Zobrazeno 1 - 10
of 2 204
pro vyhledávání: '"A Shetye"'
Autor:
Evans, Nancy Remage, Kervella, Pierre, Kuraszkiewicz, Joanna, Günther, H. Moritz, Anderson, Richard I., Proffitt, Charles, Gallenne, Alexandre, Mérand, Antoine, Trahin, Boris, Viviani, Giordano, Shetye, Shreeya
Cepheid masses continue to be important tests of evolutionary tracks for intermediate mass stars as well as important predictors of their future fate. For systems where the secondary is a B star, {\it Hubble Space Telescope} ultraviolet spectra have
Externí odkaz:
http://arxiv.org/abs/2410.01934
Autor:
Uttenthaler, S., Shetye, S., Nanni, A., Aringer, B., Eriksson, K., McDonald, I., Gobrecht, D., Höfner, S., Wolter, U., Cristallo, S., Bernhard, K.
Context: The details of the mass-loss process in the late stages of low- and intermediate-mass stellar evolution are not well understood, in particular its dependence on stellar parameters. Mira variables are highly suitable targets for studying this
Externí odkaz:
http://arxiv.org/abs/2409.19604
Autor:
Arya, Anuraag, Bilkhu, Harmanjeet Singh, Vishwakarma, Sandeep, Belatikar, Hrishikesh, Bhalerao, Varun, Ghodgaonkar, Abhijeet, Koyande, Jayprakash G., Marathe, Aditi, Mithun, N. P. S., Narang, Sanjoli, Nimbalkar, Sudhanshu, Page, Pranav, Palit, Sourav, Patel, Arpit, Shetye, Amit, Tallur, Siddharth, Tendulkar, Shriharsh, Vadawale, Santosh, Waratkar, Gaurav
Hard X-ray photons with energies in the range of hundreds of keV typically undergo Compton scattering when they are incident on a detector. In this process, an incident photon deposits a fraction of its energy at the point of incidence and continues
Externí odkaz:
http://arxiv.org/abs/2409.08822
Autor:
Maji, Moupiya, More, Surhud, Sule, Aniket, Balasubramanya, Vishaak, Bhandari, Ankit, Chand, Hum, Chavan, Kshitij, Dasgupta, Avik, De, Anindya, Gangopadhyay, Jayant, Gulati, Mamta, Hasan, Priya, Ishtiyaq, Syed, Madani, Meraj, Misra, Kuntal, N, Amoghavarsha, Oberoi, Divya, Pattnaik, Subhendu, Patwardhan, Mayuri, Ramanujam, Niruj Mohan, Ranadive, Pritesh, Sawant, Disha, Sharma, Paryag, Sharma, Twinkle, Shetye, Sai, Singhal, Akshat, Srivastava, Ajit M., Sudan, Madhu, Syed, Mumtaz, Vikranth, Pulamathi, Yadav, Virendra
We present the results of a nation-wide baseline survey, conducted by us, for the status of Astronomy education among secondary school students in India. The survey was administered in 10 different languages to over 2000 students from diverse backgro
Externí odkaz:
http://arxiv.org/abs/2406.12308
Autor:
Shetye, Shreeya S., Viviani, Giordano, Anderson, Richard I., Mowlavi, Nami, Eyer, Laurent, Evans, Nancy R., Szabados, Laszlo
Classical Cepheids provide valuable insights into the evolution of stellar multiplicity among intermediate-mass stars. Here, we present a systematic investigation of single-lined spectroscopic binaries (SB1) based on high-precision velocities measure
Externí odkaz:
http://arxiv.org/abs/2405.19840
Autor:
Anderson, Richard I., Viviani, Giordano, Shetye, Shreeya S., Mowlavi, Nami, Eyer, Laurent, Palaversa, Lovro, Holl, Berry, Blanco-Cuaresma, Sergi, Kravchenko, Kateryna, Pawlak, Michał, Reyes, Mauricio Cruz, Khan, Saniya, Netzel, Henryka E., Löbling, Lisa, Pápics, Péter I., Postel, Andreas, Roelens, Maroussia, Spetsieri, Zoi T., Thoul, Anne, Zák, Jiří, Bonvin, Vivien, Martin, David V., Millon, Martin, Saesen, Sophie, Wyttenbach, Aurélien, Figueira, Pedro, Marmier, Maxime, Prins, Saskia, Raskin, Gert, van Winckel, Hans
Publikováno v:
A&A 686, A177 (2024)
This first VELOCE data release comprises 18,225 high-precision RV measurements of 258 bona fide classical Cepheids on both hemispheres collected mainly between 2010 and 2022, alongside 1161 additional observations of 164 other stars. The median per-o
Externí odkaz:
http://arxiv.org/abs/2404.12280
Autor:
Ambilduke, Kshitij, Shetye, Aneesh, Bagade, Diksha, Bhagwatkar, Rishika, Fitter, Khurshed, Vagdargi, Prasad, Chiddarwar, Shital
Neural machine translation benefits from semantically rich representations. Considerable progress in learning such representations has been achieved by language modelling and mutual information maximization objectives using contrastive learning. The
Externí odkaz:
http://arxiv.org/abs/2401.03314
Autor:
Loganayagam, R., Shetye, Omkar
Inspired by real-time computations in AdS black holes, we propose a method to obtain the influence phase of a cosmological observer by calculating the on-shell action on a doubled spacetime geometry. The influence phase is the effective action for an
Externí odkaz:
http://arxiv.org/abs/2309.07290
Autor:
Rakshita Sukruth Kolipakala, Suranjana Basu, Senjuti Sarkar, Beneta Merin Biju, Daniela Salazar, Likhit Reddy, Pushya Pradeep, Muniraj Krishnaveni Yuvapriya, Shrijita Nath, Riley Gall, Anish Hemanth Samprathi, Harshitha Balaji, Eeshaan A. B. Koundinya, Aparna Shetye, Deepesh Nagarajan
Publikováno v:
ACS Omega, Vol 9, Iss 34, Pp 36353-36370 (2024)
Externí odkaz:
https://doaj.org/article/9beed1c300aa4d0c9e17e8f48ac6c595
New instrumental and telescopes covering the optical and ultra-violet spectral regions have revealed a range of small-scale dynamic features, many which may be related. For example, the range of spicule-like features hints towards a spectrum of featu
Externí odkaz:
http://arxiv.org/abs/2306.02945