Zobrazeno 1 - 10
of 11 909
pro vyhledávání: '"P, Pawar"'
Autor:
Rampuria, Yash, Boliya, Deep, Gupta, Shreyash, Iyengar, Gopalan, Rohilla, Ayush, Vyas, Mohak, Langde, Chaitanya, Chanda, Mehul Vijay, Matai, Ronak Gautam, Namitha, Kothapalli, Pawar, Ajinkya, Biswas, Bhaskar, Agarwal, Nakul, Khandelwal, Rajit, Kumar, Rohan, Agarwal, Shubham, Patel, Vishwam, Rathore, Abhimanyu Singh, Rahman, Amna, Mishra, Ayush, Tangri, Yash
This work presents the design and development of IIT Bombay Racing's Formula Student style autonomous racecar algorithm capable of running at the racing events of Formula Student-AI, held in the UK. The car employs a cutting-edge sensor suite of the
Externí odkaz:
http://arxiv.org/abs/2408.06113
A back-to-back semi-inclusive $J/\psi + jet$ production is a promising process to study gluon transverse momentum distribution (TMDs) at the future electron-ion collider (EIC). A back-to-back configuration allows a higher transverse momentum for $J/\
Externí odkaz:
http://arxiv.org/abs/2408.05698
Autor:
Navale, Nilam R., Pawar, Devraj, Rao, A. R., Misra, Ranjeev, Chakraborty, Sudip, Bhattacharyya, Sudip, Bambole, Vaishali A.
XB 1254-690 is a neutron star low-mass X-ray binary with an orbital period of 3.88 hrs, and it exhibits energy-dependent intensity dips, thermonuclear bursts, and flares. We present the results of an analysis of a long observation of this source usin
Externí odkaz:
http://arxiv.org/abs/2407.05371
Autor:
Moharana, Ayush, Hełminiak, K. G., Marcadon, F., Pawar, T., Pawar, G., Konacki, M., Jordán, A., Brahm, R., Espinoza, N.
Eclipsing Compact Hierarchical Triples (ECHTs) are systems with the tertiary star orbiting an eclipsing binary (EB) in an orbit of fewer than 1000 days. In a CHT, all three stars exist in a space less than 5 AU in separation. A low-mass CHT is an int
Externí odkaz:
http://arxiv.org/abs/2405.12136
Autor:
Gandhi, P., Borowski, E. S., Byrom, J., Hynes, R. I., Maccarone, T. J., Shaw, A. W., Adegoke, O. K., Altamirano, D., Baglio, M. C., Bhargava, Y., Britt, C. T., Buckley, D. A. H., Buisson, D. J. K., Casella, P., Segura, N. Castro, Charles, P. A., Corral-Santana, J. M., Dhillon, V. S., Fender, R., Gúrpide, A., Heinke, C. O., Igl, A. B., Knigge, C., Markoff, S., Mastroserio, G., McCollough, M. L., Middleton, M., Miller, J. M., Miller-Jones, J. C. A., Motta, S. E., Paice, J. A., Pawar, D. D., Plotkin, R. M., Pradhan, P., Ressler, M. E., Russell, D. M., Russell, T. D., Santos-Sanz, P., Shahbaz, T., Sivakoff, G. R., Steeghs, D., Tetarenko, A. J., Tomsick, J. A., Vincentelli, F. M., George, M., Gurwell, M., Rao, R.
We present mid-infrared (MIR) spectral-timing measurements of the prototypical Galactic microquasar GRS 1915+105. The source was observed with the Mid-Infrared Instrument (MIRI) onboard JWST in June 2023 at a MIR luminosity L(MIR)~10^{36} erg/s excee
Externí odkaz:
http://arxiv.org/abs/2406.18637
Autor:
Hansen, Colin, Glinskis, Simas, Raju, Ashwin, Kornreich, Micha, Park, JinHyeong, Pawar, Jayashri, Herzog, Richard, Zhang, Li, Odry, Benjamin
Data driven models for automated diagnosis in radiology suffer from insufficient and imbalanced datasets due to low representation of pathology in a population and the cost of expert annotations. Datasets can be bolstered through data augmentation. H
Externí odkaz:
http://arxiv.org/abs/2406.02477
We investigate the azimuthal asymmetries such as $\cos2{\phi_T}$ and Sivers symmetry for $J/\psi$ and $\pi^\pm$ production in electron-proton scattering, focusing on scenarios where the $J/\psi$ and the pion are produced in an almost back-to-back con
Externí odkaz:
http://arxiv.org/abs/2406.00271
Autor:
Kadam, S. K., Salunkhe, Sameer, Vagshette, N. D., Paul, Surajit, Sonkamble, Satish S., Pawar, P. K., Patil, M. K.
Publikováno v:
MNRAS, 531, 2024, 4060-4069
Spiral structures and cold fronts in X-rays are frequently observed in cool core galaxy clusters. However, studies on radio mini-haloes associated with such spirals and their physical connections are rare. Here, we present the detection of an extende
Externí odkaz:
http://arxiv.org/abs/2405.19750
Motion artifacts in Magnetic Resonance Imaging (MRI) are one of the frequently occurring artifacts due to patient movements during scanning. Motion is estimated to be present in approximately 30% of clinical MRI scans; however, motion has not been ex
Externí odkaz:
http://arxiv.org/abs/2405.17756
We consider the notion of finite type-ness of a site introduced by Morel and Voevodsky, for the \'etale site of a field. For a given field $k$, we conjecture that the \'etale site of $Sm/k$ is of finite type if and only if the field $k$ admits a fini
Externí odkaz:
http://arxiv.org/abs/2405.06612