Title: The Sloan Digital Sky Survey ImgCutout: The universe at your fingertips
1The Sloan Digital Sky Survey ImgCutout The
universe at your fingertips
Maria A. Nieto-Santisteban nieto_at_pha.jhu.edu Johns
Hopkins University
2The Sloan Digital Sky Survey ImgCutout The
universe at your fingertips
- 1 TByte astronomical database on the internet.
- Available to professional astronomers general
public.
- A photometric and spectral catalog of 100
million objects.
3The big picture of the sky
4The big picture of the sky
- Each tile corresponds to 5 images taken in
different wavelengths by the Sloan telescope.
- Originally in FITS format, images are "glued"
together to create a JPEG mosaic.
5The big picture of the sky
- Plates show astronomers the boundaries of
spectroscopic observations.
6The big picture of the sky
- Plates show astronomers the boundaries of
spectroscopic observations.
7The big picture of the sky
- Plates show astronomers the boundaries of
spectroscopic observations.
8The big picture of the sky
- Plates show astronomers the boundaries of
spectroscopic observations.
9The big picture of the sky
- Plates show astronomers the boundaries of
spectroscopic observations.
10The big picture of the sky
- Yellow crosses mark spectroscopic Targets.
11The big picture of the sky
- Yellow crosses mark spectroscopic Targets.
- Red squares indicate actual Spectroscopic
observations.
12The big picture of the sky
- Yellow crosses mark spectroscopic Targets.
- Red squares indicate actual Spectroscopic
observations.
- Blue circles point to Photometric observations.
13Looking at data quality
- 10 - 15 of the observations are lost due to
bad weather, bright stars, satellite trails,
meteors, etc.
14Looking at data quality
- 10 - 15 of the observations are lost due to
bad weather, bright stars, satellite trails,
meteors, etc.
- Masks delimit such bad areas.
15Looking at data quality
- 10 - 15 of the observations are lost due to
bad weather, bright stars, satellites trails,
meteors, etc.
- Masks delimit such bad areas.
16Looking at data quality
- 10 - 15 of the observations are lost due to
bad weather, bright stars, satellite trails,
meteors, etc.
- Masks delimit such bad areas.
17Looking at data quality
Meteor Trail
- Astronomers need to identify bad areas in order
to improve their science.
Bright Source
18Looking at known sources
- Astronomers can enter a list of coordinates to
get an initial view and decide whether or not
proceed further.
19Preparing new observations
Looking at known sources
- Finding charts are invaluable tools when
observing with a real telescope.
20Querying the database for new discoveries
Find galaxies with specific spectra
Search for quasars
- Users can search for new objects online and get
answers in real time.
21Querying the database for new discoveries
22Querying the database for new discoveries
- These three objects might form a previously
unknown lensed quasar!
23Querying the database for new discoveries
24Looking in detail
- Digging for more information
25Looking in detail
- Digging for more information
26Looking in detail
- Digging for more information
- Photometry, Spectro, Cross Identifications and
more
27SkyServer
- Photometry, Spectro, Cross Identifications and
more from SkyServer
28SkyServer
- Photometry, Spectro, Cross Identifications and
more from SkyServer
Quasar Spectrum
29Exploring the neighborhood
30Exploring the neighborhood
31Exploring the neighborhood
32Exploring the neighborhood
33Exploring the neighborhood
34Exploring the neighborhood
35Exploring the neighborhood
36Exploring the neighborhood
37ImgCutout
Visual exploration of
- the 1 TeraByte SkyServer database,
- its 100 million celestial objects,
- their images and spectra,
- complex spatial relations, boundaries.
Enables instantaneous discoveries.
38The Universe at your fingertips
ImgCutout
Johns Hopkins University http//skyservice.pha.jh
u.edu/dr1/ImgCutout/