Tod R. Lauer
\nAstronomer, NOIRLab<\/p>\n
We used NASA\u2019s New Horizons spacecraft to measure the cosmic optical background (COB) intensity integrated over 0.4 \u2272 \u03bb \u2272 0.9 \u03bcm. The survey comprises 16 high Galactic-latitude fields. Images were obtained with the LORRI camera when New Horizons was 57 AU distant from the Sun. As such, the sky intensity measurements were unaffected by zodiacal light, which strongly interferes with COB measurements attempted from the inner solar system. T he survey yields a highly significant detection (6.8\u03c3) of the COB at 11.16 \u00b1 1.65 (1.47 sys, 0.75 ran) nW m\u22122 sr\u22121 at the LORRI pivot wavelength of 0.608 \u03bcm. The estimated integrated intensity from background galaxies, 8.17 \u00b1 1.18 nW m\u22122 sr\u22121, can account for the great majority of this signal. The rest of the COB signal is formally classified as anomalous intensity but is not significantly different from zero. The simplest interpretation is that the COB is completely due to galaxies.<\/p>\n","protected":false},"excerpt":{"rendered":"
How Dark is Space?<\/strong> We used NASA\u2019s New Horizons spacecraft to measure the cosmic optical background (COB) intensity integrated over 0.4 \u2272 \u03bb \u2272 0.9 \u03bcm. The survey comprises 16 high Galactic-latitude fields. Images were obtained with the LORRI camera when New Horizons was 57 AU distant from the Sun. As such, the sky intensity measurements were unaffected by zodiacal light, which strongly interferes with COB measurements attempted from the inner solar system. T he survey yields a highly significant detection (6.8\u03c3) of the COB at 11.16 \u00b1 1.65 (1.47 sys, 0.75 ran) nW m\u22122 sr\u22121 at the LORRI pivot wavelength of 0.608 \u03bcm. The estimated integrated intensity from background galaxies, 8.17 \u00b1 1.18 nW m\u22122 sr\u22121, can account for the great majority of this signal. The rest of the COB signal is formally classified as anomalous intensity but is not significantly different from zero. The simplest interpretation is that the COB is completely due to galaxies.<\/p>\n","protected":false},"author":9647,"featured_media":0,"template":"","meta":{"_acf_changed":false,"_tribe_events_status":"","_tribe_events_status_reason":"","_tribe_events_is_hybrid":"","_tribe_events_is_virtual":"","_tribe_events_virtual_video_source":"","_tribe_events_virtual_embed_video":"","_tribe_events_virtual_linked_button_text":"","_tribe_events_virtual_linked_button":"","_tribe_events_virtual_show_embed_at":"","_tribe_events_virtual_show_embed_to":[],"_tribe_events_virtual_show_on_event":"","_tribe_events_virtual_show_on_views":"","_tribe_events_virtual_url":"","footnotes":"","uwm_wg_additional_authors":[]},"tags":[],"tribe_events_cat":[58],"class_list":["post-9280","tribe_events","type-tribe_events","status-publish","hentry","tribe_events_cat-physics-colloquia","cat_physics-colloquia"],"uwm_unpublish_requested":false,"yoast_head":"\n
\nTod R. Lauer
\nAstronomer, NOIRLab<\/p>\n