activity
20182021
most citedA low-luminosity core-collapse supernova very similar to SN 2005cs

14 citations · 30 across the 3 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.SR2018

Gaia Data Release 2: All-sky classification of high-amplitude pulsating stars

L. Rimoldini, B. Holl, M. Audard +23

More than half a million of the 1.69 billion sources in Gaia Data Release 2 (DR2) are published with photometric time series that exhibit light variations during the 22 months of o…

astro-ph.GA2018

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

Gaia Data Release 2: Validation of the classification of RR Lyrae and Cepheid variables with the Kepler and K2 missions

László Molnár, Emese Plachy, Áron L. Juhász +1

The second data release of the Gaia mission includes an advance catalog of variable stars. The classification of these stars are based on sparse photometry from the first 22 months…

astro-ph.IM2018

Gaia Data Release 2. Short-timescale variability processing and analysis

M. Roelens, L. Eyer, N. Mowlavi +13

The Gaia DR2 sample of short-timescale variable candidates results from the investigation of the first 22 months of Gaia photometry for a subsample of sources at the Gaia faint end…

astro-ph.IM2018

Gaia Data Release 2: Properties and validation of the radial velocities

D. Katz, P. Sartoretti, M. Cropper +51

For Gaia DR2 (GDR2), 280 million spectra, collected by the RVS instrument on-board Gaia, were processed and median radial velocities were derived for 9.8 million sources brighter t…

astro-ph.HE2018

Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods

J. Vinkó, A. Ordasi, T. Szalai +22

We present a comparative study of absolute distances to a sample of very nearby, bright Type Ia supernovae (SNe) derived from high cadence, high signal-to-noise, multi-band photome…