All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

BOOTES-IR: a robotic nIR astronomical observatory devoted to follow-up of transient phenomena

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F06%3A00234276" target="_blank" >RIV/68407700:21230/06:00234276 - isvavai.cz</a>

  • Result on the web

    <a href="http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1288144" target="_blank" >http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1288144</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1117/12.671579" target="_blank" >10.1117/12.671579</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    BOOTES-IR: a robotic nIR astronomical observatory devoted to follow-up of transient phenomena

  • Original language description

    "BOOTES-IR" is the extension of the BOOTES experiment, which has been operating in Southern Spain since 1998, to the near-infrared (nIR). The goal is to follow up the early stage of the gamma ray burst (GRB) afterglow emission in the nIR, as BOOTES doesalready at optical wavelengths. The scientific case that drives the BOOTES-IR performance is the study of GRBs with the support of spacecraft like HETE-2, INTEGRAL and SWIFT (and GLAST in the future). Given that the afterglow emission in both, the nIR and the optical, in the instances immediately following a GRB, is extremely bright (reached V = 8.9 in one case), it should be possible to detect this prompt emission at nIR wavelengths too. Combined observations by BOOTES-IR and BOOTES-1 and BOOTES-2 since 2006 can allow for real time identification of trustworthy candidates to have a ultra-high redshift (z > 6). It is expected that, few minutes after a GRB, the nIR magnitudes be H ~ 10-15, hence very high quality spectra can be obtained

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    V - Vyzkumna aktivita podporovana z jinych verejnych zdroju

Others

  • Publication year

    2006

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Ground-based and Airborne Telescopes

  • ISBN

    0-8194-6332-9

  • ISSN

    0277-786X

  • e-ISSN

  • Number of pages

    3

  • Pages from-to

  • Publisher name

    SPIE

  • Place of publication

    Orlando, Florida

  • Event location

    Orlando

  • Event date

    May 24, 2006

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000240018600019