IC1795 HOO Palette (James)

Celestial hemisphere: Northern · Constellation: Cassiopeia (Cas) · Contains: HD14510 · HD14552 · HD14695 · HD14817 · HD15069 · IC 1795 · LBN 645 · LBN 646 · LBN 647 · LBN 650 · LDN 1356 · LDN 1359 · LDN 1361 · NGC 896

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IC1795 HOO Palette

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IC1795 HOO Palette

C 1795 - The Fish Head Nebula, also known as the Northern Bear Nebula, is part of a huge star forming system of gas and dust located along the Perseus spiral arm of our Milky Way galaxy. The nebula is located in the constellation Cassiopeia approximately 6000 light-years from the Earth and is adjacent to the much larger Heart Nebula. The brighter region of IC 1795 is designated NGC 896 and is the home to many massive, young, stars. These stars radiate copious amounts of ultraviolet light. This UV radiation excites the surrounding gas and causes it shine much the same way as a neon light emits its colorful hues. [Ref: http://www.waid-observatory.com/IC1795-2016-10-15-NB.shtml]. Image captured in dual narrowband using the Optolong L-eXtreme filter and processed for the HOO color palette.

Please note: The following tables are updated every 24 hours.

Distribution of astrophotographers

This table shows the number of distinct astrophotographers who have been assigned and IOTD/TP award compared to the total number of images awarded.
	Distinct awarded users	Total awarded images
Image of the day
Top picks
Top pick nominations

Distribution of subject types

This table shows the distribution of awards per subject type, compared to the popularity of images of that subject type.
	Image of the day	Top pick	Top pick nominations	Total submitted
Deep sky
Solar system
Extremely wide field
Star trails
Northern lights
Noctilucent clouds
Landscape

Distribution of data sources

This table shows the distribution of awards per data source, compared to the popularity of images acquired from that data source.
	Image of the day	Top pick	Top pick nominations	Total submitted
Backyard
Traveller
Own remote observatory
Amateur hosting facility
Public amaeteur data
Professional, scientific grade data
Mix of multiple sources
Other
Unknown

The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

Submitted The date and time when you submitted this image for IOTD/TP consideration.	...
Views by Submitters (available since September 19th, 2023) Every image is assigned to 50% of available Submitters. In the event that at least 80% of them don't view the image before its time in the IOTD/TP process expires, it's assigned to the other 50% of Submitters and the process begins anew.
Promotions by Submitters When 3 distinct Submitters promote the image, it moves on to the next stage of the process: evaluation for Top Pick status. This requirement, in addition to anonymization of images and distribution to only a subset of them, prevents biases and ensures that the best images are selected.
Promotions by Reviewers When 3 distinct Reviewers promote the image, it moves on to the next stage of the process: evaluation for IOTD status.
Early dismissal Staff members have a lot of images to inspect on a daily basis, and they can dismiss images if they believe they don't meet the requirements for IOTD/TP selection. If an image is dismissed 5 times, it's removed from the process. This streamlines the process and ensures that any bias present in promotions could be overruled by other staff members.

Status	Advanced success
Started	...
Astrometry.net job	8956617
PixInsight job	CIIKAK2I7KYAH6MUQSMN5J4ZXKQQVHNV
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	02h25m08s.100
RA (top/left)	02h29m43s.245
RA (top/right)	02h27m30s.365
RA (bottom/right)	02h20m23s.474
RA (bottom/left)	02h22m52s.229

Dec (center)	+61°59′55″.42
Dec (top/left)	+61°28′23″.10
Dec (top/right)	+62°42′09″.80
Dec (bottom/right)	+62°30′52″.56
Dec (bottom/left)	+61°17′33″.60

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IC1795 HOO Palette

IC1795 HOO Palette

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IC1795 HOO Palette

IC1795 HOO Palette

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