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Matheson, T, Joyce, RR, Allen, LE, Saha, A, Silva, DR, Wood-vasey, WM, Adams, JJ, Anderson, RE, Beck, TL, Bentz, MC, Bershady, MA, Binkert, WS, Butler, K, Camarata, MA, Eigenbrot, A, Everett, M, Gallagher, JS, Garnavich, PM, Glikman, E, Harbeck, D, Hargis, JR, Herbst, H, Horch, EP, Howell, SB, Jha, S, Kaczmarek, JF, Knezek, P, Manne-nicholas, E, Mathieu, RD, Meixner, M, Milliman, K, Power, J, Rajagopal, J, Reetz, K, Rhode, KL, Schechtman-rook, A, Schwamb, ME, Schweiker, H
, Simmons, B, Simon, JD, Summers, D, Young, MD, Weyant, A, Wilcots, EM, Will, G & Williams, D 2012, '
The infrared light curve of SN 2011fe IN M101 and the distance to M101',
The Astrophysical Journal, vol. 754, no. 1, 19.
https://doi.org/10.1088/0004-637X/754/1/19APA
Matheson, T., Joyce, R. R., Allen, L. E., Saha, A., Silva, D. R., Wood-vasey, W. M., Adams, J. J., Anderson, R. E., Beck, T. L., Bentz, M. C., Bershady, M. A., Binkert, W. S., Butler, K., Camarata, M. A., Eigenbrot, A., Everett, M., Gallagher, J. S., Garnavich, P. M., Glikman, E., ... Williams, D. (2012).
The infrared light curve of SN 2011fe IN M101 and the distance to M101.
The Astrophysical Journal,
754(1), Article 19.
https://doi.org/10.1088/0004-637X/754/1/19Vancouver
Author
Bibtex
@article{f21a243a8ebf452a81ce32966752e491,
title = "The infrared light curve of SN 2011fe IN M101 and the distance to M101",
abstract = "We present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in Hband starting 14 days before maximum brightness in the B band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera. When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 ± 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used.",
author = "T. Matheson and Joyce, {R. R.} and Allen, {L. E.} and A. Saha and Silva, {D. R.} and Wood-vasey, {W. M.} and Adams, {J. J.} and Anderson, {R. E.} and Beck, {T. L.} and Bentz, {M. C.} and Bershady, {M. A.} and Binkert, {W. S.} and K. Butler and Camarata, {M. A.} and A. Eigenbrot and M. Everett and Gallagher, {J. S.} and Garnavich, {P. M.} and E. Glikman and D. Harbeck and Hargis, {J. R.} and H. Herbst and Horch, {E. P.} and Howell, {S. B.} and S. Jha and Kaczmarek, {J. F.} and P. Knezek and E. Manne-nicholas and Mathieu, {R. D.} and M. Meixner and K. Milliman and J. Power and J. Rajagopal and K. Reetz and Rhode, {K. L.} and A. Schechtman-rook and Schwamb, {M. E.} and H. Schweiker and B. Simmons and Simon, {J. D.} and D. Summers and Young, {M. D.} and A. Weyant and Wilcots, {E. M.} and G. Will and D. Williams",
year = "2012",
month = jul,
day = "20",
doi = "10.1088/0004-637X/754/1/19",
language = "English",
volume = "754",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "1",
}
RIS
TY - JOUR
T1 - The infrared light curve of SN 2011fe IN M101 and the distance to M101
AU - Matheson, T.
AU - Joyce, R. R.
AU - Allen, L. E.
AU - Saha, A.
AU - Silva, D. R.
AU - Wood-vasey, W. M.
AU - Adams, J. J.
AU - Anderson, R. E.
AU - Beck, T. L.
AU - Bentz, M. C.
AU - Bershady, M. A.
AU - Binkert, W. S.
AU - Butler, K.
AU - Camarata, M. A.
AU - Eigenbrot, A.
AU - Everett, M.
AU - Gallagher, J. S.
AU - Garnavich, P. M.
AU - Glikman, E.
AU - Harbeck, D.
AU - Hargis, J. R.
AU - Herbst, H.
AU - Horch, E. P.
AU - Howell, S. B.
AU - Jha, S.
AU - Kaczmarek, J. F.
AU - Knezek, P.
AU - Manne-nicholas, E.
AU - Mathieu, R. D.
AU - Meixner, M.
AU - Milliman, K.
AU - Power, J.
AU - Rajagopal, J.
AU - Reetz, K.
AU - Rhode, K. L.
AU - Schechtman-rook, A.
AU - Schwamb, M. E.
AU - Schweiker, H.
AU - Simmons, B.
AU - Simon, J. D.
AU - Summers, D.
AU - Young, M. D.
AU - Weyant, A.
AU - Wilcots, E. M.
AU - Will, G.
AU - Williams, D.
PY - 2012/7/20
Y1 - 2012/7/20
N2 - We present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in Hband starting 14 days before maximum brightness in the B band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera. When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 ± 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used.
AB - We present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in Hband starting 14 days before maximum brightness in the B band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera. When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 ± 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used.
U2 - 10.1088/0004-637X/754/1/19
DO - 10.1088/0004-637X/754/1/19
M3 - Journal article
VL - 754
JO - The Astrophysical Journal
JF - The Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 19
ER -
