activity
19982026
most citedVISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

1k citations · 17.6k across the 313 of their papers we have counts for

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16 papers · 1 filter

astro-ph.CO2023★ 22 cited

Modeling photometric reverberation mapping data for the next generation of big data surveys. Quasar accretion disks sizes with the LSST

F. Pozo Nuñez, C. Bruckmann, S. Desamutara +5

Photometric reverberation mapping can detect the radial extent of the accretion disc (AD) in Active Galactic Nuclei by measuring the time delays between light curves observed in di…

astro-ph.CO2013★ 235 cited

The Araucaria Project. The distance to the Small Magellanic Cloud from late-type eclipsing binaries

Dariusz Graczyk, Grzegorz Pietrzynski, Ian B. Thompson +12

We present a distance determination to the Small Magellanic Cloud (SMC) based on an analysis of four detached, long period, late type eclipsing binaries discovered by the OGLE Surv…

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.CO2013★ 56 cited

The Araucaria Project. A Distance Determination to the Local Group Spiral M33 from Near-Infrared Photometry of Cepheid Variables

W. Gieren, M. Gorski, G. Pietrzynski +10

Motivated by an amazing range of reported distances to the nearby Local Group spiral galaxy M33, we have obtained deep near-infrared photometry for 26 long-period Cepheids in this…

astro-ph.CO2012★ 4 cited

Cepheid distances from the Baade-Wesselink method

Wolfgang Gieren, Jesper Storm, Nicolas Nardetto +5

Recent progress on Baade-Wesselink (BW)-type techniques to determine the distances to classical Cepheids is reviewed. Particular emphasis is placed on the near-infrared surface-bri…

astro-ph.CO2012★ 33 cited

The araucaria project. An accurate distance to the late-type double-lined eclipsing binary ogle smc113.3 4007 in the small magellanic cloud

Dariusz Graczyk, Grzegorz Pietrzynski, Ian B. Thompson +13

We have analyzed the long period, double-lined eclipsing binary system OGLE SMC113.3 4007 (SC10 137844) in the SMC. The binary lies in the north-eastern part of the galaxy and cons…

astro-ph.CO2011★ 116 cited

Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance

R. -P. Kudritzki, M. A. Urbaneja, Z. Gazak +4

The quantitative spectral analysis of low resolution Keck LRIS spectra of blue supergiants in the disk of the giant spiral galaxy M81 is used to determine stellar effective tempera…

astro-ph.CO2011★ 20 cited

The Baade-Wesselink p-factor applicable to LMC Cepheids

N. Nardetto, A. Fokin, P. Fouqué +5

Context. Recent observations of LMC Cepheids bring new constraints on the slope of the period-projection factor relation (hereafter Pp relation) that is currently used in the Baade…

astro-ph.CO2011★ 166 cited

Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique I. The p-factor, the Milky Way relations, and a universal K-band relation

J. Storm, W. Gieren, P. Fouque +6

We determine Period-Luminosity relations for Milky Way Cepheids in the optical and near-IR bands. These relations can be used directly as reference for extra-galactic distance dete…

astro-ph.CO2011★ 104 cited

Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMC

J. Storm, W. Gieren, P. Fouque +5

The extragalactic distance scale builds directly on the Cepheid Period-Luminosity (PL) relation as delineated by the sample of Cepheids in the Large Magellanic Cloud (LMC). However…

astro-ph.CO2011★ 40 cited

The Magellanic Quasars Survey. II. Confirmation of 144 New Active Galactic Nuclei Behind the Southern Edge of the Large Magellanic Cloud

Szymon Kozlowski, C. S. Kochanek, A. M. Jacyszyn +9

We quadruple the number of quasars known behind the Large Magellanic Cloud (LMC) from 55 (42 in the LMC fields of the third phase of the Optical Gravitational Lensing Experiment (O…

astro-ph.CO2011★ 28 cited

The Araucaria Project. Infrared Tip of the Red Giant Branch Distances to Five Dwarf Galaxies in the Local Group

Marek Gorski, Grzegorz Pietrzynski, Wolfgang Gieren

We have obtained accurate near-infrared photometry of the Tip of the Red Giant Branches in the Local Group galaxies Sculptor, NGC 6822, NGC 3109, IC 1613 and WLM. We have used the…

astro-ph.CO2009★ 83 cited

Pushing the Boundaries of Conventional Core-Collapse Supernovae: The Extremely Energetic Supernova SN 2003ma

A. Rest, R. J. Foley, S. Gezari +34

We report the discovery of a supernova (SN) with the highest apparent energy output to date and conclude that it represents an extreme example of the Type IIn subclass. The SN, whi…

astro-ph.CO2009★ 71 cited

The Araucaria Project. The Distance to the Small Magellanic Cloud from Near-Infrared Photometry of RR Lyrae Variables

Olaf Szewczyk, Grzegorz Pietrzynski, Wolfgang Gieren +3

We have obtained deep infrared J and K band observations of nine 4.9x4.9 arcmin fields in the Small Magellanic Cloud (SMC) with the ESO New Technology Telescope equipped with the S…

astro-ph.CO2009★ 365 cited

Quantifying Quasar Variability As Part of a General Approach To Classifying Continuously Varying Sources

Szymon Kozlowski, Christopher S. Kochanek, A. Udalski +8

Robust fast methods to classify variable light curves in large sky surveys are becoming increasingly important. While it is relatively straightforward to identify common periodic s…

astro-ph.CO2009★ 82 cited

The Araucaria Project. Determination of the LMC Distance from Late-Type Eclipsing Binary Systems: I. OGLE-051019.64-685812.3

G. Pietrzynski, I. Thompson, D. Graczyk +7

We have analyzed the double-lined eclipsing binary system OGLE-051019.64-685812.3 in the LMC which consists of two G4 giant components with very similar effective temperatures. A d…