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20082026
most citedModeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk

705 citations · 12k across the 299 of their papers we have counts for

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Showing 2013Show all

18 papers · 1 filter

astro-ph.EP2013★ 9 cited

New Method to Measure Proper Motions of Microlensed Sources: Application to Candidate Free-Floating-Planet Event MOA-2011-BLG-262

Jan Skowron, Andrzej Udalski, Michał K Szymański +9

We develop a new method to measure source proper motions in microlensing events, which can partially overcome problems due to blending. It takes advantage of the fact that the sour…

astro-ph.GA2013★ 2 cited

Large Variety of New Pulsating Stars in the OGLE-III Galactic Disk Fields

P. Pietrukowicz, W. A. Dziembowski, P. Mroz +10

We present the results of a search for pulsating stars in the 7.12 deg^2 OGLE-III Galactic disk area in the direction tangent to the Centaurus Arm. We report the identification of…

astro-ph.SR2013

Eclipsing Binary Stars in the OGLE-III Fields of the Small Magellanic Cloud

M. Pawlak, D. Graczyk, I. Soszynski +10

We present a large sample of eclipsing binary stars detected in the Small Magellanic Cloud fields covering about 14 square degrees that have been monitored for eight years during t…

astro-ph.CO2013★ 85 cited

Application of Stochastic Modeling to Analysis of Photometric Reverberation Mapping Data

Ying Zu, C. S. Kochanek, Szymon Kozłowski +1

We use both simulated and real quasar light curves to explore modeling photometric reverberation-mapping (RM) data as a stochastic process. We do this using modifications to our pr…

astro-ph.SR2013★ 49 cited

Variability of Massive Stars with Known Spectral Types in the Small Magellanic Cloud Using 8 Years of OGLE-III Data

M. Kourniotis, A. Z. Bonanos, I. Soszynski +10

We present a variability study of 4646 massive stars in the Small Magellanic Cloud (SMC) with known spectral types from the catalog of Bonanos et al. (2010) using the light curves…

astro-ph.EP2013★ 66 cited

MOA-2011-BLG-322Lb: a "second generation survey" microlensing planet

Y. Shvartzvald, D. Maoz, S. Kaspi +37

Global "second-generation" microlensing surveys aim to discover and characterize extrasolar planets and their frequency, by means of round-the-clock high-cadence monitoring of a la…

astro-ph.SR2013★ 1 cited

The Kepler-SEP Mission: Harvesting the South Ecliptic Pole large-amplitude variables with Kepler

R. Szabó, L. Molnár, Z. Kołaczkowski +28

As a response to the white paper call, we propose to turn Kepler to the South Ecliptic Pole (SEP) and observe thousands of large amplitude variables for years with high cadence in…

astro-ph.CO2013★ 5 cited

A plausible (overlooked) super-luminous supernova in the SDSS Stripe 82 data

Zuzanna Kostrzewa-Rutkowska, Szymon Kozlowski, Lukasz Wyrzykowski +4

We present the discovery of a plausible super-luminous supernova (SLSN), found in the archival data of Sloan Digital Sky Survey (SDSS) Stripe 82, called PSN 000123+000504. The supe…

astro-ph.GA2013★ 4 cited

Dwarf Novae in the OGLE Data. II. Forty New Dwarf Novae in the OGLE-III Galactic Disk Fields

P. Mroz, P. Pietrukowicz, R. Poleski +9

We report the discovery of forty erupting cataclysmic variable stars in the OGLE-III Galactic disk fields: seventeen objects of U Gem type, four of Z Cam type, and nineteen stars s…

astro-ph.GA2013★ 2 cited

Eclipsing Binary Stars in the OGLE-III Galactic Disk Fields

P. Pietrukowicz, P. Mroz, I. Soszynski +9

We present the analysis of 11 589 eclipsing binary stars identified in twenty-one OGLE-III Galactic disk fields toward constellations of Carina, Centaurus, and Musca. All eclipsing…

astro-ph.EP2013★ 75 cited

Microlensing Discovery of a Tight, Low Mass-ratio Planetary-mass Object around an Old, Field Brown Dwarf

C. Han, Y. K. Jung, A. Udalski +67

Observations of accretion disks around young brown dwarfs have led to the speculation that they may form planetary systems similar to normal stars. While there have been several de…

astro-ph.EP2013★ 29 cited

Super-massive planets around late-type stars - the case of OGLE-2012-BLG-0406Lb

Radosław Poleski, Andrzej Udalski, Subo Dong +10

The core accretion theory of planetary formation does not predict that super-Jupiters will form beyond the snow line of a low mass stars. We present a discovery of 3.9 +- 1.2 M_Jup…

astro-ph.SR2013★ 29 cited

Gravitational Binary-lens Events with Prominent Effects of Lens Orbital Motion

H. Park, A. Udalski, C. Han +58

Gravitational microlensing events produced by lenses composed of binary masses are important because they provide a major channel to determine physical parameters of lenses. In thi…

astro-ph.CO2013★ 59 cited

The Magellanic Quasars Survey. III. Spectroscopic Confirmation of 758 AGNs Behind the Magellanic Clouds

Szymon Kozlowski, Christopher A. Onken, Christopher S. Kochanek +12

The Magellanic Quasars Survey (MQS) has now increased the number of quasars known behind the Magellanic Clouds by almost an order of magnitude. All survey fields in the Large Magel…

astro-ph.SR2013★ 101 cited

OGLE-2002-BLG-360: from a gravitational microlensing candidate to an overlooked red transient

R. Tylenda, T. Kaminski, A. Udalski +9

OGLE-2002-BLG-360 was discovered as a microlensing candidate by the OGLE-III project. The subsequent light curve however clearly showed that the brightening of the object could not…

astro-ph.SR2013★ 51 cited

Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs

J. -Y. Choi, C. Han, A. Udalski +121

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs are poorly understood. The multiplicity properties and minim…

astro-ph.EP2013★ 37 cited

A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251

N. Kains, R. Street, J. -Y. Choi +128

We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting micr…

astro-ph.SR2013★ 57 cited

The Dusty Aftermath of the V1309 Sco Binary Merger

C. P. Nicholls, C. Melis, I. Soszyński +9

We present mid-IR photometry and spectra of the merged binary V1309 Sco taken between 18 and 23 months after outburst. Strong mid-IR emission and a solid state absorption feature i…