VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016)

I. Arcavi; W. M. Wolf; D. A. Howell; L. Bildsten; G. Leloudas; D. Hardin; S. Prajs; D. A. Perley; G. Svirski; A. Gal-Yam; B. Katz; C. McCully; S. B. Cenko; C. Lidman; M. Sullivan; S. Valenti; P. Astier; C. Balland; R. G. Carlberg; A. Conley; D. Fouchez; J. Guy; R. Pain; N. Palanque-Delabrouille; K. Perrett; C. J. Pritchet; N. Regnault; J. Rich; V. Ruhlmann-Kleider

doi:10.26093/cds/vizier.18190035

VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016)

I. Arcavi, W. M. Wolf, D. A. Howell, L. Bildsten, G. Leloudas, D. Hardin, S. Prajs, D. A. Perley, G. Svirski, A. Gal-Yam, B. Katz, C. McCully, S. B. Cenko, C. Lidman, M. Sullivan, S. Valenti, P. Astier, C. Balland, R. G. Carlberg, A. ConleyD. Fouchez, J. Guy, R. Pain, N. Palanque-Delabrouille, K. Perrett, C. J. Pritchet, N. Regnault, J. Rich, V. Ruhlmann-Kleider

Research output: Other contribution

Abstract

PTF10iam was discovered by the Palomar 48 inch Oschin Schmidt telescope (P48) as part of the PTF survey. The three Supernova Legacy Survey (SNLS; Astier et al. 2006A&A...447...31A) events (SNLS04D4ec, SNLS05D2bk and SNLS06D1hc) were discovered by the deep survey of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS 2002), using the CFHT 3.6m telescope.

The SNLS host-galaxy magnitudes were obtained from the SNLS five-year imaging data set (D. Hardin et al. 2016, in preparation), following the general method described in Kronborg et al. (2010A&A...514A..44K). In short, photometry was performed on deep image stacks in the ugriz CFHT/Megacam filters.

(2 data files).

Original language	English
DOIs	https://doi.org/10.26093/cds/vizier.18190035
Publication status	Published - 1 May 2016

Access to Document

10.26093/cds/vizier.18190035

https://ui.adsabs.harvard.edu/abs/2016yCat..18190035A

Cite this

Arcavi, I., Wolf, W. M., Howell, D. A., Bildsten, L., Leloudas, G., Hardin, D., Prajs, S., Perley, D. A., Svirski, G., Gal-Yam, A., Katz, B., McCully, C., Cenko, S. B., Lidman, C., Sullivan, M., Valenti, S., Astier, P., Balland, C., Carlberg, R. G., ... Ruhlmann-Kleider, V. (2016, May 1). VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016). https://doi.org/10.26093/cds/vizier.18190035

@misc{224ba3409bd843f0be9b5c424b7a44f0,

title = "VizieR Online Data Catalog: Light curves of four transients from PTF \& SNLS (Arcavi+, 2016)",

abstract = "PTF10iam was discovered by the Palomar 48 inch Oschin Schmidt telescope (P48) as part of the PTF survey. The three Supernova Legacy Survey (SNLS; Astier et al. 2006A\&A...447...31A) events (SNLS04D4ec, SNLS05D2bk and SNLS06D1hc) were discovered by the deep survey of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS 2002), using the CFHT 3.6m telescope. The SNLS host-galaxy magnitudes were obtained from the SNLS five-year imaging data set (D. Hardin et al. 2016, in preparation), following the general method described in Kronborg et al. (2010A\&A...514A..44K). In short, photometry was performed on deep image stacks in the ugriz CFHT/Megacam filters. (2 data files).",

keywords = "Supernovae, Photometry: ugriz",

author = "I. Arcavi and Wolf, \{W. M.\} and Howell, \{D. A.\} and L. Bildsten and G. Leloudas and D. Hardin and S. Prajs and Perley, \{D. A.\} and G. Svirski and A. Gal-Yam and B. Katz and C. McCully and Cenko, \{S. B.\} and C. Lidman and M. Sullivan and S. Valenti and P. Astier and C. Balland and Carlberg, \{R. G.\} and A. Conley and D. Fouchez and J. Guy and R. Pain and N. Palanque-Delabrouille and K. Perrett and Pritchet, \{C. J.\} and N. Regnault and J. Rich and V. Ruhlmann-Kleider",

year = "2016",

month = may,

day = "1",

doi = "10.26093/cds/vizier.18190035",

language = "English",

type = "Other",

}

Arcavi, I, Wolf, WM, Howell, DA, Bildsten, L, Leloudas, G, Hardin, D, Prajs, S, Perley, DA, Svirski, G, Gal-Yam, A, Katz, B, McCully, C, Cenko, SB, Lidman, C, Sullivan, M, Valenti, S, Astier, P, Balland, C, Carlberg, RG, Conley, A, Fouchez, D, Guy, J, Pain, R, Palanque-Delabrouille, N, Perrett, K, Pritchet, CJ, Regnault, N, Rich, J & Ruhlmann-Kleider, V 2016, VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016).. https://doi.org/10.26093/cds/vizier.18190035

TY - GEN

T1 - VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016)

AU - Arcavi, I.

AU - Wolf, W. M.

AU - Howell, D. A.

AU - Bildsten, L.

AU - Leloudas, G.

AU - Hardin, D.

AU - Prajs, S.

AU - Perley, D. A.

AU - Svirski, G.

AU - Gal-Yam, A.

AU - Katz, B.

AU - McCully, C.

AU - Cenko, S. B.

AU - Lidman, C.

AU - Sullivan, M.

AU - Valenti, S.

AU - Astier, P.

AU - Balland, C.

AU - Carlberg, R. G.

AU - Conley, A.

AU - Fouchez, D.

AU - Guy, J.

AU - Pain, R.

AU - Palanque-Delabrouille, N.

AU - Perrett, K.

AU - Pritchet, C. J.

AU - Regnault, N.

AU - Rich, J.

AU - Ruhlmann-Kleider, V.

PY - 2016/5/1

Y1 - 2016/5/1

N2 - PTF10iam was discovered by the Palomar 48 inch Oschin Schmidt telescope (P48) as part of the PTF survey. The three Supernova Legacy Survey (SNLS; Astier et al. 2006A&A...447...31A) events (SNLS04D4ec, SNLS05D2bk and SNLS06D1hc) were discovered by the deep survey of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS 2002), using the CFHT 3.6m telescope. The SNLS host-galaxy magnitudes were obtained from the SNLS five-year imaging data set (D. Hardin et al. 2016, in preparation), following the general method described in Kronborg et al. (2010A&A...514A..44K). In short, photometry was performed on deep image stacks in the ugriz CFHT/Megacam filters. (2 data files).

AB - PTF10iam was discovered by the Palomar 48 inch Oschin Schmidt telescope (P48) as part of the PTF survey. The three Supernova Legacy Survey (SNLS; Astier et al. 2006A&A...447...31A) events (SNLS04D4ec, SNLS05D2bk and SNLS06D1hc) were discovered by the deep survey of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS 2002), using the CFHT 3.6m telescope. The SNLS host-galaxy magnitudes were obtained from the SNLS five-year imaging data set (D. Hardin et al. 2016, in preparation), following the general method described in Kronborg et al. (2010A&A...514A..44K). In short, photometry was performed on deep image stacks in the ugriz CFHT/Megacam filters. (2 data files).

KW - Supernovae

KW - Photometry: ugriz

U2 - 10.26093/cds/vizier.18190035

DO - 10.26093/cds/vizier.18190035

M3 - Other contribution

ER -

VizieR Online Data Catalog: Light curves of four transients from PTF & SNLS (Arcavi+, 2016)

Abstract

Access to Document

Fingerprint

Cite this