Search Results - "Soszy ski, I"
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Long Secondary Periods in variable red giants
Published in Monthly notices of the Royal Astronomical Society (11-11-2009)“…We present a study of a sample of Large Magellanic Cloud red giants exhibiting Long Secondary Periods (LSPs). We use radial velocities obtained from VLT…”
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Type II Cepheids Pulsating in the First Overtone from the OGLE Survey
Published in The Astrophysical journal (01-03-2019)“…We report the discovery of the first type II Cepheids (BL Herculis stars) pulsating solely in the first overtone. We found two such objects among tens of…”
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THE PANCHROMATIC VIEW OF THE MAGELLANIC CLOUDS FROM CLASSICAL CEPHEIDS. I. DISTANCE, REDDENING, AND GEOMETRY OF THE LARGE MAGELLANIC CLOUD DISK
Published in The Astrophysical journal (01-12-2016)“…ABSTRACT We present a detailed investigation of the Large Magellanic Cloud (LMC) disk using classical Cepheids. Our analysis is based on optical (I, V;…”
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SPITZER PARALLAX OF OGLE-2015-BLG-0966: A COLD NEPTUNE IN THE GALACTIC DISK
Published in The Astrophysical journal (10-03-2016)“…ABSTRACT We report the detection of a cold Neptune mplanet = 21 2 M⊕ orbiting a 0.38 M M dwarf lying 2.5-3.3 kpc toward the Galactic center as part of a…”
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FIRST SPACE-BASED MICROLENS PARALLAX MEASUREMENT OF AN ISOLATED STAR: SPITZER OBSERVATIONS OF OGLE-2014-BLG-0939
Published in The Astrophysical journal (01-04-2015)“…ABSTRACT We present the first space-based microlens parallax measurement of an isolated star. From the striking differences in the lightcurve as seen from…”
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Extracting Microlensing Signals from K2 Campaign 9
Published in Publications of the Astronomical Society of the Pacific (01-10-2017)“…The reduction of the K2's Campaign 9 (K2C9) microlensing data is challenging mostly because of the very crowded field and the unstable pointing of the…”
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THE FIRST NEPTUNE ANALOG OR SUPER-EARTH WITH A NEPTUNE-LIKE ORBIT: MOA-2013-BLG-605LB
Published in The Astrophysical journal (10-07-2016)“…ABSTRACT We present the discovery of the first Neptune analog exoplanet or super-Earth with a Neptune-like orbit, MOA-2013-BLG-605Lb. This planet has a mass…”
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Campaign 9 of the K2 Mission: Observational Parameters, Scientific Drivers, and Community Involvement for a Simultaneous Space- and Ground-based Microlensing Survey
Published in Publications of the Astronomical Society of the Pacific (01-12-2016)“…K2's Campaign 9 (K2C9) will conduct a ∼3.7 deg2 survey toward the Galactic bulge from 2016 April 22 through July 2 that will leverage the spatial separation…”
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12,660 Spotted Stars toward the OGLE Galactic Bulge Fields
Published in The Astrophysical journal (10-07-2019)“…We present the discovery and statistical analysis of 12,660 spotted variable stars toward and inside the Galactic bulge from the Optical Gravitational Lensing…”
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Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227
Published in Monthly notices of the Royal Astronomical Society (01-12-2013)“…A novel method of analysis of double-lined eclipsing binaries containing a radially pulsating star is presented. The combined pulsating-eclipsing light curve…”
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MASS MEASUREMENTS OF ISOLATED OBJECTS FROM SPACE-BASED MICROLENSING
Published in The Astrophysical journal (01-07-2016)“…ABSTRACT We report on the mass and distance measurements of two single-lens events from the 2015 Spitzer microlensing campaign. With both finite-source effect…”
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OGLE-2015-BLG-1482L: The First Isolated Low-mass Microlens in the Galactic Bulge
Published in The Astrophysical journal (01-04-2017)“…We analyze the single microlensing event OGLE-2015-BLG-1482 simultaneously observed from two ground-based surveys and from Spitzer. The Spitzer data exhibit…”
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SPITZER AS A MICROLENS PARALLAX SATELLITE: MASS AND DISTANCE MEASUREMENTS OF BINARY LENS SYSTEM OGLE-2014-BLG-1050L
Published in The Astrophysical journal (20-05-2015)“…ABSTRACT We report the first mass and distance measurements of a caustic-crossing binary system OGLE-2014-BLG-1050 L using the space-based microlens parallax…”
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DECIPHERING THE 3D STRUCTURE OF THE OLD GALACTIC BULGE FROM THE OGLE RR LYRAE STARS
Published in The Astrophysical journal (01-10-2015)“…ABSTRACT We have analyzed a sample of 27,258 fundamental-mode RR Lyrae variable stars (type RRab) detected recently toward the Galactic bulge by the Optical…”
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PATHWAY TO THE GALACTIC DISTRIBUTION OF PLANETS: COMBINED SPITZER AND GROUND-BASED MICROLENS PARALLAX MEASUREMENTS OF 21 SINGLE-LENS EVENTS
Published in The Astrophysical journal (01-05-2015)“…ABSTRACT We present microlens parallax measurements for 21 (apparently) isolated lenses observed toward the Galactic bulge that were imaged simultaneously from…”
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SPITZER IRAC PHOTOMETRY FOR TIME SERIES IN CROWDED FIELDS
Published in The Astrophysical journal (01-12-2015)“…ABSTRACT We develop a new photometry algorithm that is optimized for the Infrared Array Camera (IRAC) Spitzer time series in crowded fields and that is…”
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The dusty aftermath of the V1309 Sco binary merger
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2013)“…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…”
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OGLE-2016-BLG-1045: A Test of Cheap Space-based Microlens Parallaxes
Published in The Astrophysical journal (10-08-2018)“…Microlensing is a powerful and unique technique to probe isolated objects in the Galaxy. To study the characteristics of these interesting objects based on the…”
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A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192
Published in The Astrophysical journal (01-09-2008)“…We report the detection of an extrasolar planet of mass ratio [image] in microlensing event MOA-2007-BLG-192. The best-fit microlensing model shows both the…”
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SPITZER MICROLENS MEASUREMENT OF A MASSIVE REMNANT IN A WELL-SEPARATED BINARY
Published in The Astrophysical journal (01-12-2015)“…ABSTRACT We report the detection and mass measurement of a binary lens OGLE-2015-BLG-1285La,b, with the more massive component having M1 > 1.35 M (80%…”
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