References
-
Amblard A. et al., 2011, Submillimetre galaxies reside in dark matter haloes with masses greater than
$3{\times}10^{11}$ solar masses, Nature, 470, 510 https://doi.org/10.1038/nature09771 - Bendo G. et al., 2013, Flux calibration of the Hersche-SPIRE photometer, MNRAS, 433, 3062 https://doi.org/10.1093/mnras/stt948
- Berta S. et al., 2010, Dissecting the cosmic infra-red back- ground with Herschel/PEP, A&A, 518, L30 https://doi.org/10.1051/0004-6361/201014610
- Clements D. et al., 2010, Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns, A&A, 518, L8 https://doi.org/10.1051/0004-6361/201014581
- Dowell C., Pohlen M., Pearson C.P. et al., 2010, Status of the SPIRE photometer data processing pipelines during the early phases of the Herschel Mission, Proc. SPIE 7731, 36
- Griffin M. J. et al., 2010, The Herschel-SPIRE instrument and its inight performance, A&A, 518, L3 https://doi.org/10.1051/0004-6361/201014519
- Khan S. et al., 2007, First Constraints on Source Counts at 350 microns, ApJ, 665, 973 https://doi.org/10.1086/519239
- Lee H. M. et al., 2009, North Ecliptic Pole Wide Survey of AKARI: Survey Strategy and Data Characteristics, PASJ, 61, 375 https://doi.org/10.1093/pasj/61.2.375
- Matsuhara H. et al., 2006, Deep Extragalactic Surveys around the Ecliptic Poles with AKARI (ASTRO-F), PASJ, 58, 673 https://doi.org/10.1093/pasj/58.4.673
- Oliver, S. et al., 2010, HerMES: SPIRE galaxy number counts at 250, 350, and 500 microns, A&A, 518, L21 https://doi.org/10.1051/0004-6361/201014697
- Ott, S. 2010, The Herschel Data Processing System - HIPE and Pipelines, ASP Conference Series, 434, 139
- Pearson C., Lim T., North C. et al., 2014, SPIRE point source photometry: within the Herschel interactive processing environment (HIPE), Experimental Astronomy, 37, 175 https://doi.org/10.1007/s10686-013-9351-4
- Piazzo L., Ikhenaode D., Natoli P., Pestalozzi M., Piacentini F., Traficante A., 2012, Artifact removal for GLS map makers by means of post-processing, IEEE Trans. on Image Processing, 21, 3687 https://doi.org/10.1109/TIP.2012.2197009
- Pilbratt, G. et al., 2010, Herschel Space Observatory. An ESA facility for far-infrared and submillimetre astronomy, A&A, 518,1
- Poglitsch, A. et al. 2010, The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory, A&A, 518, L2 https://doi.org/10.1051/0004-6361/201014535
- Savage R. & Oliver S., 2007, Bayesian Methods of Astronomical Source Extraction, ApJ, 661, 1339 https://doi.org/10.1086/515393
- Traficante A. et al., 2011, Data reduction pipeline for the Hi-GAL survey, MNRAS, 416, 2932 https://doi.org/10.1111/j.1365-2966.2011.19244.x
- Wada T. et al., 2008, AKARI/IRC Deep Survey in the North Ecliptic Pole Region, PASJ, 60, 517 https://doi.org/10.1093/pasj/60.sp2.S517
Cited by
- Observations of the North Ecliptic Pole vol.234, pp.2, 2018, https://doi.org/10.3847/1538-4365/aaa07e