IIA Institutional Repository: Recent submissions

  • Manjunath, B; Sivarani, T; Surya, Arun; Yadav, Sudharsan; Unni, Athira; Parvathy, M; Divakar, Devika; Sriram, S; Prakash, A; Hasan, Amirul (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-07)
    We present a conceptual design for a fiber positioning system for multi-object high-resolution spectroscopy, designed to be compatible with the upcoming large telescopes with a wide field of view. The design incorporates ...
  • Desai, Aditi; Sallum, Steph; Banyal, R. K; Batalha, Natalie; Batalha, Natasha; Blake, Geoff; Brandt, Tim; Briesemeister, Zack; Kleer, Katherine de; Pater, Imke de; Eisner, Josh; Fong, Wen-fai; Greene, Tom; Honda, Mitsuhiko; Kain, Isabel; Kilpatrick, Charlie; Lach, Mackenzie; Liu, Mike; Macintosh, Bruce; Martinez, Raquel A.; Mawet, Dimitri; Miles, Brittany; Morley, Caroline; Powell, Diana; Sheehan, Patrick; Skemer, Andrew J.; Stelter, R. Deno; Stone, Jordan; Surya, Arun; Sivarani, T; Wagner, Kevin; Zhou, Yifan (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-07)
    SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) is a high-contrast lenslet-based integral field spectrograph (IFS) designed to characterize exoplanet atmospheres in the 2 - 5 micron wavelength ...
  • Surya, Arun; Kupke, Renate; Stelter, Deno; Hinz, Phil; Sallum, Stephanie; Hasan, Amirul; Skemer, Andrew; Sivarani, T; Banyal, R. K; Unni, Athira (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-07)
    The SCALES instrument is a high-contrast imager and integral field spectrograph that operates in the infrared wavelength and is intended to be utilized behind W.M. Keck Observatory’s adaptive optics system. The instrument ...
  • Mathur, Harsh (Indian Institute of Astrophysics, 2024)
    The chromosphere, situated between the bright photosphere and the remarkably thin transition region that precedes the million-degrees hot corona, is a highly dynamic and intricate layer within the solar atmosphere. By ...
  • Saraswathi Kalyani, S (Indian Institute of Astrophysics, 2024)
    Ground-based telescopes are severely limited in their performance by the turbulence of the Earth’s atmosphere. The wavefronts emitted by the celestial bodies are perturbed and we lose high spatial frequency information. ...
  • Saraswathi Kalyani, S; Sridharan, R (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    The Indian Institute of Astrophysics is deliberating the development of a 2-m class Solar telescope called NLST (National Large Solar Telescope) at Merak, Ladakh. It will be equipped with an adaptive optics system to realize ...
  • Radhika, Dharmadhikari; Martinez, P; Gouvret, C; Marcotto, A; Spang, A; Dejonghe, J; Beaulieu, M; Sallard, C (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    Differential optical transfer function (dOTF) is a model-independent image-based wavefront sensor for measuring the complex field. This sensor-less wavefront sensing technique is efficient for precise non-common path ...
  • Martinez, P; Radhika, Dharmadhikari; Spang, A (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    We examine several focal plane wavefront sensing (FPWFS) approaches from a theoretical perspective, specifically comparing their fundamental origins and similarities. We consider various techniques, including the differential ...
  • Shubham Jankiram, Ghatul; Bharat Chandra, P; Jain, Shubhangi; Binukumar, G; Mahesh Babu, S; Mohan, Rekhesh; Safonova, M; Murthy, J (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    We present here an STM32 microcontroller based on-board computer designed for use in small satellites and CubeSat missions that was developed using commercial-off-the-shelf (COTS) electronics components. An onboard computer ...
  • Ratliff, Chris; MacDonald, Nicholas; Cabak, J; Deich, Will; Sandford, Dale; Gonzales, Michael; Skemer, Andrew; Sallum, Stephanie; Stelter, Deno; Hunter, A; Kupke, Renate; Dillon, Daren; Marques, D; Rodriguez, C; Savage, M; Kassis, Marc; Lyke, J; Hasan, Amirul (SPIE-Society of Photo-Optical Instrumentation Engineers, 2024-08)
    SCALES is a new instrument that will be mounted on the Keck 2 Telescope just downstream of the Keck 2 AO system. SCALES is designed to take spectra of directly imaged exoplanets at multiple wavelengths in the thermal ...
  • Basheer, Alikhan; Panchal, Pramod; Jha, Sanjeev K; Sudharsan, K; Prasanna Deshmukh; Valsan, Vineeth; Sriram, S (SPIE-Society of Photo-Optical Instrumentation Engineers, 2024-08)
    As a collaborative effort within the Thirty Meter Telescope (TMT) project, India is committed to supplying 84 polished segments for the primary mirror, employing the innovative Stressed Mirror Polishing (SMP) technology ...
  • Panchal, Pramod; Jha, Sanjeev K; Basheer, Alikhan; Valsan, Vineeth; Prasanna Deshmukh; Sriram, S (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    TMT adopts Stressed Mirror Polishing (SMP) technology for the polishing of mirror segments. In this process, the meniscus type spherical shape glass blanks are converted in to a desired aspheric shape by spherical grinding ...
  • Divakar, Devika; Sivarani, T; Sethuram, Ramya; Fucik, Jason; Steidel, Chuck; Manjunath, B; Prasanna Deshmukh (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-08)
    Wide Field Optical Spectrograph (WFOS) is the first light instrument of Thirty Meter Telescope (TMT), which will be one of the wide field spectrographs for optical spectroscopy and can probe the faintest limits. In order ...
  • Subramaniam, A (Indian Institute of Astrophysics, 2024)
  • Subramaniam, A (Indian Institute of Astrophysics, 2023)
  • Dhanush, S. R; Subramaniam, A; Subramanian, S (American Astronomical Society, 2025-02-10)
    We model the kinematics of the Small Magellanic Cloud (SMC) by analyzing the proper motions (PMs) from Gaia DR3 of nine different stellar populations, including young main-sequence (MS) stars (<2 Gyr), red giant branch ...
  • Swain, Subhashree; Paliya, Vaidehi S; Saikia, D. J; Stalin, C. S (American Astronomical Society, 2025-02-01)
    The γ-ray detection from an astrophysical object indicates the presence of an extreme environment where highenergy radiation is produced. With the continuous monitoring of the γ-ray sky by the Fermi Large Area Telescope ...
  • Bhatnagar, Aditi; Avijeet Prasad; Rouppe van der Voort, L; Nobrega-Siverio, Daniel; Joshi, Jayant (EDP Sciences, 2025-01)
    Context. Quiet-Sun Ellerman bombs (QSEBs) are small-scale magnetic reconnection events in the lower atmosphere of the quiet Sun. Recent work has shown that a small percentage of them can occur co-spatially and co-temporally ...
  • Saini, Ajay Kumar; Pandey, G (American Astronomical Society, 2025-02-01)
    A fine abundance analysis of a recently discovered hydrogen-deficient carbon (HdC) star, A980, is presented. Based on the observed high-resolution optical spectrum, we ascertain that A980 is a cool extreme helium (EHe) ...
  • Murthy, Jayant; Shull, J. Michael; Postman, Marc; Parker, Joel Wm; Redfield, Seth; Cunningham, Nathaniel; Gladstone, G. Randall; Pineau, Jon P; Brandt, Pontus; Verbiscer, Anne J.; Singer, Kelsi N; Weaver, H. A; Henry, R. C; Stern, S. Alan (American Astronomical Society, 2025-02)
    We present new observations of the cosmic ultraviolet background (CUVB) at high Galactic latitudes (|b| > 40o ), made using the Alice UV spectrograph on board the New Horizons spacecraft. These observations were taken at ...

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