Difference between revisions of "Status of the verification partners"

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* Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
 
* Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
 
* Location: Loiano, Bologna, Italy
 
* Location: Loiano, Bologna, Italy
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*  
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* 1.5m
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'''TESTS:'''
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** 2011
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=== Asiago===
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* Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
 +
* Location: Padova, Italy
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* 1.82m
 +
 
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=== APT2===
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* Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
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* Location: Serra la Nave, Catania, Sicily
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* robotic 80cm Ritchey-Cretien
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=== TNT ===
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* Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it)
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* Location: Teramo, Italy,
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* 72cm Ritchey-Cretien
  
 
=== Swiss Euler ===
 
=== Swiss Euler ===
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* 1.2m
 
* 1.2m
  
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===Konkoly===
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* Contact person: Laszlo Szabados (szabados konkoly.hu)
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{| border="1" style="width:85%;"
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* Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary
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!Telescope/Observatory || Contact person (with email) || Details
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* 1m RCC,  60/90/180 cm Schmidt, 50 cm Cassegrain
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|-
 
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|Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile
 
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|-
 
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|Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time)
 
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|-
 
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|Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy
 
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|-
 
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|Padova  || Gisella Clementini || 1.82m reflector, Asiago, Italy
 
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|-
 
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|Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily
 
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|-
 
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|TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy
 
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|-
 
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|Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC,  60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary
 
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|-
 
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|}
 

Revision as of 08:08, 9 October 2012

Status of the partners preparing for the Gaia Alerts verification

Information about the requirements

In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are:

  1. react to an alert (or to a request with a target) and conduct its observations within 24h
  2. reduce the photometric data and submit to the CPCS within 24h from the observation
  3. flux calibrations better than 10% (0.1 mag)
  4. perform at least 5 (TBC) tests before June 2013.

Partners in test

Loiano

  • Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
  • Location: Loiano, Bologna, Italy
  • 1.5m

TESTS:

    • 2011

Asiago

  • Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
  • Location: Padova, Italy
  • 1.82m

APT2

  • Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it)
  • Location: Serra la Nave, Catania, Sicily
  • robotic 80cm Ritchey-Cretien

TNT

  • Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it)
  • Location: Teramo, Italy,
  • 72cm Ritchey-Cretien

Swiss Euler

  • Contact person: Laurent Eyer (laurent.eyer unige.ch)
  • La Silla, Chile
  • 1.2m

Belgian Mercatore

  • Contact person: Laurent Eyer (laurent.eyer unige.ch)
  • La Palma (Swiss time)
  • 1.2m

Konkoly

  • Contact person: Laszlo Szabados (szabados konkoly.hu)
  • Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary
  • 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain
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