Table B.2
Optical disk-integrated lightcurves used for ADAM shape modeling.
N | Epoch | Np | Δ | r | φ | Filter | Site | Observer | Reference |
---|---|---|---|---|---|---|---|---|---|
(au) | (au) | (deg) | |||||||
1 | 1968-08-13.5 | 26 | 1.13 | 2.13 | 5.4 | V | KPNO | J.L. Dunlap | Vesely & Taylor (1985) |
2 | 1968-08-14.4 | 53 | 1.13 | 2.13 | 5.1 | V | KPNO | R.C. Taylor, J.L. Dunlap | Vesely & Taylor (1985) |
3 | 1968-08-15.4 | 31 | 1.13 | 2.13 | 4.7 | V | KPNO | R.C. Taylor, J.L. Dunlap | Vesely & Taylor (1985) |
4 | 1968-08-22.4 | 36 | 1.12 | 2.13 | 4.4 | V | KPNO | J.L. Dunlap, R.E. Sather | Vesely & Taylor (1985) |
5 | 1968-08-24.3 | 108 | 1.12 | 2.12 | 4.8 | V | KPNO | J.L. Dunlap, R.E. Sather | Vesely & Taylor (1985) |
6 | 1972-08-16.0 | 36 | 1.16 | 2.17 | 5.3 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
7 | 1972-08-17.0 | 46 | 1.16 | 2.16 | 5.8 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
8 | 1972-08-18.0 | 49 | 1.17 | 2.16 | 6.4 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
9 | 1972-08-19.0 | 70 | 1.17 | 2.16 | 6.9 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
10 | 1972-08-20.0 | 65 | 1.17 | 2.16 | 7.5 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
11 | 1972-08-21.0 | 60 | 1.17 | 2.16 | 8.0 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
12 | 1972-08-24.9 | 60 | 1.18 | 2.15 | 10.1 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
13 | 1972-08-30.9 | 88 | 1.21 | 2.15 | 13.1 | V | OHP | H.J. Schober, G. Lustig | Schober & Lustig (1975) |
14 | 2009-08-23.0 | 198 | 1.34 | 2.08 | 23.8 | C | 628 | Axel Martin | Hanuš et al. (2013) |
15 | 2009-08-24.0 | 142 | 1.34 | 2.08 | 23.5 | C | 628 | Axel Martin | Hanuš et al. (2013) |
16 | 2009-08-24.1 | 14 | 1.33 | 2.08 | 23.5 | C | 628 | Axel Martin | Hanuš et al. (2013) |
17 | 2009-08-27.9 | 35 | 1.31 | 2.08 | 22.5 | C | 628 | Axel Martin | Hanuš et al. (2013) |
18 | 2009-08-28.9 | 39 | 1.30 | 2.08 | 22.3 | C | 628 | Axel Martin | Hanuš et al. (2013) |
19 | 2009-08-31.0 | 260 | 1.29 | 2.09 | 21.7 | C | 628 | Axel Martin | Hanuš et al. (2013) |
20 | 2009-08-32.0 | 165 | 1.28 | 2.09 | 21.5 | C | 628 | Axel Martin | Hanuš et al. (2013) |
21 | 2009-09-01.1 | 61 | 1.28 | 2.09 | 21.4 | C | 628 | Axel Martin | Hanuš et al. (2013) |
22 | 2009-09-09.0 | 198 | 1.23 | 2.09 | 19.2 | C | 628 | Axel Martin | Hanuš et al. (2013) |
23 | 2017-07-27.4 | 202 | 1.30 | 2.11 | 21.1 | CS3-PDS | Brian Warner | Warner (2018) | |
24 | 2017-07-28.4 | 194 | 1.29 | 2.11 | 20.9 | CS3-PDS | Brian Warner | Warner (2018) | |
25 | 2017-07-29.4 | 12 | 1.28 | 2.11 | 20.5 | CS3-PDS | Brian Warner | Warner (2018) | |
26 | 2017-07-30.4 | 269 | 1.27 | 2.11 | 20.2 | CS3-PDS | Brian Warner | Warner (2018) | |
27 | 2017-07-31.4 | 205 | 1.26 | 2.11 | 19.9 | CS3-PDS | Brian Warner | Warner (2018) | |
28 | 2017-08-05.4 | 244 | 1.23 | 2.10 | 18.3 | CS3-PDS | Brian Warner | Warner (2018) | |
29 | 2017-08-06.4 | 286 | 1.22 | 2.10 | 17.9 | CS3-PDS | Brian Warner | Warner (2018) | |
30 | 2017-09-21.2 | 553 | 1.12 | 2.08 | 11.4 | V | TRAPPIST-S | E. Jehin, M. Ferrais | This work |
31 | 2017-09-22.2 | 537 | 1.13 | 2.08 | 11.7 | V | TRAPPIST-S | E. Jehin, M. Ferrais | This work |
32 | 2017-09-23.2 | 619 | 1.13 | 2.08 | 12.1 | V | TRAPPIST-S | E. Jehin, M. Ferrais | This work |
33 | 2017-10-01.2 | 726 | 1.17 | 2.08 | 15.1 | V | TRAPPIST-S | E. Jehin, M. Ferrais | This work |
34 | 2017-11-28.0 | 522 | 1.68 | 2.10 | 27.6 | Rc | TRAPPIST-N | E. Jehin, M. Ferrais | This work |
35 | 2017-12-03.0 | 478 | 1.74 | 2.10 | 27.8 | Rc | TRAPPIST-N | E. Jehin, M. Ferrais | This work |
36 | 2017-12-07.9 | 604 | 1.80 | 2.10 | 27.9 | Rc | TRAPPIST-N | E. Jehin, M. Ferrais | This work |
37 | 2017-12-23.9 | 418 | 1.98 | 2.12 | 27.5 | Rc | TRAPPIST-N | E. Jehin, M. Ferrais | This work |
Notes. For each lightcurve, the table gives the epoch, the number of individual measurements Np, asteroid’s distances to the Earth Δ and the Sun r, phase angle φ, photometric filter and observation information. The observations by Warner (2018) were made without a filter but the reported magnitudes were on an internal system close to Johnson V. KPNO – Kitt Peak National Observatory, 41 cm telescope number 4. OHP – l’Observatoire de Haute Provence, France. 628 – Mulheim-Ruhr, Germany. CS3-PDS – Center for Solar System Studies, 446 Sycamore Ave., Eaton, CO 80615, USA. TRAPPIST-S and -N are located at La Silla Observatory (Chile) and Oukaimeden Observatory (Morocco), respectively (Jehin et al. 2011).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.