activity
20142024
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 13.7k across the 101 of their papers we have counts for

collaborators

104 papers

astro-ph.GA2024★ 129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.SR2022★ 6 cited

Do Miras show the long secondary periods?

Michal Pawlak

The long secondary period (LSP) phenomenon, which is commonly observed in pulsating red giants, has not been detected in any Mira yet. The goal of this paper is to verify, if there…

astro-ph.SR2022★ 1 cited

OGLE-BLG504.12.201843: A possible extreme dwarf nova

Camille Landri, Ondřej Pejcha, Michał Pawlak +5

We present the analysis of existing optical photometry and new optical spectroscopy of the candidate cataclysmic variable star OGLE-BLG504.12.201843. As was shown previously, this…

astro-ph.SR2021★ 15 cited

Search for Dormant Black Holes in Ellipsoidal Variables III. The OGLE BULGE Short-Period Sample

Roy Gomel, Simchon Faigler, Tsevi Mazeh +1

This is the third of a series of papers that presents an algorithm to search for close binaries with massive, possibly compact, unseen secondaries. The detection of such a binary i…

astro-ph.SR2021★ 11 cited

Connection between the Long Secondary Period phenomenon and the red giant evolution

Michał Pawlak

The mechanism behind the Long Secondary Period (LSP) observed in pulsating red giants still remains unknown. In this work, I investigate the connection between the Red Giant Branch…

astro-ph.GA2021★ 13 cited

Gaia Early Data Release 3: Structure and properties of the Magellanic Clouds

Gaia Collaboration, X. Luri, L. Chemin +417

We compare the Gaia DR2 and Gaia EDR3 performances in the study of the Magellanic Clouds and show the clear improvements in precision and accuracy in the new release. We also show…

astro-ph.GA2020★ 112 cited

Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

Gaia Collaboration, S. A. Klioner, F. Mignard +414

Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quali…

astro-ph.SR2020★ 66 cited

The ASAS-SN Catalog of Variable Stars IX: The Spectroscopic Properties of Galactic Variable Stars

T. Jayasinghe, C. S. Kochanek, K. Z. Stanek +11

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline ( yrs) band light curves for sources brighter than V mag across the whole sky.…

astro-ph.SR2019★ 41 cited

The ASAS-SN Catalog of Variable Stars VII: Contact Binaries are Different Above and Below the Kraft Break

T. Jayasinghe, K. Z. Stanek, C. S. Kochanek +11

We characterize W UMa type (EW) contact binaries, including new discoveries, using ASAS-SN -band all-sky light curves along with archival data fr…

astro-ph.SR2019★ 86 cited

The ASAS-SN Catalog of Variable Stars V: Variables in the Southern Hemisphere

T. Jayasinghe, K. Z. Stanek, C. S. Kochanek +13

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline ( yrs) light curves for sources brighter than V mag across the whole sky. As part…

astro-ph.SR2019★ 36 cited

The ASAS-SN Catalog of Variable Stars IV: Periodic Variables in the APOGEE Survey

Michal Pawlak, O. Pejcha, P. Jakubcik +12

We explore the synergy between photometric and spectroscopic surveys by searching for periodic variable stars among the targets observed by the Apache Point Observatory Galactic Ev…

astro-ph.EP2019★ 6 cited

An analysis of binary microlensing event OGLE-2015-BLG-0060

Y. Tsapras, A. Cassan, C. Ranc +83

We present the analysis of stellar binary microlensing event OGLE-2015-BLG-0060 based on observations obtained from 13 different telescopes. Intensive coverage of the anomalous par…

astro-ph.SR2019★ 12 cited

Spitzer Microlensing of MOA-2016-BLG-231L : A Counter-Rotating Brown Dwarf Binary in the Galactic Disk

Sun-Ju Chung, Andrew Gould, Jan Skowron +60

We analyze the binary microlensing event MOA-2016-BLG-231, which was observed from the ground and from Spitzer. The lens is composed of very low-mass brown dwarfs (BDs) with $M_1 =…

astro-ph.SR2019★ 3 cited

OGLE-2016-BLG-0156: Microlensing Event With Pronounced Microlens-Parallax Effects Yielding Precise Lens Mass Measurement

Youn Kil Jung, Cheongho Han, Ian A. Bond +53

We analyze the gravitational binary-lensing event OGLE-2016-BLG-0156, for which the lensing light curve displays pronounced deviations induced by microlens-parallax effects. The li…

astro-ph.HE2019★ 35 cited

Discovery and Follow-up of the Unusual Nuclear Transient OGLE17aaj

M. Gromadzki, A. Hamanowicz, L. Wyrzykowski +31

We report on the discovery and follow-up of a peculiar transient, OGLE17aaj, which occurred in the nucleus of a weakly active galaxy. We investigate whether it can be interpreted a…

astro-ph.SR2019★ 33 cited

Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye

Łukasz Wyrzykowski, P. Mróz, K. A. Rybicki +182

Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the…

astro-ph.SR2019★ 169 cited

The ASAS-SN Catalog of Variable Stars III: Variables in the Southern TESS Continuous Viewing Zone

T. Jayasinghe, K. Z. Stanek, C. S. Kochanek +13

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline ( yrs) light curves for sources brighter than V mag across the whole sky. The Tran…

astro-ph.EP2018★ 12 cited

First assessment of the binary lens OGLE-2015_BLG-0232

E. Bachelet, V. Bozza, C. Han +51

We present an analysis of the microlensing event OGLE-2015-BLG-0232. This event is challenging to characterize for two reasons. First, the light curve is not well sampled during th…

astro-ph.SR2018★ 8 cited

OGLE-2017-BLG-0039: Microlensing Event with Light from the Lens Identified from Mass Measurement

C. Han, Y. K. Jung, A. Udalski +58

We present the analysis of the caustic-crossing binary microlensing event OGLE-2017-BLG-0039. Thanks to the very long duration of the event, with an event time scale $t_{\rm E}\sim…

astro-ph.SR2018

ASAS-SN Identification of FY Sct as a detached eclipsing binary system with a ~2.6 year period

T. Jayasinghe, K. Z. Stanek, C. S. Kochanek +7

We report the identification of the bright (V mag) star FY Sct as a long period detached eclipsing binary using a combined ASAS-SN and ASAS light curve spanning 2000-20…

astro-ph.SR2018★ 195 cited

The ASAS-SN Catalog of Variable Stars II: Uniform Classification of 412,000 Known Variables

T. Jayasinghe, K. Z. Stanek, C. S. Kochanek +12

The variable stars in the VSX catalog are derived from a multitude of inhomogeneous data sources and classification tools. This inhomogeneity complicates our understanding of varia…

astro-ph.SR2018★ 8 cited

OGLE-2017-BLG-0537: Microlensing Event with a Resolvable Lens in years from High-resolution Follow-up Observations

Y. K. Jung, C. Han, A. Udalski +29

We present the analysis of the binary-lens microlensing event OGLE-2017-BLG-0537. The light curve of the event exhibits two strong caustic-crossing spikes among which the second ca…

astro-ph.GA2018★ 8.6k cited

Gaia Data Release 2. Summary of the contents and survey properties

Gaia Collaboration, A. G. A. Brown, A. Vallenari +4

We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources…

astro-ph.SR2018★ 33 cited

Microlensing Parallax for OGLE-2017-BLG-0896 Reveals a Counter-Rotating Low-Mass Brown Dwarf

Yossi Shvartzvald, Jennifer C. Yee, Jan Skowron +63

The kinematics of isolated brown dwarfs in the Galaxy, beyond the solar neighborhood, is virtually unknown. Microlensing has the potential to probe this hidden population, as it ca…