IAUC 5901 available at Central Bureau for Astronomical Telegrams.
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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GRO J0422+32Zhao, P. et al.121993
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GRO J0422+32
IAUC 5907 available at Central Bureau for Astronomical Telegrams.
Zhao, P. et al.Advertised on:
121993 -
Ground-Based Detection of Terrestrial-Sized Extrasolar Planets Around Small Eclipsing Binary Systems
We have photometrically searched the circumstellar habitable zone (about 95 eclipsing binary system CM Draconis for evidence of planetary transits. With 1014 hours of imaging data we have reached a detection limit of about 2.3 Earth radii (less than 1 60 days or less, marginally demonstrating that the ground-based detection of large terrestrial
Doyle, L. R. et al.Advertised on:
122000 -
Ground-based follow-up in relation to Kepler asteroseismic investigation
The Kepler space mission, successfully launched in March 2009, is providing continuous and high-precision photometry of thousands of stars simultaneously. The uninterrupted time-series of stars of all known pulsation types are a precious source for asteroseismic studies. The Kepler data do not provide information on the physical parameters, such as
Uytterhoeven, K. et al.Advertised on:
122010 -
Ground-based multi-color photometry of the γ Doradus-δ Scuti hybrid star KIC 6761539
We present a preliminary analysis of the first three nights of multi-color photometric data for a γ Doradus-δ Scuti hybrid star (KIC 6761539) that is also being observed with the Kepler space telescope. We find that up to four (depending on the filter) of the highest amplitude modes, whose frequencies could be determined from Kepler data, are
Roth, M. et al.Advertised on:
122012 -
GT2318+620 - a Galactic Low-Mass X-Ray Binary or a Radio Loud AGN?
GT2318+620 is a variable radio source exhibiting a jet-like feature on both sides of an unresolved core (Taylor et al., Nature 351, 1991), and it is possibly associated with an UHURU X-ray source. A red 20th magnitude star coincident with the radio core was identified as the optical counterpart. Based on a neutral hydrogen absorption spectrum and
Muhli, P. et al.Advertised on:
121998