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most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

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184 papers · 1 filter

astro-ph2008★ 8 cited

Modelling solar-like variability for the detection of Earth-like planetary transits. II) Performance of the three-spot modelling, harmonic function fitting, iterative non-linear filtering and sliding boxcar filtering

A. S. Bonomo, S. Aigrain, P. Bordé +1

We present a comparison of four methods of filtering solar-like variability to increase the efficiency of detection of Earth-like planetary transits by means of box-shaped transit…

astro-ph2008★ 45 cited

The WEBT Campaign on the Intermediate BL Lac Object 3C66A in 2007-2008

M. Boettcher, K. Fultz

Prompted by a high optical state in September 2007, the Whole Earth Blazar Telescope (WEBT) consortium organized an intensive optical, near-IR (JHK) and radio observing campaign on…

astro-ph2008★ 18 cited

Magnetic activity in the photosphere of CoRoT-Exo-2a. Active longitudes and short-term spot cycle in a young Sun-like star

A. F. Lanza, I. Pagano, G. Leto +18

The space experiment CoRoT has recently detected transits by a hot Jupiter across the disc of an active G7V star (CoRoT-Exo-2a) that can be considered as a good proxy for the Sun a…

astro-ph2008★ 21 cited

Science with the World Space Observatory - Ultraviolet

Ana I. Gomez de Castro, Isabella Pagano, Mikhail Sachkov +4

The World Space Observatory-Ultraviolet (WSO-UV) will provide access to the UV range during the next decade. The instrumentation on board will allow to carry out high resolution im…

astro-ph2008★ 136 cited

Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007

V. M. Larionov, S. G. Jorstad, A. P. Marscher +2

We present radio-to-optical data taken by the WEBT, supplemented by VLBA and RXTE observations, of 3C 279. Our goal is to use this extensive database to draw inferences regarding t…

astro-ph2008★ 1 cited

Multiline Zeeman signatures as demonstrated through the Pseudo-line

M. Semel, J. C. Ramirez Velez, M. J. Stift +3

In order to get a significant Zeeman signature in the polarised spectra of a magnetic star, we usually 'add' the contributions of numerous spectral lines; the ultimate goal is to r…

astro-ph2008★ 32 cited

HINODE Observations of Chromospheric Brightenings in the Ca II H Line during small-scale Flux Emergence Events

S. L. Guglielmino, F. Zuccarello, P. Romano +1

\ion{Ca}{2} H emission is a well-known indicator of magnetic activity in the Sun and other stars. It is also viewed as an important signature of chromospheric heating. However, the…

astro-ph2008★ 101 cited

A new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008

C. M. Raiteri, M. Villata, V. M. Larionov +2

We present and analyse the WEBT multifrequency observations of 3C 454.3 in the 2007-2008 observing season, including XMM-Newton observations and near-IR spectroscopic monitoring, a…

astro-ph2008★ 4 cited

CCD and photon-counting photometric observations of asteroids carried out at Padova and Catania observatories

Davide Gandolfi, Massimo Cigna, Daniele Fulvio +1

We present the results of observational campaigns of asteroids performed at Asiago Station of Padova Astronomical Observatory and at M.G. Fracastoro Station of Catania Astrophysica…

astro-ph2008★ 79 cited

X-ray emission from dense plasma in CTTSs: Hydrodynamic modeling of the accretion shock

G. G. Sacco, C. Argiroffi, S. Orlando +3

High spectral resolution X-ray observations of CTTSs demonstrate the presence of plasma at T~2-3X10^6 K and n_e~10^11-10^13 cm^-3, unobserved in non-accreting stars. Stationary mod…

astro-ph2008★ 39 cited

Eleven years of radio monitoring of the Type IIn supernova SN 1995N

Poonam Chandra, Christopher J. Stockdale, Roger A. Chevalier +6

We present radio observations of the optically bright Type IIn supernova SN 1995N. We observed the SN at radio wavelengths with the Very Large Array (VLA) for 11 years. We also obs…

astro-ph2008★ 225 cited

A time - luminosity correlation for Gamma Ray Bursts in the X - rays

M. G. Dainotti, V. F. Cardone, S. Capozziello

Gamma ray bursts (GRBs) have recently attracted much attention as a possible way to extend the Hubble diagram to very high redshift. However, the large scatter in their intrinsic p…

astro-ph2008

CoRoT and stellar activity: preliminary results from the modelling of CoRoT-Exo-2a

A. F. Lanza, I. Pagano, G. Leto +3

We present a preliminary analysis of the photospheric activity of CoRoT-Exo-2a, a young G7V star accompanied by a transiting hot Jupiter recently discovered by CoRoT. We apply spot…

astro-ph2008★ 158 cited

A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

Torben Arentoft, Hans Kjeldsen, Timothy R. Bedding +45

We have carried out a multi-site campaign to measure oscillations in the F5 star Procyon A. We obtained high-precision velocity observations over more than three weeks with eleven…

astro-ph2008★ 9 cited

New triple systems in the RasTyc sample of stellar X-ray sources

A. Klutsch, A. Frasca, P. Guillout +4

During the study of a large set of late-type stellar X-ray sources, we discovered a large fraction of multiple systems. In this paper we investigate the orbital elements and kinema…

astro-ph2008★ 95 cited

Transiting exoplanets from the CoRoT space mission IV: CoRoT-Exo-4b: A transiting planet in a 9.2 day synchronous orbit

S. Aigrain, A. Collier Cameron, M. Ollivier +32

CoRoT, the first space-based transit search, provides ultra-high precision light curves with continuous time-sampling over periods, of up to 5 months. This allows the detection of…

astro-ph2008★ 19 cited

Radio continuum properties of young planetary nebulae

L. Cerrigone, G. Umana, C. Trigilio +3

We have selected a small sample of post-AGB stars in transition towards the planetary nebula and present new Very Large Array multi-frequency high-angular resolution radio observat…

astro-ph2008★ 258 cited

The metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae

Paolo A. Mazzali, Stefano Valenti, Massimo Della Valle +38

The only supernovae (SNe) to have shown early gamma-ray or X-ray emission thus far are overenergetic, broad-lined Type Ic SNe (Hypernovae - HNe). Recently, SN 2008D shows several n…

astro-ph2008

Magnetic activity in the young star SAO 51891

K. Biazzo, A. Frasca, E. Marilli +3

We present preliminary results on a study based on contemporaneous photometric and spectroscopic observations of the young K0-1V star SAO 51891. We find that SAO 51891, a possible…

astro-ph2008★ 83 cited

The star formation in the L1615/L1616 cometary cloud

Davide Gandolfi, Juan M. Alcalá, Silvio Leccia +6

The present work aims at performing a comprehensive census and characterisation of the pre-main sequence (PMS) population in the cometary cloud L1615/L1616, in order to assess the…

astro-ph2008★ 107 cited

Solar twins in M67

L. Pasquini, K. Biazzo, P. Bonifacio +2

The discovery of true solar analogues is fundamental for a better understanding of the Sun and of the solar system. The open cluster M67 offers a unique opportunity to search for s…

astro-ph2008★ 58 cited

AGN Jet-induced Feedback in Galaxies. I. Suppression of Star Formation

V. Antonuccio-Delogu, J. Silk

(Abridged) We study the interaction of relativistic jets from AGNs with the ISM in their host galaxy, using a series of Adaptive Mesh Refinement simulations of the evolution of the…

astro-ph2008★ 6 cited

The gas turbulence in planetary nebulae: quantification and multi-D maps from long-slit, wide-spectral range echellogram

F. Sabbadin, M. Turatto, S. Benetti +2

This methodological paper is part of a short series dedicated to the long-standing astronomical problem of de-projecting the bi-dimensional, apparent morphology of a three-dimensio…

astro-ph2008

Comparing the performance of stellar variability filters for the detection of planetary transits

A. S. Bonomo, A. F. Lanza

We have developed a new method to improve the transit detection of Earth-sized planets in front of solar-like stars by fitting stellar microvariability by means of a spot model. A…