Rosette Nebula NGC_2239 SHO (Jason)

Celestial hemisphere: Northern · Constellation: Monoceros (Mon) · Contains: 12 Mon · NGC 2237 · NGC 2238 · NGC 2239 · NGC 2244 · NGC 2246 · NGC 2252 · Rosette A · Rosette B · Rosette Nebula · Sh2-275 · The star 12Mon

Powered byPixInsight

Rosette Nebula NGC_2239 SHO

Powered byPixInsight

Rosette Nebula NGC_2239 SHO

Rosette Nebula in narrowband taken 10 Feb. 4 hours of exposure in 600s images.

Lucky with no moon and quite clear skies but window of visibility also coincides with the street lights being on. For teh short about of data it seems to come out well. Not sure it's the final rendition of the data...

Pixinsight Process details:

Rosette Nebula

H Ref 007

O Ref 001

S Ref 005

SHO

10/02 8,9,7

Pre-Processing:

WBPP for calibration

Batch format conversion of calibrated images with output with "compression-codec lz4hc+sh"

SubFrame Selection

Registration of all against best Ha Frame, output with "no-compression"

Integration of SHO channels with Automatic Normalisation

Linear Stage:

All S, H, O channels:

Dynamic crop of all to suit trim of combined data edges

ABE of each chn (Interpol function = 1, subtract, no normilization)

Ha data only:

EzDecon (Itt=59, Pixmath=10, defaults for rest of settings)

EzDenoise (defaults)

HT stretch from SFT after LRGB combine!

SHO:

LRGB combine in SHO

Image solved

Photometric calibration Narrowband SHO R=672 G=656.30 B=500.70 all 7mm

HT based on STF stretch

SCNR

LRGB Combo to add H to lum channel

Lum mask (RGBWS=1,1,1,1 and HT with low = -0.5 High = 1.5 and adjust mid point to center output peak)

HDRMultiscaleTransform Layers 6 Iterations 2

Curves K S curve with large boost around 60% and small saturation boost.

ACDNR

LocalHistogramEqualisation (Kernal = 146, contrast=2.5 Amount = 0.41, Resolution 8bit)

(LHE applied twice)

Darkstructure Enhance script (defaults)

EzStarReduction

Original
Final
B

B

Description: Reprocess of data in SHO with some newer workflow than when I created teh last revision. Now using the batch gradient script

Uploaded: ...

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	4699921
PixInsight job	UPMIG3N4XRLBYYBUX46GSWP1H6YU2TI8
PixInsight queue size	n/a
PixInsight stage	n/a

RA (center)	06h31m57s.36
RA (top/left)	06h35m03s.78
RA (top/right)	06h34m36s.64
RA (bottom/right)	06h28m50s.39
RA (bottom/left)	06h29m18s.54

Dec (center)	+04°56′44″.6
Dec (top/left)	+04°01′52″.2
Dec (top/right)	+05°56′43″.5
Dec (bottom/right)	+05°51′33″.9
Dec (bottom/left)	+03°56′44″.7

Image Index:

Contribution Index (beta):

Rosette Nebula NGC_2239 SHO

Rosette Nebula NGC_2239 SHO

Equipment

Acquisition details

Description

Comments

Revisions

B

Sky plot

Histogram

		...
You have no new notifications.

Image Index:

Contribution Index (beta):

Rosette Nebula NGC_2239 SHO

Rosette Nebula NGC_2239 SHO

Equipment

Acquisition details

Description

Comments

Revisions

B

Sky plot

Histogram

Notifications

AstroBin is in READ ONLY mode

Sorry :-(

Sorry :-(

Sorry :-(

Are you really sure?

Warning!

Warning!

Are you sure?

Report abuse

Slideshow settings

IOTD/TP stats (last [x] days)

Distribution of astrophotographers

Distribution of subject types

Distribution of data sources

Sorry

Sorry

Share

Upload new revision

Upload uncompressed source (XISF/FITS/PSD/TIFF)

Delete image and all its revisions?

Delete original image?

Delete all other versions?

Delete all revisions?

Delete this revision?

IOTD/TP stats

The following people like this image

The following people bookmarked this image

Warning

Flag malfunctioning thumbnails

Contains

Remove yourself as a collaborator

Plate-solving information