Sloan digital sky survey multicolor observations of GRB 010222

Brian C. Lee; Douglas L. Tucker; Daniel E. Vanden Berk; Brian Yanny; Daniel E. Reichart; Jennifer Adelman; Bing Chen; Mike Harvanek; Arne Henden; Željko Ivezić; Scot Kleinman; Don Lamb; Dan Long; Russet Mcmillan; Peter R. Newman; Atsuko Nitta; Povilas Palunas; Donald P. Schneider; Steph Snedden; Don York; John W. Briggs; J. Brinkmann; Istvan Csabai; Greg S. Hennessy; Stephen Kent; Robert Lupton; Heidi Jo Newberg; Chris Stoughton

doi:10.1086/322981

Sloan digital sky survey multicolor observations of GRB 010222

Brian C. Lee, Douglas L. Tucker, Daniel E. Vanden Berk, Brian Yanny, Daniel E. Reichart, Jennifer Adelman, Bing Chen, Mike Harvanek, Arne Henden, Željko Ivezić, Scot Kleinman, Don Lamb, Dan Long, Russet Mcmillan, Peter R. Newman, Atsuko Nitta, Povilas Palunas, Donald P. Schneider, Steph Snedden, Don YorkJohn W. Briggs, J. Brinkmann, Istvan Csabai, Greg S. Hennessy, Stephen Kent, Robert Lupton, Heidi Jo Newberg, Chris Stoughton

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Abstract

The discovery of an optical counterpart to GRB 010222 (detected by BeppoSAX) was announced 4.4 hr after the burst by Henden. The Sloan Digital Sky Survey's 0.5 m photometric telescope (PT) and 2.5 m survey telescope were used to observe the afterglow of GRB 010222 starting 4.8 hr after the gamma-ray burst. The 0.5 m PT observed the afterglow in five 300 s g*-band exposures over the course of half an hour, measuring a temporal decay rate in this short period of F_v ∝ t^-1±0.5. The 2.5 m camera imaged the counterpart nearly simultaneously in five filters (u*, g*, r*, i*, z*), with r* = 18.74 ± 0.02 at 12:10 UT. These multicolor observations, corrected for reddening and the afterglow's temporal decay, are well-fitted by the power law F_v ∝ v^-0.90±0.03 with the exception of the u*-band UV flux which is 20% below this slope. We examine possible interpretations of this spectral shape, including source extinction in a star-forming region.

Original language	English (US)
Pages (from-to)	183-188
Number of pages	6
Journal	Astrophysical Journal
Volume	561
Issue number	1 PART 1
DOIs	https://doi.org/10.1086/322981
State	Published - Nov 1 2001

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/322981

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Lee, B. C., Tucker, D. L., Vanden Berk, D. E., Yanny, B., Reichart, D. E., Adelman, J., Chen, B., Harvanek, M., Henden, A., Ivezić, Ž., Kleinman, S., Lamb, D., Long, D., Mcmillan, R., Newman, P. R., Nitta, A., Palunas, P., Schneider, D. P., Snedden, S., ... Stoughton, C. (2001). Sloan digital sky survey multicolor observations of GRB 010222. Astrophysical Journal, 561(1 PART 1), 183-188. https://doi.org/10.1086/322981

@article{84edd5d74f4d48e7a9a8a75da90ad2d3,

title = "Sloan digital sky survey multicolor observations of GRB 010222",

abstract = "The discovery of an optical counterpart to GRB 010222 (detected by BeppoSAX) was announced 4.4 hr after the burst by Henden. The Sloan Digital Sky Survey's 0.5 m photometric telescope (PT) and 2.5 m survey telescope were used to observe the afterglow of GRB 010222 starting 4.8 hr after the gamma-ray burst. The 0.5 m PT observed the afterglow in five 300 s g*-band exposures over the course of half an hour, measuring a temporal decay rate in this short period of Fv ∝ t-1±0.5. The 2.5 m camera imaged the counterpart nearly simultaneously in five filters (u*, g*, r*, i*, z*), with r* = 18.74 ± 0.02 at 12:10 UT. These multicolor observations, corrected for reddening and the afterglow's temporal decay, are well-fitted by the power law Fv ∝ v-0.90±0.03 with the exception of the u*-band UV flux which is 20% below this slope. We examine possible interpretations of this spectral shape, including source extinction in a star-forming region.",

author = "Lee, {Brian C.} and Tucker, {Douglas L.} and {Vanden Berk}, {Daniel E.} and Brian Yanny and Reichart, {Daniel E.} and Jennifer Adelman and Bing Chen and Mike Harvanek and Arne Henden and {\v Z}eljko Ivezi{\'c} and Scot Kleinman and Don Lamb and Dan Long and Russet Mcmillan and Newman, {Peter R.} and Atsuko Nitta and Povilas Palunas and Schneider, {Donald P.} and Steph Snedden and Don York and Briggs, {John W.} and J. Brinkmann and Istvan Csabai and Hennessy, {Greg S.} and Stephen Kent and Robert Lupton and Newberg, {Heidi Jo} and Chris Stoughton",

year = "2001",

month = nov,

day = "1",

doi = "10.1086/322981",

language = "English (US)",

volume = "561",

pages = "183--188",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

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Lee, BC, Tucker, DL, Vanden Berk, DE, Yanny, B, Reichart, DE, Adelman, J, Chen, B, Harvanek, M, Henden, A, Ivezić, Ž, Kleinman, S, Lamb, D, Long, D, Mcmillan, R, Newman, PR, Nitta, A, Palunas, P, Schneider, DP, Snedden, S, York, D, Briggs, JW, Brinkmann, J, Csabai, I, Hennessy, GS, Kent, S, Lupton, R, Newberg, HJ & Stoughton, C 2001, 'Sloan digital sky survey multicolor observations of GRB 010222', Astrophysical Journal, vol. 561, no. 1 PART 1, pp. 183-188. https://doi.org/10.1086/322981

TY - JOUR

T1 - Sloan digital sky survey multicolor observations of GRB 010222

AU - Lee, Brian C.

AU - Tucker, Douglas L.

AU - Vanden Berk, Daniel E.

AU - Yanny, Brian

AU - Reichart, Daniel E.

AU - Adelman, Jennifer

AU - Chen, Bing

AU - Harvanek, Mike

AU - Henden, Arne

AU - Ivezić, Željko

AU - Kleinman, Scot

AU - Lamb, Don

AU - Long, Dan

AU - Mcmillan, Russet

AU - Newman, Peter R.

AU - Nitta, Atsuko

AU - Palunas, Povilas

AU - Schneider, Donald P.

AU - Snedden, Steph

AU - York, Don

AU - Briggs, John W.

AU - Brinkmann, J.

AU - Csabai, Istvan

AU - Hennessy, Greg S.

AU - Kent, Stephen

AU - Lupton, Robert

AU - Newberg, Heidi Jo

AU - Stoughton, Chris

PY - 2001/11/1

Y1 - 2001/11/1

N2 - The discovery of an optical counterpart to GRB 010222 (detected by BeppoSAX) was announced 4.4 hr after the burst by Henden. The Sloan Digital Sky Survey's 0.5 m photometric telescope (PT) and 2.5 m survey telescope were used to observe the afterglow of GRB 010222 starting 4.8 hr after the gamma-ray burst. The 0.5 m PT observed the afterglow in five 300 s g*-band exposures over the course of half an hour, measuring a temporal decay rate in this short period of Fv ∝ t-1±0.5. The 2.5 m camera imaged the counterpart nearly simultaneously in five filters (u*, g*, r*, i*, z*), with r* = 18.74 ± 0.02 at 12:10 UT. These multicolor observations, corrected for reddening and the afterglow's temporal decay, are well-fitted by the power law Fv ∝ v-0.90±0.03 with the exception of the u*-band UV flux which is 20% below this slope. We examine possible interpretations of this spectral shape, including source extinction in a star-forming region.

AB - The discovery of an optical counterpart to GRB 010222 (detected by BeppoSAX) was announced 4.4 hr after the burst by Henden. The Sloan Digital Sky Survey's 0.5 m photometric telescope (PT) and 2.5 m survey telescope were used to observe the afterglow of GRB 010222 starting 4.8 hr after the gamma-ray burst. The 0.5 m PT observed the afterglow in five 300 s g*-band exposures over the course of half an hour, measuring a temporal decay rate in this short period of Fv ∝ t-1±0.5. The 2.5 m camera imaged the counterpart nearly simultaneously in five filters (u*, g*, r*, i*, z*), with r* = 18.74 ± 0.02 at 12:10 UT. These multicolor observations, corrected for reddening and the afterglow's temporal decay, are well-fitted by the power law Fv ∝ v-0.90±0.03 with the exception of the u*-band UV flux which is 20% below this slope. We examine possible interpretations of this spectral shape, including source extinction in a star-forming region.

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U2 - 10.1086/322981

DO - 10.1086/322981

M3 - Article

AN - SCOPUS:0035510949

SN - 0004-637X

VL - 561

SP - 183

EP - 188

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 1

ER -

Sloan digital sky survey multicolor observations of GRB 010222

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