Articles written in Journal of Astrophysics and Astronomy
Volume 37 Issue 4 December 2016 Article ID 0038 Review
Stars and planetary systems are formed out of molecular clouds in the interstellar medium. Although the sequence of steps involved in star formation are generally known, a comprehensive theory which describes the details of the processes that drive formation of stars is still missing. The Square Kilometre Array (SKA), with its unprecedented sensitivity and angular resolution, will play a major role in filling these gaps in our understanding. In this article, we present a few science cases that the Indian star formation community is interested in pursuing with SKA, which include investigation of AU-sized structures in the neutral ISM, the origin of thermal and non-thermal radio jets from protostars and the accretion history of protostars, and formation of massive stars and their effect on the surrounding medium.
Volume 43 All articles Published: 31 May 2022 Article ID 0032 OBSERVATIONAL FACILITIES
G. C. ANUPAMA G. MAHESWAR S. SRIRAM T. SIVARANI P. S. PARIHAR S. NAGABHUSHAN DORJE ANGCHUK S. BARWAY B. C. BHATT R. BANYAL ALIKHAN BASHEER PRASANNA DESHMUKH DEVIKA DIVAKAR TSEWANG DORJAI ARUNA GOSWAMI K. V. GOVINDA SONAM JORPHAIL U. S. KAMATH MADAN MOHAN KEMKAR TASHI TSERING MAHAY S. MUNEER C. MUTHUMARIAPPAN SHANTIKUMAR SINGH NINGOMBAM G. PANDEY B. E. REDDY D. K. SAHU D. S. SANDEEP RAMYA SETHURAM C. S. STALIN S. SUBRAMANIAN STANZIN TSEWANG A. SUBRAMANIAM
An observatory class national large optical-IR telescope (NLOT), is proposed to be built and located in the country. The telescope consists of a 10–12 m segmented primary. In order to cater to a diversity of observational programs, the telescope is designed with high throughput in both the optical and IRregions (0.3–5 $\mu$m). It should perform reasonably well up to 30 $\mu$m. The telescope and instruments should have remote operations capability, allowing for the queue as well as classical scheduling and high reliability and robustness. This article provides a brief description of the science cases that drive the telescope requirements, activities related to optics design and some thoughts on the instruments.
Volume 43 All articles Published: 12 November 2022 Article ID 0086 OBSERVATIONAL FACILITIES
THIRUPATHI SIVARANI RAMYA SETHURAM S. SRIRAM DEVIKA DIVAKAR ARUN SURYA HARI MOHAN VARSHNEY SUDARSHAN KAMBALA AMIRUL HASAN AJIN PRAKASH K. V. GOVINDA VISWANATHA G. C. ANUPAMA G. MAHESWAR D. OJHA S. B. PANDEY J. PANDEY M. PURAVANKARA A. N. RAMAPRAKASH B. E. REDDY SARANG S. SHAH R. SRIANAND A. SUBRAMANIAM S. SUBRAMANIAN
The future of astronomy in the coming decades will be shaped by the upcoming three extremely large optical telescopes, the Thirty Meter Telescope (TMT), the Giant Magellan Telescope (GMT) and the European Large Telescope (ELT). The USA astronomy and astrophysics 2020 decadal survey and the Canadian long-range plan for astronomy have recently recommended these large observatories as a top priority for ground-based astronomy for the upcoming decade. India is a 10% partner in one of these large observatories, the TMT, which is jointly funded by the Department of Science and Technology (DST) and Department of Atomic Energy (DAE). Here, we highlight India’s contributions to the development of the telescope and science instruments. The size of back-end science instruments scale with telescope aperture, hence, science instruments for TMT will be the biggest ever built for any telescope. Designing and building them requires broad collaboration within India, across TMT partnership and industries. India contributes >30% of the work share towards the development of wide field optical spectrometer (WFOS). India is part of the development of other first-light instruments, the infrared imaging spectrograph (IRIS) and multi-object diffraction-limited high-resolution infrared spectrograph (MODHIS). Infrared guide star catalog is an important contribution from India to these adaptive optics (AO)-assisted instruments. India leads the development of high-resolution optical spectrograph (HROS), a major workhorse among the first decade instruments of TMT. India is also part of the instrument development team of other first-decade instruments. Concerted efforts have been made to contribute to some of the TMT precursor instruments that will help us to maximize the scientific productivity when TMT is operational, especially in the area of exoplanet science and observations that require AO. India-TMT is part of the science team for the Keck high-resolution infrared spectrograph for exoplanet characterization (HISPEC), a precursor instrument to TMT-MODHIS. In addition, Indian Institute of Astrophysics (IIA) is participating in the science and development of Santa Cruz array of lenslets for exoplanet spectroscopy (SCALES) project for Keck, which is a direct imaging spectrograph for exoplanet studies and a precursor to the TMT planetary system imager.
Volume 44, 2023
Continuous Article Publishing mode
Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.
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