Ultraviolet to optical diffuse sky emission as seen by the Hubble Space Telescope Faint Object Spectrograph
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Timothy D. Brandt | K. Kawara | S. Oyabu | S. Oyabu | H. Sameshima | K. Kawara | Y. Matsuoka | K. Tsumura | T. Brandt | Y. Matsuoka | K. Sano | H. Sameshima | K. Tsumura | N. Ienaka | N. Ienaka | K. Sano
[1] M. Eracleous,et al. The Speedy Magnetic Propeller in the Cataclysmic Variable AE Aquarii , 1996 .
[2] Measurements of the Diffuse Ultraviolet Background and the Terrestrial Airglow with the Space Telescope Imaging Spectrograph , 2000, astro-ph/0004147.
[3] T. Mukai,et al. HIGH-RESOLUTION IMAGING OF THE GEGENSCHEIN AND THE GEOMETRIC ALBEDO OF INTERPLANETARY DUST , 2013, 1302.3316.
[4] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[5] H. Ferguson,et al. Ultraviolet Galaxy Counts from Space Telescope Imaging Spectrograph Observations of the Hubble Deep Fields , 2000 .
[6] Richard G. Arendt,et al. Interstellar Dust Models Consistent with Extinction, Emission, and Abundance Constraints , 2003, astro-ph/0312641.
[7] L. Cambresy,et al. The Cosmic Infrared Background at 1.25 and 2.2 Microns Using DIRBE and 2MASS: A Contribution Not Due to Galaxies? , 2001 .
[8] L. A. Antonelli,et al. Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe? , 2008, Science.
[9] C. A. Oxborrow,et al. Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation , 2013, 1309.0382.
[10] Jayant Murthy,et al. MAPPING THE DIFFUSE ULTRAVIOLET SKY WITH THE GALAXY EVOLUTION EXPLORER , 2010 .
[11] Toshio Matsumoto,et al. Rocket-borne observations of the zodiacal light in the near-infrared wavelengths. , 1995 .
[12] S. Bowyer,et al. Discovery and imaging of a Galactic cirrus cloud with the far ultraviolet space telescope , 1995 .
[13] Lucia Pozzetti,et al. Deep galaxy counts, extragalactic background light and the stellar baryon budget , 1999, astro-ph/9907315.
[14] Min Gyu Kim,et al. MEASUREMENTS OF THE MEAN DIFFUSE GALACTIC LIGHT SPECTRUM IN THE 0.95–1.65 μm BAND FROM CIBER , 2015, 1503.04926.
[15] Mark S. Robinson,et al. Ultraviolet spectral reflectance properties of common planetary minerals , 2008 .
[16] Toshio Matsumoto,et al. Low-Resolution Spectrum of the Extragalactic Background Light with the AKARI InfraRed Camera , 2013, 1307.6740.
[17] V. V. Hristov,et al. OBSERVATIONS OF THE NEAR-INFRARED SPECTRUM OF THE ZODIACAL LIGHT WITH CIBER , 2010, 1004.5445.
[18] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[19] S. Oyabu,et al. COSMIC OPTICAL BACKGROUND: THE VIEW FROM PIONEER 10/11 , 2011, Proceedings of the International Astronomical Union.
[20] T. Totani,et al. Diffuse Extragalactic Background Light versus Deep Galaxy Counts in the Subaru Deep Field: Missing Light in the Universe? , 2001, astro-ph/0102328.
[21] Douglas P. Finkbeiner,et al. A Full-Sky Hα Template for Microwave Foreground Prediction , 2003, astro-ph/0301558.
[22] H. Kataza,et al. MEASUREMENTS OF DIFFUSE SKY EMISSION COMPONENTS IN HIGH GALACTIC LATITUDES AT 3.5 AND 4.9 μm USING DIRBE AND WISE DATA , 2015, 1512.08072.
[23] J. Weingartner,et al. Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud , 2001 .
[24] E. L. Wright,et al. Number Counts at 3 μm < λ < 10 μm from the Spitzer Space Telescope , 2004 .
[25] E. L. Wright,et al. Tentative Detection of the Cosmic Infrared Background at 2.2 and 3.5 Microns Using Ground-based and Space-based Observations , 1999, astro-ph/9909428.
[26] E. L. Wright,et al. DIRBE Minus 2MASS: Confirming the CIRB in 40 New Regions at 2.2 and 3.5 μm , 2007, 0704.1498.
[27] W. Duley,et al. Ultraviolet Absorption in Amorphous Carbons: Polycyclic Aromatic Hydrocarbons and the 2175 Å Extinction Feature , 2004 .
[28] L. Bianchi,et al. GALEX OBSERVATIONS OF DIFFUSE UV RADIATION AT HIGH SPATIAL RESOLUTION FROM THE SANDAGE NEBULOSITY , 2008, 0807.0189.
[29] P. Pilewskie,et al. Recent variability of the solar spectral irradiance and its impact on climate modelling , 2012, 1303.5577.
[30] M. V. Fernandes,et al. Measurement of the extragalactic background light imprint on the spectra of the brightest blazars observed with H.E.S.S. , 2012, 1212.3409.
[31] M. Kawada,et al. Infrared Telescope in Space Observations of the Near-Infrared Extragalactic Background Light , 2004, astro-ph/0411593.
[32] Hideo Ohashi,et al. Simulation of space weathering of planet-forming materials: Nanosecond pulse laser irradiation and proton implantation on olivine and pyroxene samples , 1999 .
[33] J. L. Weinberg,et al. Zodiacal light and the asteroid belt: The view from Pioneer 10 , 1974 .
[34] H. Murakami,et al. IRTS Observation of the Near-Infrared Spectrum of the Zodiacal Light , 1996 .
[35] G. Rieke,et al. The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background. , 2006, astro-ph/0603208.
[36] Jayant Murthy,et al. Mapping the Diffuse Ultraviolet Sky with GALEX , 2010 .
[37] Richard P. Binzel,et al. MUSES‐C target asteroid (25143) 1998 SF36: A reddened ordinary chondrite , 2001 .
[38] S. Matsuura,et al. FIRST DETECTION OF GALACTIC LATITUDE DEPENDENCE OF NEAR-INFRARED DIFFUSE GALACTIC LIGHT FROM DIRBE RENALYSIS , 2016, 1603.07732.
[39] M. Mapelli,et al. Background radiation from sterile neutrino decay and reionization , 2005, astro-ph/0508413.
[40] B. Peterson,et al. DIFFUSE GALACTIC LIGHT IN THE FIELD OF THE TRANSLUCENT HIGH GALACTIC LATITUDE CLOUD MBM32 , 2013, 1303.0938.
[41] M. Köhler,et al. Dust in the solar system and in extra-solar planetary systems , 2006 .
[42] F. DeMeo,et al. INTERPLANETARY DUST PARTICLES AS SAMPLES OF ICY ASTEROIDS , 2015 .
[43] L. Colina,et al. The 0.12-2.5 micron Absolute Flux Distribution of the Sun for Comparison With Solar Analog Stars , 1996 .
[44] M. C. Cooper,et al. Extragalactic background light inferred from AEGIS galaxy-SED-type fractions , 2010, 1103.4534.
[45] S. Andrews,et al. MEASUREMENTS OF EXTRAGALACTIC BACKGROUND LIGHT FROM THE FAR UV TO THE FAR IR FROM DEEP GROUND- AND SPACE-BASED GALAXY COUNTS , 2016, 1605.01523.
[46] R. Bernstein,et al. The Optical Extragalactic Background Light: Revisions and Further Comments , 2007 .
[47] Stuart Bowyer,et al. The 1997 reference of diffuse night sky brightness , 1998 .
[48] Harold F. Levison,et al. COMETARY ORIGIN OF THE ZODIACAL CLOUD AND CARBONACEOUS MICROMETEORITES. IMPLICATIONS FOR HOT DEBRIS DISKS , 2009, 0909.4322.
[49] Sophia A. Khan,et al. DETECTION OF THE COSMIC FAR-INFRARED BACKGROUND IN AKARI DEEP FIELD SOUTH , 2010, 1002.3674.
[50] Bradley M. Peterson,et al. A Search for Ultrarapid Microvariability in the Seyfert Galaxy NGC 7469 with the Hubble Space Telescope , 1998 .
[51] E. al.,et al. Number Counts of GALEX Sources in FUV (1530A) and NUV (2310A) Bands , 2004, astro-ph/0411317.
[52] L. Bianchi,et al. GALEX OBSERVATIONS OF DIFFUSE ULTRAVIOLET EMISSION FROM DRACO , 2010, 1009.3348.
[53] R. Arendt,et al. The Near-Infrared Background: Interplanetary Dust or Primordial Stars? , 2005, astro-ph/0508262.
[54] K. Lumme,et al. Photometric properties of zodiacal light particles , 1985 .
[55] Sho Sasaki,et al. Pulse-laser irradiation experiments of Murchison CM2 chondrite for reproducing space weathering on C-type asteroids , 2015 .
[56] E. L. Wright. DIRBE minus 2MASS: Confirming the Cosmic Infrared Background at 2.2 Microns , 2000, astro-ph/0004192.
[57] E. L. Wright,et al. Detection of the Cosmic Infrared Background at 2.2 and 3.5 Microns Using DIRBE Observations , 1999, astro-ph/9912523.
[58] M. Zolensky,et al. Thermal metamorphism of the C, G, B, and F asteroids seen from the 0.7 μm, 3 μm, and UV absorption strengths in comparison with carbonaceous chondrites , 1996 .
[59] A. Noutsos,et al. A low level of extragalactic background light as revealed by γ-rays from blazars , 2005, Nature.
[60] A. Mickaelian. DSS1/DSS2 astrometry for 1101 First Byurakan Survey blue stellar objects: Accurate positions and other results , 2004 .
[61] Timothy D. Brandt,et al. THE SPECTRUM OF THE DIFFUSE GALACTIC LIGHT: THE MILKY WAY IN SCATTERED LIGHT , 2011, 1109.4175.
[62] M. Jura. Observational consequences of scattering clouds above the galactic disk. , 1979 .
[63] Astronomy,et al. Infrared Emission from the Radio Supernebula in NGC 5253: A Proto-Globular Cluster? , 2001, astro-ph/0103101.
[64] E. L. Wright,et al. The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. II. Model of the Interplanetary Dust Cloud , 1997, astro-ph/9806250.
[65] K. Tsumura,et al. REANALYSIS OF THE NEAR-INFRARED EXTRAGALACTIC BACKGROUND LIGHT BASED ON THE IRTS OBSERVATIONS , 2015, 1501.01359.
[66] T. Onaka,et al. MODELING OF THE ZODIACAL EMISSION FOR THE AKARI/IRC MID-INFRARED ALL-SKY DIFFUSE MAPS , 2016, 1601.05553.
[67] H. Kataza,et al. DERIVATION OF A LARGE ISOTOPIC DIFFUSE SKY EMISSION COMPONENT AT 1.25 AND 2.2 μm FROM THE COBE/DIRBE DATA , 2015, 1508.02806.
[68] Richard P. Binzel,et al. Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: The Observations , 2002 .
[69] E. L. Wright,et al. The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections , 1998, astro-ph/9806167.
[70] Hongu Yang,et al. ORIGIN OF INTERPLANETARY DUST THROUGH OPTICAL PROPERTIES OF ZODIACAL LIGHT , 2015, 1509.07184.