UWISH2 -- The UKIRT Widefield Infrared Survey for H2
D., Froebrich, C.J., Davis, G., Ioannidis, T.M., Gledhill, M., Takami,, A., Chrysostomou, J., Drew, J., Eisl\"offel, A., Gosling, R., Gredel, J.,, Hatchell, K.W., Hodapp, M.S.N., Kumar, P.W., Lucas, H., Matthews, M.G.,, Rawlings, M.D., Smith, B., Stecklum, W.P., Varricatt, H.T.

TL;DR
The UWISH2 survey provides high-resolution near-infrared imaging of the First Galactic Quadrant, revealing star formation activities, planetary nebulae, and variable stars, complementing existing surveys and enhancing understanding of dynamic processes in the galaxy.
Contribution
This survey offers the first comprehensive, high-resolution narrow-band imaging of the region, uncovering new astrophysical phenomena and objects related to star formation and stellar evolution.
Findings
Detection of jets and outflows from young stellar objects
Discovery of new planetary nebulae
Identification of numerous variable stars
Abstract
We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). This area includes most of the Giant Molecular Clouds and massive star forming regions in the northern hemisphere. The survey is centred on the 1-0S(1) ro-vibrational line of H2, a proven tracer of hot, dense molecular gas in star-forming regions, around evolved stars, and in supernova remnants. The observations complement existing and upcoming photometric surveys (Spitzer-GLIMPSE, UKIDSS-GPS, JCMT-JPS, AKARI, Herschel Hi-GAL, etc.), though we probe a dynamically active component of star formation not covered by these broad-band surveys. Our narrow-band survey is currently more than 60% complete. The median seeing in our images is 0.73arcsec. The images have a 5sigma detection limit of point sources of K=18mag and the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
