2018AcA....68..183B


Query : 2018AcA....68..183B

2018AcA....68..183B - Acta Astron., 68, 183-203 (2018/August-0)

An Almanac of Predicted Microlensing Events for the 21st Century.

BRAMICH D.M. and NIELSEN M.B.

Abstract (from CDS):

Using Gaia data release 2 (GDR2), we present an almanac of 2509 predicted microlensing events, caused by 2130 unique lens stars, that will peak between July 25, 2026 and the end of the century. This work extends and completes a thorough search for future microlensing events initiated by Bramich and Nielsen using GDR2. The almanac includes 161 lenses that will cause at least two microlensing events each. A few highlights are presented and discussed, including: (i) an astrometric microlensing event with a peak amplitude of ≃9.7 mas, (ii) an event that will probe the planetary system of a lens with three known planets, and (iii) an event (resolvable from space) where the blend of the lens and the minor source image will brighten by a detectable amount (≃2 mmag) due to the appearance of the minor source image. All of the predicted microlensing events in the almanac will exhibit astrometric signals that are detectable by observing facilities with an angular resolution and astrometric precision similar to, or better than, that of the Hubble Space Telescope ( e.g., NIRCam on the James Webb Space Telescope), although the events with the most extreme source-to-lens contrast ratios may be challenging. Ground-based telescopes of at least 1 m in diameter can be used to observe many of the events that are also expected to exhibit a photometric signal.

Abstract Copyright:

Journal keyword(s): gravitational lensing: micro - Methods: data analysis - Catalogs - Astrometry - Stars: fundamental parameters

VizieR on-line data: <Available at CDS (J/AcA/68/183): table2.dat>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 15

goto View the references in ADS

Number of rows : 15
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 HD 1326 Er* 00 18 22.8849799680 +44 01 22.637951588   10.120   7.3   M2V 542 0
2 HD 1326B Er* 00 18 25.8251408611 +44 01 38.092431857   12.84 11.04 10.3   M3.5V 286 0
3 Wolf 28 WD* 00 49 09.8983373329 +05 23 18.993828947 12.984 12.92 12.374 12.106 11.854 DZ7.5 250 0
4 Ross 322 PM* 01 07 47.8417363419 +34 12 30.544309449   14.94 13.35 12.2   M3 29 0
5 EGGR 180 WD* 04 31 12.5714396826 +58 58 41.292707803 12.29 12.77   12.8   DC5 128 0
6 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17432 0
7 HD 39194 PM* 05 44 31.9179600882 -70 08 36.857795874   8.841 8.075     K0V 129 1
8 PM J07228-3042 WD* 07 22 51.3793277526 -30 42 34.378614303   18.3   17.4 17.2 DA 8 0
9 L 143-23 PM* 10 44 21.2329114167 -61 12 35.275360415   15.74 13.920 12.33 10.31 M5.5V 65 0
10 LAWD 37 WD* 11 45 42.9169346379 -64 50 29.461957832 11.08 11.725 11.513 11.34 11.163 DQ 267 0
11 WG 21 WD* 12 26 42.0226230528 -66 12 18.467291952   14.37 13.97     DA6.6 43 0
12 NAME Proxima Centauri Er* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1299 0
13 CD-40 9712 PM* 15 32 12.9323109019 -41 16 32.130433884 11.918 10.815 9.311 8.265 6.947 M2.5V 141 0
14 HD 145417 PM* 16 13 48.5588453721 -57 34 13.843989664 8.663 8.365 7.540 7.054 6.588 K3VFe-1.7 163 0
15 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

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