J/ApJS/230/28 The populations of Carina. II. Abundances (Norris+, 2017)
The populations of Carina.
II. Chemical enrichment.
Norris J.E., Yong D., Venn K.A., Gilmore G., Casagrande L., Dotter A.
<Astrophys. J. Suppl. Ser., 230, 28-28 (2017)>
=2017ApJS..230...28N 2017ApJS..230...28N (SIMBAD/NED BibCode)
ADC_Keywords: Abundances ; Stars, giant ; Equivalent widths ; Radial velocities
Photometry, UBVRI ; Photometry, infrared ; Cross identifications
Keywords: galaxies: abundances; galaxies: dwarf;
galaxies: individual: Carina; stars: abundances
Abstract:
Chemical abundances are presented for 19 elements in a sample of 63
red giants in the Carina dwarf spheroidal galaxy (dSph), based on
homogeneous 1D/LTE model atmosphere analyses of our own observations
(32 stars) and data available in the literature (a further 31
independent stars). The (Fe) metallicity and [α/Fe] distribution
functions have mean values and dispersions of -1.59 and 0.33dex
([Fe/H] range: -2.68 to -0.64) and 0.07 and 0.13dex ([α/Fe]
range: -0.27 to 0.25), respectively. We confirm the finding of Venn+
(2012, J/ApJ/751/102) that a small percentage (some 10% in the present
investigation) of the sample shows clear evidence for significant
enrichment by Type Ia supernova (SN Ia) ejecta. Calcium, with the most
accurately determined abundance of the α-elements, shows an
asymmetric distribution toward smaller values of [Ca/Fe] at all
[Fe/H], most significantly over -2.0<[Fe/H]←1.0, suggestive of
incomplete mixing of the ejecta of SNe Ia with the ambient medium of
each of Carina's generations. Approximate color-magnitude diagram age
estimates are presented for the sample, and together with our chemical
abundances, compared with the results of our previous synthetic
color-magnitude diagram analysis, which reported the details of
Carina's four well-defined populations. We searched for the Na-O
anticorrelation universally reported in the Galaxy's globular clusters
and confirm that this phenomenon does not exist in Carina. We also
found that one of the 32 stars in our sample has an extremely enhanced
lithium abundance-A(Li)NLTE=+3.36, consistent with membership of the
∼1% group of Li-rich stars in dSph described by
Kirby+ (2012ApJ...752L..16K 2012ApJ...752L..16K).
Description:
Our selection of objects is based on unpublished CCD V, I observations
that we have made of the Carina galaxy.
High-resolution, moderate-S/N spectra were obtained of 39 Carina red
giants, during 2007 November-2008 March, with the FLAMES system at the
8.2m Kueyen (VLT/UT2) telescope at Cerro Paranal. The spectra cover
the wavelength ranges 4800-5750Å and 5840-6800Å. The resolving
power was R=47000.
Photometry has been obtained from several sources: P. B. Stetson
provided us with homogenized BVI, M. J. Irwin furnished JHK from ESO
VISTA survey photometry, and M. Gullieuszik supplied BVIJHKs.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 78 32 Coordinates, photometry, and radial velocities
for 32 Carina red giants
ews.dat 46 6752 Atomic data and equivalent widths (mÅ)
for 32 Carina red giants (tables 2, 3 and 4)
table5.dat 31 32 Model atmosphere parameters for 32 Carina red giants
table6.dat 47 672 Chemical abundances for 32 Carina red giants
table8.dat 288 32 Summary of [Fe/H], [X/Fe], and total errors
for 32 Carina red giants
table9.dat 94 49 Coordinates, photometry, and atmospheric parameters
for 49 Carina red giants from the literature
table10.dat 282 14 Summary of [Fe/H], [X/Fe], and total errors
for 14 literature (Venn+ (2012, J/ApJ/751/102) &
Shetrone+ (2003AJ....125..684S 2003AJ....125..684S)) Carina red giants
table11.dat 139 35 Summary of [Fe/H], [X/Fe], and total errors
for 35 Lemasle+ (2012, J/A+A/538/A100)
Carina red giants
table12.dat 83 30 alpha/Fe values and errors for 30 Carina red giants
table13.dat 34 63 Fraction of Type Ia material, <d[Xi/Fe]>, and
[Ba/Fe] in the Carina red giants
table14.dat 52 63 Cross-identification and coordinates of program stars
table15.dat 222 63 Average [Fe/H], [X/Fe], and errors
for the 63 independent Carina red giants
--------------------------------------------------------------------------------
See also:
J/ApJS/99/637 : Equivalent widths for 54 red giants (Norris+ 1995)
J/A+AS/121/95 : Giant stars abundances in 24 clusters (Carretta+ 1997)
J/AJ/114/1458 : The Carina Dwarf (Mighell 1997)
J/AJ/115/1840 : BV photometry in Carina dwarf galaxy (Hurley-Keller+ 1998)
J/AJ/120/1841 : Abundances & Kinematics of Halo & Disk Stars (Fulbright 2000)
J/A+A/439/129 : HERES II. Spectroscopic analysis (Barklem+, 2005)
J/ApJ/626/446 : Effective temperature scale of FGK stars (Ramirez+, 2005)
J/MNRAS/373/13 : Lower main-sequence stars parameters (Casagrande+, 2006)
J/ApJ/649/201 : Velocities & Washington phot. in Carina dSph (Munoz+, 2006)
J/AJ/131/895 : Stars in the Carina dwarf spheroidal galaxy (Koch+, 2006)
J/MNRAS/383/183 : CaII triplet of RGB from VLT/FLAMES obs. (Battaglia+, 2008)
J/AJ/135/1580 : Element abundances in ten red giants of Car dSph (Koch+, 2008)
J/A+A/503/541 : Neutral Li in late-type stars (Lind+, 2009)
J/AJ/137/3100 : Radial velocities of 4 dSph galaxies (Walker+, 2009)
J/ApJ/711/350 : Metal-poor giant Boo-1137 abundances (Norris+, 2010)
J/ApJS/194/15 : CCCP: Carina's diffuse X-ray emission (Townsley+, 2011)
J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)
J/A+A/534/A136 : Halo red giants from the SEGUE survey (Martell+, 2011)
J/ApJ/733/46 : Velocity measurements in Segue 1 (Simon+, 2011)
J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)
J/PASP/124/519 : Iron abundances of red giants in Carina gal. (Fabrizio+, 2012)
J/A+A/538/A100 : Abundances red giants in Carina dSph (Lemasle+, 2012)
J/ApJ/757/164 : Oxygen abundances of dwarf stars (Ramirez+, 2012)
J/ApJ/751/102 : Equivalent widths of 9 RGB in Carina dSph (Venn+, 2012)
J/ApJ/763/61 : Abundances of 7 red giant members of BootesI (Gilmore+, 2013)
J/ApJ/778/149 : Abundances for 3 stars in Sgr dSph (McWilliam+, 2013)
J/ApJ/762/26 : Most metal-poor stars. II. Galactic halo stars (Yong+, 2013)
J/A+A/572/A10 : (BV) photometry in Carina dSph (de Boer+, 2014)
J/A+A/580/A18 : Carina Project VIII. α-element abund. (Fabrizio+, 2015)
J/ApJ/830/126 : The Carina project. X. Radial velocities (Fabrizio+, 2016)
J/ApJS/225/24 : NuGrid stellar data set I. Yields (Pignatari+, 2016)
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name
9- 10 I2 h RAh [06] Hour of Right Ascension (J2000)
12- 13 I2 min RAm [40/42] Minute of Right Ascension (J2000)
15- 19 F5.2 s RAs Second of Right Ascension (J2000)
21 A1 --- DE- [-] Sign of the Declination (J2000)
22- 23 I2 deg DEd [50/51] Degree of Declination (J2000)
25- 26 I2 arcmin DEm Arcminute of Declination (J2000)
28- 31 F4.1 arcsec DEs Arcsecond of Declination (J2000)
33- 37 F5.2 mag Vmag [17.6/18.7] V band magnitude,
Johnson-Kron-Cousins system (G1)
39- 42 F4.2 mag B-V B-V color index, Johnson-Kron-Cousins system (G1)
44- 48 F5.2 mag Imag [16.1/17.5] I band magnitude,
Johnson-Kron-Cousins system (G1)
50- 54 F5.2 mag Jmag [15/16.7] J band magnitude, 2MASS system (G2)
56- 60 F5.2 mag Hmag H band magnitude, 2MASS system (G2)
62- 66 F5.2 mag Ksmag Ks band magnitude, 2MASS system (G2)
68- 73 F6.2 km/s RVel [215/237] Derived Radial Velocity
75- 78 F4.2 km/s e_RVel [0.07/0.3] Uncertainty in RVel
--------------------------------------------------------------------------------
Byte-by-byte Description of file: ews.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name
9- 13 A5 --- Ion Atomic species
15- 21 F7.2 0.1nm lambda [5302.3/6774.3] Wavelength in Angstroms
23- 26 F4.2 eV ExPot [0/5.8] Excitation Potential
28- 33 F6.3 --- log(gf) [-9.8/0.7] Log of oscillator strength
35- 35 A1 --- l_EW Limit flag on EW
36- 40 F5.1 0.1pm EW [10.5/238]? Equivalent width of star at lambda
42- 43 I2 --- SNR [7/23]? SNR for the star (1)
45- 46 I2 0.1pm min [14/34]? Minimum EW for the star
--------------------------------------------------------------------------------
Note (1): S/N per ∼0.28Å pixel at 5300-5700Å.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name
9- 12 I4 K Teff [4230/4695] Derived surface effective temperature
14- 16 I3 K e_Teff Uncertainty in Teff
18- 21 F4.2 [cm/s2] logg [0.6/1.4] Derived surface gravity, cgs units
23- 26 F4.1 [Sun] [M/H] [-2.3/-1.2] Log metallicity,
eq. to iron abundance [Fe/H]
28- 31 F4.2 km/s Vturb [1.8/2.5] Microturbulent velocity
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name
10- 14 A5 --- Ion Atomic species
16- 16 A1 --- l_loge(X) Limit flag on loge(X)
17- 21 F5.2 [-] loge(X) [-1.4/8]? Mean absolute abundance (1)
23- 26 F4.2 [-] e_loge(X) ? Standard error of the mean, loge(X)
28- 29 I2 --- Nl [1/82]? Number of lines analyzed
31- 31 A1 --- l_[X/Fe] Limit flag on [X/Fe]
32- 37 F6.2 [Sun] [X/Fe] [-2.5/1.8]? Abundance relative to Fe (2)
39- 42 F4.2 [Sun] s_[X/Fe] ? Systematic error, [X/Fe]
44- 47 F4.2 [Sun] e_[X/Fe] ? Total error, [X/Fe]
--------------------------------------------------------------------------------
Note (1): loge(X)=log(NX/NH)+12.0
Note (2): Abundance relative to Fe except for Fe atomic species which are
relative to hydrogen, [Fe/H]
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table8.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name
10- 14 F5.2 [Sun] [Fe/H] [-2.5/-1.2]? [Fe/H] abundance
16- 16 A1 --- l_O Limit flag on O
17- 21 F5.2 [Sun] O [0.1/1.3]? [O/Fe] abundance
23- 23 A1 --- l_Na Limit flag on Na
24- 29 F6.2 [Sun] Na [-0.8/0.8]? [Na/Fe] abundance
31- 35 F5.2 [Sun] Mg [-0.5/0.9]? [Mg/Fe] abundance
37- 37 A1 --- l_Al Limit flag on Al
38- 42 F5.2 [Sun] Al [0.06/1.8]? [Al/Fe] abundance
44- 47 F4.2 [Sun] Si [0.06/0.9]? [Si/Fe] abundance
49- 53 F5.2 [Sun] Ca [-0.4/0.3]? [Ca/Fe] abundance
55- 59 F5.2 [Sun] Sc [-0.9/0.5]? [Sc/Fe] abundance
61- 65 F5.2 [Sun] TiI [-0.4/0.7]? [TiI/Fe] abundance
67- 71 F5.2 [Sun] TiII [-0.2/0.6]? [TiII/Fe] abundance
73- 77 F5.2 [Sun] V ? [V/Fe] abundance
79- 83 F5.2 [Sun] Cr [-0.5/0.2]? [Cr/Fe] abundance
85- 89 F5.2 [Sun] Mn [-0.9/0.5]? [Mn/Fe] abundance
91- 95 F5.2 [Sun] FeII [-0.01/0.7]? [FeII/Fe] abundance
97-101 F5.2 [Sun] Co ? [Co/Fe] abundance
103-107 F5.2 [Sun] Ni [-0.5/0.5]? [Ni/Fe] abundance
109-113 F5.2 [Sun] Cu ? [Cu/Fe] abundance
115-119 F5.2 [Sun] Ba [-1/0.6]? [Ba/Fe] abundance
121-124 F4.2 [Sun] La ? [La/Fe] abundance
126-130 F5.2 [Sun] Nd ? [Nd/Fe] abundance
132-135 F4.2 [Sun] Eu ? [Eu/Fe] abundance
137-140 F4.2 [Sun] e_[Fe/H] ? Total Error in [Fe/H]
142-145 F4.2 [Sun] e_O ? Total Error in [O/Fe]
147-150 F4.2 [Sun] e_Na ? Total Error in [Na/Fe]
152-155 F4.2 [Sun] e_Mg ? Total Error in [Mg/Fe]
157-160 F4.2 [Sun] e_Al ? Total Error in [Al/Fe]
162-165 F4.2 [Sun] e_Si ? Total Error in [Si/Fe]
167-170 F4.2 [Sun] e_Ca ? Total Error in [Ca/Fe]
172-175 F4.2 [Sun] e_Sc ? Total Error in [Sc/Fe]
177-180 F4.2 [Sun] e_TiI ? Total Error in [TiI/Fe]
182-185 F4.2 [Sun] e_TiII ? Total Error in [TiII/Fe]
187-190 F4.2 [Sun] e_V ? Total Error in [V/Fe]
192-195 F4.2 [Sun] e_Cr ? Total Error in [Cr/Fe]
197-200 F4.2 [Sun] e_Mn ? Total Error in [Mn/Fe]
202-205 F4.2 [Sun] e_FeII ? Total Error in [FeII/Fe]
207-210 F4.2 [Sun] e_Co ? Total Error in [Co/Fe]
212-215 F4.2 [Sun] e_Ni ? Total Error in [Ni/Fe]
217-220 F4.2 [Sun] e_Cu ? Total Error in [Cu/Fe]
222-225 F4.2 [Sun] e_Ba ? Total Error in [Ba/Fe]
227-230 F4.2 [Sun] e_La ? Total Error in [La/Fe]
232-235 F4.2 [Sun] e_Nd ? Total Error in [Nd/Fe]
237-240 F4.2 [Sun] e_Eu ? Total Error in [Eu/Fe]
242-243 I2 --- o_[Fe/H] ? Number of Fe lines observed
245-245 I1 --- o_O ? Number of O lines observed
247-247 I1 --- o_Na ? Number of Na lines observed
249-249 I1 --- o_Mg ? Number of Mg lines observed
251-251 I1 --- o_Al ? Number of Al lines observed
253-253 I1 --- o_Si ? Number of Si lines observed
255-256 I2 --- o_Ca ? Number of Ca lines observed
258-258 I1 --- o_Sc ? Number of Sc lines observed
260-260 I1 --- o_TiI ? Number of TiI lines observed
262-262 I1 --- o_TiII ? Number of TiII lines observed
264-265 I2 --- o_V ? Number of V lines observed
267-267 I1 --- o_Cr ? Number of Cr lines observed
269-269 I1 --- o_Mn ? Number of Mn lines observed
271-272 I2 --- o_FeII ? Number of FeII lines observed
274-274 I1 --- o_Co ? Number of Co lines observed
276-277 I2 --- o_Ni ? Number of Ni lines observed
279-279 I1 --- o_Cu ? Number of Cu lines observed
281-281 I1 --- o_Ba ? Number of Ba lines observed
283-283 I1 --- o_La ? Number of La lines observed
285-285 I1 --- o_Nd ? Number of Nd lines observed
287-288 I2 --- o_Eu ? Number of Eu lines observed
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table9.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 8 A8 --- ID Object name
10- 10 I1 --- Ref Literature sources (1)
12- 13 I2 h RAh [06] Hour of Right Ascension (J2000)
15- 16 I2 min RAm [40/42] Minute of Right Ascension (J2000)
18- 22 F5.2 s RAs Second of Right Ascension (J2000)
24- 24 A1 --- DE- [-] Sign of the Declination (J2000)
25- 26 I2 deg DEd [50/51] Degree of Declination (J2000)
28- 29 I2 arcmin DEm Arcminute of Declination (J2000)
31- 34 F4.1 arcsec DEs Arcsecond of Declination (J2000)
36- 40 F5.2 mag Vmag [17.6/19.3] V band magnitude,
Johnson- Kron-Cousins system (G1)
42- 45 F4.2 mag B-V B-V color index, Johnson- Kron-Cousins system (G1)
47- 51 F5.2 mag Imag [16/18.2] I band magnitude,
Johnson- Kron-Cousins system (G1)
53- 57 F5.2 mag Jmag [15/17.4] J band magnitude, 2MASS system (G2)
59- 63 F5.2 mag Hmag H band magnitude, 2MASS system (G2)
65- 69 F5.2 mag Kmag K band magnitude, 2MASS system (G2)
71- 74 I4 K Teff [4230/4832] Derived surface effective temperature
76- 78 I3 K e_Teff Uncertainty in Teff
80- 83 F4.2 [cm/s2] logg [0.6/1.7] Derived surface gravity, cgs units
85- 89 F5.2 [Sun] [M/H] [-2.8/-0.7] Log metallicity,
eq. to iron abundance [Fe/H]
91- 94 F4.2 km/s Vturb [1.7/2.7] Microturbulent velocity
--------------------------------------------------------------------------------
Note (1): Literature Sources as follows:
1 = Venn et al. (2012, J/ApJ/751/102; <[VSI2012] Car-NNNN> in Simbad)
2 = Shetrone et al. (2003AJ....125..684S 2003AJ....125..684S; <[MOP93] NN> in Simbad);
3 = Lemasle et al. (2012, J/A+A/538/A100; <[LHT2012] MKVNNNN> in Simbad)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table10.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 9 A9 --- ID Object name, Venn+ (2012, J/ApJ/751/102)
or Shetrone+ (2003AJ....125..684S 2003AJ....125..684S)
11- 15 F5.2 [Sun] [Fe/H] [-2.7/-1.3]? [Fe/H] abundance
17- 20 F4.2 [Sun] O [0.2/0.7]? [O/Fe] abundance
22- 26 F5.2 [Sun] Na [-0.5/0.01]? [Na/Fe] abundance
28- 32 F5.2 [Sun] Mg [-0.6/0.5]? [Mg/Fe] abundance
34- 38 F5.2 [Sun] Al [-0.02/0.2]? [Al/Fe] abundance
40- 43 F4.2 [Sun] Si [0.1/0.6]? [Si/Fe] abundance
45- 49 F5.2 [Sun] Ca [-0.5/0.2]? [Ca/Fe] abundance
51- 55 F5.2 [Sun] Sc [-0.5/0.3]? [Sc/Fe] abundance
57- 61 F5.2 [Sun] TiI [-0.4/0.4]? [TiI/Fe] abundance
63- 67 F5.2 [Sun] TiII [-0.2/0.6]? [TiII/Fe] abundance
69- 73 F5.2 [Sun] V ? [V/Fe] abundance
75- 79 F5.2 [Sun] Cr [-0.8/0.2]? [Cr/Fe] abundance
81- 85 F5.2 [Sun] Mn [-0.5/-0.1]? [Mn/Fe] abundance
87- 90 F4.2 [Sun] FeII [0.03/0.4]? [FeII/Fe] abundance
92- 96 F5.2 [Sun] Co ? [Co/Fe] abundance
98-102 F5.2 [Sun] Ni [-0.3/0.2]? [Ni/Fe] abundance
104-108 F5.2 [Sun] Cu ? [Cu/Fe] abundance
110-114 F5.2 [Sun] Ba [-1.1/0.5]? [Ba/Fe] abundance
116-119 F4.2 [Sun] La ? [La/Fe] abundance
121-125 F5.2 [Sun] Nd ? [Nd/Fe] abundance
127-130 F4.2 [Sun] Eu ? [Eu/Fe] abundance
132-135 F4.2 [Sun] e_[Fe/H] ? Total Error in [Fe/H]
137-140 F4.2 [Sun] e_O ? Total Error in [O/Fe]
142-145 F4.2 [Sun] e_Na ? Total Error in [Na/Fe]
147-150 F4.2 [Sun] e_Mg ? Total Error in [Mg/Fe]
152-155 F4.2 [Sun] e_Al ? Total Error in [Al/Fe]
157-160 F4.2 [Sun] e_Si ? Total Error in [Si/Fe]
162-165 F4.2 [Sun] e_Ca ? Total Error in [Ca/Fe]
167-170 F4.2 [Sun] e_Sc ? Total Error in [Sc/Fe]
172-175 F4.2 [Sun] e_TiI ? Total Error in [TiI/Fe]
177-180 F4.2 [Sun] e_TiII ? Total Error in [TiII/Fe]
182-185 F4.2 [Sun] e_V ? Total Error in [V/Fe]
187-190 F4.2 [Sun] e_Cr ? Total Error in [Cr/Fe]
192-195 F4.2 [Sun] e_Mn ? Total Error in [Mn/Fe]
197-200 F4.2 [Sun] e_FeII ? Total Error in [FeII/Fe]
202-205 F4.2 [Sun] e_Co ? Total Error in [Co/Fe]
207-210 F4.2 [Sun] e_Ni ? Total Error in [Ni/Fe]
212-215 F4.2 [Sun] e_Cu ? Total Error in [Cu/Fe]
217-220 F4.2 [Sun] e_Ba ? Total Error in [Ba/Fe]
222-225 F4.2 [Sun] e_La ? Total Error in [La/Fe]
227-230 F4.2 [Sun] e_Nd ? Total Error in [Nd/Fe]
232-235 F4.2 [Sun] e_Eu ? Total Error in [Eu/Fe]
237-238 I2 --- o_[Fe/H] ? Number of Fe lines observed
240-240 I1 --- o_O ? Number of O lines observed
242-242 I1 --- o_Na ? Number of Na lines observed
244-244 I1 --- o_Mg ? Number of Mg lines observed
246-246 I1 --- o_Al ? Number of Al lines observed
248-248 I1 --- o_Si ? Number of Si lines observed
250-251 I2 --- o_Ca ? Number of Ca lines observed
253-253 I1 --- o_Sc ? Number of Sc lines observed
255-255 I1 --- o_TiI ? Number of TiI lines observed
257-257 I1 --- o_TiII ? Number of TiII lines observed
259-260 I2 --- o_V ? Number of V lines observed
262-262 I1 --- o_Cr ? Number of Cr lines observed
264-264 I1 --- o_Mn ? Number of Mn lines observed
266-267 I2 --- o_FeII ? Number of FeII lines observed
269-269 I1 --- o_Co ? Number of Co lines observed
271-271 I1 --- o_Ni ? Number of Ni lines observed
273-273 I1 --- o_Cu ? Number of Cu lines observed
275-275 I1 --- o_Ba ? Number of Ba lines observed
277-277 I1 --- o_La ? Number of La lines observed
279-279 I1 --- o_Nd ? Number of Nd lines observed
281-282 I2 --- o_Eu ? Number of Eu lines observed
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table11.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 8 A8 --- ID Object name, Lemasle+ (2012, J/A+A/538/A100)
10- 14 F5.2 [Sun] [Fe/H] [-2.4/-0.6]? [Fe/H] abundance
16- 20 F5.2 [Sun] Mg [-0.9/0.7]? [Mg/Fe] abundance
22- 26 F5.2 [Sun] Ca [-0.6/0.6]? [Ca/Fe] abundance
28- 32 F5.2 [Sun] TiI [-0.5/1.4]? [TiI/Fe] abundance
34- 38 F5.2 [Sun] TiII [-0.2/0.9]? [TiII/Fe] abundance
40- 44 F5.2 [Sun] Cr [-0.7/0.6]? [Cr/Fe] abundance
46- 50 F5.2 [Sun] Mn [-0.7/0.2]? [Mn/Fe] abundance
52- 56 F5.2 [Sun] FeII [-0.01/1]? [FeII/Fe] abundance
58- 61 F4.2 [Sun] Ni [0/0.6]? [Ni/Fe] abundance
63- 67 F5.2 [Sun] Ba [-1/0.6]? [Ba/Fe] abundance
69- 72 F4.2 [Sun] e_[Fe/H] ? Total Error in [[Fe/H]
74- 77 F4.2 [Sun] e_Mg ? Total Error in [Mg/Fe]
79- 82 F4.2 [Sun] e_Ca ? Total Error in [Ca/Fe]
84- 87 F4.2 [Sun] e_TiI ? Total Error in [TiI/Fe]
89- 92 F4.2 [Sun] e_TiII ? Total Error in [TiII/Fe]
94- 97 F4.2 [Sun] e_Cr ? Total Error in [Cr/Fe]
99-102 F4.2 [Sun] e_Mn ? Total Error in [Mn/Fe]
104-107 F4.2 [Sun] e_FeII ? Total Error in [FeII/Fe]
109-112 F4.2 [Sun] e_Ni ? Total Error in [Ni/Fe]
114-117 F4.2 [Sun] e_Ba ? Total Error in [Ba/Fe]
119-120 I2 --- o_[Fe/H] ? Number of [Fe/H] lines observed
122-122 I1 --- o_Mg ? Number of Mg lines observed
124-124 I1 --- o_Ca ? Number of Ca lines observed
126-126 I1 --- o_TiI ? Number of TiI lines observed
128-128 I1 --- o_TiII ? Number of TiII lines observed
130-130 I1 --- o_Cr ? Number of Cr lines observed
132-132 I1 --- o_Mn ? Number of Mn lines observed
134-134 I1 --- o_FeII ? Number of FeII lines observed
136-136 I1 --- o_Ni ? Number of Ni lines observed
138-139 I2 --- o_Ba ? Number of Ba lines observed
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table12.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object observed in this paper
9- 16 A8 --- ID Literature source
18- 22 F5.2 [Sun] [Fe/H] [-2.7/-1.2] Fe/H abundance
24- 27 F4.2 [Sun] e_[Fe/H] [0.09/0.2] Uncertainty in [Fe/H]
29- 33 F5.2 [Sun] [Mg/Fe] [-0.5/0.8] Mg/Fe abundance
35- 38 F4.2 [Sun] e_[Mg/Fe] Uncertainty in [Mg/H]
40- 43 F4.2 [Sun] [Si/Fe] [0.06/0.9]? Si/Fe abundance
45- 48 F4.2 [Sun] e_[Si/Fe] ? Uncertainty in [Si/H]
50- 54 F5.2 [Sun] [Ca/Fe] [-0.5/0.3] Ca/Fe abundance
56- 59 F4.2 [Sun] e_[Ca/Fe] Uncertainty in [Ca/H]
61- 65 F5.2 [Sun] [Ti/Fe] [-0.2/0.6] Ti/Fe abundance
67- 70 F4.2 [Sun] e_[Ti/Fe] Uncertainty in [Ti/H]
72- 77 F6.3 [Sun] [alpha/Fe] [-0.3/0.3] Alpha-to-iron abundance ratio
79- 83 F5.3 [Sun] e_[alpha/Fe] Uncertainty in [alpha/H]
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table13.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 8 A8 --- ID Object Name
10 I1 --- f_ID ? 1=Insufficient information,
too few elements observable
12- 17 A6 --- Type ? Iwamoto type (1)
19- 22 F4.2 --- Frac [0/0.6]? Fraction of Type Ia material involved
24- 28 F5.2 [Sun] <d[Xi/Fe]> [-0.6/0.3]? Mean difference, relative abundances
30- 34 F5.2 [Sun] d[Ba/Fe] [-0.8/0.7]? Difference relative abundance, Ba
--------------------------------------------------------------------------------
Note (1): Iwamoto et al. (1999ApJS..125..439I 1999ApJS..125..439I) Type Ia model admixed in the
best-fitting model.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table14.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- Name Object name, this paper
9- 16 A8 --- [VSI2012] Venn+ (2012, J/ApJ/751/102) ID
18- 20 A3 --- [MOP93] Shetrone+ (2003AJ....125..684S 2003AJ....125..684S) ID;
<[MOP93] NN> in Simbad
22- 28 A7 --- [LHT2012] Lemasle+ (2012, J/A+A/538/A100) ID
30- 31 I2 h RAh [06] Hour of Right Ascension (J2000)
33- 34 I2 min RAm [40/42] Minute of Right Ascension (J2000)
36- 40 F5.2 s RAs Second of Right Ascension (J2000)
42 A1 --- DE- [-] Sign of the Declination (J2000)
43- 44 I2 deg DEd [50/51] Degree of Declination (J2000)
46- 47 I2 arcmin DEm Arcminute of Declination (J2000)
49- 52 F4.1 arcsec DEs Arcsecond of Declination (J2000)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table15.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 8 A8 --- ID Object name
10- 17 A8 --- OName Additional object name (1)
19- 23 F5.2 [Sun] <[Fe/H]> [-2.7/-0.6]? Average [Fe/H] abundance
25- 28 F4.2 [Sun] ? Average [O/Fe] abundance
30- 34 F5.2 [Sun] <Na> ? Average [Na/Fe] abundance
36- 40 F5.2 [Sun] <Mg> [-0.9/0.8]? Average [Mg/Fe] abundance
42- 45 F4.2 [Sun] <Si> ? Average [Si/Fe] abundance
47- 51 F5.2 [Sun] <Ca> [-0.6/0.6]? Average [Ca/Fe] abundance
53- 57 F5.2 [Sun] <Sc> ? Average [Sc/Fe] abundance
59- 63 F5.2 [Sun] <Ti> [-0.3/0.9]? Average [Ti/Fe] abundance
65- 69 F5.2 [Sun] ? Average [V/Fe] abundance
71- 75 F5.2 [Sun] <Cr> [-0.7/0.6]? Average [Cr/Fe] abundance
77- 81 F5.2 [Sun] <Mn> [-0.9/0.5]? Average [Mn/Fe] abundance
83- 87 F5.2 [Sun] <FeII> [-0.01/1]? Average [FeII/Fe] abundance
89- 93 F5.2 [Sun] <Co> ? Average [Co/Fe] abundance
95- 99 F5.2 [Sun] <Ni> [-0.4/0.6]? Average [Ni/Fe] abundance
101-105 F5.2 [Sun] <Cu> ? Average [Cu/Fe] abundance
107-111 F5.2 [Sun] <Ba> [-1.1/0.6]? Average [Ba/Fe] abundance
113-116 F4.2 [Sun] <La> ? Average [La/Fe] abundance
118-122 F5.2 [Sun] <Nd> ? Average [Nd/Fe] abundance
124-127 F4.2 [Sun] <Eu> ? Average [Eu/Fe] abundance
129-132 F4.2 [Sun] e_<[Fe/H]> ? Total uncertainty in <[Fe/H]>
134-137 F4.2 [Sun] e_ ? Total uncertainty in <[O/Fe]>
139-142 F4.2 [Sun] e_<Na> ? Total uncertainty in <[Na/Fe]>
144-147 F4.2 [Sun] e_<Mg> ? Total uncertainty in <[Mg/Fe]>
149-152 F4.2 [Sun] e_<Si> ? Total uncertainty in <[Si/Fe]>
154-157 F4.2 [Sun] e_<Ca> ? Total uncertainty in <[Ca/Fe]>
159-162 F4.2 [Sun] e_<Sc> ? Total uncertainty in <[Sc/Fe]>
164-167 F4.2 [Sun] e_<Ti> ? Total uncertainty in <[Ti/Fe]>
169-172 F4.2 [Sun] e_ ? Total uncertainty in <[V/Fe]>
174-177 F4.2 [Sun] e_<Cr> ? Total uncertainty in <[Cr/Fe]>
179-182 F4.2 [Sun] e_<Mn> ? Total uncertainty in <[Mn/Fe]>
184-187 F4.2 [Sun] e_<FeII> ? Total uncertainty in <[FeII/Fe]>
189-192 F4.2 [Sun] e_<Co> ? Total uncertainty in <[Co/Fe]>
194-197 F4.2 [Sun] e_<Ni> ? Total uncertainty in <[Ni/Fe]>
199-202 F4.2 [Sun] e_<Cu> ? Total uncertainty in <[Cu/Fe]>
204-207 F4.2 [Sun] e_<Ba> ? Total uncertainty in <[Ba/Fe]>
209-212 F4.2 [Sun] e_<La> ? Total uncertainty in <[La/Fe]>
214-217 F4.2 [Sun] e_<Nd> ? Total uncertainty in <[Nd/Fe]>
219-222 F4.2 [Sun] e_<Eu> ? Total uncertainty in <[Eu/Fe]>
--------------------------------------------------------------------------------
Note (1): If an object name is given for OName then two observations were
available for the calculation.
--------------------------------------------------------------------------------
Global notes:
Note (G1): Homogenized BVI photometry from P.B. Stetson, M. Gullieuszik
corrected to be on the Johnson-Kron-Cousins system,
following Stetson (2005PASP..117..563S 2005PASP..117..563S).
Note (G2): JHK from ESO VISTA survey photometry from M.J. Irwin, and JHKs data
from M. Gullieuszik corrected to be on the 2MASS system.
--------------------------------------------------------------------------------
History:
From electronic version of the journal
References:
Norris et al. Paper I. 2017ApJS..230...27N 2017ApJS..230...27N
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 08-Aug-2017