FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2079344579> ?p ?o ?g. }

• W2079344579 endingPage "L15" @default.
• W2079344579 startingPage "L15" @default.
• W2079344579 abstract "We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the <i>Herschel<i/> Lensing Survey (HLS) Program. We describe in detail a photometric procedure designed to recover robust fluxes and deblend faint <i>Herschel<i/> sources near the confusion noise. The method is based on the use of the positions of <i>Spitzer<i/>/MIPS 24 <i>μ<i/>m sources as priors. Our catalogs are able to reliably (5<i>σ<i/>) recover galaxies with fluxes above 6 and 10 mJy in the PACS 100 and 160 <i>μ<i/>m channels, respectively, and 12 to 18 mJy in the SPIRE bands. We also obtain spectral energy distributions covering the optical through the far-infrared/millimeter spectral ranges of all the <i>Herschel<i/> detected sources, and analyze them to obtain independent estimations of the photometric redshift based on either stellar population or dust emission models. We exemplify the potential of the combined use of <i>Spitzer<i/> position priors plus independent optical and IR photometric redshifts to robustly assign optical/NIR counterparts to the sources detected by <i>Herschel<i/> and other (sub-)mm instruments." @default.
• W2079344579 created "2016-06-24" @default.
• W2079344579 creator A5001172613 @default.
• W2079344579 creator A5003656561 @default.
• W2079344579 creator A5003953079 @default.
• W2079344579 creator A5004193106 @default.
• W2079344579 creator A5009664387 @default.
• W2079344579 creator A5012069547 @default.
• W2079344579 creator A5012224131 @default.
• W2079344579 creator A5022611236 @default.
• W2079344579 creator A5023314136 @default.
• W2079344579 creator A5026496927 @default.
• W2079344579 creator A5027849832 @default.
• W2079344579 creator A5028898239 @default.
• W2079344579 creator A5031916357 @default.
• W2079344579 creator A5039844544 @default.
• W2079344579 creator A5041494992 @default.
• W2079344579 creator A5042027319 @default.
• W2079344579 creator A5044798918 @default.
• W2079344579 creator A5051029980 @default.
• W2079344579 creator A5052031270 @default.
• W2079344579 creator A5052127987 @default.
• W2079344579 creator A5052954301 @default.
• W2079344579 creator A5055320940 @default.
• W2079344579 creator A5062010375 @default.
• W2079344579 creator A5062504729 @default.
• W2079344579 creator A5064812526 @default.
• W2079344579 creator A5068869030 @default.
• W2079344579 creator A5069252746 @default.
• W2079344579 creator A5073859219 @default.
• W2079344579 creator A5074214640 @default.
• W2079344579 creator A5074788204 @default.
• W2079344579 creator A5078587946 @default.
• W2079344579 creator A5081131289 @default.
• W2079344579 creator A5081451517 @default.
• W2079344579 creator A5084677176 @default.
• W2079344579 creator A5085375529 @default.
• W2079344579 creator A5087897086 @default.
• W2079344579 creator A5088205374 @default.
• W2079344579 creator A5090073897 @default.
• W2079344579 creator A5090080680 @default.
• W2079344579 date "2010-07-01" @default.
• W2079344579 modified "2023-10-18" @default.
• W2079344579 title "Improving the identification of high-<i>z</i><i>Herschel</i>sources with position priors and optical/NIR and FIR/mm photometric redshifts" @default.
• W2079344579 cites W1681063222 @default.
• W2079344579 cites W1826064388 @default.
• W2079344579 cites W1841113251 @default.
• W2079344579 cites W1914598719 @default.
• W2079344579 cites W1971182901 @default.
• W2079344579 cites W1972308849 @default.
• W2079344579 cites W1990919732 @default.
• W2079344579 cites W1999046479 @default.
• W2079344579 cites W2006316173 @default.
• W2079344579 cites W2007741717 @default.
• W2079344579 cites W2017100570 @default.
• W2079344579 cites W2027297109 @default.
• W2079344579 cites W2043533977 @default.
• W2079344579 cites W2045213752 @default.
• W2079344579 cites W2083821946 @default.
• W2079344579 cites W2115157422 @default.
• W2079344579 cites W2119392211 @default.
• W2079344579 cites W2120875714 @default.
• W2079344579 cites W2132735762 @default.
• W2079344579 cites W2135536375 @default.
• W2079344579 cites W2142238829 @default.
• W2079344579 cites W2147223987 @default.
• W2079344579 cites W2147847259 @default.
• W2079344579 cites W2148801975 @default.
• W2079344579 cites W2164106029 @default.
• W2079344579 cites W2167262338 @default.
• W2079344579 cites W2168126149 @default.
• W2079344579 cites W3098166889 @default.
• W2079344579 cites W3098853664 @default.
• W2079344579 cites W3099956274 @default.
• W2079344579 cites W3100054476 @default.
• W2079344579 cites W3100106758 @default.
• W2079344579 cites W3100638626 @default.
• W2079344579 cites W3102827423 @default.
• W2079344579 cites W3103281616 @default.
• W2079344579 cites W3103868583 @default.
• W2079344579 cites W3105713365 @default.
• W2079344579 cites W3105821843 @default.
• W2079344579 cites W3106529437 @default.
• W2079344579 cites W3121508074 @default.
• W2079344579 cites W3126089333 @default.
• W2079344579 cites W4293003757 @default.
• W2079344579 doi "https://doi.org/10.1051/0004-6361/201014593" @default.
• W2079344579 hasPublicationYear "2010" @default.
• W2079344579 type Work @default.
• W2079344579 sameAs 2079344579 @default.
• W2079344579 citedByCount "28" @default.
• W2079344579 countsByYear W20793445792012 @default.
• W2079344579 countsByYear W20793445792013 @default.
• W2079344579 countsByYear W20793445792014 @default.
• W2079344579 countsByYear W20793445792016 @default.
• W2079344579 countsByYear W20793445792017 @default.
• W2079344579 countsByYear W20793445792018 @default.
• W2079344579 countsByYear W20793445792019 @default.

• next