Gamma-Ray Burst Optical/Near-Infrared Detector

{{Redirect|Grond|other topics of the same name|Grond (disambiguation)}}

Image:GROND ESO first light.jpg (a dark blue cylinder at the lower left)]]

The Gamma-Ray Burst Optical/Near-Infrared Detector (GROND) is an imaging instrument used to investigate Gamma-Ray Burst afterglows and for doing follow-up observations on exoplanets using transit photometry.{{cite journal |title=OGLE2-TR-L9b: an exoplanet transiting a rapidly rotating F3 star |url=http://www.mpe.mpg.de/~saglia/journals_pdf/snellen2009.pdf |last1=Snellen |first1=I. A. G. |last2=Koppenhoefer |first2=J. |journal=Astronomy & Astrophysics |doi=10.1051/0004-6361/200810917 |date=2008 |bibcode=2009A&A...497..545S |volume=497 |issue=2 |pages=545–550|arxiv=0812.0599 |s2cid=15639369 }}{{Cite journal|url=http://www.aanda.org/articles/aa/full_html/2012/03/aa18336-11/aa18336-11.html|doi = 10.1051/0004-6361/201118336|title = WASP-4b transit observations with GROND|year = 2012|last1 = Nikolov|first1 = N.|last2 = Henning|first2 = Th.|last3 = Koppenhoefer|first3 = J.|last4 = Lendl|first4 = M.|last5 = MacIejewski|first5 = G.|last6 = Greiner|first6 = J.|journal = Astronomy & Astrophysics|volume = 539|pages = A159|arxiv = 1201.5727|bibcode = 2012A&A...539A.159N|s2cid = 59017585}}

{{cite press release

|title = GROND Takes Off

|publisher = European Organisation for Astronomical Research in the Southern Hemisphere (ESO)

|date = 2007-07-06

|url = http://www.eso.org/public/outreach/press-rel/pr-2007/pr-30-07.html

|accessdate = 2009-02-23

|url-status = dead

|archiveurl = https://web.archive.org/web/20090225100400/http://www.eso.org/public/outreach/press-rel/pr-2007/pr-30-07.html

|archivedate = 2009-02-25

}} It is operated at the 2.2-metre MPG/ESO telescope at ESO's La Silla Observatory in the southern part of the Atacama desert, about 600 kilometres north of Santiago de Chile and at an altitude of 2,400 metres.

Discoveries

  • On 13 September 2008, Swift detected gamma-ray burst 080913. GROND and VLT subsequently placed the GRB at 12.8 Gly distant, making it the most-distant GRB observed, as well as the second-most-distant object to be spectroscopically confirmed.{{cite press release

| title = NASA's Swift Catches Farthest Ever Gamma-Ray Burst

| publisher = NASA

| date = 2008-09-19

| url = http://www.nasa.gov/mission_pages/swift/bursts/farthest_grb.html

| accessdate = 2009-02-23}}{{cite journal

| first = Jochen

| last = Greiner

| title = GRB 080913 at redshift 6.7

| year = 2009

| arxiv = 0810.2314

|display-authors=etal

| doi=10.1088/0004-637X/693/2/1610

| bibcode=2009ApJ...693.1610G

| volume=693

| journal=The Astrophysical Journal

| issue = 2

| pages=1610–1620| s2cid = 14713585

}}

  • On 15 September 2008, NASA's Fermi Gamma-ray Space Telescope detected gamma-ray burst 080916C. On 19 February 2009, NASA announced that the GROND team's work shows that the GRB was the most energetic yet observed, and 12.2 Gly distant.{{cite press release

| title = NASA's Fermi Telescope Sees Most Extreme Gamma-ray Blast Yet

| publisher = NASA

| date = 2009-02-19

| url = http://www.nasa.gov/mission_pages/GLAST/news/high_grb.html

| accessdate = 2009-02-23}}{{cite journal

| first = Jochen

| last = Greiner

| title = The redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C

| date = 2009-02-04

| arxiv = 0902.0761

|display-authors=etal

| doi=10.1051/0004-6361/200811571

| bibcode=2009A&A...498...89G

| volume=498

| journal=Astronomy and Astrophysics

| issue = 1

| pages=89–94| s2cid = 6758498

}}

See also

References

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