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Sample Program of Study - Nurse Anesthetist Program 126 Credits* (Specialty coursework in BOLD) Year One – Preclinical Year Summer Cr Fall Cr Spring Cr NAN 543 Principles of Anesthesia I 3 NAN 718 Prof Aspects NA I 1 NAN 544 Principles of Anes II 2 NGC 501 Conceptual Foundations 3 NGC 527 Eval and Gen Evidence for HC II 3 NAN 544L Principles of Anes II Lab 1 NGC 518 Health Promotion 3 NGC 527L Eval and Gen Evidence II Lab 1 NAN 672 Pharm Anesth/Adj Drugs 3 NGC 520 Scientific Communications 2 NGC 634 Organizational Leadership 3 NAN 719 Prof Aspects NA II 1 NGC 625 Pathophysiology for APN I 3 NGC 575 Adv Helth Assessmnt (CRNA) 2 NGC 502 Informatics 3 NGC 612 Pharmacotherapeutics 4 NGC 509 Ethics* 3 NGC 626 Pathophysiology for APN II 3 NGC 526 Eval and Gen Evidence for HC I 4 Total Credits 14 Total Credits 17 Total Credits 17 Year Two – Clinical Year I Summer Fall Spring NAN 598 Intro to NA Clin Prac (1 d/wk) 2 NAN 545 Principles of Anes III 3 NAN 546 Principles of Anes IV 3 NAN 601 NA Clin Pract I (3 d/wk) 6 NAN 602 NA Clin Pract II (4 d/wk) 8 NAN 603 NA Clin Pract III (4 d/wk) 8 NGC 632 Interpreting HC Policy 3 NAN 711 Current Top Anes 1 NAN 712 Current Top Anes II 1 NGC 692 Grantsmanship 1 NGC 701 State of the Science 3 NAN 721 Anes Crisis Res Mgt I 1 NGC 638 Program Evaluation 3 Total Credits 12 Total Credits 15 Total Credits 16 Year Three – Clinical Year II Summer Fall Spring NAN 604 NA Clin Pract IV (4 d/wk) 6 NAN 605 NA Clin Pract V (4 d/wk) 6 NAN 547 Principles of Anes V 3 NGC 725 DNP Advanced Clinical Prac I 2 NAN 713 Current Top Anes III 1 NAN 606 NA Clin Pract VI (4 d/wk) 8 NGC 798 DNP Capstone Course I 1 NAN 722 Anes Crisis Res Mgt II 1 NAN 714 Current Top Anes IV 1 NGC 533 Teaching in Nursing 3 NGC 726 DNP Advanced Clinical Prac II 2 NGC 799 DNP Capstone Course II 1 Total Credits 9 Total Credits 14 Total Credits 12 *Effective for all students matriculating Spring 2015 and thereafter, N509 is not a required course and the total credits will be 123. 6-19-2015 .

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Infrared Spectroscopy of Nearby Radio Active Elliptical Galaxies
The Astrophysical Journal Supplement Series, 203:14 (11pp), 2012 November doi:10.1088/0067-0049/203/1/14 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES Jeremy Mould1,2,9, Tristan Reynolds3, Tony Readhead4, David Floyd5, Buell Jannuzi6, Garret Cotter7, Laura Ferrarese8, Keith Matthews4, David Atlee6, and Michael Brown5 1 Centre for Astrophysics and Supercomputing Swinburne University, Hawthorn, Vic 3122, Australia; [email protected] 2 ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) 3 School of Physics, University of Melbourne, Melbourne, Vic 3100, Australia 4 Palomar Observatory, California Institute of Technology 249-17, Pasadena, CA 91125 5 School of Physics, Monash University, Clayton, Vic 3800, Australia 6 Steward Observatory, University of Arizona (formerly at NOAO), Tucson, AZ 85719 7 Department of Physics, University of Oxford, Denys, Oxford, Keble Road, OX13RH, UK 8 Herzberg Institute of Astrophysics Herzberg, Saanich Road, Victoria V8X4M6, Canada Received 2012 June 6; accepted 2012 September 26; published 2012 November 1 ABSTRACT In preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ , and [Fe ii]. We consider the inﬂuence of radio power and black hole mass in relation to the spectra. Access to the spectra is provided here as a community resource. Key words: galaxies: elliptical and lenticular, cD – galaxies: nuclei – infrared: general – radio continuum: galaxies ∼ 1. INTRODUCTION 30% of the most massive galaxies are radio continuum sources (e.g., Fabbiano et al.
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HUBBLE SPACE TELESCOPE and GROUND-BASED OBSERVATIONS of the TYPE Iax SUPERNOVAE SN 2005Hk and SN 2008A
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ATNF News Issue No
Galaxy Pair NGC 1512 / NGC 1510 ATNF News Issue No. 67, October 2009 ISSN 1323-6326 Questacon "astronaut" street performer and visitors at the Parkes Open Days 2009. Credit: Shaun Amy, CSIRO. Cover page image Cover Figure: Multi-wavelength color-composite image of the galaxy pair NGC 1512/1510 obtained using the Digitised Sky Survey R-band image (red), the Australia Telescope Compact Array HI distribution (green) and the Galaxy Evolution Explorer NUV -band image (blue). The Spitzer 24µm image was overlaid just in the center of the two galaxies. We note that in the outer disk the UV emission traces the regions of highest HI column density. See article (page 28) for more information. 2 ATNF News, Issue 67, October 2009 Contents From the Director ...................................................................................................................................................................................................4 CSIRO Medal Winners .........................................................................................................................................................................................5 CSIRO Astronomy and Space Science Unit Formed ........................................................................................................................6 ATNF Distinguished Visitors Program ........................................................................................................................................................6 ATNF Graduate Student Program ................................................................................................................................................................7
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A Basic Requirement for Studying the Heavens Is Determining Where In
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A DEEP SEARCH for PROMPT RADIO EMISSION from THERMONUCLEAR SUPERNOVAE with the VERY LARGE ARRAY Laura Chomiuk1,11, Alicia M
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Arxiv:1801.08245V2 [Astro-Ph.GA] 14 Feb 2018
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X-Ray Luminosities for a Magnitude-Limited Sample of Early-Type Galaxies from the ROSAT All-Sky Survey
Mon. Not. R. Astron. Soc. 302, 209±221 (1999) X-ray luminosities for a magnitude-limited sample of early-type galaxies from the ROSAT All-Sky Survey J. Beuing,1* S. DoÈbereiner,2 H. BoÈhringer2 and R. Bender1 1UniversitaÈts-Sternwarte MuÈnchen, Scheinerstrasse 1, D-81679 MuÈnchen, Germany 2Max-Planck-Institut fuÈr Extraterrestrische Physik, D-85740 Garching bei MuÈnchen, Germany Accepted 1998 August 3. Received 1998 June 1; in original form 1997 December 30 Downloaded from https://academic.oup.com/mnras/article/302/2/209/968033 by guest on 30 September 2021 ABSTRACT For a magnitude-limited optical sample (BT # 13:5 mag) of early-type galaxies, we have derived X-ray luminosities from the ROSATAll-Sky Survey. The results are 101 detections and 192 useful upper limits in the range from 1036 to 1044 erg s1. For most of the galaxies no X-ray data have been available until now. On the basis of this sample with its full sky coverage, we ®nd no galaxy with an unusually low ¯ux from discrete emitters. Below log LB < 9:2L( the X-ray emission is compatible with being entirely due to discrete sources. Above log LB < 11:2L( no galaxy with only discrete emission is found. We further con®rm earlier ®ndings that Lx is strongly correlated with LB. Over the entire data range the slope is found to be 2:23 60:12. We also ®nd a luminosity dependence of this correlation. Below 1 log Lx 40:5 erg s it is consistent with a slope of 1, as expected from discrete emission.
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2.5-11 Micron Spectroscopy and Imaging of Agns: Implication For
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