Pregled bibliografske jedinice broj: 998574
Short time-scale variables in the Gaia era: detection and characterization by structure function analysis
Short time-scale variables in the Gaia era: detection and characterization by structure function analysis // Monthly notices of the Royal Astronomical Society, 472 (2017), 3; 3230-3245 doi:10.1093/mnras/stx2115 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 998574 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Short time-scale variables in the Gaia era:
detection and characterization by structure
function analysis
Autori
Roelens, Maroussia ; Eyer, Laurent ; Mowlavi, Nami ; Lecoeur-Taïbi, Isabelle ; Rimoldini, Lorenzo ; Blanco-Cuaresma, Sergi ; Palaversa, Lovro ; Süveges, Maria ; Charnas, Jonathan ; Wevers, Thomas
Kolaboracija
Gaia Collaboration
Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 472
(2017), 3;
3230-3245
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
methods: data analysis ; methods: numerical ; techniques: photometric ; surveys ; stars ; variables: general
Sažetak
We investigate the capabilities of the ESA Gaia mission for detecting and characterizing short time-scale variability, from tens of seconds to a dozen hours. We assess the efficiency of the variogram analysis, for both detecting short time-scale variability and estimating the underlying characteristic time-scales from Gaia photometry, through extensive light-curve simulations for various periodic and transient short time-scale variable types. We show that, with this approach, we can detect fast periodic variability, with amplitudes down to a few millimagnitudes, as well as some M dwarf flares and supernovae explosions, with limited contamination from longer time-scale variables or constant sources. Time-scale estimates from the variogram give valuable information on the rapidity of the underlying variation, which could complement time-scale estimates from other methods, like Fourier-based periodograms, and be reinvested in preparation of ground- based photometric follow-up of short time-scale candidates evidenced by Gaia. The next step will be to find new short time-scale variable candidates from real Gaia data, and to further characterize them using all the Gaia information, including colour and spectrum.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus