A Scientific Workflow System for Satellite Data Processing with Real-Time Monitoring. (arXiv:1812.02236v1 [astro-ph.IM])

A Scientific Workflow System for Satellite Data Processing with Real-Time Monitoring. (arXiv:1812.02236v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Nguyen_M/0/1/0/all/0/1">Minh Duc Nguyen</a> (1) ((1) Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics) This paper provides a case study on satellite data processing, storage, and distribution in the space weather domain by introducing the Satellite Data Downloading System (SDDS). The […]

Monitoring activities of satellite data processing services in real-time with SDDS Live Monitor. (arXiv:1812.02239v1 [astro-ph.IM])

Monitoring activities of satellite data processing services in real-time with SDDS Live Monitor. (arXiv:1812.02239v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Nguyen_M/0/1/0/all/0/1">Minh Duc Nguyen</a> (1) ((1) Lomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics) This work describes Live Monitor, the monitoring subsystem of SDDS – an automated system for space experiment data processing, storage, and distribution created at SINP […]

A Galactic Plane Defined by the Milky Way HII Region Distribution. (arXiv:1812.02244v1 [astro-ph.GA])

A Galactic Plane Defined by the Milky Way HII Region Distribution. (arXiv:1812.02244v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Anderson_L/0/1/0/all/0/1">L. D. Anderson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wenger_T/0/1/0/all/0/1">Trey V. Wenger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Armentrout_W/0/1/0/all/0/1">W. P. Armentrout</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Balser_D/0/1/0/all/0/1">Dana S. Balser</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bania_T/0/1/0/all/0/1">T. M. Bania</a> We develop a framework for a new definition of the Galactic midplane, allowing for tilt (rotation about Galactic azimuth 90deg.), and roll […]

Atmospheric Charm, QCD and Neutrino Astronomy. (arXiv:1812.02248v1 [hep-ph])

Atmospheric Charm, QCD and Neutrino Astronomy. (arXiv:1812.02248v1 [hep-ph]) <a href="http://arxiv.org/find/hep-ph/1/au:+Benzke_M/0/1/0/all/0/1">Michael Benzke</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Garzelli_M/0/1/0/all/0/1">Maria V. Garzelli</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kniehl_B/0/1/0/all/0/1">Bernd A. Kniehl</a> We present predictions for the prompt-neutrino flux arising from the decay of charmed mesons and baryons produced by the interactions of high-energy cosmic rays in the Earth’s atmosphere, making use of a QCD approach on the […]

The Draco Constellation

The Draco Constellation Located in the northern hemisphere, between the two “dippers”, is the Draco constellation – one of the 48 compiled by Ptolemy and one of the 88 recognized by the IAU. The post The Draco Constellation appeared first on Universe Today. Universe Today Go to Source

InSight’s Robot Arm is Ready to go to Work

InSight’s Robot Arm is Ready to go to Work Some new images sent home by the InSight Lander show the robotic arm and the craft’s instruments waiting on deck, on the surface of Mars. The lander is still having its systems tested, and isn’t quite ready to get to work. It’ll use its arm to […]

The Breakthrough Listen Search for Intelligent Life: No Evidence of Claimed Periodic Spectral Modulations in High Resolution Optical Spectra of Nearby Stars. (arXiv:1812.02258v1 [astro-ph.SR])

The Breakthrough Listen Search for Intelligent Life: No Evidence of Claimed Periodic Spectral Modulations in High Resolution Optical Spectra of Nearby Stars. (arXiv:1812.02258v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Isaacson_H/0/1/0/all/0/1">Howard Isaacson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Siemion_A/0/1/0/all/0/1">Andrew P. V. Siemion</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Marcy_G/0/1/0/all/0/1">Geoffrey W. Marcy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hickish_J/0/1/0/all/0/1">Jack Hickish</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Price_D/0/1/0/all/0/1">Danny C. Price</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Enriquez_J/0/1/0/all/0/1">J. Emilio Enriquez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gizani_N/0/1/0/all/0/1">Nectaria Gizani</a> We report on high-resolution spectra […]

Fast Switch and Spline Scheme for Accurate Inversion of Nonlinear Functions: The New First Choice Solution to Kepler’s Equation. (arXiv:1812.02273v1 [physics.comp-ph])

Fast Switch and Spline Scheme for Accurate Inversion of Nonlinear Functions: The New First Choice Solution to Kepler’s Equation. (arXiv:1812.02273v1 [physics.comp-ph]) <a href="http://arxiv.org/find/physics/1/au:+Tommasini_D/0/1/0/all/0/1">Daniele Tommasini</a>, <a href="http://arxiv.org/find/physics/1/au:+Olivieri_D/0/1/0/all/0/1">David N. Olivieri</a> Numerically obtaining the inverse of a function is a common task for many scientific problems, often solved using a Newton iteration method. Here we describe an alternative […]

How Many Hydrated NEOs Are There?. (arXiv:1812.02285v1 [astro-ph.EP])

How Many Hydrated NEOs Are There?. (arXiv:1812.02285v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Rivkin_A/0/1/0/all/0/1">Andrew S. Rivkin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+DeMeo_F/0/1/0/all/0/1">Francesca E. DeMeo</a> Hydrated minerals are tracers of early solar system history, and have been proposed as a possible focus for economic activity in space. Near-Earth objects (NEOs) are important to both of these, especially the most accessible members of that community. […]

Solar Neutrino Measurements. (arXiv:1812.02326v1 [nucl-ex])

Solar Neutrino Measurements. (arXiv:1812.02326v1 [nucl-ex]) <a href="http://arxiv.org/find/nucl-ex/1/au:+Pocar_A/0/1/0/all/0/1">Andrea Pocar</a> We present the most recent results from the two currently running solar neutrino experiments, Borexino at the Gran Sasso laboratory in Italy and SuperK at Kamioka mine in Japan. SuperK has released the most precise yet measurement of the 8B solar neutrino interaction rate, with a precision […]

Null test for interactions in the dark sector. (arXiv:1812.02333v1 [astro-ph.CO])

Null test for interactions in the dark sector. (arXiv:1812.02333v1 [astro-ph.CO]) <a href="http://arxiv.org/find/astro-ph/1/au:+Marttens_R/0/1/0/all/0/1">Rodrigo von Marttens</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Marra_V/0/1/0/all/0/1">Valerio Marra</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Casarini_L/0/1/0/all/0/1">Luciano Casarini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gonzalez_J/0/1/0/all/0/1">J. E. Gonzalez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Alcaniz_J/0/1/0/all/0/1">Jailson Alcaniz</a> Since there is no known symmetry in Nature that prevents a non-minimal coupling between the dark energy (DE) and cold dark matter (CDM) components, such a possibility constitutes […]

GMRT Archive Processing Project. (arXiv:1812.02358v1 [astro-ph.IM])

GMRT Archive Processing Project. (arXiv:1812.02358v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Deshpande_S/0/1/0/all/0/1">Shubhankar Deshpande</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wadadekar_Y/0/1/0/all/0/1">Yogesh Wadadekar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Intema_H/0/1/0/all/0/1">Huib Intema</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ratnakumar_B/0/1/0/all/0/1">B. Ratnakumar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+George_L/0/1/0/all/0/1">Lijo George</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Desai_R/0/1/0/all/0/1">Rathin Desai</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sakhadeo_A/0/1/0/all/0/1">Archit Sakhadeo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shaikh_S/0/1/0/all/0/1">Shadab Shaikh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ishwara_Chandra_C/0/1/0/all/0/1">C. H. Ishwara-Chandra</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Oberoi_D/0/1/0/all/0/1">Divya Oberoi</a> The GMRT Online Archive now houses over 120 terabytes of interferometric observations obtained with the GMRT since the […]

Gaia-DR2 confirms VLBA parallaxes in Ophiuchus, Serpens and Aquila. (arXiv:1812.02360v1 [astro-ph.SR])

Gaia-DR2 confirms VLBA parallaxes in Ophiuchus, Serpens and Aquila. (arXiv:1812.02360v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Ortiz_Leon_G/0/1/0/all/0/1">Gisela N. Ortiz-Le&#xf3;n</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Loinard_L/0/1/0/all/0/1">Laurent Loinard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dzib_S/0/1/0/all/0/1">Sergio A. Dzib</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kounkel_M/0/1/0/all/0/1">Marina Kounkel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Galli_P/0/1/0/all/0/1">Phillip A. B. Galli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tobin_J/0/1/0/all/0/1">John J. Tobin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Evans_N/0/1/0/all/0/1">Neal J. Evans II</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hartmann_L/0/1/0/all/0/1">Lee Hartmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rodriguez_L/0/1/0/all/0/1">Luis F. Rodr&#xed;guez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Briceno_C/0/1/0/all/0/1">Cesar Brice&#xf1;o</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Torres_R/0/1/0/all/0/1">Rosa M. Torres</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mioduszewski_A/0/1/0/all/0/1">Amy […]

On the minimum jet power of TEV BL Lac objects in the p-$gamma$ model. (arXiv:1812.02398v1 [astro-ph.HE])

On the minimum jet power of TEV BL Lac objects in the p-$gamma$ model. (arXiv:1812.02398v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Xue_R/0/1/0/all/0/1">Rui Xue</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_R/0/1/0/all/0/1">Ruo-Yu Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_X/0/1/0/all/0/1">Xiang-Yu Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yan_H/0/1/0/all/0/1">Huirong Yan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bottcher_M/0/1/0/all/0/1">Markus B&#xf6;ttcher</a> We study the requirement on the jet power in the conventional p-$gamma$ models (photopion production and Bethe-Heitler pair production) for TeV BL Lac objects. […]

Calculation of molecular line intensity in stellar atmospheres. (arXiv:1812.02414v1 [astro-ph.SR])

Calculation of molecular line intensity in stellar atmospheres. (arXiv:1812.02414v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Barbuy_B/0/1/0/all/0/1">B. Barbuy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Trevisan_J/0/1/0/all/0/1">J. Trevisan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Almeida_A/0/1/0/all/0/1">A. de Almeida</a> Molecular line intensity calculations are not a straightforward task. We present a description of the basics for including molecular linesin synthetic spectra, and of the input data needed. We aim both at describing ways in […]

HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation. (arXiv:1812.02432v1 [astro-ph.IM])

HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation. (arXiv:1812.02432v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Fuschino_F/0/1/0/all/0/1">F. Fuschino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Campana_R/0/1/0/all/0/1">R. Campana</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Labanti_C/0/1/0/all/0/1">C. Labanti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Evangelista_Y/0/1/0/all/0/1">Y. Evangelista</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Feroci_M/0/1/0/all/0/1">M. Feroci</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burderi_L/0/1/0/all/0/1">L. Burderi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fiore_F/0/1/0/all/0/1">F. Fiore</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ambrosino_F/0/1/0/all/0/1">F. Ambrosino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baldazzi_G/0/1/0/all/0/1">G. Baldazzi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bellutti_P/0/1/0/all/0/1">P. Bellutti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertacin_R/0/1/0/all/0/1">R. Bertacin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertuccio_G/0/1/0/all/0/1">G. Bertuccio</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Borghi_G/0/1/0/all/0/1">G. Borghi</a>, […]

Planet-star interactions with precise transit timing. I. The refined orbital decay rate for WASP-12 b and initial constraints for HAT-P-23 b, KELT-1 b, KELT-16 b, WASP-33 b, and WASP-103 b. (arXiv:1812.02438v1 [astro-ph.EP])

Planet-star interactions with precise transit timing. I. The refined orbital decay rate for WASP-12 b and initial constraints for HAT-P-23 b, KELT-1 b, KELT-16 b, WASP-33 b, and WASP-103 b. (arXiv:1812.02438v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Maciejewski_G/0/1/0/all/0/1">G. Maciejewski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fernandez_M/0/1/0/all/0/1">M. Fern&#xe1;ndez</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aceituno_F/0/1/0/all/0/1">F. Aceituno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Martin_Ruiz_S/0/1/0/all/0/1">S. Mart&#xed;n-Ruiz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ohlert_J/0/1/0/all/0/1">J. Ohlert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dimitrov_D/0/1/0/all/0/1">D. Dimitrov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Szyszka_K/0/1/0/all/0/1">K. Szyszka</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+vonEssen_C/0/1/0/all/0/1">C. […]

The Limits of the Primitive Equations of Dynamics for Warm, Slowly Rotating Small Neptunes and Super Earths. (arXiv:1812.02451v1 [astro-ph.EP])

The Limits of the Primitive Equations of Dynamics for Warm, Slowly Rotating Small Neptunes and Super Earths. (arXiv:1812.02451v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Mayne_N/0/1/0/all/0/1">N. J. Mayne</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Drummond_B/0/1/0/all/0/1">B. Drummond</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Debras_F/0/1/0/all/0/1">F. Debras</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jaupart_E/0/1/0/all/0/1">E. Jaupart</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Manners_J/0/1/0/all/0/1">J. Manners</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boutle_I/0/1/0/all/0/1">I. A. Boutle</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baraffe_I/0/1/0/all/0/1">I. Baraffe</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kohary_K/0/1/0/all/0/1">K. Kohary</a> We present significant differences in the simulated atmospheric flow for […]

Detection of He I $lambda10830$ AA{} absorption on HD 189733 b with CARMENES high-resolution transmission spectroscopy. (arXiv:1812.02453v1 [astro-ph.EP])

Detection of He I $lambda10830$ AA{} absorption on HD 189733 b with CARMENES high-resolution transmission spectroscopy. (arXiv:1812.02453v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Salz_M/0/1/0/all/0/1">M. Salz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Czesla_S/0/1/0/all/0/1">S. Czesla</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schneider_P/0/1/0/all/0/1">P. C. Schneider</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nagel_E/0/1/0/all/0/1">E. Nagel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schmitt_J/0/1/0/all/0/1">J. H. M. M. Schmitt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nortmann_L/0/1/0/all/0/1">L. Nortmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Alonso_Floriano_F/0/1/0/all/0/1">F. J. Alonso-Floriano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lopez_Puertas_M/0/1/0/all/0/1">M. L&#xf3;pez-Puertas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lampon_M/0/1/0/all/0/1">M. Lamp&#xf3;n</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bauer_F/0/1/0/all/0/1">F. F. Bauer</a>, <a […]