Results 91 to 100 of about 141,789 (261)

FINE STRUCTURE OF ANOMALOUSLY INTENSE PULSES OF PSR J0814+7429 RADIO EMISSION IN THE DECAMETER RANGE

Radio Physics and Radio Astronomy, 2017
Purpose: The fine structure of the anomalously intense pulses of PSR J0814+7429 (В0809+74) has been studied. The pulsar radio emission fine structure is investigated to determine its parameters in the lowest part of spectrum available for groundbased ...
A. O. Skoryk, O. M. Ulyanov, V. V. Zakharenko, A. I. Shevtsova, I. Y. Vasylieva, M. S. Plakhov, I. M. Kravtsov   +6 more
doaj   +1 more source

Extended Emission from the PSR B1259-63/SS 2883 Binary Detected with Chandra

, 2011
PSR B1259-63 is a middle-aged radio pulsar (P=48 ms, tau=330 kyr, Edot=8.3*10^{35} erg/s) in an eccentric binary (P_orb =3.4 yr, e=0.87) with a high-mass Be companion, SS 2883.
Chulhoon Chang, Cordes, Durant, Gaensler, George G. Pavlov, Hirayama, Johnston, Juda, Kargaltsev, Kargaltsev, Kargaltsev, Kargaltsev, Kashyap, Mori, Nicastro, Oleg Kargaltsev, Pavlov, Pavlov, Pavlov, Tavani, Tsunemi, Uchiyama   +21 more
core   +1 more source

Single‐Position Peptide Clustering for Peptidomics Reveals Novel Disease Biomarkers and Dysregulated Proteolytic Characteristics

Advanced Science, Volume 13, Issue 5, 27 January 2026.
A novel amino acid (aa)‐score‐based single‐position peptide clustering strategy is developed for peptidomics, enabling precise profiling of protein proteolysis in plasma from β‐thalassemia cohort. The method identifies new aa position‐based peptide cluster biomarkers validated by heavy‐labeled peptides, visualizes aggregated changes, uncovers disease ...
Na Li, Yaxin Zhu, Yumeng Yan, Jifeng Wang, Lili Niu, Xiang Ding, Mengmeng Zhang, Zhensheng Xie, Tanxi Cai, Xiaojing Guo, Jianming Luo, Peng An, Xiangqian Guo, Fuquan Yang   +13 more
wiley   +1 more source

Calculation of radar signals delay to second order in the frame of the General Relativity Theory

ACI Avances en Ciencias e Ingenierías, 2014
From the Schwarzschild metric, the light delay due to a gravitational field is calculated to second order approximation in the gravitational potential. We analize the contribution of the second order terms for strong gravitational fields as the generated
Joaquín Valerio Grefa, Carlos A. Marín
doaj   +1 more source

HST optical polarimetry of the Vela pulsar & nebula

, 2014
Polarisation measurements of pulsars offer an unique insight into the geometry of the emission regions in the neutron star magnetosphere. Therefore, they provide observational constraints on the different models proposed for the pulsar emission ...
Mignani, R. P., Moran, P., Shearer, A.
core   +1 more source

Multi‐scale maternal behavioral responses by white‐tailed deer to coyote predation risk

The Journal of Wildlife Management, Volume 90, Issue 1, January 2026.
In the piedmont region of the southeastern US, white‐tailed deer adjust maternal care strategies in response to variation in risk of encountering coyotes. In areas frequented by coyotes, adult female deer (i.e., does) increase their use of space, likely to avoid drawing coyotes to the location where a fawn is hidden.
Michael S. Muthersbaugh, Wesley W. Boone, Elizabeth A. Saldo, Alex J. Jensen, Charles Ruth, Jay Cantrell, John C. Kilgo, David S. Jachowski   +7 more
wiley   +1 more source

Cherenkov Telescope Array Observatory: Die Zukunft der Gammaastronomie

Physik in unserer Zeit, Volume 57, Issue 1, Page 10-18, January 2026.
Im Jahr 1989 hat das Wipple‐Observatorium die erste Quelle hochenergetischer Gammastrahlung entdeckt. 2002 waren dann sechs Quellen bekannt, 2024 schon mehr als 300. Und das ist immer noch lediglich die Spitze des Eisbergs in der jungen Geschichte der Gammaastronomie.
Daniela Hadasch, Daniel Mazin
wiley   +1 more source

The identification of the optical companion to the binary millisecond pulsar J0610-2100 in the Galactic field

, 2012
We have used deep V and R images acquired at the ESO Very Large Telescope to identify the optical companion to the binary pulsar PSR J0610-2100, one of the black-widow millisecond pulsars recently detected by the Fermi Gamma-ray Telescope in the Galactic
A. Possenti, Abdo, B. Lanzoni, C. Pallanca, Cocozza, Cordes, E. Dalessandro, E. Sabbi, Edmonds, F. R. Ferraro, Ferraro, Ferraro, King, Kızıltan, Lasker, M. Burgay, Manchester, Moffat, Ozel, Pallanca, R. P. Mignani, Roberts, Stappers, Stappers, Stappers, Stappers, van Kerkwijk, Voges   +27 more
core   +1 more source

X-ray observations of the Large Magellanic Cloud pulsar PSR B0540-69 and its PWN

, 2008
PSR B0540-69 is a young pulsar in the Large Magellanic Cloud that has similar properties with respect to the Crab Pulsar, and is embedded in a Pulsar Wind Nebula.
A. De Rosa, A. J. Dean, Bird, Cusumano, Cusumano, de Jager, de Jager, de Plaa, Dean, Deeter, E. Massaro, Ferrando, Fichtel, Finley, Forot, Freedman, Gehrels, Goldwurm, Gotthelf, Götz, Hirayama, Hoffmann, Hwang, Jahoda, Kaaret, Kargaltsev, L. Bassani, Landi, Lebrun, Lin, Livingstone, Manchester, Massaro, Massaro, McBride, Middleditch, Mineo, Mineo, Petre, R. Campana, Rothschild, Schaefer, Serafimovich, Seward, Sreekumar, T. Mineo, Takata, Thompson, Ubertini   +48 more
core   +1 more source

Red Noise Suppression in Pulsar Timing Array Data Using Adaptive Splines

Universe
Noise in Pulsar Timing Array (PTA) data is commonly modeled as a mixture of white and red noise components. While the former is related to the receivers, and easily characterized by three parameters (EFAC, EQUAD and ECORR), the latter arises from a mix ...
Yi-Qian Qian, Yan Wang, Soumya D. Mohanty   +2 more
doaj   +1 more source