J/A+A/605/A89 Abundances of microlensed Bulge dwarf stars. VI. (Bensby+, 2017)
Chemical evolution of the Galactic bulge as traced by microlensed dwarfs and
subgiant stars.
VI. Age and abundance structure of the stellar populations in the central
sub-kpc of the Milky Way.
Bensby T., Feltzing S., Gould A., Yee, J.C., Johnson J.A., Asplund M.,
Melendez J., Lucatello S., Howes L.M., McWilliam A., Udalski A.,
Szymanski M.K., Soszynski I., Poleski R., Wyrzykowski L., Ulaczyk K.,
Kozlowski S., Pietrukowicz P., Skowron J., Mroz P., Pawlak, M., Abe F.,
Asakura Y., Bhattacharya A., Bond I.A., Bennett D.P., Hirao Y.,
Nagakane M., Koshimoto N., Sumi T., Suzuki D., Tristram P.J.
<Astron. Astrophys. 605, A89 (2017)>
=2017A&A...605A..89B 2017A&A...605A..89B (SIMBAD/NED BibCode)
ADC_Keywords: Gravitational lensing ; Abundances ; Equivalent widths
Keywords: gravitational lensing: micro - Galaxy: bulge - Galaxy: formation -
Galaxy: evolution - stars: abundances
Abstract:
We perform a detailed elemental abundance analysis of dwarf stars in
the Galactic bulge, based on high-resolution spectra that were
obtained while the stars were optically magnified during gravitational
microlensing events. The analysis method is the same as for a large
sample of F and G dwarf stars in the Solar neighbourhood, enabling a
fully differential comparison between the Bulge and the local stellar
populations in the Galactic disc.
Description:
For each spectral line we give the lower excitation potential,
measured equivalent widths, and derived absolute abundances.
We also give median abundances for each star, normalised to the Sun,
and errors in the median abundances.
These tables contain data for all so far 91 microlensed dwarf stars,
and superseeds the tables in Bensby et al. (2009, Cat. J/A+A/499/737),
Bensby et al. (2010, Cat. J/A+A/512/A41), Bensby et al. (2011, Cat.
J/A+A/533/A134), and Bensby et al. (2013, Cat. J/A+A/549/A147).
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
tablea2.dat 561 91 Abundance ratios and uncertainties, stellar
parameters, radial velocities, stellar ages,
masses, photometry, and more
tablea1.dat 1038 494 Equivalent widths and absolute abundances for
individual lines
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See also:
J/A+A/499/737 : Microlensed dwarf & subgiant stars abundances (Bensby+, 2009)
J/A+A/512/A41 : Microlensed stars in the Bulge abundances (Bensby+, 2010)
J/A+A/533/A134 : Microlensed stars in the Bulge abundances (Bensby+, 2011)
J/A+A/549/A147 : Microlensed Bulge stars abundances (Bensby+, 2013)
Byte-by-byte Description of file: tablea2.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 I6 --- Num Internal numbering of star
11- 29 A19 --- Name Name of microlensing source star
31- 32 I2 h RAh Right ascension (J2000)
34- 35 I2 min RAm Right ascension (J2000)
37- 41 F5.2 s RAs Right ascension (J2000)
43 A1 --- DE- Declination sign (J2000)
44- 45 I2 deg DEd Declination (J2000)
47- 48 I2 arcmin DEm Declination (J2000)
50- 54 F5.2 arcsec DEs Declination (J2000)
56- 60 F5.2 deg GLON [] Galactic longitude
62- 66 F5.2 deg GLAT Galactic latitude
68- 71 I4 d Tevent ? Duration of microlensing event
73- 79 F7.2 d Tmax Time of maximum magnification (HJD)
81- 84 I4 --- Amax ? Maximum magnification
86- 93 F8.3 d Tobs Time when observed (MJD)
95- 99 I5 s ExpTime Exposure time
103-105 I3 --- snr S/N per pixel at 640 nm
107-113 A7 --- Spec Spectrograph that was used
115-119 I5 --- R Spectral resolving power
122-125 I4 K Teff Effective temperature
128-131 I4 K e_Teff Effective temperature uncertainty
134-137 F4.2 [cm/s2] logg Surface gravity
140-143 F4.2 [cm/s2] e_logg Surface gravity uncertainty
146-149 F4.2 km/s xit Microturbulence parameter
152-155 F4.2 km/s e_xit Microturbulence uncertainty
157-161 F5.2 [Sun] [Fe/H] Iron abundance normalised to Sun
164-167 F4.2 [Sun] e_[Fe/H] Iron abundance uncertainty
171-173 I3 --- o_FeI Number of Fe I lines
178-179 I2 --- o_FeII ? Number of Fe II lines
182-185 F4.2 [Sun] s_FeI Fe I line-to-line scatter
188-191 F4.2 [Sun] s_FeII ? Fe II line-to-line scatter
193-199 F7.1 km/s HRV Heliocentric radial velocity
201-207 F7.1 km/s vGC Galactocentric radial velocity
210-213 F4.2 Sun M Stellar mass
216-219 F4.2 Sun b_M ? Lower limit on stellar mass
222-225 F4.2 Sun B_M ? Upper limit on stellar mass
228-231 F4.1 Gyr Age Stellar age
234-237 F4.1 Gyr b_Age ? Lower limit on stellar age
240-243 F4.1 Gyr B_Age ? Upper limit on stellar age
245-249 F5.2 mag (V-I)0 (V-I)_0 colour from spectroscopy
251-255 F5.2 mag b_(V-I)0 Lower limit on (V-I)_0 colour
257-261 F5.2 mag B_(V-I)0 Upper limit on (V-I)_0 colour
263-267 F5.2 mag VMAG Absolute V magnitude from spectroscopy
269-273 F5.2 mag b_VMAG Lower limit on absolute V magnitude
275-279 F5.2 mag B_VMAG Upper limit on absolute V magnitude
281-285 F5.2 mag IMAGmu ? Absolute I magnitude from microlensing
287-291 F5.2 mag (V-I)0mu ? Colour from microlensing
294-297 I4 K Teffmu ? Effective temperature from microlensing
299-303 F5.2 [Sun] [Na/Fe] ? [Na/Fe] normalised abundance ratio
306-309 F4.2 [Sun] e_[Na/Fe] ? Error in abundance ratio
313-315 I3 --- o_Na ? Number of Na lines used
318-321 F4.2 [Sun] s_Na ? Line-to-line scatter from Na lines
323-327 F5.2 [Sun] [Mg/Fe] ? [Mg/Fe] normalised abundance ratio
330-333 F4.2 [Sun] s_[Mg/Fe] ? Error in abundance ratio
337-339 I3 --- o_Mg ? Number of Mg lines used
342-345 F4.2 [Sun] s_Mg ? Line-to-line scatter from Mg lines
347-351 F5.2 [Sun] [Al/Fe] ? [Al/Fe] normalised abundance ratio
354-357 F4.2 [Sun] e_[Al/Fe] ? Error in abundance ratio [Al/Fe]
361-363 I3 --- o_Al ? Number of Al lines used
366-369 F4.2 [Sun] s_Al ? Line-to-line scatter from Al lines
371-375 F5.2 [Sun] [Si/Fe] ? [Si/Fe] normalised abundance ratio
378-381 F4.2 [Sun] e_[Si/Fe] ? Error in abundance ratio [Si/Fe]
385-387 I3 --- o_Si ? Number of Si lines used
390-393 F4.2 [Sun] s_Si ? Line-to-line scatter from Si lines
395-399 F5.2 [Sun] [Ca/Fe] ? [Ca/Fe] normalised abundance ratio
402-405 F4.2 [Sun] e_[Ca/Fe] ? Error in abundance ratio [Ca/Fe]
409-411 I3 --- o_Ca ? Number of Ca lines used
414-417 F4.2 [Sun] s_Ca ? Line-to-line scatter from Ca lines
419-423 F5.2 [Sun] [Ti/Fe] ? [Ti/Fe] normalised abundance ratio
426-429 F4.2 [Sun] e_[Ti/Fe] ? Error in abundance ratio [Ti/Fe]
433-435 I3 --- o_Ti ? Number of Ti lines used
438-441 F4.2 [Sun] s_Ti ? Line-to-line scatter from Ti lines
443-447 F5.2 [Sun] [Cr/Fe] ? [Cr/Fe] normalised abundance ratio
450-453 F4.2 [Sun] e_[Cr/Fe] ? Error in abundance ratio [Cr/Fe]
457-459 I3 --- o_Cr ? Number of Cr lines used
462-465 F4.2 [Sun] s_Cr ? Line-to-line scatter from Cr lines
467-471 F5.2 [Sun] [Ni/Fe] ? [Ni/Fe] normalised abundance ratio
474-477 F4.2 [Sun] e_[Ni/Fe] ? Error in abundance ratio [Ni/Fe]
481-483 I3 --- o_Ni ? Number of Ni lines used
486-489 F4.2 [Sun] s_Ni ? Line-to-line scatter from Ni lines
491-495 F5.2 [Sun] [Zn/Fe] ? [Zn/Fe] normalised abundance ratio
498-501 F4.2 [Sun] e_[Zn/Fe] ? Error in abundance ratio [Zn/Fe]
505-507 I3 --- o_Zn ? Number of Zn lines used
510-513 F4.2 [Sun] s_Zn ? Line-to-line scatter from Zn lines
515-519 F5.2 [Sun] [Y/Fe] ? [Y/Fe] normalised abundance ratio
522-525 F4.2 [Sun] e_[Y/Fe] ? Error in abundance ratio [Y/Fe]
529-531 I3 --- o_Y ? Number of Y lines used
534-537 F4.2 [Sun] s_Y ? Line-to-line scatter from Y lines
539-543 F5.2 [Sun] [Ba/Fe] ? [Ba/Fe] normalised abundance ratio
546-549 F4.2 [Sun] e_[Ba/Fe] ? Error in abundance ratio [Ba/Fe]
553-555 I3 --- o_Ba ? Number of Ba lines used
558-561 F4.2 [Sun] s_Ba ? Line-to-line scatter from Ba lines
--------------------------------------------------------------------------------
Byte-by-byte Description of file: tablea1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- Element Element
4 I1 --- Ion Ionisation (1=neutral)
6- 13 F8.3 0.1nm Lambda Wavelength
15- 19 F5.3 eV LEP Lower excitation potential
21- 26 F6.3 --- loggf Oscillator strength
28- 32 F5.1 0.1pm EWSun ? Equivalent width for Sun
34- 37 F4.2 [-] ASun ? Sun absolute abundance
(log scale, A(H)=12)
39- 43 F5.1 0.1pm EW1 ? Equivalent width for MOA-2009-BLG-174
45- 48 F4.2 --- A1 ? Absolute abundance MOA-2009-BLG-174
50- 54 F5.1 0.1pm EW2 ? Equivalent width for MOA-2009-BLG-259
56- 59 F4.2 --- A2 ? Absolute abundance MOA-2009-BLG-259
61- 65 F5.1 0.1pm EW3 ? Equivalent width for MOA-2010-BLG-167
67- 70 F4.2 --- A3 ? Absolute abundance MOA-2010-BLG-167
72- 76 F5.1 0.1pm EW4 ? Equivalent width for MOA-2010-BLG-311
78- 81 F4.2 --- A4 ? Absolute abundance MOA-2010-BLG-311
83- 87 F5.1 0.1pm EW5 ? Equivalent width for MOA-2010-BLG-446
89- 92 F4.2 --- A5 ? Absolute abundance MOA-2010-BLG-446
94- 98 F5.1 0.1pm EW6 ? Equivalent width for MOA-2010-BLG-523
100- 103 F4.2 --- A6 ? Absolute abundance MOA-2010-BLG-523
105- 109 F5.1 0.1pm EW7 ? Equivalent width for OGLE-2011-BLG-0950
111- 114 F4.2 --- A7 ? Absolute abundance OGLE-2011-BLG-0950
116- 120 F5.1 0.1pm EW8 ? Equivalent width for OGLE-2011-BLG-0969
122- 125 F4.2 --- A8 ? Absolute abundance OGLE-2011-BLG-0969
127- 131 F5.1 0.1pm EW9 ? Equivalent width for MOA-2011-BLG-034
133- 136 F4.2 --- A9 ? Absolute abundance MOA-2011-BLG-034
138- 142 F5.1 0.1pm EW10 ? Equivalent width for MOA-2011-BLG-058
144- 147 F4.2 --- A10 ? Absolute abundance MOA-2011-BLG-058
149- 153 F5.1 0.1pm EW11 ? Equivalent width for OGLE-2011-BLG-1072
155- 158 F4.2 --- A11 ? Absolute abundance OGLE-2011-BLG-1072
160- 164 F5.1 0.1pm EW12 ? Equivalent width for MOA-2011-BLG-090
166- 169 F4.2 --- A12 ? Absolute abundance MOA-2011-BLG-090
171- 175 F5.1 0.1pm EW13 ? Equivalent width for MOA-2011-BLG-104
177- 180 F4.2 --- A13 ? Absolute abundance MOA-2011-BLG-104
182- 186 F5.1 0.1pm EW14 ? Equivalent width for OGLE-2011-BLG-1105
188- 191 F4.2 --- A14 ? Absolute abundance OGLE-2011-BLG-1105
193- 197 F5.1 0.1pm EW15 ? Equivalent width for MOA-2011-BLG-174
199- 202 F4.2 --- A15 ? Absolute abundance MOA-2011-BLG-174
204- 208 F5.1 0.1pm EW16 ? Equivalent width for MOA-2011-BLG-191
210- 213 F4.2 --- A16 ? Absolute abundance MOA-2011-BLG-191
215- 219 F5.1 0.1pm EW17 ? Equivalent width for MOA-2011-BLG-234
221- 224 F4.2 --- A17 ? Absolute abundance MOA-2011-BLG-234
226- 230 F5.1 0.1pm EW18 ? Equivalent width for MOA-2011-BLG-278
232- 235 F4.2 --- A18 ? Absolute abundance MOA-2011-BLG-278
237- 241 F5.1 0.1pm EW19 ? Equivalent width for OGLE-2011-BLG-1410
243- 246 F4.2 --- A19 ? Absolute abundance OGLE-2011-BLG-1410
248- 252 F5.1 0.1pm EW20 ? Equivalent width for MOA-2011-BLG-445
254- 257 F4.2 --- A20 ? Absolute abundance MOA-2011-BLG-445
259- 263 F5.1 0.1pm EW21 ? Equivalent width for MOA-2012-BLG-022
265- 268 F4.2 --- A21 ? Absolute abundance MOA-2012-BLG-022
270- 274 F5.1 0.1pm EW22 ? Equivalent width for OGLE-2012-BLG-0026
276- 279 F4.2 --- A22 ? Absolute abundance OGLE-2012-BLG-0026
281- 285 F5.1 0.1pm EW23 ? Equivalent width for MOA-2012-BLG-187
287- 290 F4.2 --- A23 ? Absolute abundance MOA-2012-BLG-187
292- 296 F5.1 0.1pm EW24 ? Equivalent width for MOA-2012-BLG-202
298- 301 F4.2 --- A24 ? Absolute abundance MOA-2012-BLG-202
303- 307 F5.1 0.1pm EW25 ? Equivalent width for OGLE-2012-BLG-0211
309- 312 F4.2 --- A25 ? Absolute abundance OGLE-2012-BLG-0211
314- 318 F5.1 0.1pm EW26 ? Equivalent width for OGLE-2012-BLG-0270
320- 323 F4.2 --- A26 ? Absolute abundance OGLE-2012-BLG-0270
325- 329 F5.1 0.1pm EW27 ? Equivalent width for MOA-2012-BLG-291
331- 334 F4.2 --- A27 ? Absolute abundance MOA-2012-BLG-291
336- 340 F5.1 0.1pm EW28 ? Equivalent width for MOA-2012-BLG-391
342- 345 F4.2 --- A28 ? Absolute abundance MOA-2012-BLG-391
347- 351 F5.1 0.1pm EW29 ? Equivalent width for MOA-2012-BLG-410
353- 356 F4.2 --- A29 ? Absolute abundance MOA-2012-BLG-410
358- 362 F5.1 0.1pm EW30 ? Equivalent width for OGLE-2012-BLG-0521
364- 367 F4.2 --- A30 ? Absolute abundance OGLE-2012-BLG-0521
369- 373 F5.1 0.1pm EW31 ? Equivalent width for MOA-2012-BLG-532
375- 378 F4.2 --- A31 ? Absolute abundance MOA-2012-BLG-532
380- 384 F5.1 0.1pm EW32 ? Equivalent width for OGLE-2012-BLG-0563
386- 389 F4.2 --- A32 ? Absolute abundance OGLE-2012-BLG-0563
391- 395 F5.1 0.1pm EW33 ? Equivalent width for OGLE-2012-BLG-0617
397- 400 F4.2 --- A33 ? Absolute abundance OGLE-2012-BLG-0617
402- 406 F5.1 0.1pm EW34 ? Equivalent width for OGLE-2012-BLG-0816
408- 411 F4.2 --- A34 ? Absolute abundance OGLE-2012-BLG-0816
413- 417 F5.1 0.1pm EW35 ? Equivalent width for OGLE-2012-BLG-1156
419- 422 F4.2 --- A35 ? Absolute abundance OGLE-2012-BLG-1156
424- 428 F5.1 0.1pm EW36 ? Equivalent width for OGLE-2012-BLG-1217
430- 433 F4.2 --- A36 ? Absolute abundance OGLE-2012-BLG-1217
435- 439 F5.1 0.1pm EW37 ? Equivalent width for OGLE-2012-BLG-1274
441- 444 F4.2 --- A37 ? Absolute abundance OGLE-2012-BLG-1274
446- 450 F5.1 0.1pm EW38 ? Equivalent width for OGLE-2012-BLG-1279
452- 455 F4.2 --- A38 ? Absolute abundance OGLE-2012-BLG-1279
457- 461 F5.1 0.1pm EW39 ? Equivalent width for OGLE-2012-BLG-1526
463- 466 F4.2 --- A39 ? Absolute abundance OGLE-2012-BLG-1526
468- 472 F5.1 0.1pm EW40 ? Equivalent width for OGLE-2012-BLG-1534
474- 477 F4.2 --- A40 ? Absolute abundance OGLE-2012-BLG-1534
479- 483 F5.1 0.1pm EW41 ? Equivalent width for MOA-2013-BLG-063
485- 488 F4.2 --- A41 ? Absolute abundance for MOA-2013-BLG-063
490- 494 F5.1 0.1pm EW42 ? Equivalent width for MOA-2013-BLG-068
496- 499 F4.2 --- A42 ? Absolute abundance for MOA-2013-BLG-068
501- 505 F5.1 0.1pm EW43 ? Equivalent width for MOA-2013-BLG-299
507- 510 F4.2 --- A43 ? Absolute abundance for MOA-2013-BLG-299
512- 516 F5.1 0.1pm EW44 ? Equivalent width for MOA-2013-BLG-402
518- 521 F4.2 --- A44 ? Absolute abundance for MOA-2013-BLG-402
523- 527 F5.1 0.1pm EW45 ? Equivalent width for OGLE-2013-BLG-0446
529- 532 F4.2 --- A45 ? Absolute abundance for OGLE-2013-BLG-0446
534- 538 F5.1 0.1pm EW46 ? Equivalent width for MOA-2013-BLG-517
540- 543 F4.2 --- A46 ? Absolute abundance for MOA-2013-BLG-517
545- 549 F5.1 0.1pm EW47 ? Equivalent width for MOA-2013-BLG-524
551- 554 F4.2 --- A47 ? Absolute abundance for MOA-2013-BLG-524
556- 560 F5.1 0.1pm EW48 ? Equivalent width for MOA-2013-BLG-605
562- 565 F4.2 --- A48 ? Absolute abundance for MOA-2013-BLG-605
567- 571 F5.1 0.1pm EW49 ? Equivalent width for OGLE-2013-BLG-0692
573- 576 F4.2 --- A49 ? Absolute abundance for OGLE-2013-BLG-0692
578- 582 F5.1 0.1pm EW50 ? Equivalent width for OGLE-2013-BLG-0835
584- 587 F4.2 --- A50 ? Absolute abundance for OGLE-2013-BLG-0835
589- 593 F5.1 0.1pm EW51 ? Equivalent width for OGLE-2013-BLG-0911
595- 598 F4.2 --- A51 ? Absolute abundance for OGLE-2013-BLG-0911
600- 604 F5.1 0.1pm EW52 ? Equivalent width for OGLE-2013-BLG-1015
606- 609 F4.2 --- A52 ? Absolute abundance for OGLE-2013-BLG-1015
611- 615 F5.1 0.1pm EW53 ? Equivalent width for OGLE-2013-BLG-1114
617- 620 F4.2 --- A53 ? Absolute abundance for OGLE-2013-BLG-1114
622- 626 F5.1 0.1pm EW54 ? Equivalent width for OGLE-2013-BLG-1125
628- 631 F4.2 --- A54 ? Absolute abundance for OGLE-2013-BLG-1125
633- 637 F5.1 0.1pm EW55 ? Equivalent width for OGLE-2013-BLG-1147
639- 642 F4.2 --- A55 ? Absolute abundance for OGLE-2013-BLG-1147
644- 648 F5.1 0.1pm EW56 ? Equivalent width for OGLE-2013-BLG-1259
650- 653 F4.2 --- A56 ? Absolute abundance for OGLE-2013-BLG-1259
655- 659 F5.1 0.1pm EW57 ? Equivalent width for OGLE-2013-BLG-1768
661- 664 F4.2 --- A57 ? Absolute abundance for OGLE-2013-BLG-1768
666- 670 F5.1 0.1pm EW58 ? Equivalent width for OGLE-2013-BLG-1793
672- 675 F4.2 --- A58 ? Absolute abundance for OGLE-2013-BLG-1793
677- 681 F5.1 0.1pm EW59 ? Equivalent width for OGLE-2013-BLG-1868
683- 686 F4.2 --- A59 ? Absolute abundance for OGLE-2013-BLG-1868
688- 692 F5.1 0.1pm EW60 ? Equivalent width for OGLE-2013-BLG-1938
694- 697 F4.2 --- A60 ? Absolute abundance for OGLE-2013-BLG-1938
699- 703 F5.1 0.1pm EW61 ? Equivalent width for MOA-2014-BLG-131
705- 708 F4.2 --- A61 ? Absolute abundance for MOA-2014-BLG-131
710- 714 F5.1 0.1pm EW62 ? Equivalent width for OGLE-2014-BLG-0157
716- 719 F4.2 --- A62 ? Absolute abundance for OGLE-2014-BLG-0157
721- 725 F5.1 0.1pm EW63 ? Equivalent width for OGLE-2014-BLG-0801
727- 730 F4.2 --- A63 ? Absolute abundance for OGLE-2014-BLG-0801
732- 736 F5.1 0.1pm EW64 ? Equivalent width for OGLE-2014-BLG-0953
738- 741 F4.2 --- A64 ? Absolute abundance for OGLE-2014-BLG-0953
743- 747 F5.1 0.1pm EW65 ? Equivalent width for OGLE-2014-BLG-0987
749- 752 F4.2 --- A65 ? Absolute abundance for OGLE-2014-BLG-0987
754- 758 F5.1 0.1pm EW66 ? Equivalent width for OGLE-2014-BLG-1122
760- 763 F4.2 --- A66 ? Absolute abundance for OGLE-2014-BLG-1122
765- 769 F5.1 0.1pm EW67 ? Equivalent width for OGLE-2014-BLG-1370
771- 774 F4.2 --- A67 ? Absolute abundance for OGLE-2014-BLG-1370
776- 780 F5.1 0.1pm EW68 ? Equivalent width for OGLE-2014-BLG-1418
782- 785 F4.2 --- A68 ? Absolute abundance for OGLE-2014-BLG-1418
787- 791 F5.1 0.1pm EW69 ? Equivalent width for OGLE-2014-BLG-1469
793- 796 F4.2 --- A69 ? Absolute abundance for OGLE-2014-BLG-1469
798- 802 F5.1 0.1pm EW70 ? Equivalent width for OGLE-2014-BLG-2040
804- 807 F4.2 --- A70 ? Absolute abundance for OGLE-2014-BLG-2040
809- 813 F5.1 0.1pm EW71 ? Equivalent width for OGLE-2015-BLG-0078
815- 818 F4.2 --- A71 ? Absolute abundance for OGLE-2015-BLG-0078
820- 824 F5.1 0.1pm EW72 ? Equivalent width for MOA-2015-BLG-111
826- 829 F4.2 --- A72 ? Absolute abundance for MOA-2015-BLG-111
831- 835 F5.1 0.1pm EW73 ? Equivalent width for OGLE-2015-BLG-0159
837- 840 F4.2 --- A73 ? Absolute abundance for OGLE-2015-BLG-0159
842- 846 F5.1 0.1pm EW74 ? Equivalent width for MOA-2010-BLG-037
848- 851 F4.2 --- A74 ? Absolute abundance MOA-2010-BLG-037
853- 857 F5.1 0.1pm EW75 ? Equivalent width for MOA-2010-BLG-049
859- 862 F4.2 --- A75 ? Absolute abundance MOA-2010-BLG-049
864- 868 F5.1 0.1pm EW76 ? Equivalent width for OGLE-2009-BLG-076
870- 873 F4.2 --- A76 ? Absolute abundance OGLE-2009-BLG-076
875- 879 F5.1 0.1pm EW77 ? Equivalent width for MOA-2010-BLG-078
881- 884 F4.2 --- A77 ? Absolute abundance MOA-2010-BLG-078
886- 890 F5.1 0.1pm EW78 ? Equivalent width for MOA-2006-BLG-099
892- 895 F4.2 --- A78 ? Absolute abundance MOA-2006-BLG-099
897- 901 F5.1 0.1pm EW79 ? Equivalent width for MOA-2009-BLG-133
903- 906 F4.2 --- A79 ? Absolute abundance MOA-2009-BLG-133
908- 912 F5.1 0.1pm EW80 ? Equivalent width for OGLE-2008-BLG-209
914- 917 F4.2 --- A80 ? Absolute abundance OGLE-2008-BLG-209
919- 923 F5.1 0.1pm EW81 ? Equivalent width for OGLE-2006-BLG-265
925- 928 F4.2 --- A81 ? Absolute abundance OGLE-2006-BLG-265
930- 934 F5.1 0.1pm EW82 ? Equivalent width for MOA-2010-BLG-285
936- 939 F4.2 --- A82 ? Absolute abundance MOA-2010-BLG-285
941- 945 F5.1 0.1pm EW83 ? Equivalent width for MOA-2008-BLG-310
947- 950 F4.2 --- A83 ? Absolute abundance MOA-2008-BLG-310
952- 956 F5.1 0.1pm EW84 ? Equivalent width for MOA-2008-BLG-311
958- 961 F4.2 --- A84 ? Absolute abundance MOA-2008-BLG-311
963- 967 F5.1 0.1pm EW85 ? Equivalent width for OGLE-2007-BLG-349
969- 972 F4.2 --- A85 ? Absolute abundance OGLE-2007-BLG-349
974- 978 F5.1 0.1pm EW86 ? Equivalent width for MOA-2009-BLG-456
980- 983 F4.2 --- A86 ? Absolute abundance MOA-2009-BLG-456
985- 989 F5.1 0.1pm EW87 ? Equivalent width for MOA-2009-BLG-475
991- 994 F4.2 --- A87 ? Absolute abundance MOA-2009-BLG-475
996- 1000 F5.1 0.1pm EW88 ? Equivalent width for MOA-2009-BLG-489
1002 -1005 F4.2 --- A88 ? Absolute abundance MOA-2009-BLG-489
1007 -1011 F5.1 0.1pm EW89 ? Equivalent width for MOA-2009-BLG-493
1013 -1016 F4.2 --- A89 ? Absolute abundance MOA-2009-BLG-493
1018 -1022 F5.1 0.1pm EW90 ? Equivalent width for OGLE-2007-BLG-514
1024 -1027 F4.2 --- A90 ? Absolute abundance OGLE-2007-BLG-514
1029 -1033 F5.1 0.1pm EW91 ? Equivalent width for MACH-1999-BLG-022
1035 -1038 F4.2 --- A91 ? Absolute abundance MACH-1999-BLG-022
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Acknowledgements:
Thomas Bensby, tbensby(at)astro.lu.se
References:
Bensby et al., Paper I 2009A&A...499..737B 2009A&A...499..737B, Cat. J/A+A/499/737
Bensby et al., Paper II 2010A&A...512A..41B 2010A&A...512A..41B, Cat. J/A+A/512/A41
Bensby et al., Paper III 2010A&A...521L..57B 2010A&A...521L..57B
Bensby et al., Paper IV 2011A&A...533A.134B 2011A&A...533A.134B, Cat. J/A+A/533/A134
Bensby et al., Paper V 2013A&A...549A.147B 2013A&A...549A.147B, Cat. J/A+A/549/A147
(End) Thomas Bensby [Lund Obs., Sweden], Patricia Vannier [CDS] 17-Jul-2017