VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014)

Y. -C. Pan; M. Sullivan; K. Maguire; I. M. Hook; P. E. Nugent; D. A. Howell; I. Arcavi; J. Botyanszki; S. B. Cenko; J. Derose; H. K. Fakhouri; A. Gal-Yam; E. Hsiao; S. R. Kulkarni; R. R. Laher; C. Lidman; J. Nordin; E. S. Walker; D. Xu

VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014)

Y. -C. Pan, M. Sullivan, K. Maguire, I. M. Hook, P. E. Nugent, D. A. Howell, I. Arcavi, J. Botyanszki, S. B. Cenko, J. Derose, H. K. Fakhouri, A. Gal-Yam, E. Hsiao, S. R. Kulkarni, R. R. Laher, C. Lidman, J. Nordin, E. S. Walker, D. Xu

Research School of Astronomy & Astrophysics

Research output: Other contribution

Abstract

The SNe Ia studied in this paper were discovered by the PTF, a project which operated from 2009 to 2012 and used the CFH12k wide-field survey camera mounted on the Samuel Oschin 48 inch telescope (P48) at the Palomar Observatory. The observational cadences used to discover the SNe ranged from hours up to ~5d. SN candidates were identified in image subtraction data and ranked using both simple cuts on the detection parameters and a machine learning algorithm (Bloom et al. 2012PASP..124.1175B), and then visually confirmed by members of the PTF collaboration or, from mid-2010 onwards, via the citizen science project 'Galaxy Zoo: Supernova' (Smith et al., 2011MNRAS.412.1309S). The latter identified eight of the SNe studied in this paper.

(4 data files).

Original language	English
Publication status	Published - 1 Nov 2014

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Pan, Y. .-C., Sullivan, M., Maguire, K., Hook, I. M., Nugent, P. E., Howell, D. A., Arcavi, I., Botyanszki, J., Cenko, S. B., Derose, J., Fakhouri, H. K., Gal-Yam, A., Hsiao, E., Kulkarni, S. R., Laher, R. R., Lidman, C., Nordin, J., Walker, E. S., & Xu, D. (2014, Nov 1). VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014). https://ui.adsabs.harvard.edu/abs/2014yCat..74381391P

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title = "VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014)",

abstract = "The SNe Ia studied in this paper were discovered by the PTF, a project which operated from 2009 to 2012 and used the CFH12k wide-field survey camera mounted on the Samuel Oschin 48 inch telescope (P48) at the Palomar Observatory. The observational cadences used to discover the SNe ranged from hours up to ~5d. SN candidates were identified in image subtraction data and ranked using both simple cuts on the detection parameters and a machine learning algorithm (Bloom et al. 2012PASP..124.1175B), and then visually confirmed by members of the PTF collaboration or, from mid-2010 onwards, via the citizen science project 'Galaxy Zoo: Supernova' (Smith et al., 2011MNRAS.412.1309S). The latter identified eight of the SNe studied in this paper. (4 data files).",

keywords = "Supernovae",

author = "Pan, {Y. -C.} and M. Sullivan and K. Maguire and Hook, {I. M.} and Nugent, {P. E.} and Howell, {D. A.} and I. Arcavi and J. Botyanszki and Cenko, {S. B.} and J. Derose and Fakhouri, {H. K.} and A. Gal-Yam and E. Hsiao and Kulkarni, {S. R.} and Laher, {R. R.} and C. Lidman and J. Nordin and Walker, {E. S.} and D. Xu",

year = "2014",

month = nov,

day = "1",

language = "English",

type = "Other",

}

TY - GEN

T1 - VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014)

AU - Pan, Y. -C.

AU - Sullivan, M.

AU - Maguire, K.

AU - Hook, I. M.

AU - Nugent, P. E.

AU - Howell, D. A.

AU - Arcavi, I.

AU - Botyanszki, J.

AU - Cenko, S. B.

AU - Derose, J.

AU - Fakhouri, H. K.

AU - Gal-Yam, A.

AU - Hsiao, E.

AU - Kulkarni, S. R.

AU - Laher, R. R.

AU - Lidman, C.

AU - Nordin, J.

AU - Walker, E. S.

AU - Xu, D.

PY - 2014/11/1

Y1 - 2014/11/1

N2 - The SNe Ia studied in this paper were discovered by the PTF, a project which operated from 2009 to 2012 and used the CFH12k wide-field survey camera mounted on the Samuel Oschin 48 inch telescope (P48) at the Palomar Observatory. The observational cadences used to discover the SNe ranged from hours up to ~5d. SN candidates were identified in image subtraction data and ranked using both simple cuts on the detection parameters and a machine learning algorithm (Bloom et al. 2012PASP..124.1175B), and then visually confirmed by members of the PTF collaboration or, from mid-2010 onwards, via the citizen science project 'Galaxy Zoo: Supernova' (Smith et al., 2011MNRAS.412.1309S). The latter identified eight of the SNe studied in this paper. (4 data files).

AB - The SNe Ia studied in this paper were discovered by the PTF, a project which operated from 2009 to 2012 and used the CFH12k wide-field survey camera mounted on the Samuel Oschin 48 inch telescope (P48) at the Palomar Observatory. The observational cadences used to discover the SNe ranged from hours up to ~5d. SN candidates were identified in image subtraction data and ranked using both simple cuts on the detection parameters and a machine learning algorithm (Bloom et al. 2012PASP..124.1175B), and then visually confirmed by members of the PTF collaboration or, from mid-2010 onwards, via the citizen science project 'Galaxy Zoo: Supernova' (Smith et al., 2011MNRAS.412.1309S). The latter identified eight of the SNe studied in this paper. (4 data files).

KW - Supernovae

M3 - Other contribution

ER -

VizieR Online Data Catalog: Host galaxies of Type Ia SN from PTF (Pan+, 2014)

Abstract

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