AstroGrid

Navigation
Log in


Forgot your password?
 

This website (www2.astrogrid.org) is now deprecated - please go to www.astrogrid.org for up to date information.

Document Actions

IPHAS Database Access

This page describes the access to the IPHAS catalogue.

1   The IPHAS Survey

IPHAS is a survey in r, i and Halpha of the galactic plane carried out using the Wide Field Camera on the Isaac Newton Telescope, La Palma.

2   Database Access

The access through AstroGrid is done using the workbench.

  1. Follow this link for help in downloading and setting up the workbench.
  2. Once up and running click on the data analysis tab and in the Task Launcher icon.
  3. Select then the IPHAS object catalogue as shown in this guide.
  4. See also the end of this page for some example queries and how to run them.

3   Data Coverage

The released data contains the observations carried out in the first two years of observations from 2003 to the end of 2005. The database contains about 200 million objects (most of them repeated twice) covering an area of 1700 sq. deg.. The figure below shows the coverage of these data in galactic coordinates.

edr_coverage_galactic2.gif

4   The main catalogue database

PhotoObjBest is the main catalogue table. Below a description of columns.

Name Description Units
ra Right Ascension, J2000 deg
dec Declination, J2000 deg
glon Galactic Longitude deg
glat Galactic Latitude deg
coremag_r Aperture magnitude in r band mag (Vega)
coremag_i Aperture magnitude in r band mag (Vega)
coremag_ha Aperture magnitude in Halpha band mag (Vega)
coremagerr_r Aperture magnitude error in r band mag (Vega)
coremagerr_i Aperture magnitude error in i band mag (Vega)
coremagerr_ha Aperture magnitude error in Halpha band mag (Vega)
class_r Classification index in r band  
class_i Classification index in i band  
class_ha Classification index in ha band  
ellipt_r Ellipticity on r band  
ellipt_i Ellipticity on i band  
ellipt_ha Ellipticity on Halpha band  
posang_r Position angle in r band deg
posang_i Position angle in i band deg
posang_ha Position angle in Halpha band deg
seeing_flag Seeing flag  
ellipt_flag Ellipticity flag  
photom_flag Photometric quality flag  
class_flag Classification flag  
chip_r_id Index of r band chip in table ChipAll  
chip_i_id Index of i band chip in table ChipAll  
chip_ha_id Index of Halpha band chip in table ChipAll  
field_id Index in table FieldsAll (pointer to field)  

The class_? flags are defined as follows:

Class Meaning
-9 means saturated
-8 indicative of poor match
-1 stellar
-2 probably stellar
-3 compact but probably not stellar
1 non-stellar (ie. would be galaxy normally)
0 noise-like

5   Example Queries

5.1   Search for objects around a position

For rectangular queries one can use:

--- Retrieve all objects in a rectangle
SELECT * FROM
  PhotoObj as P
WHERE
  P.ra > 15.4 AND P.ra < 15.6
  AND
  P.dec > 59.0 AND P.dec < 60.1

The table getObjCirc is used in the following example to retrieve all objects within a radius of 10 arcmin from the position RA=15.45, Dec=60.50:

--- Retrieve all objects within 10 arcmin of
--- the position RA=15.45, Dec=60.50
--- uses HTM to speed the query
SELECT * FROM 
  PhotoObj as P, getObjCirc as G
WHERE
  --- Insert here the ra, dec and radius in arcmin
  G._ra=15.45 AND G._dec=60.50 AND G._radius=10.0 
AND
  --- getObjCirc returns a table with id numbers
  --- satisfying the circular query
  G.id = P.id

The image below shows the result ra, dec distribution of the returned sources as well as their r band magnitude distribution.

iphas_cone_comb.png

5.2   Extracting colours

The following example selects positions and colours for sources observed in fields which match '7300':

SELECT 
   P.ra, P.dec, 
   P.coremag_r, P.coremag_i, P.coremag_ha,
   F.name
FROM PhotoObj as P, FieldsAll as F
--- ADQL does not support JOIN keyword
WHERE P.field_id = F.id AND F.name LIKE '%7300o%'

The following plot shows a colour-colour diagram extracted for the field 7300o. The plot on the right shows different objects as function of their magnitude (magenta: r<14, blue: r<16, grey: r<18 and green: r<20).

iphas_7300o_cc.png

5.3   Selecting by magnitude limit

The following query selects all the objects which are observed in frames where the r-band magnitude is greater or equal to 22.0 (the result is 366763 objects):

SELECT
   P.ra, P.dec, P.coremag_r, P.coremag_i, P.coremag_ha, F.name
FROM PhotoObj as P, PhotoPtr as T, FieldsAll as F, ChipAll as C 
WHERE P.pptr_id=T.id And T.chip_r_id=C.id And T.field_id=F.id and C.maglim>22.0

5.4   Adding additional constrains

In some cases you will want to retrieve objects which have been observed in a particular field, or only in those observations with a good seeing and/or good photometric conditions:

--- Select objects which have been observed in good conditions
SELECT TOP 1000 * FROM PhotoObj as P
WHERE
   --- Only objects observed in seeing <= 1.7 arcsec
   --- we may add more codes to different seeing values
   seeing_flag =1
AND
   --- Only objects observed with ellipticity <= 0.25
   --- we may add more codes to different ellipt values
   ellipt_flag = 1
AND
   --- Skip objects saturated in one or more bands
   class_flag <> -9
AND
   --- Only objects for which r, i and Ha have been obtained the same night
   night_flag = 1

5.5   Example Query Files

In order to load these queries follow this tutorial.

  1. iphas_rect.q performs a simple selection in ra and dec
  2. iphas_cone.q performs a simple cone search query using the HTM tree.
  3. iphas_field.q resturns all objects observed in a particular field.

6   Python Scripts

The script below shows an example of submitting a workflow from python. It is a single task workflow which runs a cone search in the database:

$> python iphas-cone.py 15.45 60.50 2.0 iphas_out.vot
Job: jes:galahad.star.le.ac.uk/143.210.36.238/ed@uk.ac.le.star/586
Status: RUNNING
Status: RUNNING
Result saved into MySpace file: ivo://uk.ac.le.star/ed#/iphas/iphas-20061027-151823.vot
Result saved into local file iphas_out.vot

where the arguments are the RA, Dec in decimal degrees and the radius in arcmin and the name of the output votable. Click on the file name below to get the script. Note that you still need the workench to be running to execute the script.

  1. iphas-cone.py

Docutils System Messages

System Message: INFO/1 (<string>, line 72)

External hyperlink target "schema" is not referenced.

System Message: ERROR/3 (<string>, line 74); backlink

Unknown target name: "class".