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ADFOSC
SPIM SPIM
IMAGER IMAGER
TANSPEC TANSPEC
TIRCAM TIRCAM2

ARIES Devasthal Faint Object Spectrograph and Camera (ADFOSC)

ADFOSC is a low-resolution slit-spectrograph and camera having sensitivity in the wavelength range 350 nm to 1050 nm. It uses a 4096 x 4096 deep-depletion fringe-suppressed E2V CCD camera with a pixel (px) scale of ~0.2 arcsec, and it covers a field of view of 13.6 x 13.6 arcmin. The available filters are broad-band SDSS u,g,r,i,z and narrow-band (10.2 nm width) with central wavelengths at 491.6, 660.9, 674.3, and 683.3 nm. The spectral dispersions provided by different grisms are in the range of 0.1 to 0.7 nm/px and an 8’ long slit with different available widths (0.4” - 3.2”) can be used. Imaging observations show that the instrument has the capability to detect sources up to ~24.5 mag AB (i-band) with 10% photometric accuracy in r-band in effective exposure of ~2 hours in dark nights. Stellar images with a FWHM of 0.9 arcsec in r-band were recorded in May 2020 in the best sky conditions. Spectroscopic observations with the instrument show that a spectroscopic trace of g=19 mag source at a 5-sigma level can be detected in 10 minutes of exposure at ~0.2 nm/px dispersion. Hg-Ar, Ne, and continuum lamps are available for spectral calibration.

Instrument parameters

Parameters Value
Type Imaging and spectroscopy
Mount position Main axial port
Wavelength range 350-1050 nm
Array size 4096 x 4096 pixel2
Pixel size 15 μm
Pixel scale 0”.2
Field of view Broad-band imaging: 13’.6 X 13’.6, Narrow-band imaging: 11’ diameter
Spectral resolution <2000
Readout noise 8 e-
Readout time 35 s
Gain 1.6e-/ADU
Minimum exposure 0.9 sec
Available filters broadband: SDSS u,g,r,i,z and narrowband
Grism range 0.1 - 0.7 nm/pixel
Slits Length:8”, Widths: 0’.4 - 3’.2
Limiting magnitude for photometry 24.5 mag in i-band for an exposure of 2 hours
Limiting magnitude for spectroscopy g=19 mag with 10 minute exposure at 0.2 nm/px dispersion
Calibration lamp Hg-Ar, Ne, and continuum
The picture shows ADFOSC mounted on axial main port of 3.6m DOT.

Latest update

  • 2020-12-24: Notes on observing with the ADFOSC instrument are rewritten. It includes earlier notes as well. Click HERE.
  • 2020-12-17: Preliminary notes on observing with the ADFOSC instrument, click HERE.

Documents for users

Recent publications

  1. A Relook at the Black Hole Binary Candidate J1328+2752 with VLBI
    Sumana Nandi, Preeti Kharb, Anderson Caproni, Rupak Roy, and Biny Sebastian;
    2024, ApJ, 965, 1, id.9, 8pp
  2. Spectrophotometric Reverberation Mapping of Intermediate-mass Black Hole NGC 4395
    Shivangi Pandey, Suvendu Rakshit, Krishan Chand, C. S. Stalin, Hojin Cho, Jong-Hak Woo, Priyanka Jalan, Amit Kumar Mandal, Amitesh Omar, Jincen Jose, Archana Gupta;
    2024, ApJ, 976, 1, id.116, 13pp
  3. Investigation of the central system of the Black Hole Binary Candidate J1328+2752
    Sumana Nandi, Preeti Kharb, Anderson Caproni, Rupak Roy, and Biny Sebastian;
    2024, 42nd meeting of the Astronomical Society of India (ASI), held 31 January-04 February 2024, in Bengaluru, India. Hosted jointly by Indian Institute of Science (IISc), Indian Space Research Organisation (ISRO) and Jawaharlal Nehru Planetarium (JNP). Online at https://www.astron-soc.in/asi2024, id.P82
  4. Optical spectroscopy of Gaia detected protostars with DOT: Can we probe protostellar photospheres?
    Mayank Narang, Manoj P., Himanshu Tyagi, Prasanta K. Nayak, Saurabh Sharma, Arun Surya, Bihan Banerjee, Blesson Mathew, Arpan Ghosh, Ayushi Verma;
    2023, JApA, 44, 99N
  5. Characterization of a deep-depletion 4K × 4K charge-coupled device detector system designed for ARIES Devasthal faint object spectrograph
    Dimple Panchal, Tripurari S. Kumar, Amitesh Omar, Kuntak Misra;
    2023, Journal of Astronomical Telescopes, Instruments, and Systems, 9, 018002
  6. SN 2020jfo: A Short-plateau Type II Supernova from a Low-mass Progenitor
    R. S. Teja, A. Singh, D. K. Sahu, G. C. Anupama, B. Kumar, A. J. Nayana;
    2022, ApJ, 930, 1, id.34, 19pp
  7. Optical spectroscopic characterization of Fermi blazar candidates of uncertain type with TNG and DOT: first results
    Amanda Olmo-Garcia, Vaidehi S. Paliya, Nuria Alvarez Crespo, Brajesh Kumar, Alberto Dominguez, Armando Gil de Paz, Patricia Sanchez-Blazquez ;
    2022, MNRAS, 516, 4, pp.5702-5711
  8. SN 2020sck: Deflagration in a Carbon-Oxygen White Dwarf
    A. Dutta, D. K. Sahu, G. C. Anupama, S. Joharle, B. Kumar, A. J. Nayana, A. Singh, H. Kumar, V. Bhalerao, and S. Barway;
    2022, ApJ, 925(2):217
  9. GRB 210217A: A short or a long GRB?
    Dimple, K. Misra, A. Ghosh, K. G. Arun, R. Gupta, A. Kumar, L. Resmi, S. B. Pandey, and L. Yadav;
    2022, JApA, 43, 2-39
  10. Intranight variability of ultraviolet emission from powerful blazars
    K. Chand, Gopal-Krishna, A. Omar, H. Chand, S. Mishra, P. S. Bisht, and S. Britzen;
    2022, MNRAS, 511(1):13–18
  11. First-light images from low dispersion spectrograph-cum-imager on 3.6- meter Devasthal Optical Telescope
    A. Omar, T. S. Kumar, B. Krishna Reddy, J. Pant, M. Mahto;
    2019, Current Science, 116, 1472-1478
  12. Optical detection of a GMRT-detected candidate high- redshift radio galaxy with 3.6-m Devasthal optical telescope
    Amitesh Omar, A. Saxena, K. Chand, et al. ; 2019, JApA, 40, 9; (arXiv : 1902.05856)
  13. Design and development of control unit and software for the ADFOSC instrument of the 3.6 m Devasthal optical telescope
    T. S. Kumar;
    2016, Proceedings of the SPIE, 9908, 99084Y 6 pp
  14. Design of FOSC for 360-cm Devasthal Optical Telescope
    A. Omar, R. K. S. Yadav, V. Shukla, S. Mondal, and J. Pant;
    2012, I. S. McLean, S. K. Ramsay, and H. Takami, editors, Ground-based and Airborne Instrumentation for Astronomy IV, volume 8446 of Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, page 844614
  15. Preliminary Design of ARIES-Devasthal Faint Object Spectrograph and Camera
    Soumen Mondal, Ramakant S. Yadav, Mahendra Singh;
    2009, eprint arXiv:0905.0360