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ata_testing [2018/04/10 20:59] jrsetiata_testing [2023/10/28 18:36] (current) – external edit 127.0.0.1
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-==ATA Testing==+===ATA Testing===
  
-===Thoughts from Andrew and Griffin===+==Feed Measurements== 
 + 
 +  * [[feed_measurements|Feed Measurements]] 
 +  * [[sefd_measurements|SEFD Measurements]] 
 + 
 +==Data Gathers== 
 + 
 +  * [[data_gathered|These sources have been observed with the Beamformer]] 
 + 
 +==Pulsar Finding== 
 + 
 +  * [[pulsar_finding|Pulsars]] 
 + 
 +==Handful of Sources== 
 + 
 +  * http://adsbit.harvard.edu//full/1994A%26A...284..331O/0000335.000.html 
 +  * [[http://www.atnf.csiro.au/people/pulsar/psrcat/|Pulsars]] 
 + 
 +  * [[https://github.com/UCBerkeleySETI/breakthrough/blob/master/doc/RAW-File-Format.md|GUPPI Raw format]] 
 +  * [[https://github.com/UCBerkeleySETI/gbt_seti/blob/master/src/filterbank_mkheader.c|Filterbank header]] 
 +  * [[http://astro.berkeley.edu/~davidm/rb-blgbt.git|Filterbank Ruby code from Dave]] 
 +  * [[http://sigproc.sourceforge.net/sigproc.pdf|Filterbank header spec (see section 3)]] 
 +  * [[https://github.com/UCBerkeleySETI/breakthrough/blob/master/GBT/voyager/voyager.ipynb|Filterbank Voyager1 Tutorial/Jupyter]] 
 + 
 +==Thoughts from Andrew and Griffin==
  
 Email from August 07, 2017 from Griffin: Email from August 07, 2017 from Griffin:
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   Positions for these sources can be found on SIMBAD, e.g.: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=3C48&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id   Positions for these sources can be found on SIMBAD, e.g.: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=3C48&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id
 +  
   I would recommend cross scans at the nominal position in addition to the ON/OFF, as was done in the reference    I would recommend cross scans at the nominal position in addition to the ON/OFF, as was done in the reference 
   above.   above.
 +  
   For the purposes of analyzing these observations, we will want to be able to produce coarsely channelized and    For the purposes of analyzing these observations, we will want to be able to produce coarsely channelized and 
   integrated spectral data, e.g. ~1s time integration and 1 MHz frequency resolution.  This should keep the data rate    integrated spectral data, e.g. ~1s time integration and 1 MHz frequency resolution.  This should keep the data rate 
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 +==Pulsars==
 +
 +PSR B0329+54
 +  RA: 03h 32m 59.368s
 +  Dec: +54° 34′ 43.57″
 +  In hours,degrees: 3.5498244,54.5787694
 +  
 +PSR B0531+21 (Crab Pulsar)
 +  RA: 05h 34m 31.97s
 +  Dec: +22° 00' 52.1"
 +  In hours,degrees: 5.5755472,22.0144722
 +  
 +PSR B0950+08
 +  RA: 09h 53m 09.310s
 +  Dec: +07° 55' 35.75"
 +  In hours,degrees: 9.8859194,7.9265972
  
ata_testing.1523393956.txt.gz · Last modified: 2023/10/28 18:36 (external edit)

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