Experience Report on an Undergraduate Project in Distributed Systems

Omar, A.; Bance, Jared; Behan, Christopher W; Bowden, Brian; Crites, Sebastian; Dhillon, Arshdeep; Dimond, Eric; Eliopoulos, Ian; Fawcett, Alexandria; Friesen, Micheal; Hossain, Nayem; Jantzen, Kurtis; Kelly, A. J.; Kenny, David A.; Kernaghan, Kayleigh; Kim, Sunah; Kruger, Brenton; Lysov, Anton; Ma, Siyuan; McGregor, Bryan; Meston, Levi; Pham, Richard; Phan, Quan Anh; Rehman, Zia Ur; Sawatzky, Mitchell; Schulze, Peter; Seguin, Stuart; Senger, Rebecca; Settle, Patrick; Shabash, Yehonatan; Syed, Masroor; Tarannum, Mehnaz; Thompson, Colin; Tomar, Saurabh; Unarce, Kevin; Egmond, Joel van; Verwaayen, Michael; Vogelaar, Steven; Williamson, Aaron; Yu, Selena; Giv, Mehrdad Jafari; Kawash, Jalal

doi:10.1109/csci49370.2019.00159

Cited by 1 publication

(1 citation statement)

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“…The FOSC-type instrument (hereafter ADFOSC; ARIES-Devasthal FOSC), developed in ARIES (Aryabhatta Research Institute of observational sciences), Nainital, is presently undergoing commissioning. Details of the ADFOSC and the Charge-Coupled Device (CCD) camera are presented elsewhere (Omar et al 2012;Omar et al 2019). The ADFOSC has a collimator and focal-reducer optics, converting the f/9 beam from the DOT to ∼f/4.3 Notes:…”

Section: Instrument Description and Observationsmentioning

confidence: 99%

Optical detection of a GMRT-detected candidate high-redshift radio galaxy with 3.6-m Devasthal optical telescope

et al. 2019

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We report optical observations of TGSS J1054+5832, a candidate high-redshift (z = 4.8 ± 2) steepspectrum radio galaxy, in r and i bands using the faint object spectrograph and camera mounted on 3.6-m Devasthal Optical Telescope (DOT). The source previously detected at 150 MHz from Giant Meterwave Radio Telescope and at 1420 MHz from Very Large Array has a known counterpart in near-infrared bands with K-band magnitude of AB 22. The source is detected in i-band with AB24.3 ± 0.2 magnitude in the DOT images presented here. The source remains undetected in the r-band image at a 2.5σ depth of AB 24.4 mag over an 1.2 × 1.2 aperture. An upper limit to i − K color is estimated to be ∼2.3, suggesting youthfulness of the galaxy with active star formation. These observations highlight the importance and potential of the 3.6-m DOT for detections of faint galaxies.

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Section: Instrument Description and Observationsmentioning

confidence: 99%