Differences

This shows you the differences between two versions of the page.

--- start [2018/03/06 02:21] – [Interactive Access] intema
+++ start [2024/06/25 13:14] (current) – intema
@@ Line 22: / Line 22: @@
 News will be posted here and on our [[https://www.facebook.com/TGSSADR/|Facebook page]].
+   * 22-Aug-2018: Since 1-2 weeks there have been some issues with the VO server where TGSS ADR is hosted. As a result, also NASA SkyView has not been working correctly for TGSS ADR. Please know that the problem is being addressed, and SkyView is expected to properly work again in a matter of days.
    * 01-Dec-2017: A special version of TGSS ADR1 has been combined with NVSS to create a spectral index map and catalog of approx. 80 percent of the radio sky. The public data release page is found [[spidx|here]].
    * 15-Nov-2016: The TGSS-based LOFAR Sky Model Creator now has a flux cutoff option to exclude sources below a certain threshold. This can be used to speed up the initial calibration by using fewer model sources.
@@ Line 46: / Line 47: @@
 The TGSS ADR survey products are hosted by the ASTRON virtual observatory (VO) system. This system complies with the VO standard and can be accessed directly by tools like [[http://www.star.bris.ac.uk/~mbt/topcat/|TOPCAT]]. The VO system provides three services, for which web-based interfaces are available:
-   * [[http://vo.astron.nl/tgssadr/q_fits/imgs/form|TGSSADR Image Archive]] containing 5336 mosaic images of 5x5 square degrees covering the survey area.
+   * [[https://vo.astron.nl/tgssadr/q_fits/imgs/form|TGSSADR Image Archive]] containing 5336 mosaic images of 5x5 square degrees covering the survey area.
-   * [[http://vo.astron.nl/tgssadr/q_fits/cutout/form|TGSSADR Image Cutout Service]] provides cutout images of up to 1x1 square degrees anywhere in the survey area.
+   * [[https://vo.astron.nl/tgssadr/q_fits/cutout/form|TGSSADR Image Cutout Service]] provides cutout images of up to 1x1 square degrees anywhere in the survey area.
-   * [[http://vo.astron.nl/tgssadr/q/cone/form|TGSSADR Source Catalogue]] provides access to the 0.63 Million radio source catalog extracted from the full survey area.
+   * [[https://vo.astron.nl/tgssadr/q/cone/form|TGSSADR Source Catalogue]] provides access to the 0.63 Million radio source catalog extracted from the full survey area.
 The VO service links are given here:
-   * [[http://vo.astron.nl/tgssadr/q/cone/scs.xml|TGSSADR VO Source Cone Search (SCS)]]
+   * [[https://vo.astron.nl/tgssadr/q/cone/scs.xml|TGSSADR VO Source Cone Search (SCS)]]
-   * [[http://vo.astron.nl/tgssadr/q_fits/imgs/siap.xml|TGSSADR VO Simple Image Access (SIA)]]
+   * [[https://vo.astron.nl/tgssadr/q_fits/imgs/siap.xml|TGSSADR VO Simple Image Access (SIA)]]
 The 5x5 square degree mosaic images that form the basis of TGSS ADR1 are available for direct download [[http://tgssadr.strw.leidenuniv.nl/mosaics/|here]] (5336 FITS images; 32 MB each). Note that there is a factor 3.6(!) redundancy in the sky coverage, mainly to guarantee up to 1x1 square degree cutouts anywhere in the survey area.
@@ Line 73: / Line 74: @@
 <code python>
 import pyvo as vo
-url = 'http://vo.astron.nl/tgssadr/q/cone/scs.xml'
+url = 'https://vo.astron.nl/tgssadr/q/cone/scs.xml'
 t = vo.conesearch( url, pos = vo.object2pos( 'NGC 5939' ), radius = 30.0 )
 print t.votable
@@ Line 103: / Line 104: @@
 You can use the TGSS ADR source catalog for generating a BBS-compatible Global Sky Model to calibrate your LOFAR data. Either fill out the form below, or run something like \\
-//wget -O GSM.txt <nowiki>'http://tgssadr.strw.leidenuniv.nl/cgi-bin/gsmv3.cgi?coord=3c323&radius=3&unit=deg&deconv=y&cutoff=0.3'</nowiki>
+//wget -O GSM.txt <nowiki>'https://tgssadr.strw.leidenuniv.nl/cgi-bin/gsmv5.cgi?coord=3c323&radius=3&unit=deg&deconv=y&cutoff=0.3'</nowiki>
 //
 <html>
-<form name="TGSSGSM" method="POST" action="cgi-bin/gsmv3.cgi">
+<form name="TGSSGSM" method="POST" action="cgi-bin/gsmv5.cgi">
 Position =  <input type="text" name="coord" />
 (NED/Simbad Object or RA,Dec)
@@ Line 152: / Line 153: @@
   - D.A. Frail, P. Jagannathan, K.P. Mooley, H.T. Intema, 2016 (ApJ in press), [[https://arxiv.org/abs/1606.00449|arXiv:1606.00449]], \\ //Known Pulsars Identified in the GMRT 150 MHz All-Sky Survey//
   - S.J. Tingay, P.J. Hancock, R.B. Wayth, H. Intema, P. Jagannathan, K. Mooley, 2016 (AAS accepted), [[https://arxiv.org/abs/1606.01761|arXiv:1606.01761]] \\ //A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field//
+... and many many more.
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