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Fe J/A+A/365/266 XXIII fine structure level oscillator strengths (Tully+, 2001) ================================================================================ Oscillator strengths between fine structure levels of Fe XXIII. Tully J.A., Chidichimo M.C. <Astron. Astrophys. 365, 266 (2001)> =2001A&A...365..266T ================================================================================ ADC_Keywords: Atomic physics Keywords: Atomic data Abstract: We tabulate theoretical line strengths, f-values and transition energies for the beryllium-like ion Fe XXIII. Transitions are between levels 2l_1_2l_2_S'L'J' and 2l_3_nl_4_SLJ with n = 2, 3, 4. The calculation uses the well known configuration interaction program CIV3 in which relativistic effects are allowed for by means of the Breit-Pauli approximation. We give a detailed comparison of our oscillator strengths with those which Chen & Ong (1998, Phys. Rev. A, 58, 1070) obtained using the relativistic Dirac code GRASP2. File Summary: -------------------------------------------------------------------------------FileName Lrecl Records Explanations -------------------------------------------------------------------------------ReadMe 80 . This file table1.dat 23 26 Fe XXIII radial orbital parameters table2.dat 78 44 Odd parity single configuration states table3.dat 91 49 Even parity single configuration states table4.dat 84 15 Fe XXIII line strengths and f-values for 2s2s ^1^S_0_ -> 2l_3_nl_4_, n = 2, 3, 4 table5.dat 82 14 Fe XXIII line strengths and f-values for 2s2p ^3^P^o^_0_ -> 2l_3_nl_4_, n = 2, 3, 4 table6.dat 82 37 Fe XXIII line strengths and f-values for 2s2p ^3^P^o^_1_ -> 2l_3_nl_4_, n = 2, 3, 4 table7.dat 83 37 Fe XXIII line strengths and f-values for 2s2p ^3^P^o^_2_ -> 2l_3_nl_4_, n = 2, 3, 4 table8.dat 82 37 Fe XXIII line strengths and f-values for 2s2p ^1^P^o^_1_ -> 2l_3_nl_4_, n = 2, 3, 4 table9.dat 82 14 Fe XXIII line strengths and f-values for 2p2p ^3^P_0_ -> 2l_3_nl_4_, n = 2, 3, 4 table10.dat 82 33 Fe XXIII line strengths and f-values for 2p2p ^3^P_1_ -> 2l_3_nl_4_, n = 2, 3, 4 table11.dat 82 35 Fe XXIII line strengths and f-values for 2p2p ^3^P_2_ -> 2l_3_nl_4_, n = 2, 3, 4 table12.dat 82 35 Fe XXIII line strengths and f-values for 2p2p ^1^D_2_ -> 2l_3_nl_4_, n = 2, 3, 4 table13.dat 82 14 Fe XXIII line strengths and f-values for 2p2p ^1^S_0_ -> 2l_3_nl_4_, n = 2, 3, 4 table14.dat 23 243 Present length oscillator strengths compared to those of Chen & Ong 1998 (Phys. Rev. A, 58, 1070) CO/TC {equiv} f(CO)/f(TC). table15.dat 45 46 Fe XXIII theoretical level energies relative to the ground state. table16.dat 84 16 Comparing present f-values with those of Cheng et al (1979), Nussbaumer & Storey (1979), Bhatia & Mason (1981), Safronova et al. (1992) and Zhang & Sampson (1992) table17.dat 59 22 Comparing present line strengths with those of Sampson et al. (1980ApJS...44..193S, 1984, Atomic Data & Nuclear Data Tables 30, 125) -------------------------------------------------------------------------------See also: J/A+AS/103/273 J/A+A/283/319 J/A+AS/108/1 J/A+A/293/953 J/A+A/293/967 J/A+AS/109/193 J/A+AS/119/509 J/A+AS/119/523 J/A+AS/120/361 J/A+AS/123/159 J/A+AS/123/575 J/A+AS/126/373 J/A+AS/131/499 J/A+AS/131/153 J/A+AS/135/347 J/A+AS/136/395 J/A+AS/137/165 J/A+AS/143/483 J/A+AS/144/141 J/A+AS/147/111 J/A+AS/147/253 J/A+A/365/268 : : : : : : : : : : : : : : : : : : : : : : IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON IRON Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project Project II III V VI VII VIII XVII XVIII XIX XXII XXIII XXVII XXIX XXXI XXXV XXXVII XXXVIII XLII XLIII XLIV XLV XLVII IR collision strengths of C-like ions B-like ions Collision strengths of O-like ions Fe II collision strengths Fe II radiative transitions Electron excitation of Ti-like ions Radiative transition in Fe III Electron impact for Fe III Fe II radiative transitions C and O radiative rates Fe XXII excitation rate coefficients Fe IV collision strengths Boron isoelectronic sequence Fe XII electron excitation Fe XXIV & Fe XXV oscillator strengths Fe VI collision strengths Fe XV fine-structure transitions Fe XXI electron impact excitation Fe V transition probabilities Fe VI trans. prob. & line ratio Ar XIII, Fe XXI trans. probabilities Ni III electron impact excitation Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 2 A2 --nl nl order (1) 4- 12 F9.6 --cjnl c_jnl_ coefficient (1) 14 I1 --Ijnl I_jnl_ coefficient (1) 16- 23 F8.5 --zetajnl {zeta}_jnl_ coefficient (1) -------------------------------------------------------------------------------Note The (1): atomic orbitals P_nl_(r) have the following analytic form P_nl_(r) = {sum, j=1 to k} c_jnl_* {(2{zeta}_jnl_)^I_jnl_+1/2_)/[(2I_jnl_)!]^1/2^}*r^I_jnl_^exp(-{zeta}_jnl_(r)) -------------------------------------------------------------------------------Byte-by-byte Description of file: table2.dat, table3.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 2 I2 --No Sequential number 4- 16 A13 ---J=0 J=0 configuration 19- 31 A13 ---J=1 J=1 configuration 34- 46 A13 ---J=2 J=2 configuration 49- 61 A13 ---J=3 J=3 configuration 64- 76 A13 ---J=4 J=4 configuration 79- 91 A13 --J=5 J=5 configuration -------------------------------------------------------------------------------Byte-by-byte Description of file: table4.dat, table5.dat, table6.dat, table7.dat Byte-by-byte Description of file: table8.dat, table9.dat, table10.dat Byte-by-byte Description of file: table11.dat, table12.dat, table13.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 9 E9.3 --Sl Length line strength (in atomic units) 11- 18 E8.3 --Sv Velocity line strength (in atomic units) 20- 28 E9.3 --fl length oscillator strength 30- 37 E8.3 --fv Velocity absorption oscillator strength 39- 49 F11.7 Ry Eij Calculated transition energy 52- 82 A31 --Trans Transition -------------------------------------------------------------------------------Byte-by-byte Description of file: table14.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 2 I2 --i Initial level 3 A1 ----[-] 4- 5 I2 --j Final level 8 A1 --n_Per Note on Per (1) 9- 10 I2 % Per Percentage difference between f(CO1998) and f(this paper) 12- 17 F6.4 --f(CO)/f(TC) Length oscillator strength ratio (2) -------------------------------------------------------------------------------Note (1): A negative percentage difference means that f(CO) < f(TC) Note (2): Chen & Ong (1998, Phys. Rev. A, 58, 1070) to this paper value ratio -------------------------------------------------------------------------------Byte-by-byte Description of file: table15.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 2 I2 --i Initial level (1) 4- 11 F8.5 Ry E2000 Present energy level (2000) obtained from a 78 state calculation (2) 13- 20 F8.5 Ry E1999 Energy level of Chidichimo et al. (1999A&AS..137..175C) (2) 22- 29 F8.5 Ry E1998 Energy level of Chen & Ong (1998, Phys. Rev. A, 58, 1070) (2) 31- 45 A15 --Trans Transition -------------------------------------------------------------------------------Note (1): Levels with indexes 13 and 14 are almost degenerate in energy Note (2): The energy unit is Ry = 109737.32 cm^-1^ -------------------------------------------------------------------------------Byte-by-byte Description of file: table16.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 8 E8.3 --Present Present f-value 10- 17 E8.3 --Cheng f-value of Cheng et al. (1979, At. Data Nucl. Data Tables, 24, 111) 19- 26 E8.3 --Nussba f-value of Nussbaumer & Storey (1979, J. Phys. B, 12, 1647) 28- 35 E8.3 --Bhatia f-value of Bhatia & Mason (1981A&A...103..324B) 36- 43 E8.3 --Safron f-value of Safronova et al. (1992, Phys. Scr, 46, 409) ? f-value of Zhang & Sampson (1992, At. Data Nucl. Data Tables, 52, 143) 52- 84 A33 --Trans Transition -------------------------------------------------------------------------------Byte-by-byte Description of file: table17.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 8 E8.3 --Present Present line strength 10- 17 E8.3 --1980 ? Sampson et al. (1980ApJS...44..193S) line strength 19- 26 E8.3 --1984 ? Sampson et al. (1984, Atomic Data and Nuclear Data Tables 30, 125) line strength 29- 58 A30 --Trans Transition -------------------------------------------------------------------------------History: From electronic version of the journal ================================================================================ (End) Patricia Bauer [CDS] 07-May-2001 44- 51 E8.3 --- Zhang
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J/ApJ/455/60 CFRS II: 0000-00 and 1000+25 fields (Le Fevre+ 1995) = The Canada-France Redshift Survey: II. Spectroscopic program : data for the 0000-00 and 1000+25 fields Le Fevre O., Crampton D., Lilly S.J., Hammer F., Tresse L. <Astrophys. J. 455, ...
Maryland >> HIST >> 461 (Fall, 2008)
J/ApJS/126/461 Equivalent Widths in the Spectrum of Sirius (Zhao+, 2000) = Equivalent Widths in the Spectrum of Sirius Zhao G., Qiu H.M., Chen Y.Q., Li Z.W. <Astrophys. J. Suppl. 126, 461 (2000)> =2000ApJS.126.461Z = ADC_Keywords: Atlases ; Line Prof...
Maryland >> HIST >> 462 (Fall, 2008)
A Conceptual Framework for Text Filtering Douglas W. Oard Medical Informatics and Computational Intelligence Laboratory Electrical Engineering Department and Gary Marchionini Human-Computer Interaction Laboratory Center for Automation Research and Di...
Maryland >> HIST >> 471 (Fall, 2008)
J/ApJ/471/L5 Redshift clustering in the Hubble Deep Field (Cohen+ 1996) = Redshift clustering in the Hubble Deep Field. Cohen J.G., Cowie L.L., Hogg D.W., Songaila A., Blandford R., Hu E.M., Shopbell P. <Astrophys. J. 471, L5 (1996)> =1996ApJ.471L.5C...
Maryland >> HIST >> 473 (Fall, 2008)
J/ApJ/473/822 APS Catalog of Galaxies behind Virgo (Hoffman+ 1996) = A Minnesota automated plate scanner catalog of galaxies behind the Virgo cluster and toward its antipode Hoffman G.L., Dickey J.M., Lu N.Y., Fromhold-Treu R. <Astrophys. J. 473, 822...
Maryland >> HIST >> 475 (Fall, 2008)
J/ApJS/129/475 The CNOC2 survey. I. (Yee+, 2000) = The CNOC2 field galaxy redshift survey. I. The survey and the catalog for the patch CNOC 0223+00. Yee H.K.C., Morris S.L., Lin H., Carlberg R.G., Hall P.B., Sawicki M., Patton D.R., Wirth G.D., Ellin...
Maryland >> HIST >> 475 (Fall, 2008)
J/ApJ/475/445 VIK photometry of faint field galaxies (Moustakas+ 1997) = Colors and K-band counts of extremely faint field galaxies. Moustakas L.A., Davis M., Graham J.R., Silk J., Peterson B.A., Yoshii Y. <Astrophys. J. 475, 445 (1997)> =1997ApJ.475...
Maryland >> HIST >> 475 (Fall, 2008)
J/A+AS/101/475 Spectroscopic observations of A3571 (Quintana+, 1993) = Spectroscopic observations of the galaxy cluster A 3571 (SC 1344-325) Quintana H., De Souza R. <Astron. Astrophys. Suppl. Ser. 101, 475 (1993)> =1993A&AS.101.475Q (SIMBAD/NED BibC...
Maryland >> HIST >> 480 (Fall, 2008)
Elastic Windows: A Hierarchical Multi-Window World-Wide Web Browser Eser Kandogan and Ben Shneiderman* Department of Computer Science, Human-Computer Interaction Laboratory Institute for Advanced Computer Studies University of Maryland, College Park,...
Maryland >> HIST >> 481 (Fall, 2008)
Homegrown House Members: A Vanishing Breed? Matthew Alejandro Castillo Summer Research Initiative 2006 University of Maryland at College Park Research Question Why are some congressional districts more hospitable to candidates born outside the state ...
Maryland >> HIST >> 482 (Fall, 2008)
Viewing personal history records: A comparison of Tabular format and graphical presentation using LifeLines Diane Lindwarm Alonso2, Anne Rose1, Catherine Plaisant1, Kent L. Norman2 1Human-Computer Interaction Laboratory University of Maryland Instit...
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