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TANSPEC
SPIM SPIM
IMAGER IMAGER
ADFOSC ADFOSC
TIRCAM TIRCAM2

TIFR ARIES Near-IR Spectrograph (TANSPEC)

TANSPEC is a medium-resolution spectrograph and camera having sensitivity in the wavelength range from 550 to 2540 nm. It employs a 1024 x 1024 H1RG array with a pixel scale of 0.25 arcsec and it covers a field of view of 1 arcmin x 1 arcmin. It offers broad-band photometry in r, i, Y, J, H, K and narrow-band H2 and BrG filters. Stellar images with FWHM of 0.5 arcsec in K-band were recorded in February 2020 in the best conditions. The object of 18 mag in K has been successfully imaged and detected in 1-min exposure. It is possible to detect sources at J, H, K of 19.5, 18.9, 18.4 mag respectively at 10 sigma level in 10 minutes exposure. R~23 mag source is detected in 1 hour exposure.
  For spectroscopy, it employs a 2048 x 2048 H2RG array, and it can be used in cross-dispersed mode (R~2750) as well as in prism mode (R~100-350). The slits available in these modes have widths between 0.5 to 4.0 arcsec. By our theoretical calculations, It can be possible to take R ~ 2750 (~100-350) spectra of J=14.3 (17.3) mag source in 1 hour at 100-sigma level for stellar sources with FWHM of 1 arcsec. TANSPEC can only be mounted on the axial-port of the telescope. Proposals should be considered for science verification in the early cycles, when the focus will be on stabilizing the TANSPEC instrument.
  For high-resolution spectroscopic mode, the proposers should add about 50% of the overhead (excluding lamp / standard stars). In the imaging mode, the overhead is about 30% (for dithering, filter change, readout, etc).

Instrument parameters

Parameters Value
Type Imaging and spectroscopy
Mount position Main axial port
Wavelength range 550 - 2540 nm
Array size Imaging: 1024 X 1024 pixel2, Spectroscopy: 2048 x 2048 pixel2
Pixel size 18 μm
Pixel scale 0”.25
Field of view 1’ X 1’
Readout noise Imaging: 3.5 ADU, Spectroscopy: 20.7 (high-gain), 5.3 (low-gain)
Readout time Imaging: 1.89s, Spectroscopy: 5.26s
Gain Imaging: 4.3e-/ADU, Spectroscopy: 1.1 (high-gain), 4.5 (low-gain)
Minimum exposure time for imaging 0.9 s
Spectroscopy modes Cross-dispersion and prism
Spectral resolution Cross-dispersion mode: 2750, Prism mode: 100-350
Available filters broadband: r, i, Y, J, H, K and narrowband: H2, BrG
Slits Widths: 0”.5-4”.0
Limiting magnitudes for imaging 18 mag in K-band for an exposure of 1 min, 19.5,, 18.9, 18.4 mag in J, H, K bands, respectively, with an exposures of 10 min
Limiting magnitude for spectroscopy Cross dispersion mode: J=14.3 with 1 hour exposure, Prism mode: J=17.3 with 1 hour exposure
The image shows TANSPEC mounted on axial port of the 3.6m DOT.

Latest update

  • 2020-12-29: The grating wheel has been repaired and high-resolution mode (cross-dispersion) will be available during cycle 2021-DOT-C1.
  • 2020-11-26: For new plots on SNR vs exposure time in prism mode from the latest data, click here.
  • 2020-11-21: For new plots on sensitivity and resolution from the latest data, click here.
  • 2020-11-18: The Grating wheel has developed some technical issues and hence any spectroscopic observations cannot be executed at the moment, though the proposers may like to utilise the instrument in the imaging mode if that suits their science requirement. The technical issue is unlikely to be resolved in cycle 2020-DOT-C2. The grating wheel is expected to be repaired for cycle 2021-DOT- C1.

Documents for users

 

Recent publications

  1. Peering into the Heart of the Giant Molecular Cloud G148.24+00.41: A Deep Near-infrared View of the Newly Hatched Cluster FSR 655
    Vineet Rawat, M. R. Samal, D. K. Ojha, Brajesh Kumar, Saurabh Sharma, J. Jose, Ram Sagar, R. K. Yadav
    2024, AJ, 168, 3, id 136, 14 pp
  2. Understanding the Magnetic Activity of M Dwarfs: Optical and Near-Infrared Spectroscopic Studies
    Diya Ram, Soumen Mondal, Samrat Ghosh, Santosh Joshi, Dusmants Patra, Rajib Kumbhakar
    2024, Bulletin de la Société Royale des Sciences de Liège, 93, No.2- Proceedings of the 3rd BINA Workshop on the Scientific Potential of the Indo-Belgian Cooperation, pp. 358-369
  3. Infrared Astronomy at TIFR over the years
    D. K. Ojha, TIFR Infrared Astronomy Group
    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).
  4. Quiescence of an outburst of a low-mass young stellar object: LDN1415-IRS
    Koshvendra Singh, Devendra K. Ojha, Joe P. Ninan, Saurabh Sharma, Supriyo Ghosh, Arpan Ghosh, Bhuwan C. Bhatt, Devendra K. Sahu;
    2023, JApA, 44, 2, id.58
  5. Kronberger 55: A candidate for end-dominated collapse scenario
    Ayushi Verma, Saurabh Sharma, Lokesh Dewangan, Rakesh Pandey, Tapas Baug, Devendra K. Ojha, Arpan Ghosh, Harmeen Kaur;
    2023, JApA, 44, 1, id 52
  6. Spectroscopy of nine eruptive young variables using TANSPEC
    Arpan Ghosh, Saurabh Sharma, Joe P. Ninan, Devendra K. Ojha, A. S. Gour, Rakesh Pandey, Tirthendu Sinha, Ayushi Verma, Koshvendra Singh, Supriyo Ghosh, Harmeen Kaur;
    2023, JApA, 44, 1, id 50
  7. Teutsch 76: A deep near-infrared study
    Saurabh Sharma, Lokesh Dewangan, Neelam Panwar, Harmeen Kaur, Devendra K. Ojha, Ramkesh Yadav, Ayushi Verma, Tapas Baug, Tirthendu Sinha, Rakesh Pandey, Arpan Ghosh, Tarak Chand;
    2023, JApA, 44, 1, id 46
  8. PYTANSPEC: A data reduction package for TANSPEC
    Supriyo Ghosh, Joe P. Ninan, Devendra K. Ojha, Saurabh Sharma;
    2023, JApA, 44, 1, id 30
  9. pyTANSPEC: Python tool for extracting 1D TANSPEC spectra from 2D images
    Supriyo Ghosh, Joe P. Ninan, Devendra K. Ojha, Saurabh Sharma;
    2022, Astrophysics Source Code Library, record ascl:2212.014
  10. Optical and near-infrared spectroscopy of Nova V2891 Cygni: evidence for shock-induced dust formation
    V. Kumar, M. K. Srivastava, D. P. K. Banerjee, C. E. Woodward, U. Munari, A. Evans, V. Joshi, S. Dallaporta, and K. L. Page;
    2022, MNRAS, 510(3):4265–4283
  11. Gaia 20eae: A Newly Discovered Episodically Accreting Young Star
    A. Ghosh, S. Sharma, J. P. Ninan, D. K. Ojha, B. C. Bhatt, S. Kanodia, S. Mahadevan, G. Stefansson, R. K. Yadav, A. S. Gour, R. Pandey, T. Sinha, N. Panwar, J. P. Wisniewski, C. I. Cañas, A. S. J. Lin, A. Roy, F. Hearty, L. Ramsey, P. Robertson, and C. Schwab;
    2022, ApJ, 926(1):68
  12. TANSPEC: TIFR-ARIES Near-infrared Spectrometer
    Saurabh Sharma, Devendra K. Ojha, Arpan Ghosh, Joe P. Ninan, Supriyo Ghosh, Swarna K. Ghosh, Manoj, Milind B. Naik, Savio L. A. D'Costa, B. Krishna Reddy, Nandish Nanjappa, Rakesh Pandey, Tirthendu Sinha, Neelam Panwar, Susmitha Antony, Harmeen Kaur, Sanjit Sahu, Tarun Bangia, Satheesha S. Poojary, Rajesh B. Jadhav, Shailesh B. Bhagat, Ganesh S. Meshram, Harshit Shah, John T. Rayner, Douglas Toomey, Pradeep R. Sandimani;
    2022, PASP, 134, 1038, id 085002, 23pp
  13. TIFR Treasures for Astronomy from Ground to Space.
    S. Ghosh, D. K. Ojha, S. Sharma, and M. B. Naik;
    2022, JApA, 43, 16
  14. 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; (arXiv : 1902.05857)
  15. 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)
  16. Prospects for star formation studies with infrared instruments (TIRCAM2 and TANSPEC) on the 3.6-m Devasthal Optical Telescope
    Devendra Ojha; Swarna Kanti Ghosh; Saurabh Sharma; Anil Kumar Pandey, ; Tapas Baug; Joe Philip Ninan, ; Brijesh Kumar, Manoj Puravankara, Savio D'Costa; Milind Naik; Satheesha Poojari, ; Shailesh Bhagat, ; Rajesh Jadhav, ; Ganesh Meshram, ; Pradeep Sandimani, Sanjay Gharat; Chandrakant Bakalkar
    2018, BSRSL, 87, 58-87
  17. Prospects of star formation studies with near-infrared instruments on 2-4 meter class Indian ground-based telescopes
    Devendra Kumar Ojha, S. K. Ghosh, Tapas Baug, Priyanka Chaturvedi, Puravankara Manoj, Savio L. A. DCosta, Milind B. Naik, Sateesh s. Poojary, Pradeep R. Sandimani, J. P. Ninan, Saurabh Sharma, A. K. Pandey;
    2018, The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life. Edited by Takafumi Ootsubo, Issei Yamamura, Kazumi Murata and Takashi Onaka. pp.257-260