2019A&A...623A.164L


Query : 2019A&A...623A.164L

2019A&A...623A.164L - Astronomy and Astrophysics, volume 623A, 164-164 (2019/3-1)

Recovering saturated images for high dynamic kernel-phase analysis. Application to the determination of dynamical masses for the system Gl 494AB.

LAUGIER R., MARTINACHE F., CEAU A., MARY D., N'DIAYE M. and BEUZIT J.-L.

Abstract (from CDS):

Kernel-phase observables extracted from mid- to high-Strehl images are proving to be a powerful tool to probe within a few angular resolution elements of point sources. The attainable contrast is limited, however, by the dynamic range of the imaging sensors. The Fourier interpretation of images with pixels exposed beyond the saturation has so far been avoided. In cases where the image is dominated by the light of a point source, we show that we can use an interpolation to reconstruct the otherwise lost pixels with an accuracy sufficient to enable the extraction of kernel-phases from the patched image. We demonstrate the usability of our method by applying it to archive images of the Gl 494AB system taken with the Hubble Space Telescope in 1997. Using this new data point along with other resolved observations and radial velocity measurements, we produce improved constraints on the orbital parameters of the system, and consequently the masses of its components.

Abstract Copyright: © R. Laugier et al. 2019

Journal keyword(s): techniques: image processing - techniques: interferometric - techniques: high angular resolution - stars: low-mass - binaries: close

Simbad objects: 33

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Number of rows : 33
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 LP 469-67 LM* 02 02 16.2429995239 +10 20 13.937753422       15.711   M5.5V 53 0
2 Ross 47 BY* 05 42 09.2676872099 +12 29 21.604835564 14.264 13.130 11.509 10.298 8.709 M4V 268 0
3 HD 42581 Er* 06 10 34.6149358167 -21 51 52.656352926 10.801 9.607 8.125 7.164 6.121 M1V 478 0
4 HD 260655 PM* 06 37 10.7988015297 +17 33 53.333221083 12.303 11.104 9.593 8.661 7.718 M0.0V 176 0
5 G 109-35 PM* 06 59 28.8164986147 +19 20 55.857870053   16.78   10.6   M5.0Ve 76 0
6 HD 296991 * 09 44 05.2932242424 -46 17 19.571067492   10.76 9.37     K5 4 0
7 HD 85512 PM* 09 51 07.0518026760 -43 30 10.023686079 9.963 8.83 7.651 6.934 6.319 K6Vk: 213 1
8 L 143-23 PM* 10 44 21.2329114167 -61 12 35.275360415   15.74 13.920 12.33 10.31 M5.5V 65 0
9 Ross 128 Er* 11 47 44.3972681420 +00 48 16.400337591 14.223 12.905 11.153 9.859 8.184 dM4 420 0
10 G 122-49 PM* 11 50 57.7205259231 +48 22 38.561183125       12.95   M4.5V 118 0
11 * bet CVn ** 12 33 44.5442516547 +41 21 26.921352859 4.91 4.86 4.25 3.73 3.42 G0V 579 0
12 Wolf 461 Er* 13 00 33.5221795982 +05 41 07.996620384   15.12   13.041   M4.5Ve 133 0
13 BD+13 2618 Er* 13 00 46.5566863405 +12 22 32.677229903 12.314 11.233 9.750 8.785 7.653 M0V 348 1
14 L 339-19 PM* 16 40 45.2528895868 -45 59 59.302886578   13.70 12.73 12.320 10.19 M3.0V 36 0
15 G 19-7 Er* 16 57 05.7362228328 -04 20 56.318033870   13.92 12.25 10.99 9.432 dM4 101 0
16 BD+25 3173 PM* 16 58 08.8496107083 +25 44 38.974052855 12.342 11.139 9.655 8.685 7.602 M2V 224 1
17 G 203-42 PM* 17 03 23.8838600746 +51 24 22.868680261   15.31   13.301   M5.0V 67 0
18 HD 157881 PM* 17 25 45.2324302566 +02 06 41.123732402 10.126 8.865 7.56 6.649 5.89 K7V 336 0
19 CD-46 11540 LM* 17 28 39.9455781571 -46 53 42.688095874 12.177 10.973 9.407 8.337 7.006 M3V 254 1
20 BD+18 3421 PM* 17 37 53.3468417549 +18 35 30.164096453 12.315 11.109 9.577 8.599 7.525 M1.5V 211 0
21 HD 165222 PM* 18 05 07.5787518746 -03 01 52.749184670 12.09 10.878 9.360 8.385 7.304 M0V 230 0
22 G 227-29 PM* 18 22 27.0947595389 +62 03 01.746625489   14.8   13.060   M4.0V 81 0
23 G 185-18 PM* 19 21 38.7001955897 +20 52 03.284705570   15.13 13.42 13.116 10.44 M4.0Ve 72 0
24 * del Pav PM* 20 08 43.6088716052 -66 10 55.442769229 4.78 4.32 3.56 2.95 2.61 G8IV 390 0
25 HD 191849 PM* 20 13 53.3962498530 -45 09 50.470550834 10.627 9.419 7.966 7.053 6.124 M0V 166 0
26 HD 192310 PM* 20 15 17.3913760474 -27 01 58.711625384   6.63 5.723 5.98 8.74 K2+V 318 1
27 G 262-15 PM* 20 30 32.0453969319 +65 26 58.411357864   12.00   10.124   M3V 165 0
28 HD 204961 PM* 21 33 33.9751191976 -49 00 32.399427028 11.359 10.176 8.672 7.665 6.479 M2/3V 290 1
29 * eps Ind PM* 22 03 21.6536261624 -56 47 09.522795714   5.75 4.69     K5V 551 0
30 L 49-19 PM* 22 55 45.5127596213 -75 27 31.203633959 13.004 11.873 10.377 9.312 7.958 M3V 74 0
31 G 157-77 PM* 23 35 10.4624266947 -02 23 20.613547105   16.60 14.69 14.447   M5.0Ve 94 0
32 G 130-4 PM* 23 43 06.3118372752 +36 32 13.137302361   14.27 12.67 11.4   M4.5Ve 93 0
33 V* BR Psc BY* 23 49 12.5250852078 +02 24 04.405476893 11.532 10.427 8.993 8.029 6.946 dM1 326 0

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