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Grant Proposals, 1991-1999 Finding aid prepared by Smithsonian Institution Archives Smithsonian Institution Archives Washington, D.C. Contact us at [email protected] Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Descriptive Entry.............................................................................................................. 1 Names and Subjects ...................................................................................................... 1 Container Listing ............................................................................................................. 2 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Collection Overview Repository: Smithsonian Institution Archives, Washington, D.C., [email protected] Title: Grant Proposals Identifier: Accession 99-171 Date: 1991-1999 Extent: 17 cu. ft. (17 record storage boxes) Creator:: Smithsonian Astrophysical Observatory. Contracts and Procurement Office Language: English Administrative Information Prefered Citation Smithsonian Institution Archives, Accession 99-171, Smithsonian Astrophysical Observatory, Contracts and Procurement Office, Grant Proposals Descriptive Entry This accession consists of records documenting Smithsonian Astrophysical Observatory projects and activities. Materials include proposals, correspondence, progress reports, cost estimates, notes, final project reports, research announcements, and memoranda. Names and Subject Terms This collection is indexed in the online catalog of the Smithsonian Institution under the following terms: Subjects: Astronomy Astrophysical observatories Astrophysics Contracts Types of Materials: Manuscripts Page 1 of 48 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Container Listing Box 1 Box 1 of 17 P2405-4-91, High Resolution X-ray Observation of M81, 04/01/1991-10/04/1991 Box 1 of 17 P2406-4-91, Hunting for Cool Loops: The Dividing Line Revisited, 04/01/1991-05/05/1992 Box 1 of 17 P2407-4-91, PSPC X-ray Spectral Observations of Supernova Remnant E0102.2-72.2 in the Small Magellanic Cloud, 04/01/1991-10/04/1991 Box 1 of 17 P2408-4-91, A Comparison of Non-thermal Pressure in Radio Features with Gas Pressure in Clusters and Super Clusters, 04/01/1991-08/19/1991 Box 1 of 17 P2409-4-91, ROSAT Selected Area Survey - DRACO, 04/01/1991-08/19/1991 Box 1 of 17 P2410-4-91, An X-ray Study of Cluster Gravitational Lenses, 04/01/1991-10/04/1991 Box 1 of 17 P2411-4-91, Evidence for a Multiphase ISM in Early Type Galaxies, 04/01/1991-10/04/1991 Box 1 of 17 P2412-4-91, The Inner Accretion Disk of Black Hole A0620-00, 04/01/1991-10/02/1991 Box 1 of 17 P2413-4-91, Gravitational Lensing of Active Galaxies, 04/01/1991-08/19/1991 Box 1 of 17 P2414-4-91, The Interstellar Matters of NGC 1052, 04/01/1991-08/19/1991 Box 1 of 17 P2415-4-91, Distribution of dark and Luminous Matter in Clusters, 04/01/1991-10/04/1991 Box 1 of 17 P2416-4-91, Is There an IR/X-Ray Connection for Radio-Quiet Quasars?, 03/26/1991-09/18/1992 Box 1 of 17 P2417-4-91, ROSAT PSPC Observations of Three Clusters of Galaxies: Targets for the Sunyaev_Zeldovich Effect, 04/01/1991-08/23/1991 Box 1 of 17 P2418-4-91, How Do the Spectra of AGN in the Einstein Medium Sensitivity Survey Relate to the Production of the Diffuse Background, 04/01/1991-04/02/1991 Page 2 of 48 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Box 1 of 17 P2419-4-91, The Multiphase Interstellar Medium of M86, 04/01/1991-08/19/1991 Box 1 of 17 P2420-4-91, Centaurus A- The Nearest Bright Elliptical Galaxy, 04/01/1991-08/19/1991 Box 1 of 17 P2421-4-91, The Soft X-Ray Flux of SN1987A, 04/01/1991-12/09/1991 Box 1 of 17 P2422-4-91, Study of Lunar Internal Structure Using Lunar Laser Ranging Data, 01/01/1991-04/10/1991 Box 1 of 17 P2423-4-91, ROSAT High Spatial Resolution Observations of Kepler's Supernova Remnant, 03/29/1991-12/09/1991 Box 1 of 17 P2424-4-91, Investigation of The Large Amounts of Cold, X-Ray Absorbing Matter in Clusters of Galaxies, 03/28/1991-10/04/1991 Box 1 of 17 P2425-4-91, Soft X-Ray Spectra of AGN Discovered via Their Hard X-Ray Emission, 03/28/1991-10/02/1991 Box 1 of 17 P2426-4-91, ROSAT PSPC and HRI Observations of Supernova Remnant G292.0+1.8, 03/28/1991-09/28/1992 Box 1 of 17 P2427-4-91, Hot Intergalactic Medium in Edge on Spirals, 03/29/1991-08/19/1991 Box 1 of 17 P2428-4-91, The Soft X-Ray Emission Component of Spiral Galaxies, 03/29/1991-03/04/1992 Box 1 of 17 P2429-4-91, Identification and Study of BL LAC Objects in the Einstein Medium Sensitivity Survey , 03/29/1991-10/04/1991 Box 1 of 17 P2430-4-91, A194-A low X-Ray Luminosity, E /SO Rich Linear Cluster, 03/29/1991-10/04/1991 Box 1 of 17 P2431-4-91, Are Large Core Radius Clusters Merging Systems?, 03/29/1991-08/19/1991 Box 1 of 17 P2432-4-91, The Origin of X-Ray Emission in Late B-type Stars: HD 100841, a Case Study, 03/28/1991-08/19/1991 Box 1 of 17 P2433-4-91, Wind Interaction in Planetary Nebulae, 03/29/1991-04/04/1991 Box 1 of 17 P2434-4-91, A Deep X-ray of the Pleiades, 03/28/1991-12/09/1991 Page 3 of 48 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Box 1 of 17 P2435-4-91, ROSAT Observations of the X-ray Binary HD 154791, 03/29/1991-04/04/1991 Box 1 of 17 P2436-4-91, A Search For Substructure in High X-ray Luminosity Clusters of Galaxies, 04/02/1991-07/15/1992 Box 1 of 17 P2437-4-91, Deep Imaging in Taurus: Dark Cloud Cores With and Without T Tauri Stars, 04/02/1991-07/15/1992 Box 1 of 17 P2438-4-91, Classical Cepheids: Chromospheric Heating and Formation of the Helium Spectrum, 04/02/1991-04/04/1991 Box 1 of 17 P2439-4-91, X-ray Variability: A Probe of Heating Mechanisms of Inactive Coronae, 03/27/1991-04/04/1991 Box 1 of 17 P2440-4-91, The Soft X-ray Excess and The Big Blue Bump in Quasar, 03/27/1991-04/04/1991 Box 1 of 17 P2441-4-91, Coordinated ROSAT and Speckle Observations of the Mira AB System, 04/03/1991-10/17/1991 Box 1 of 17 P2442-4-91, Measuring the Gas Mass in Clusters, 03/27/1991-10/04/1991 Box 1 of 17 P2443-4-91, Inverse Compton Emission From Relic Radio Sources, 03/25/1991-08/19/1991 Box 1 of 17 P2444-4-91, Red Quasars, 03/26/1991-04/04/1991 Box 1 of 17 P2445-4-91, X-ray Quiet (But Detected) Quasars, 03/26/1991-10/02/1991 Box 1 of 17 P2446-4-91, "X-ray Transients in the 5-kpc Arm," 03/27/1991-08/19/1991 Box 1 of 17 P2447-4-91, A Grand Design Spiral Galaxy With an Interacting Companion N5194 and N5195, 03/29/1991-10/02/1991 Box 1 of 17 P2448-4-91, Astrometric Observations of Comets and Asteroids and Subsequent Orbital Investigations, 03/28/1991-10/08/1991 Box 1 of 17 P2449-4-91, Measurements of Atomic Interactions and Frequency Stability with a Cryogenic Hydrogen Maser, 04/05/1991-04/15/1991 Box 1 of 17 P2450-4-91, Repair P-1 Maser and Prepare to Ship Maser to Australia, 04/15/1991-09/24/1991 Page 4 of 48 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Box 1 of 17 P2451-4-91, An UltraViolet Coronagraph Spectrometer for SOHO, 04/18/1991-02/26/1992 Box 1 of 17 P2452-4-91, Increasing Resonant Frequency of An UltraViolet Coronagraph Spectrometer for Soho, 04/22/1991-02/26/1992 Box 1 of 17 P2453-4-91, Two Advanced Hydrogen Masers Incorporating an Adiabatic Fast Passage Selection System, 02/28/1991-10/31/1991 Box 1 of 17 P2454-4-91, The Luminosity Function of the Trapezium Cluster - An Observational Test of Bi Modal Star Formation Models, 04/24/1991-04/29/1991 Box 1 of 17 P2455-4-91, The Resonance Lines of Mg II as Diagnostics of the Upper Solar Chromosphere, 04/30/1991-05/02/1991 Box 2 Box 2 of 17 P2456-5-91, Design and Manufacture of High Speed Charge-Coupled Device Wavefront Images, 05/01/1991-10/24/1991 Box 2 of 17 P2457-5-91, Enhancements to Financial Reporting Cost Growth in Materials and Subcontracting, and Cost Growth Due to Negotiated Forward Pricing Rates, 01/09/1990-10/24/1991 Box 2 of 17 P2458-5-91, Development of Points as a Planetology Instrument, 05/10/1991-01/15/1992 Box 2 of 17 P2459-5-91, Cost Associated With Multiple Iterations of EID Part A, 05/21/1991-12/10/1991 Box 2 of 17 P2460-5-91, The X-ray Structure of Centaurus A: the Nearest Jet and Its Host, 05/21/1991-05/31/1991 Box 2 of 17 P2461-5-91, SAO Participation in the Cooling of Molecular Gas By Far- Infrared and Submillimeter Line Emission, 02/29/1991-11/27/1991 Box 2 of 17 P2462-5-91, A Consortium Request for Space Telescope Director's Discretionary Time, 05/29/1991-06/05/1991 Box 2 of 17 P2463-6-91, Analysis and Interpretation of Coordinated Solar Eclipse Observations, 06/04/1991-06/12/1991 Box 2 of 17 P2464-6-91, Exotic Molecules in Space, 06/04/1991-08/16/1994 Page 5 of 48 Grant Proposals https://siarchives.si.edu/collections/siris_arc_251859 Box 2 of 17 P2465-6-91, A Spectroscopic Investigation of the Comet- Asteroid Interrelation, 06/07/1991-06/10/1991 Box 2 of 17 P2466-6-91, Research on Infrared Spectroscopy, Opacity and Atmospheres, 06/06/1991-04/07/1994 Box 2 of 17 P2467-6-91, Repair MIT Maser, S/N P-2, 06/06/1991-06/11/1991 Box 2 of 17 P2468-6-91, A Ginga Visiting Investigator Program of LAC/Slew Survey Intercomparisons, 06/11/1991-06/13/1991 Box 2 of 17 P2469-6-91, A Ginga Visiting Investigator Program Studies of Clusters of Galaxies and Supernova Remnants, 06/11/1991-11/04/1991 Box 2 of 17 P2470-6-91, Lift Table to Support AXAF Synchrotron Program, 06/13/1991-06/18/1991 Box 2 of
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    An X-Ray Upper Limit on the Presence of a Neutron Star for the Small

    An X-ray upper limit on the presence of a Neutron Star for the Small Magellanic Cloud and Supernova Remnant 1E0102.2-7219 M.J. Rutkowski1, E. M. Schlegel2, J. W. Keohane3 and R. A. Windhorst1 [email protected] ABSTRACT We present Chandra X-ray Observatory archival observations of the supernova rem- nant 1E0102.2-7219, a young Oxygen-rich remnant in the Small Magellanic Cloud. Combining 28 ObsIDs for 324 ks of total exposure time, we present an ACIS image with an unprecedented signal-to-noise ratio (mean S/N √S 6; maximum S/N > ≃ ∼ 35) . We search within the remnant, using the source detection software wavdetect, for point sources which may indicate a compact object. Despite finding numerous de- tections of high significance in both broad and narrow band images of the remnant, we are unable to satisfactorily distinguish whether these detections correspond to emission from a compact object. We also present upper limits to the luminosity of an obscured compact stellar object which were derived from an analysis of spectra extracted from the high signal-to-noise image. We are able to further constrain the characteristics of a potential neutron star for this remnant with the results of the analysis presented here, though we cannot confirm the existence of such an object for this remnant. 1. Introduction The supernova remnant 1E 0102.2-7219 (SNR 1E0102.2-7219, hereafter, “E0102”) was first identified by Seward & Mitchell (1981) in a survey of the Small Magellanic Cloud (SMC) with the Einstein X-Ray Observatory. While this oxygen-rich remnant resides at a distance of 59 kpc (van den Bergh 1999), it is far less extincted than many Galactic remnants due to its high galactic arXiv:1005.0635v1 [astro-ph.GA] 4 May 2010 latitude (l –45◦).
  • Search for Gamma-Ray Emission from AE Aquarii with Seven Years of FERMI-LAT Observations

    Search for Gamma-Ray Emission from AE Aquarii with Seven Years of FERMI-LAT Observations

    Search for gamma-ray emission from AE Aquarii with seven years of FERMI-LAT observations Jian Li1, Diego F. Torres1,2, Nanda Rea1,3, Emma de O˜na Wilhelmi1, Alessandro Papitto4, Xian Hou5, & Christopher W. Mauche6 ABSTRACT AE Aquarii (AE Aqr) is a cataclysmic binary hosting one of the fastest rotating (Pspin = 33.08 s) white dwarfs known. Based on seven years of Fermi Large Area Tele- scope (LAT) Pass 8 data, we report on a deep search for gamma-ray emission from æ. Using X-ray observations from ASCA, XMM-Newton, Chandra, Swift, Suzaku, and NuSTAR, spanning 20 years, we substantially extend and improve the spin ephemeris of æ. Using this ephemeris, we searched for gamma-ray pulsations at the spin period of the white dwarf. No gamma-ray pulsations were detected above 3 σ significance. Neither phase-averaged gamma-ray emission nor gamma-ray variability of æ is de- tected by Fermi-LAT. We impose the most restrictive upper limit to the gamma-ray flux from æ to date: 1.3 × 10−12 erg cm−2 s−1 in the 100 MeV–300 GeV energy range, providing constraints on models. Subject headings: gamma rays: stars — cataclysmic binary: individual: æ 1. Introduction Cataclysmic variables (CVs) are semi-detached binaries consisting of a white dwarf (WD) and a companion star, usually a red dwarf. æ is a bright (V≈11, Welsh et al. 1999) CV hosting one of the fastest rotating WDs known (Pspin = 33.08 s, Patterson 1979) and a K 4-5 V secondary; it is arXiv:1608.06662v1 [astro-ph.HE] 23 Aug 2016 1Institute of Space Sciences (IEEC-CSIC), Campus UAB, Carrer de Magrans s/n, 08193 Barcelona, Spain 2Instituci´oCatalana de Recerca i Estudis Avanc¸ats (ICREA), E-08010 Barcelona, Spain 3Anton Pannekoek Institute, University of Amsterdam, Postbus 94249, NL-1090-GE Amsterdam, The Netherlands 4INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00040 Monte Porzio Catone, Roma, Italy 5Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China.