Noor AftabAndrew, XunheAndrew, Zhang, David R. Mittelman, Dennis di Cicco, Sean Walker, David H. Sliski, Julia Homa, Colin Holm-Hansen, Mary Putman, David Schiminovich, Arne Henden, Gary Walker
{"title":"MDW Hα 巡天观测第 0 版数据","authors":"Noor AftabAndrew, XunheAndrew, Zhang, David R. Mittelman, Dennis di Cicco, Sean Walker, David H. Sliski, Julia Homa, Colin Holm-Hansen, Mary Putman, David Schiminovich, Arne Henden, Gary Walker","doi":"arxiv-2409.11481","DOIUrl":null,"url":null,"abstract":"The Mittelman-di Cicco-Walker (MDW) H$\\alpha$ Sky Survey is an\nautonomously-operated and ongoing all-sky imaging survey in the narrowband\nH$\\alpha$ wavelength. The survey was founded by amateur astronomers, and is\npresented here in its first stage of refinement for rigorous scientific use.\nEach field is exposed through an H$\\alpha$ filter with a 3nm bandwidth for a\ntotal of four hours, with a pixel scale of 3.2 arcsec. Here, we introduce the\nfirst Data Release of the MDW H$\\alpha$ Survey (Data Release 0, or DR0),\nspanning 238 fields in the region of Orion (~3100 deg$^2$). DR0 includes:\ncalibrated mean fields, star-removed mean fields, a point source catalog\nmatched to Data Release 1 of the Panoramic Survey Telescope and Rapid Response\nSystem (Pan-STARRS1) and the INT Galactic Plane Survey (IGAPS), and mosaics.","PeriodicalId":501068,"journal":{"name":"arXiv - PHYS - Solar and Stellar Astrophysics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The MDW Hα Sky Survey: Data Release 0\",\"authors\":\"Noor AftabAndrew, XunheAndrew, Zhang, David R. Mittelman, Dennis di Cicco, Sean Walker, David H. Sliski, Julia Homa, Colin Holm-Hansen, Mary Putman, David Schiminovich, Arne Henden, Gary Walker\",\"doi\":\"arxiv-2409.11481\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Mittelman-di Cicco-Walker (MDW) H$\\\\alpha$ Sky Survey is an\\nautonomously-operated and ongoing all-sky imaging survey in the narrowband\\nH$\\\\alpha$ wavelength. The survey was founded by amateur astronomers, and is\\npresented here in its first stage of refinement for rigorous scientific use.\\nEach field is exposed through an H$\\\\alpha$ filter with a 3nm bandwidth for a\\ntotal of four hours, with a pixel scale of 3.2 arcsec. Here, we introduce the\\nfirst Data Release of the MDW H$\\\\alpha$ Survey (Data Release 0, or DR0),\\nspanning 238 fields in the region of Orion (~3100 deg$^2$). DR0 includes:\\ncalibrated mean fields, star-removed mean fields, a point source catalog\\nmatched to Data Release 1 of the Panoramic Survey Telescope and Rapid Response\\nSystem (Pan-STARRS1) and the INT Galactic Plane Survey (IGAPS), and mosaics.\",\"PeriodicalId\":501068,\"journal\":{\"name\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.11481\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Solar and Stellar Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11481","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The Mittelman-di Cicco-Walker (MDW) H$\alpha$ Sky Survey is an
autonomously-operated and ongoing all-sky imaging survey in the narrowband
H$\alpha$ wavelength. The survey was founded by amateur astronomers, and is
presented here in its first stage of refinement for rigorous scientific use.
Each field is exposed through an H$\alpha$ filter with a 3nm bandwidth for a
total of four hours, with a pixel scale of 3.2 arcsec. Here, we introduce the
first Data Release of the MDW H$\alpha$ Survey (Data Release 0, or DR0),
spanning 238 fields in the region of Orion (~3100 deg$^2$). DR0 includes:
calibrated mean fields, star-removed mean fields, a point source catalog
matched to Data Release 1 of the Panoramic Survey Telescope and Rapid Response
System (Pan-STARRS1) and the INT Galactic Plane Survey (IGAPS), and mosaics.