations in singly ionized ytterbium",
J. Phys. B: At. Mol. Opt. Phys. 35, 4743-4749 (2002).
- M. Reyniers, H. Van Winckel, E. Biémont and P. Quinet,
"Cerium: the lithium substitute in post-AGB stars",
Astron. Astrophys. 395, L35-L38 (2002).
- H. Xu, Z. Jiang, Z.G. Zhang, Z. Dai, S. Svanberg, P. Quinet and
E. Biémont,
"Radiative lifetime measurements in Er II by time-resolved laser
spectroscopy",
J. Phys. B: At. Mol. Opt. Phys. 36, 1771-1781 (2003).
- E. Biémont, H.P. Garnir, U. Litzén, K. Nielsen, P. Quinet, S. Svanberg,
G. Wahlgren and Z.G. Zhang,
"Radiative lifetime and oscillator strength determinations in Sm III",
Astron. Astrophys. 399, 343-349 (2003).
- Z. Dai, Z. Jiang, H. Xu, Z.G. Zhang, S. Svanberg, E. Biémont,
P.H. Lefèbvre and P. Quinet,
"Time-resolved laser-induced fluorescence measurements of Rydberg
states in Lu I and comparison with theory",
J. Phys. B: At. Mol. Opt. Phys. 36, 479-487 (2003).
- E. Biémont and P. Quinet,
"Recent advances in study of lanthanide atoms and ions",
Phys. Scr. T105, 38-54 (2003).
- P. Quinet and E. Biémont,
"Radiative lifetime, oscillator strength and Landé factor calculations
in doubly ionized europium (Eu III)",
Mon. Not. R. Astr. Soc. 340, 463-467 (2003).
- E. Biémont, P.H. Lefèbvre, P. Quinet, S. Svanberg and H. Xu,
"Radiative lifetime measurements and oscillator strength determination
for transitions in singly ionized praseodymium (Pr II)",
Eur. Phys. J. D 27, 33-41 (2003).
- H. Xu, S. Svanberg, R.D. Cowan, P.H. Lefèbvre, P. Quinet and
E. Biémont,
"Theoretical and experimental lifetime determination in singly ionized
neodymium (Nd II)",
Mon. Not. R. Astr. Soc. 346, 433-440 (2003).
- H. Xu, S. Svanberg, P. Quinet, H.P. Garnir and E. Biémont,
"Time-resolved laser-induced fluorescence lifetime measurements and
relativistic Hartree-Fock calculations of transition probabilities
in Sm II",
J. Phys. B: At. Mol. Opt. Phys. 36, 4773-4787 (2003).
- P. Quinet and E. Biémont,
"Landé g-factors for experimentally determined energy levels in doubly
ionized lanthanides",
At. Data Nucl. Data Tables 87, 207-230 (2004).
- E. Biémont, P. Quinet, S. Svanberg and H.L. Xu,
"Experimental lifetime determination in neutral praseodymium (Pr I)
and neodymium (Nd I)",
J. Phys. B: At. Mol. Opt. Phys. 37, 1381-1389 (2004).
- E. Biémont, P. Quinet, S. Svanberg and H.L. Xu,
"Lifetime measurements and calculations in La I",
Eur. Phys. J. D 30, 157-162 (2004).
- E. Biémont and P. Quinet,
"A database of astrophysical interest covering the UV region",
J. Electr. Spectrosc. Rel. Phen. (in press, 2004).
3. Database
The different tables are accessible directly
by clicking on the ion considered in the following list.
Lanthanum (Z = 57)........
La III
Cerium (Z = 58)...............
Ce II,
Ce III
Praseodymium (Z = 59)...
Pr II,
Pr III
Neodymium (Z = 60).......
Nd II,
Nd III
Promethium (Z = 61).......
Samarium (Z = 62)..........
Sm II,
Sm III
Europium (Z = 63)...........
Eu III
Gadolinium (Z = 64)........
Gd III
Terbium (Z = 65).............
Tb III
Dysprosium (Z = 66)........
Dy III
Holmium (Z = 67)............
Ho III
Erbium (Z = 68)...............
Er II,
Er III
Thulium (Z = 69).............
Tm II,
Tm III
Lutetium (Z = 71)...........
Lu I,
Lu II,
Lu III
Thorium (Z = 90)............
Th III
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