Showing 121 - 140 results of 207 for search '"space observatory"', query time: 0.16s Refine Results
  1. 121
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    Advances in optical engineering for future telescopes by Daewook Kim, Heejoo Choi, Trenton Brendel, Henry Quach, Marcos Esparza, Hyukmo Kang, Yi-Ting Feng, Jaren N. Ashcraft, Xiaolong Ke, Tianyi Wang, Ewan S. Douglas

    Published 2021-06-01
    “…Among these, the Nautilus space observatory requires challenging alignment of segmented multi-order diffractive elements. …”
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    Article
  4. 124

    A compact receiver system for simultaneous measurements of mesospheric CO and O<sub>3</sub> by P. Forkman, O. M. Christensen, P. Eriksson, B. Billade, V. Vassilev, V. M. Shulga

    Published 2016-02-01
    “…The first measurement series from October 2014 until April 2015 taken at the Onsala Space Observatory, OSO (57&deg; N, 12&deg; E), is analysed. …”
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    Article
  5. 125
  6. 126

    Bi-Spectral Infrared Algorithm for Cloud Coverage over Oceans by the JEM-EUSO Mission Program by David Santalices, Susana Briz, Antonio J. de Castro, Fernando López

    Published 2021-09-01
    “…Specifically, this article evaluates a method to determine the cloud map from the images provided by a simple bi-spectral infrared camera within the framework of JEM-EUSO (The Joint Experiment Missions-Extrem Universe Space Observatory). This program involves different experiments whose aim is determining properties of Ultra-High Energy Cosmic Ray (UHECR) via the detection of atmospheric fluorescence light. …”
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    Article
  7. 127
  8. 128

    Spektr–UF Mission Spectrograph Space Qualified CCD Detector Subsystem by Andrey Shugarov, Mikhail Sachkov

    Published 2023-09-01
    “…Spektr–UF (World Space Observatory Ultraviolet, WSO-UV) is a Russian-led international collaboration aiming to develop a large space-borne 1.7 m Ritchey–Chretién telescope with science instruments to study the Universe in ultraviolet wavelengths. …”
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    Article
  9. 129

    Far-infrared properties of submillimeter and optically faint radio galaxies by Magnelli, B, Lutz, D, Berta, S, Altieri, B, Andreani, P, Aussel, H, Castaneda, H, Cava, A, Cepa, J, Cimatti, A, Daddi, E, Dannerbauer, H, Dominguez, H, Elbaz, D, Schreiber, N, Genzel, R, Grazian, A, Gruppioni, C, Magdis, G, Maiolino, R, Nordon, R, Perez Fournon, I, Garcia, I, Poglitsch, A, Popesso, P

    Published 2010
    “…We use deep observations obtained with the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel Space Observatory to study the far-infrared (FIR) properties of submillimeter and optically faint radio galaxies (SMGs and OFRGs). …”
    Journal article
  10. 130

    Far-infrared properties of submillimeter and optically faint radio galaxies by Magnelli, B, Lutz, D, Berta, S, Altieri, B, Andreani, P, Aussel, H, Castañeda, H, Cava, A, Cepa, J, Cimatti, A, Daddi, E, Dannerbauer, H, Dominguez, H, Elbaz, D, Förster Schreiber, N, Genzel, R, Grazian, A, Gruppioni, C, Magdis, G, Maiolino, R, Nordon, R, Pérez Fournon, I, Pérez García, I, Poglitsch, A, Popesso, P

    Published 2010
    “…We use deep observations obtained with the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel Space Observatory to study the far-infrared (FIR) properties of submillimeter and optically faint radio galaxies (SMGs and OFRGs). …”
    Journal article
  11. 131

    The LOFAR two-metre sky survey deep fields: the star-formation rate–radio luminosity relation at low frequencies by Smith, DJB, Haskell, P, Gürkan, G, Best, PN, Hardcastle, MJ, Kondapally, R, Williams, W, Duncan, KJ, Cochrane, RK, McCheyne, I, Röttgering, HJA, Sabater, J, Shimwell, TW, Tasse, C, Bonato, M, Bondi, M, Jarvis, MJ, Leslie, SK, Prandoni, I, Wang, L

    Published 2021
    “…The LOFAR Surveys Key Science Project is transforming our understanding of the low-frequency radio sky, with the 150 MHz data over the European Large Area Infrared Space Observatory Survey-North 1 field reaching an rms sensitivity of 20 μJy beam−1 over 10 deg2 at 6 arcsec resolution. …”
    Journal article
  12. 132

    Goods-Herschel measurements of the dust attenuation of typical star-forming galaxies at high redshift: Observations of ultraviolet-selected galaxies at z ∼ 2 by Reddy, N, Dickinson, M, Elbaz, D, Morrison, G, Giavalisco, M, Ivison, R, Papovich, C, Scott, D, Buat, V, Burgarella, D, Charmandaris, V, Daddi, E, Magdis, G, Murphy, E, Altieri, B, Aussel, H, Dannerbauer, H, Dasyra, K, Hwang, H, Kartaltepe, J, Leiton, R, Magnelli, B, Popesso, P

    Published 2012
    “…We take advantage of the sensitivity and resolution of the Herschel Space Observatory at 100 and 160 μm to directly image the thermal dust emission and investigate the infrared luminosities (L IR) and dust obscuration of typical star-forming (L*) galaxies at high redshift. …”
    Journal article
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  17. 137

    Waves and Magnetism in the Solar Atmosphere (WAMIS) by Yuan-Kuen eKo, John Daniel Moses, John Martin Laming, Leonard eStrachan, Samuel eTun Beltran, Steven eTomczyk, Sarah E. Gibson, Frederic eAuchere, Roberto eCasini, Silvano eFineschi, Michael eKnoelker, Clarence eKorendyke, Scott William McIntosh, Marco eRomoli, Jan eRybak, Dennis G. Socker, Angelos eVourlidas, Qian eWu

    Published 2016-02-01
    “…These comprehensive observations are not provided by any current single ground-based or space observatory. The fundamental advancements achieved by the near-space observations of WAMIS on coronal field would point the way for future ground based and orbital instrumentation.…”
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    Article
  18. 138

    The need for a multi-purpose, optical–NIR space facility after HST and JWST by Jahnke, Knud, Krause, Oliver, Rix, Hans-Walter, Courbin, Frédéric, Fontana, Adriano, Heymans, Catherine, Martin, Nicolas, Oesch, Pascal, Taylor, Andy, Gaudi, B. S, Kiessling, Alina, Mennesson, Bertrand, Seager, Sara, Stern, Daniel, Warfield, Keith

    Published 2021
    “…Abstract In the early 2030s, after the end of operations for the epochal Hubble Space Telescope and the long-anticipated James Webb Space Telescope, astrophysics will lose access to a general purpose high-spatial resolution space observatory to cover the UV–optical–NIR wavelength range with a variety of imaging bandpasses and high-multiplexing mid-resolution spectroscopy. …”
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    Article
  19. 139

    The evolution of the dust temperatures of galaxies in the SFR-M-* plane up to z similar to 2 by Magnelli, B, Lutz, D, Saintonge, A, Berta, S, Santini, P, Symeonidis, M, Altieri, B, Andreani, P, Aussel, H, Bethermin, M, Bock, J, Bongiovanni, A, Cepa, J, Cimatti, A, Conley, A, Daddi, E, Elbaz, D, Schreiber, N, Genzel, R, Ivison, R, Le Floc'h, E, Magdis, G, Maiolino, R, Nordon, R, Oliver, S

    Published 2014
    “…We study the evolution of the dust temperature of galaxies in the SFR-Mâ̂- plane up to z ~ 2 using far-infrared and submillimetre observations from the Herschel Space Observatory taken as part of the PACS Evolutionary Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) guaranteed time key programmes. …”
    Journal article
  20. 140

    Herschel unveils a puzzling uniformity of distant dusty galaxies by Elbaz, D, Hwang, H, Magnelli, B, Daddi, E, Aussel, H, Altieri, B, Amblard, A, Andreani, P, Arumugam, V, Auld, R, Babbedge, T, Berta, S, Blain, A, Bock, J, Bongiovanni, A, Boselli, A, Buat, V, Burgarella, D, Castro-Rodriguez, N, Cava, A, Cepa, J, Chanial, P, Chary, R, Cimatti, A, Clements, D

    Published 2010
    “…The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. …”
    Journal article