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TIRCAM2 is the facility near-infrared Imager at the Devasthal 3.6-m telescope in northern India, equipped with an Aladdin III InSb array detector. We have pioneered the use of TIRCAM2 for very fast photometry, with the aim of recording…

We present a program of routine lunar occultations, at optical and near-IR wavelengths, recently started at the 1.5m Spanish telescope at the Calar Alto Observatory. Both a CCD and an infrared array detector are used. The program is aimed…

天体物理学 · 物理学 2007-05-23 O. Fors , A. Richichi , J. Nunez , A. Prades

We present an update of the lunar occultation program which is routinely carried out in the near-IR at the Calar Alto Observatory. A total of 350 events were recorded since our last report (Fors et al. 2004). In the course of eight runs we…

天体物理学 · 物理学 2016-08-30 A. Richichi , O. Fors , M. Merino , X. Otazu , J. Nunez , A. Prades , U. Thiele , D. Perez-Ramirez , F. J. Montojo

The TIFR Near Infrared Imaging Camera-II (TIRCAM2) is being used at the Devasthal Optical Telescope (DOT) operated by Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, Uttarakhand, India. In addition to the normal…

天体物理仪器与方法 · 物理学 2023-06-07 Milind B. Naik , Devendra K. Ojha , Saurabh Sharma , Shailesh B. Bhagat , Savio L. D'Costa , Arpan Ghosh , Koshvendra Singh

We report on 25 sub-arcsecond binaries, detected for the first time by means of lunar occultations in the near-infrared as part of a long-term program using the ISAAC instrument at the ESO Very Large Telescope. The primaries have magnitudes…

太阳与恒星天体物理 · 物理学 2015-06-16 A. Richichi , O. Fors , F. Cusano , M. Moerchen

We report on 13 sub-arcsecond binaries, detected by means of lunar occultations in the near-infrared at the ESO Very Large Telescope. They are all first-time detections, except for the visual binary HD~158122 which we resolved for the first…

太阳与恒星天体物理 · 物理学 2015-06-18 Andrea Richichi , Octavi Fors , Felice Cusano , Valentin Ivanov

(Abridged) Lunar occultations (LO) are a very efficient and powerful technique, that achieves the best combination of high angular resolution and sensitivity possible today at near-infrared wavelengths. Given that the events are fixed in…

太阳与恒星天体物理 · 物理学 2015-05-19 A. Richichi , O. Fors , W-P. Chen , E. Mason

The TIFR Near Infrared Imaging Camera-II (TIRCAM2) is being used at the 3.6 m Devasthal Optical Telescope (DOT) operated by Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, Uttarakhand, India. Earlier, the TIRCAM2…

The 3.6 meter Indo-Belgian Devasthal optical telescope (DOT) has been used for optical and near-infrared (NIR) observations of celestial objects. The telescope has detected stars of B = 24.5+-0.2; R = 24.6+-0.12 and g = 25.2+-0.2 mag in…

天体物理仪器与方法 · 物理学 2020-12-17 Ram Sagar , Brijesh Kumar , Saurabh Sharma

We report further results from the program of lunar occultation (LO) observations started at the 2.4-m Thai National Telescope (TNT) in 2014. We have recorded LO events of 18 stellar sources, leading to the detection of four angular…

太阳与恒星天体物理 · 物理学 2015-12-22 A. Richichi , O. Tasuya , P. Irawati , B. Soonthornthum , V. S. Dhillon , T. R. Marsh

We report the angular diameters of two Mira variables (U Ari and Z Sco), three semiregular (SR) and irregular variables (SW Vir, eta Gem and mu Gem) and a supergiant SR variable (TV Gem) by lunar occultation observations in the near-IR…

天体物理学 · 物理学 2008-11-26 Soumen Mondal , T. Chandrasekhar

We present lunar occultation observations obtained in August 2006 with the recently demonstrated burst mode of the ISAAC instrument at the ESO VLT. The results presented here follow the previously reported observations carried out in March…

天体物理学 · 物理学 2009-11-13 A. Richichi , O. Fors , E. Mason

Lunar occultations (LO) provide a unique combination of high angular resolution and sensitivity at near-infrared wavelenghts. At the ESO Very Large Telescope, it is possible to achieve about 1 milliarcsecond (mas) resolution and detect…

太阳与恒星天体物理 · 物理学 2015-05-28 A. Richichi , W. P. Chen , O. Fors , P. F. Wang

For the first time, the lunar occultation technique has been employed on a very large telescope in the near-IR with the aim of achieving systematically milliarcsecond resolution on stellar sources. We have demonstrated the burst mode of the…

天体物理学 · 物理学 2009-11-13 A. Richichi , O. Fors , E. Mason , J. Stegmaier , T. Chandrasekhar

TIFR Near Infrared Imaging Camera-II is a closed-cycle Helium cryo-cooled imaging camera equipped with a Raytheon 512 x 512 pixels InSb Aladdin III Quadrant focal plane array having sensitivity to photons in the 1-5 microns wavelength band.…

The recently inaugurated 2.4\,m Thai National Telescope (TNT) is equipped, among other instruments, with the ULTRASPEC low-noise, frame-transfer EMCCD camera. At the end of its first official observing season, we report on the use of this…

太阳与恒星天体物理 · 物理学 2015-06-22 A. Richichi , P. Irawati , B. Soonthornthum , V. S. Dhillon , T. R. Marsh

India and Belgium have jointly established two 4 meter class optical telescopes at Devasthal located in Nainital, India. After successful installation of the 3.6-m modern new technology Devasthal Optical Telescope (DOT) in 2015, it was…

天体物理仪器与方法 · 物理学 2019-09-02 Ram Sagar , Brijesh Kumar , Annapurni Subramaniam

By cross-matching the eclipsing binary catalog from TESS with that from LAMOST MRS, semi-detached eclipsing binaries with radial velocities coverage spanning more than 0.3 phases were authenticated. The absolute parameters for these systems…

太阳与恒星天体物理 · 物理学 2024-12-11 Yajuan Lei , Guiping Zhou , Liang Wang , Guangwei Li , Kai Li , Tuan Yi

Context: Trans-Neptunian objects are distant bodies that retain valuable information about the origin and evolution of the Solar System. Many of these objects constitute binary systems. Studying binaries allows us to further characterise…

地球与行星天体物理 · 物理学 2026-05-22 J. M. Gómez-Limón , R. Leiva , J. L. Ortiz , P. Santos-Sanz , M. Kretlow , Y. Kilic , J. L. Rizos , A. Álvarez-Candal , T. G. Müller

TIRCAM2 (TIFR Near Infrared Imaging Camera - II) is a closed cycle cooled imager that has been developed by the Infrared Astronomy Group at the Tata Institute of Fundamental Research for observations in the near infrared band of 1 to 3.7…

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