ARCADE 2 Measurement of the Absolute Sky Brightness at 3-90 GHz
The ARCADE 2 instrument has measured the absolute temperature of the sky at frequencies 3, 8, 10, 30, and 90 GHz, using an open-aperture cryogenic instrument observing at balloon altitudes with no emissive windows between the beam-forming optics and the sky. An external blackbody calibrator provides...
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description | The ARCADE 2 instrument has measured the absolute temperature of the sky at frequencies 3, 8, 10, 30, and 90 GHz, using an open-aperture cryogenic instrument observing at balloon altitudes with no emissive windows between the beam-forming optics and the sky. An external blackbody calibrator provides an in situ reference. Systematic errors were greatly reduced by using differential radiometers and cooling all critical components to physical temperatures approximating the cosmic microwave background (CMB) temperature. A linear model is used to compare the output of each radiometer to a set of thermometers on the instrument. Small corrections are made for the residual emission from the flight train, balloon, atmosphere, and foreground Galactic emission. The ARCADE 2 data alone show an excess radio rise of 54 ? 6 mK at 3.3 GHz in addition to a CMB temperature of 2.731 ? 0.004 K. Combining the ARCADE 2 data with data from the literature shows an excess power-law spectrum of T = 24.1 ? 2.1 (K) ( Delta *n/ Delta *n0)--2.599 ? 0.036 from 22 MHz to 10 GHz ( Delta *n0 = 310 MHz) in addition to a CMB temperature of 2.725 ? 0.001 K. |
doi_str_mv | 10.1088/0004-637X/734/1/5 |
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Small corrections are made for the residual emission from the flight train, balloon, atmosphere, and foreground Galactic emission. The ARCADE 2 data alone show an excess radio rise of 54 ? 6 mK at 3.3 GHz in addition to a CMB temperature of 2.731 ? 0.004 K. Combining the ARCADE 2 data with data from the literature shows an excess power-law spectrum of T = 24.1 ? 2.1 (K) ( Delta *n/ Delta *n0)--2.599 ? 0.036 from 22 MHz to 10 GHz ( Delta *n0 = 310 MHz) in addition to a CMB temperature of 2.725 ? 0.001 K.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/734/1/5</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Astronomy ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; BRIGHTNESS ; Earth, ocean, space ; ELECTROMAGNETIC RADIATION ; EMISSION ; Exact sciences and technology ; MEASURING INSTRUMENTS ; MICROWAVE RADIATION ; OPTICAL PROPERTIES ; PHYSICAL PROPERTIES ; RADIATION DETECTORS ; RADIATIONS ; RADIOMETERS ; RELICT RADIATION ; SKY ; THERMOMETERS</subject><ispartof>The Astrophysical journal, 2011-06, Vol.734 (1), p.5-jQuery1323907509973='48'</ispartof><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c444t-e64848685fc06a74d368dabc887bc7ce240b7dad843829f4502ce833bf1b9da83</citedby><cites>FETCH-LOGICAL-c444t-e64848685fc06a74d368dabc887bc7ce240b7dad843829f4502ce833bf1b9da83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/0004-637X/734/1/5/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,881,27605,27901,27902,53906</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/0004-637X/734/1/5$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=24249073$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/21576705$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Fixsen, D. 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Combining the ARCADE 2 data with data from the literature shows an excess power-law spectrum of T = 24.1 ? 2.1 (K) ( Delta *n/ Delta *n0)--2.599 ? 0.036 from 22 MHz to 10 GHz ( Delta *n0 = 310 MHz) in addition to a CMB temperature of 2.725 ? 0.001 K.</description><subject>Astronomy</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>BRIGHTNESS</subject><subject>Earth, ocean, space</subject><subject>ELECTROMAGNETIC RADIATION</subject><subject>EMISSION</subject><subject>Exact sciences and technology</subject><subject>MEASURING INSTRUMENTS</subject><subject>MICROWAVE RADIATION</subject><subject>OPTICAL PROPERTIES</subject><subject>PHYSICAL PROPERTIES</subject><subject>RADIATION DETECTORS</subject><subject>RADIATIONS</subject><subject>RADIOMETERS</subject><subject>RELICT RADIATION</subject><subject>SKY</subject><subject>THERMOMETERS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp1kMtKw0AUhgdRsFYfwN2AiC6MmVsyk52x1laoCF7A3TCZTGw0TWJmsqhP47P4ZCakdCOuDof_Oz-HD4BjjC4xEsJHCDEvpPzV55T52A92wAgHVHiMBnwXjLb5Pjiw9r1fSRSNwFX8OIlvppDAe6Ns25iVKR2sMuiWBsaJrYrWGfj0sYbXTf62dKWxFioHqRehn-_Z_OsQ7GWqsOZoM8fg5Xb6PJl7i4fZ3SReeJox5jwTMsFEKIJMo1BxltJQpCrRQvBEc20IQwlPVSoYFSTKWICINoLSJMNJlCpBx-Bk6K2sy6XVuTN6qauyNNpJggMechR01NlA1U312Rrr5Cq32hSFKk3VWhkRJFCEKO9IPJC6qaxtTCbrJl-pZi0xkr1S2TuSvTLZKZVY9u2nm3ZltSqyRpU6t9tDwgiLEKcddz5weVVv0z91sk6zDr34i_7_wS8PjI2z</recordid><startdate>20110610</startdate><enddate>20110610</enddate><creator>Fixsen, D. 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subjects | Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BRIGHTNESS Earth, ocean, space ELECTROMAGNETIC RADIATION EMISSION Exact sciences and technology MEASURING INSTRUMENTS MICROWAVE RADIATION OPTICAL PROPERTIES PHYSICAL PROPERTIES RADIATION DETECTORS RADIATIONS RADIOMETERS RELICT RADIATION SKY THERMOMETERS |
title | ARCADE 2 Measurement of the Absolute Sky Brightness at 3-90 GHz |
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