1999
DOI: 10.1086/312018
|View full text |Cite
|
Sign up to set email alerts
|

MACHO Mass Determination Based on Space Telescope Observation

Abstract: We investigate the possibility of lens mass determination for a caustic crossing microlensing event based on a space telescope observation. We demonstrate that the parallax due to the orbital motion of a space telescope causes a periodic fluctuation of the light curve, from which the lens distance can be derived. Since the proper motion of the lens relative to the source is also measurable for a caustic crossing event, one can find a full solution for microlensing properties of the event, including the lens ma… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
18
1

Year Published

2001
2001
2016
2016

Publication Types

Select...
7
1
1

Relationship

0
9

Authors

Journals

citations
Cited by 18 publications
(19 citation statements)
references
References 14 publications
0
18
1
Order By: Relevance
“…Therefore, if that magnification pattern has a non-zero second derivative, such as when the source crosses a caustic (where the magnification diverges to infinity), the physical size of the source limits the observed magnification, leading to a rounded feature in the light curve whose width directly reflects the source size (Gould 1994a;Witt & Mao 1994). The microlens parallax p E is measured through observations from either a single accelerating platform (Gould 1992(Gould , 2013Honma 1999) or two wellseparated observatories (Refsdal 1966;Gould 1994bGould , 1997.…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, if that magnification pattern has a non-zero second derivative, such as when the source crosses a caustic (where the magnification diverges to infinity), the physical size of the source limits the observed magnification, leading to a rounded feature in the light curve whose width directly reflects the source size (Gould 1994a;Witt & Mao 1994). The microlens parallax p E is measured through observations from either a single accelerating platform (Gould 1992(Gould , 2013Honma 1999) or two wellseparated observatories (Refsdal 1966;Gould 1994bGould , 1997.…”
Section: Introductionmentioning
confidence: 99%
“…Hence, the oscillations would typically be minuscule. To overcome this obstacle, Honma (1999) proposed that the observations should be made during caustic crossings, which he showed dramatically increase the strength of the signal. However, alerting HST to imminent caustic crossings is extremely difficult, more so for planetary events, and in fact such measurements have never been carried out, nor even attempted.…”
Section: Introductionmentioning
confidence: 99%
“…The Earth and various space telescopes are all accelerating platforms. This acceleration can be seen in the light curve of the microlensing event, provided the event timescale is a significant fraction of the orbit [38,39,40]. Second, a microlensing event from two different locations will have a different observed light curve for each location because of the parallax effect [41,42,43,44].…”
Section: Pos(bash2015)002mentioning
confidence: 99%