• No results found

The MACHO PROJECT: 45 Candidate microlensing events

Candidate microlensing events from M31 observations with the Loiano
  telescope

Candidate microlensing events from M31 observations with the Loiano telescope

... The only clear outlier is the bright and short set B mi- crolensing candidate. We discuss the selected candidates in detail in Sect. 5.2. Comparing with the efficiency simulation analysis, a few points are worth ...

12

Candidate gravitational microlensing events for future direct lens imaging

Candidate gravitational microlensing events for future direct lens imaging

... of microlensing events toward the Galactic bulge with high relative lens-source proper motion that are therefore good candidates for constraining the lens mass with future high-resolution ...all ...

11

Microlensing Binaries with Candidate Brown Dwarf Companions

Microlensing Binaries with Candidate Brown Dwarf Companions

... dwarf candidate (Bozza et ...dwarf events is the difficulty in analyzing binary-lensing light curves due to the complexity of the light ...binary-lensing events in which the mass ratio between the ...

10

A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event

A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event

... gravitational microlensing via their light-bending gravity. Microlensing events due to terrestrial-mass rogue planets are expected to have extremely small angular Einstein radii ...shortest-timescale ...

8

Distribution of Caustic-Crossing Intervals for Galactic Binary-Lens Microlensing Events

Distribution of Caustic-Crossing Intervals for Galactic Binary-Lens Microlensing Events

... However, the expected most frequent caustic-crossing interval of ∼ 1.5 day is shorter than the current preparation time of the followup observations. Then, if the preparation time is shortened by adopting more aggressive ...

6

Gravitational Microlensing

Gravitational Microlensing

... of microlensing events have since been observed, although the idea that MACHOs contribute to dark matter has largely been ...first microlensing events were observed, Mao and Paczynski ...

78

Microlensing in Galactic Halos

Microlensing in Galactic Halos

... Conclusions Microlensing searches towards the Magellanic Clouds and the Andromeda galaxy, M31, have given, in recent years, first exciting though somewhat contradictory conclu- ...of microlensing ...

10

First searches for optical counterparts to gravitational-wave candidate events

First searches for optical counterparts to gravitational-wave candidate events

... We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for providing the kilonova model light curves that we have used in our Figures 4–7. The authors gratefully acknowledge the support of the United States National ...

25

First searches for optical counterparts to gravitational-wave candidate events

First searches for optical counterparts to gravitational-wave candidate events

... We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for providing the kilonova model light curves that we have used in our Figures 4–7. The authors gratefully acknowledge the support of the United States National ...

26

First Searches for Optical Counterparts to Gravitational-Wave Candidate Events

First Searches for Optical Counterparts to Gravitational-Wave Candidate Events

... We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for providing the kilonova model light curves that we have used in our Figures 4–7. The authors gratefully acknowledge the support of the United States National ...

27

First searches for optical counterparts to gravitational-wave candidate events

First searches for optical counterparts to gravitational-wave candidate events

... We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for providing the kilonova model light curves that we have used in our Figures 4–7. The authors gratefully acknowledge the support of the United States National ...

25

First Searches for Optical Counterparts to Gravitational-Wave Candidate Events

First Searches for Optical Counterparts to Gravitational-Wave Candidate Events

... We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for providing the kilonova model light curves that we have used in our Figures 4 – 7 . The authors gratefully acknowledge the support of the United States National ...

26

Candidate Brief. Nutrition Project Manager CABI

Candidate Brief. Nutrition Project Manager CABI

... • Ensure accurate and timely management of the funds and track budget utilization with support from the concerned persons and teams • Support the Strategic Business Development Programme Manager on the development of ...

6

Galactic Aspects of Gravitational Microlensing: High Magnification Events and Stellar Limb-darkening of a Source Star in the Galactic bulge

Galactic Aspects of Gravitational Microlensing: High Magnification Events and Stellar Limb-darkening of a Source Star in the Galactic bulge

... main project, we reviewed all high mgnification events observed during the 2006 season in order to select a well-covered subset of events which could hide a planetary ...magnification events, ...

83

Identification and classification of interesting variable stars in the macho database

Identification and classification of interesting variable stars in the macho database

... The macho database [1, 3] is an astronomical database consisting of the intensities of about 20 million stars recorded approximately every night for several ...rare events called microlensing when a ...

19

Measuring polarization in microlensing events

Measuring polarization in microlensing events

... The study of these events, integrated by a Monte Carlo analysis, allows us to estimate the expected polarization profiles and to predict for which source stars and at which time is most [r] ...

8

Measuring polarization in microlensing events

Measuring polarization in microlensing events

... Here and in the following we indicate with the subscript ‘int ’ dereddened quantities of the unlensed source star.6 Given the physical parameters of the source stars, by using equations [r] ...

8

Modelling of Planetary Gravitational Microlensing Events

Modelling of Planetary Gravitational Microlensing Events

... Beaulieu, J., Bennett, D. P., Fouqu´e, P., Williams, A., Dominik, M., Jørgensen, U. G., Kubas, D., Cassan, A., Coutures, C., Greenhill, J., Hill, K., Menzies, J., Sackett, P. D., Albrow, M., Brillant, S., Caldwell, J. A. ...

209

A spectroscopic and photometric study of gravitational microlensing events

A spectroscopic and photometric study of gravitational microlensing events

... Also, extinction effects towards the Galactic bulge have been shown to have a non-negligible effect on the observed optical depth, the effects of which can be seen in the reddening of[r] ...

299

The advantages of using a Lucky Imaging camera for observations of microlensing events

The advantages of using a Lucky Imaging camera for observations of microlensing events

... min . (16) The crucial point regarding the sampling interval is that we set it to ∼10 min once at least three data points deviate from the simple microlensing light curve by more than 2 σ . Once the anomaly is ...

12

Show all 10000 documents...

Related subjects