Zobrazeno 1 - 10
of 31 497
pro vyhledávání: '"A. A., Pawar"'
Autor:
Shaw, A. W., Kaplan, D. L., Gandhi, P., Maccarone, T. J., Borowski, E. S., Britt, C. T., Buckley, D. A. H., Burdge, K. B., Charles, P. A., Dhillon, V. S., French, R. G., Heinke, C. O., Hynes, R. I., Knigge, C., Littlefair, S. P., Pawar, Devraj, Plotkin, R. M., Ressler, M. E., Santos-Sanz, P., Shahbaz, T., Sivakoff, G. R., Stevens, A. L.
JWST, despite not being designed to observe astrophysical phenomena that vary on rapid time scales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the sub-second infrared timescale
Externí odkaz:
http://arxiv.org/abs/2411.02238
Autor:
Bhan, Nirav, Gupta, Shival, Manaswini, Sai, Baba, Ritik, Yadav, Narun, Desai, Hillori, Choudhary, Yash, Pawar, Aman, Shrivastava, Sarthak, Biswas, Sudipta
Large Language Models (LLMs) have shown remarkable capabilities in various domains, yet their economic impact has been limited by challenges in tool use and function calling. This paper introduces ThorV2, a novel architecture that significantly enhan
Externí odkaz:
http://arxiv.org/abs/2410.17950
Autor:
Pawar, T., Hełminiak, K. G., Moharana, A., Pawar, G., Pyatnytskyy, M., Lala, H. N., Konacki, M.
Pulsating stars in eclipsing binaries (EBs) provide an excellent opportunity to obtain precise, model-independent stellar parameters for studying oscillations in detail. One common class of pulsators in these EBs exhibits delta Scuti-type oscillation
Externí odkaz:
http://arxiv.org/abs/2410.00590
We present results of high-resolution spectroscopic observations of detached eclipsing binaries (DEBs) with total eclipses, for which UVES spectra were obtained during the phase of totality. With the additional, independent information on effective t
Externí odkaz:
http://arxiv.org/abs/2409.20144
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:
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
Autor:
Moharana, Ayush, Hełminiak, K. G., Marcadon, F., Pawar, T., Pawar, G., Konacki, M., Jordán, A., Brahm, R., Espinoza, N.
Publikováno v:
A&A 690, A153 (2024)
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