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Abstract abridged. Eclipsing binary systems provide the opportunity to measure the fundamental parameters of their component stars in a stellar-model-independent way. This makes them ideal candidates for testing and calibrating theories of…

Instrumentation and Methods for Astrophysics · Physics 2024-02-12 Luc W. IJspeert , Andrew Tkachenko , Cole Johnston , Andrej Prša , Mark A. Wells , Conny Aerts

The ExoClock project has been created with the aim of increasing the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates over an extended period, in order to…

Earth and Planetary Astrophysics · Physics 2023-02-22 A. Kokori , A. Tsiaras , B. Edwards , A. Jones , G. Pantelidou , G. Tinetti , L. Bewersdorff , A. Iliadou , Y. Jongen , G. Lekkas , A. Nastasi , E. Poultourtzidis , C. Sidiropoulos , F. Walter , A. Wünsche , R. Abraham , V. K. Agnihotri , R. Albanesi , E. Arce-Mansego , D. Arnot , M. Audejean , C. Aumasson , M. Bachschmidt , G. Baj , P. R. Barroy , A. A. Belinski , D. Bennett , P. Benni , K. Bernacki , L. Betti , A. Biagini , P. Bosch , P. Brandebourg , L. Brát , M. Bretton , S. M. Brincat , S. Brouillard , A. Bruzas , A. Bruzzone , R. A. Buckland , M. Caló , F. Campos , A. Carreno , J. -A. Carrion Rodrigo , R. Casali , G. Casalnuovo , M. Cataneo , C. -M. Chang , L. Changeat , V. Chowdhury , R. Ciantini , M. Cilluffo , J. -F. Coliac , G. Conzo , M. Correa , G. Coulon , N. Crouzet , M. V. Crow , I. Curtis , D. Daniel , S. Dawes , B. Dauchet , M. Deldem , D. Deligeorgopoulos , G. Dransfield , R. Dymock , T. Eenmäe , P. Evans , N. Esseiva , C. Falco , R. G. Farfán , E. Fernández-Lajús , S. Ferratfiat , S. L. Ferreira , A. Ferretti , J. Fiołka , M. Fowler , S. R. Futcher , D. Gabellini , T. Gainey , J. Gaitan , P. Gajdoš , A. García-Sánchez , J. Garlitz , C. Gillier , C. Gison , F. Grau Horta , G. Grivas , J. Gonzales , D. Gorshanov , P. Guerra , T. Guillot , C. A. Haswell , T. Haymes , V. -P. Hentunen , K. Hills , K. Hose , T. Humbert , F. Hurter , T. Hynek , M. Irzyk , J. Jacobsen , A. L. Jannetta , K. Johnson , P. Jóźwik-Wabik , A. E. Kaeouach , W. Kang , H. Kiiskinen , T. Kim , Ü. Kivila , B. Koch , U. Kolb , H. Kučáková , S. -P. Lai , D. Laloum , S. Lasota , L. A. Lewis , G. -I. Liakos , F. Libotte , C. Lopresti , F. Lomoz , R. Majewski , A. Malcher , M. Mallonn , M. Mannucci , A. Marchini , J. -M. Mari , A. Marino , G. Marino , J. -C. Mario , J. -B. Marquette , F. A. Martínez-Bravo , M. Mašek , P. Matassa , P. Michel , J. Michelet , M. Miller , E. Miny , T. Mollier , D. Molina , B. Monteleone , N. Montigiani , M. Morales-Aimar , F. Mortari , M. Morvan , L. V. Mugnai , G. Murawski , L. Naponiello , R. Naves , J. -L. Naudin , D. Néel , R. Neito , S. Neveu , A. Noschese , Y. Öğmen , O. Ohshima , Z. Orbanic , E. P. Pace , C. Pantacchini , N. I. Paschalis , C. Pereira , I. Peretto , V. Perroud , M. Phillips , P. Pintr , J. -B. Pioppa , J. Plazas , A. J. Poelarends , A. Popowicz , J. Purcell , N. Quinn , M. Raetz , D. Rees , F. Regembal , M. Rocchetto , P. -F. Rocci , M. Rockenbauer , R. Roth , L. Rousselot , X. Rubia , N. Ruocco , E. Russo , M. Salisbury , F. Salvaggio , A. Santos , J. Savage , F. Scaggiante , D. Sedita , S. Shadick , A. F. Silva , N. Sioulas , V. Školník , M. Smith , M. Smolka , A. Solmaz , N. Stanbury , D. Stouraitis , T. -G. Tan , M. Theusner , G. Thurston , F. -P. Tifner , A. Tomacelli , A. Tomatis , J. Trnka , M. Tylšar , P. Valeau , J. -P. Vignes , A. Villa , A. Vives Sureda , K. Vora , M. Vrašťák , D. Walliang , B. Wenzel , D. E. Wright , R. Zambelli , M. Zhang , M. Zíbar

One challenge in strong gravitational lensing cosmography is the measurement of time delays between multiple lensed images, which are essential for constraining the Hubble constant (\(H_0\)). In this study, we investigate how assumptions…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-20 Guanhua Rui , Bin Hu , Wei Du

Scale invariance is expected in empty Universe models, while the presence of matter tends to suppress it. As shown recently, scale invariance is certainly absent in cosmological models with densities equal to or above the critical value…

Earth and Planetary Astrophysics · Physics 2022-11-24 Andre Maeder , Vesselin Gueorguiev

As space exploration extends into cislunar space and further towards Mars, understanding the relativistic effects on clocks on Mars, particularly in relation to multibody gravitational influences, becomes increasingly important for accurate…

General Relativity and Quantum Cosmology · Physics 2025-09-17 Neil Ashby , Bijunath R. Patla

Despite the ever-growing number of exoplanets discovered and the extensive analyses carried out to find their potential satellites, only two exomoon candidates, Kepler-1625b-i and Kepler-1708 b-i, have been discovered to date. A…

Earth and Planetary Astrophysics · Physics 2023-11-09 Sz. Kálmán , Sz. Csizmadia , A. E. Simon , K. W. F. Lam , A. Deline , J. -V. Harre , Gy. M. Szabó

Time-delay strong lensing provides a unique way to directly measure the Hubble constant ($H_{0}$). The precision of the $H_{0}$ measurement depends on the uncertainties in the time-delay measurements, the mass distribution of the main…

Using observations of pulsars from the Parkes Pulsar Timing Array (PPTA) project we develop the first pulsar-based timescale that has a precision comparable to the uncertainties in international atomic timescales. Our ensemble of pulsars…

Terrestrial timescales show instabilities due to the physical limitations of the atomic clocks. Stricter environmental isolation and increased numbers of improved cesium clocks and cavity-tuned hydrogen masers have resulted in time scales…

Astrophysics · Physics 2007-05-23 Demetrios N. Matsakis , Roger S. Foster

In the last decade, over 7000 eclipsing binaries have been discovered in the Local Group through various variability surveys. Measuring fundamental parameters of these eclipsing binaries has become feasible with 8 meter class telescopes,…

Astrophysics · Physics 2009-02-18 A. Z. Bonanos

The ExoClock project is an open platform aiming to monitor exoplanets by integrating observations from space and ground based telescopes. This study presents an updated catalogue of 620 exoplanet ephemerides, integrating 30000 measurements…

Earth and Planetary Astrophysics · Physics 2025-11-19 A. Kokori , A. Tsiaras , G. Pantelidou , A. Jones , A. Siakas , B. Edwards , G. Tinetti , A. Wünsche , Y. Jongen , F. Libotte , M. Correa , L. V. Mugnai , A. Bocchieri , A. R. Capildeo , E. Poultourtzidis , C. Sidiropoulos , L. Bewersdorff , G. Lekkas , G. Grivas , R. A. Buckland , S. R. -L. Futcher , P. Matassa , J. -P. Vignes , A. O. Kovacs , M. Raetz , B. E. Martin , A. Popowicz , D. Gakis , P. Batsela , V. Michalaki , A. Nastasi , C. Pereira , A. Iliadou , F. Walter , N. I. Paschalis , K. Vats , N. A-thano , R. Abraham , V. K. Agnihotri , M. Á. Álava-Amat , R. Albanesi , T. Alderweireldt , J. Alonso-Santiago , D. Q. Amat , L. Andrade , V. Anzallo , J. Aragones , E. Arce-Mansego , D. Arnot , R. A. Artola , C. Aumasson , M. Bachschmidt , R. Barberá-Córdoba , J. -F. Barrois , P. R. Barroy , M. Bastoni , V. Béjar , A. A. Belinski , A. Ben Lassoued , P. Bendjoya , B. Benei , D. Bennett , K. Bernacki , G. O. Bernard , L. Betti , G. Biesse , M. Billiani , P. Bosch-Cabot , V. Boucher , R. C. Boufleur , D. Boulakos , P. J. -M. Brandebourg , S. M. Brincat , X. Bros , A. Brosio , S. Brouillard , A. -M. Bruzzone , L. Cabona , C. Calamai , G. Calapai , Y. Calatayud-Borràs , M. Caló , F. Campos , A. Carbognani , F. Carretero , R. Casas , M. L. Castanheira , G. Catanzaro , L. Cavaglioni , C. -M. Chang , M. Chella , W. -H. Chen , P. -J. Chiu , R. Ciantini , J. -F. Coliac , J. Collins , F. Conti , G. Conzo , W. R. Cooney, , L. N. Correa , S. P. Cosentino , N. Crouzet , M. V. Crow , B. V. -H. -V. da-Silva , A. Damonte , D. Daniel , S. Dawes , L. de Almeida , P. De Backer , A. de Melo , M. Deldem , D. Deligeorgopoulos , Y. Delisle , F. Denjean , F. Dias , S. Diaz Lopez , T. Dittadi , N. Dodd , S. Doman , G. Domènech-Rams , T. G. Dooley , S. Drapkin-Junyent , F. Dubois , A. Dustor , R. Dymock , T. Eenmäe , M. Emilio , E. Esparza-Borges , J. Estevez , C. Falco , R. G. Farfán , P. Farissier , G. Farrall , G. Fernandez Rodriguez , A. Ferretti , G. Ferrini , L. Fini , J. Fiołka , G. Fleerackers , J. Flores-Martín , g. follero , S. Foschino , L. Fossi , M. Fowler , A. Frasca , E. Frigeni , I. Fukuda , A. Fukui , G. Furlato , D. Gabellini , T. Gainey , P. Gajdoš , D. Galán-Diéguez , P. Gamache , E. García Navarro , N. A. Garcia , A. García-Sánchez , A. Garmash , T. Gesser , A. Ginard , I. Gkolias , E. Gomez , G. F. Gonçalves , J. González-Edo , J. González-Rodríguez , G. Gruntz , B. Guillet , T. Guillot , M. N. Günther , H. Hautecler , Y. Hayashi , E. Herrero , K. Hills , H. S. Hodkinson , G. Holtkamp , G. R. Hunt , N. Iannascoli , M. Iozzi , M. Irzyk , K. Isogai , K. Johnson , P. Jóźwik-Wabik , A. E. Kaeouach , S. Kartal , H. Kiiskinen , Ü. Kivila , U. Kolb , J. Korth , D. Kustrin , S. -P. Lai , S. Lasota , F. Le Rhun , Y. H. Lee , D. Lefoulon , F. Legrele , H. Leipold , A. Liberti , T. Lien , Y. -H. Lin , F. Linsalata , J. H. Livingston , C. Lopresti , S. Lora , E. R. Lorenz , D. Madison , M. Mannucci , A. Marchini , A. Marino , J. -C. Mario , E. Maris , J. -B. Marquette , N. A. Maslennikova , A. E. McGregor , A. Mengoudis , P. Meni , M. Mesarč , M. Michelagnoli , J. Michelet , J. Mieglitz , M. Mifsud , M. Miller , S. A. Mills , E. Miny , S. Miquel Romero , D. Molina , S. Montchaud , B. Monteleone , M. Monticelli , N. Montigiani , M. Morales-Aimar , G. Morello , L. Moretti , M. Mori , F. Mortari , M. Müller , D. Mura , F. Murgas , N. Narita , A. Nath , R. Nicollerat , V. Noce , P. Norridge , A. J. Norton , Y. Ogmen , Z. Orbanic , J. Owen-Lloyd-Walters , E. P. Pace , E. Pakštienė , A. F. Pala , E. Palle , C. Pantacchini , I. Parenti , D. Patterson , E. Pavoni , A. W. Pereira , I. Peretto , V. Perroud , S. W. Peterson , V. Pettina , M. Phillips , J. Philpot , D. Pica , P. Pintr , J. -B. Pioppa , T. J. Plunkett , T. G. Prado , A. Prasad , R. A. Prestes , A. Putz , F. Régembal , L. Ribe , D. F. Rocha , J. Rodrigues , R. Roth , L. Rousselot , N. Rozand , X. Rubia , N. Ruocco , M. Salisbury , T. Salomon , L. Sassaro , J. E. -G. Savage , T. Savin , F. Scaggiante , F. -X. Schmider , M. Serrau , I. D. Sharp , D. Shave-Wall , A. F. Silva , V. Školník , A. Solmaz , A. Sonka , M. Spiller , T. H. Sprecher , R. Stanga , M. Stefanini , D. Stouraitis , M. Stratigou-Psarra , O. Suarez , D. Suys , M. Szkudlarek , M. F. Talafha , A. N. Tarasenkov , G. Tartalo-Montardit , C. Titescu , A. Tomacelli , A. H. Triaud , S. Tsavdaridis , K. Tsiganis , M. A. van der Grijp , S. Vanaverbeke , j. -p. vergne , J. Verheyden , J. Vilalta , P. Vuylsteke , P. Wagner , D. Walliang , C. H. Wang , I. Weller , D. E. Wright , K. O. Xenos , R. Yorke , O. Zamora , J. Zapata , M. Zejmo , M. Zulian

The error pattern correcting code (EPCC) can be constructed to provide a syndrome decoding table targeting the dominant error events of an inter-symbol interference channel at the output of the Viterbi detector. For the size of the syndrome…

Information Theory · Computer Science 2010-03-31 Hakim Alhussien , Jaekyun Moon

The ICARUS T600 LAr TPC is the far detector of the Short Baseline Program at FNAL. As it will have to work at shallow depth in the Booster Neutrino Beam, a large cosmic rays background ($\sim 11$ kHz) will be present. To reduce it, precise…

Instrumentation and Detectors · Physics 2020-06-24 M. Bonesini , R. Benocci , R. Bertoni , A. Falcone , R. Mazza , M. Torti , A. Menegolli , G. L. Raselli , M. Rossella

We have developed a new laser-based time calibration system for highly segmented scintillator counters like the MEG II pixelated Timing Counter (pTC), consisting of 512-centimeter scale scintillator counters read out by silicon…

This work investigates the use of stellar occultation measurements to enhance the orbit determination performance of the Lunar Meteoroid Impact Observer (LUMIO) mission, operating from a quasi-Halo orbit around the Earth-Moon L2 point.…

Earth and Planetary Astrophysics · Physics 2025-09-05 Davide Banzi , Riccardo Lasagni Manghi , Marco Zannoni

Context. Among options for definition of the lunar reference time, the option taking Lunar Coordinate Time (O1) has its simplicity but cannot be realized by any clock without steering, while another option adopting the lunar geoid…

Instrumentation and Methods for Astrophysics · Physics 2026-04-08 Tian-Ning Yang , Ren-Fang Geng , Jing Zhang , Chong Yang , Yong Huang , Yi Xie

Optical clock network requires the establishment of optical frequency transmission link between multiple optical clocks, utilizing narrow linewidth lasers. Despite achieving link noise levels of 10${^{-20}}$, the final accuracy is limited…

Irregularly sampled time series forecasting, characterized by non-uniform intervals, is prevalent in practical applications. However, previous research have been focused on regular time series forecasting, typically relying on transformer…

Machine Learning · Computer Science 2024-10-01 Byunghyun Kim , Jae-Gil Lee

Analysis of transit times in exoplanetary systems accurately provides an instantaneous orbital period, $P(t)$, of their member planets. A long-term monitoring of those transiting planetary systems puts limits on the variability of $P(t)$,…

General Relativity and Quantum Cosmology · Physics 2016-03-21 Kento Masuda , Yasushi Suto

Lunar Laser Ranging (LLR) measurements are crucial for advanced exploration of the evolutionary history of the lunar orbit, the laws of fundamental gravitational physics, selenophysics and geophysics as well as for future human missions to…

General Relativity and Quantum Cosmology · Physics 2009-02-23 Sergei Kopeikin