The source catalog includes 662 sources, reaches a limiting unabsorbed luminosity of ∼2.4 ×10 34 erg s −1 in the 0.35–8.0 keV energy band, and contains source positions, source net counts, fluxes and significances in several energy bands, and information on source variability. With a total exposure time of 1.4 Ms, ChASeM33 covers ∼70% of the D 25 isophote ( R ≈ 4.0 kpc) of M33 and provides the deepest, most complete, and detailed look at a spiral galaxy in X-rays.
This study presents the final source catalog of the Chandra ACIS Survey of M33 (ChASeM33).
WD DRIVE UTILITIES 2.0 0.71 CODE
1 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USAģ NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USAĤ Astronomy Department, University of Washington, Seattle, WA 98195, USAĥ Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, 85741 Garching, GermanyĦ Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USAħ Institut für Astronomie und Astrophysik, Eberhard Karls Universität, Tübingen, GermanyĨ Department of Physics, Middlebury College, Middlebury, VT 05753, USAĩ Space Science Center, 235 Martindale Drive, Morehead State University, Morehead, KY 40351, USAġ0 Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USAġ1 Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019, USAġ2 School of Physics and Astronomy, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israelġ3 Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive, Santa Barbara, CA 93117, USAġ4 Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93106, USA
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