2017A&A...598A...5P


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.10CEST06:30:46

2017A&A...598A...5P - Astronomy and Astrophysics, volume 598A, 5-5 (2017/2-1)

The Gaia-ESO Survey: Calibration strategy.

PANCINO E., LARDO C., ALTAVILLA G., MARINONI S., RAGAINI S., COCOZZA G., BELLAZZINI M., SABBI E., ZOCCALI M., DONATI P., HEITER U., KOPOSOV S.E., BLOMME R., MOREL T., SIMON-DIAZ S., LOBEL A., SOUBIRAN C., MONTALBAN J., VALENTINI M., CASEY A.R., BLANCO-CUARESMA S., JOFRE P., WORLEY C.C., MAGRINI L., HOURIHANE A., FRANCOIS P., FELTZING S., GILMORE G., RANDICH S., ASPLUND M., BONIFACIO P., DREW J.E., JEFFRIES R.D., MICELA G., VALLENARI A., ALFARO E.J., ALLENDE PRIETO C., BABUSIAUX C., BENSBY T., BRAGAGLIA A., FLACCOMIO E., HAMBLY N., KORN A.J., LANZAFAME A.C., SMILJANIC R., VAN ECK S., WALTON N.A., BAYO A., CARRARO G., COSTADO M.T., DAMIANI F., EDVARDSSON B., FRANCIOSINI E., FRASCA A., LEWIS J., MONACO L., MORBIDELLI L., PRISINZANO L., SACCO G.G., SBORDONE L., SOUSA S.G., ZAGGIA S. and KOCH A.

Abstract (from CDS):

The Gaia-ESO survey (GES) is now in its fifth and last year of observations and has produced tens of thousands of high-quality spectra of stars in all Milky Way components. This paper presents the strategy behind the selection of astrophysical calibration targets, ensuring that all GES results on radial velocities, atmospheric parameters, and chemical abundance ratios will be both internally consistent and easily comparable with other literature results, especially from other large spectroscopic surveys and from Gaia. The calibration of GES is particularly delicate because of (i) the large space of parameters covered by its targets, ranging from dwarfs to giants, from O to M stars; these targets have a large wide of metallicities and also include fast rotators, emission line objects, and stars affected by veiling; (ii) the variety of observing setups, with different wavelength ranges and resolution; and (iii) the choice of analyzing the data with many different state-of-the-art methods, each stronger in a different region of the parameter space, which ensures a better understanding of systematic uncertainties. An overview of the GES calibration and homogenization strategy is also given, along with some examples of the usage and results of calibrators in GES iDR4, which is the fourth internal GES data release and will form the basis of the next GES public data release. The agreement between GES iDR4 recommended values and reference values for the calibrating objects are very satisfactory. The average offsets and spreads are generally compatible with the GES measurement errors, which in iDR4 data already meet the requirements set by the main GES scientific goals.

Abstract Copyright: © ESO, 2017

Journal keyword(s): surveys - Galaxy: general - stars: abundances - techniques: spectroscopic - techniques: radial velocities

VizieR on-line data: <Available at CDS (J/A+A/598/A5): table2.dat>

Status at CDS:   All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 98

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Number of rows : 98

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 HD 283 PM* 00 07 32.5418081805 -23 49 07.398024948   9.50 8.70     G9.5V 55 0
2 * gam Peg bC* 00 13 14.1512308 +15 11 00.936759 1.75 2.61 2.84 2.94 3.13 B2IV 660 0
3 NGC 104 GlC 00 24 05.359 -72 04 53.20   5.78 4.09     ~ 3548 0
4 * bet Hyi PM* 00 25 45.07036 -77 15 15.2860 3.52 3.41 2.79 2.28 1.94 G0V 544 0
5 NGC 362 GlC 01 03 14.26 -70 50 55.6     6.58     ~ 938 0
6 HD 6512 PM* 01 06 12.6312001066 +13 15 09.877746638       7.7   G0 47 0
7 * tau Cet PM* 01 44 04.0834226 -15 56 14.926552 4.43 4.22 3.50 2.88 2.41 G8V 1091 1
8 * psi Phe LP* 01 53 38.7410337 -46 18 09.604795 7.71 6.00 4.41 2.68 1.17 M4III 97 0
9 * eps For PM* 03 01 37.6304831834 -28 05 29.376723799   6.68 5.85     G9:V 157 0
10 * alf Cet LP? 03 02 16.77307 +04 05 23.0596 6.10 4.17 2.53 1.18 0.02 M1.5IIIa 439 0
11 NGC 1261 GlC 03 12 16.21 -55 12 58.4   9.79 8.63     ~ 426 0
12 * eps Eri BY* 03 32 55.8449634 -09 27 29.731165 5.19 4.61 3.73 3.00 2.54 K2V 1697 1
13 HD 22879 Pe* 03 40 22.0654223510 -03 13 01.124769689 7.146 7.222 6.667 6.346 6.016 G0VmF2 434 0
14 HD 27947 * 04 25 00.3251206411 +11 58 40.535954503   9.05 8.40     G0 29 0
15 * del03 Tau a2* 04 25 29.38340 +17 55 40.4579   4.369 4.298 6.18 4.24 A2IV-Vs 381 0
16 * alf Tau LP? 04 35 55.23907 +16 30 33.4885 4.32 2.40 0.86 -0.37 -1.31 K5+III 1178 1
17 NGC 1851 GlC 05 14 06.76 -40 02 47.6   8.80 7.23     ~ 1241 0
18 M 79 GlC 05 24 10.59 -24 31 27.3   9.21 8.16     ~ 717 0
19 HD 36395 PM* 05 31 27.3958475290 -03 40 38.021551815 10.626 9.443 7.968 6.996 5.913 M1.5Ve 428 0
20 V* V2689 Ori RS* 05 36 30.9904303980 +11 19 40.331999226 11.508 10.276 8.898 7.963 7.140 K6V 112 0
21 HD 38459 PM* 05 43 26.4569110795 -47 49 22.710164014   9.37 8.50     K1IV-V 45 0
22 NAME Gal Anticenter reg 05 46 +28.9           ~ 720 0
23 * 134 Tau * 05 49 32.9297423 +12 39 04.758221 4.68 4.811 4.875     B9IV 178 0
24 HD 42581 Fl* 06 10 34.6152510171 -21 51 52.658021185 10.801 9.607 8.125 7.164 6.121 M1V 396 0
25 NGC 2243 OpC 06 29 34 -31 17.0   10.12 9.4     ~ 210 0
26 HD 46828 PM* 06 35 03.0323467851 -12 36 27.579641038   8.17 7.70     F6V 25 0
27 HD 48381 * 06 41 42.9532280933 -33 28 11.101369729   9.57 8.50     K0IV 21 0
28 HD 49035 PM* 06 42 23.2469863554 -61 13 29.890169196   9.27 8.53     G5/6IV/V 39 0
29 HD 49933 ** 06 50 49.831 -00 32 27.18           F3V 326 1
30 HD 51754 PM* 06 58 38.5387307770 -00 28 49.697886299 9.60 9.567 9.009 8.663 8.334 G2V 110 0
31 HD 56613 Pu* 07 17 31.6049283914 -05 49 21.499268021   7.12 7.21     B8V 10 0
32 Cl Melotte 71 OpC 07 37 34 -12 03.3   7.44 7.1     ~ 94 0
33 NGC 2420 OpC 07 38 23 +21 34.4   9.0 8.3     ~ 398 0
34 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1758 0
35 NGC 2477 OpC 07 52 10 -38 31.8   6.64 5.8     ~ 256 0
36 HD 64942 * 07 55 58.2270625134 -09 47 49.933268457   9.00 8.34     G3/5V 47 0
37 HD 68450 * 08 11 01.6834504504 -37 17 32.541641609 5.58 6.42 6.44 7.43   O9.7II 124 0
38 NGC 2682 OpC 08 51 18 +11 48.0           ~ 2032 0
39 * rho01 Cnc PM* 08 52 35.8113282132 +28 19 50.956901366 7.45 6.82   5.4   K0IV-V 969 1
40 IRAS 09110-6439 GlC 09 12 03.10 -64 51 48.6   7.77 5.69     ~ 1245 0
41 HD 79601 PM* 09 13 44.6281531458 -42 18 37.470774830   8.55 8.02     G2V 77 0
42 Ross 85 PM* 09 41 10.3603705950 +13 12 34.424857126 13.097 11.891 10.370 9.371 8.182 M2.5V 102 0
43 HD 84273 PM* 09 43 20.2759924707 -29 48 14.427801074   9.05 8.40     G5V 31 0
44 HD 84937 PM* 09 48 56.09801 +13 44 39.3237 8.49 8.68 8.32 7.97 7.70 F8Vm-5 717 0
45 HD 88725 PM* 10 14 08.3345668419 +03 09 04.675865338 8.34 8.33 7.73 7.24 6.89 G3/5V 170 0
46 BD+20 2465 Er* 10 19 36.2808024653 +19 52 12.014037746   10.82 9.52 9.19   M4Vae 1146 0
47 BD-09 3070 PM* 10 25 10.8370935977 -10 13 43.289558706 12.834 11.631 10.139 9.161 8.051 M1V 112 0
48 NGC 3293 OpC 10 35 49 -58 13.8   4.84 4.7     ~ 282 0
49 * tet Car SB* 10 42 57.4019674 -64 23 40.020796 1.53 2.54 2.76 2.87 3.10 B0Vp 313 0
50 HD 93128 SB* 10 43 54.3955430232 -59 32 57.496584258 8.82 8.97 8.77 9.40 8.71 O3.5V((fc))z 83 1
51 NGC 3532 OpC 11 05 39 -58 45.2           ~ 264 0
52 * ksi Hya ** 11 33 00.1150559 -31 51 27.443449 5.17 4.47 3.54 2.84 2.36 G7IIIb 231 0
53 Ross 905 PM* 11 42 11.0933874353 +26 42 23.658083337   12.06 10.613 10.272 8.24 M3V 495 1
54 * bet Vir PM* 11 50 41.7182390 +01 45 52.991019 4.26 4.15 3.60 3.13 2.85 F9V 856 0
55 HD 103932 PM* 11 57 56.2063624042 -27 42 25.364242481 9.23 8.114 6.964 6.298 5.758 K4+V 141 0
56 * c Vir PM* 12 20 20.9813348 +03 18 45.260365 7.27 6.12 4.96 4.07 3.46 K0.5IIIbFe-0.5 335 0
57 NGC 4372 GlC 12 25 45.43 -72 39 32.7   10.86 9.85     ~ 263 0
58 NGC 4833 GlC 12 59 33.92 -70 52 35.4   8.72 7.79     ~ 350 0
59 NAME Centaurus A Sy2 13 25 27.61509104 -43 01 08.8056025   8.18 6.84 6.66   ~ 3999 3
60 BD+11 2576 PM* 13 29 59.7856884759 +10 22 37.784822214 11.728 10.524 9.029 8.07 7.013 M1.0Ve 198 0
61 HD 117600 PM* 13 32 16.1161518291 -47 25 06.759578947   9.99 9.16     K2IV/V(p) 29 0
62 HD 119850 Fl* 13 45 43.7754528655 +14 53 29.473195472 10.989 9.894 8.50 7.465 6.363 M2V 289 0
63 NAME Cen B QSO 13 46 49.04327124 -60 24 29.3552337         15.74 ~ 125 0
64 * eta Boo SB* 13 54 41.07892 +18 23 51.7946 3.440 3.250 2.680 2.24 1.95 G0IV 654 1
65 HD 122563 Pe* 14 02 31.8456299772 +09 41 09.942736952 7.47 7.10 6.19 5.37 4.79 G8:III:Fe-5 746 0
66 * alf Boo RG* 14 15 39.67207 +19 10 56.6730 2.46 1.18 -0.05 -1.03 -1.68 K1.5IIIFe-0.5 2133 0
67 V* V645 Cen Er* 14 29 42.9451234609 -62 40 46.170818907 14.21 12.95 11.13 9.45 7.41 M5.5Ve 958 0
68 BD-07 4003 BY* 15 19 26.8271336166 -07 43 20.190958776 13.403 11.76 10.560 9.461 8.911 M3V 534 2
69 NGC 5927 GlC 15 28 00.69 -50 40 22.9   10.13 8.86     ~ 404 0
70 HD 140283 Pe* 15 43 03.0967798658 -10 56 00.595803430 7.508 7.711 7.212 6.63 8.21 F9VkA5mA1 852 0
71 HD 141105 PM* 15 47 24.1458440377 -01 03 48.301224918   8.83 8.04     G8V 22 0
72 * 18 Sco PM* 16 15 37.2703721200 -08 22 09.981989277   6.15 5.50     G2Va 484 0
73 HD 147518 PM* 16 24 56.3594475504 -51 25 44.234007688   10.00 9.38     G3/5V(w) 36 0
74 * tau Sco * 16 35 52.9528530 -28 12 57.661515 1.55 2.56 2.81 2.93 3.18 B0.2V 854 0
75 NAME Galactic Center Spur Rad 16 41 -39.1           ~ 12 1
76 M 12 GlC 16 47 14.18 -01 56 54.7   8.52 6.07     ~ 579 0
77 NGC 6253 OpC 16 59 05 -52 42.0     10.2     ~ 144 0
78 HD 319699 * 17 19 30.4179094473 -35 42 36.122491362 10.17 10.31 9.63 9.81 8.91 O5V((fc)) 56 0
79 * bet Ara * 17 25 17.9883527 -55 31 47.586765 5.87 4.31 2.85     K0/1Ib 114 0
80 HD 157881 PM* 17 25 45.2323043669 +02 06 41.123668100 10.126 8.865 7.56 6.649 5.89 K7V 310 0
81 * mu. Ara PM* 17 44 08.7036342277 -51 50 02.591049123   5.85 5.15     G3IV-V 465 2
82 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11540 0
83 NAME Barnard's star BY* 17 57 48.4997994034 +04 41 36.111354228 12.497 11.24 9.511 8.298 6.741 M4V 655 2
84 HD 163758 s*b 17 59 28.3670166132 -36 01 15.588119230 6.46 7.35 7.32 8.38   O6.5Iafp 144 0
85 NGC 6553 GlC 18 09 15.68 -25 54 27.9   9.08       ~ 535 0
86 NGC 6705 OpC 18 51 05 -06 16.2   6.32 5.8     ~ 354 0
87 HD 175607 PM* 19 01 05.4888630172 -66 11 33.642423195   9.31 8.61     G6V 52 0
88 NGC 6752 GlC 19 10 52.11 -59 59 04.4   6.96 6.28     ~ 1807 0
89 * gam Sge PM* 19 58 45.4286265 +19 29 31.728079 6.97 5.04 3.47 2.27 1.35 M0-III 241 0
90 HD 201219 PM* 21 07 56.5198482794 +07 25 58.594323368       7.6   G5 55 0
91 HD 203021 PM* 21 21 23.5928467156 -51 45 09.421141853   7.40 6.75     G8/K1III+(F/G) 24 0
92 M 15 GlC 21 29 58.33 +12 10 01.2   3       ~ 2907 0
93 HD 204587 PM* 21 30 02.7560686865 -12 30 36.246696764 11.59 10.36 9.075 8.28 7.586 K7Vk: 104 0
94 M 2 GlC 21 33 27.02 -00 49 23.7     6.25     ~ 899 1
95 HD 207970 PM* 21 53 41.8139891944 -28 40 14.205578459   8.55 7.82     G7V 43 0
96 HD 216899 PM* 22 56 34.8047291749 +16 33 12.353727149 11.323 10.143 8.638 7.657 6.542 M1.5Ve 234 0
97 HD 217357 PM* 23 00 16.1224771183 -22 31 27.651428500 10.494 9.251 7.869 7.014 6.238 K7+Vk 158 0
98 * 7 Psc PM* 23 20 20.5830620142 +05 22 52.700020565   6.262 5.069     K1IV 107 0

    Equat.    Gal    SGal    Ecl

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2020.07.10-06:30:46

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