Building-up a database of spectro-photometric standards from the UV to the NIR

J. Vernet; F. Kerber; V. Mainieri; T. Rauch; F. Saitta; S. D'Odorico; R. Bohlin; V. Ivanov; C. Lidman; E. Mason; A. Smette; J. Walsh; R. Fosbury; P. Goldoni; P. Groot; F. Hammer; L. Kaper; M. Horrobin; P. Kjaergaard-Rasmussen; F. Royer

doi:10.1017/S1743921310010574

Building-up a database of spectro-photometric standards from the UV to the NIR

J. Vernet, F. Kerber, V. Mainieri, T. Rauch, F. Saitta, S. D'Odorico, R. Bohlin, V. Ivanov, C. Lidman, E. Mason, A. Smette, J. Walsh, R. Fosbury, P. Goldoni, P. Groot, F. Hammer, L. Kaper, M. Horrobin, P. Kjaergaard-Rasmussen, F. Royer

Research School of Astronomy & Astrophysics

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Abstract

We present results of a project aimed at establishing a set of 12 spectro-photometric standards over a wide wavelength range from 320 to 2500 nm. Currently no such set of standard stars covering the near-IR is available. Our strategy is to extend the useful range of existing well-established optical flux standards (Oke 1990, Hamuy et al. 1992, 1994) into the near-IR by means of integral field spectroscopy with SINFONI at the VLT combined with state-of-the-art white dwarf stellar atmospheric models (TMAP, Holberg et al. 2008). As a solid reference, we use two primary HST standard white dwarfs GD71 and GD153 and one HST secondary standard BD+17 4708. The data were collected through an ESO “Observatory Programme” over ~40 nights between February 2007 and September 2008.

Original language	English
Pages (from-to)	535
Number of pages	1
Journal	Highlights of Astronomy
Volume	15
DOIs	https://doi.org/10.1017/S1743921310010574
Publication status	Published - 1 Nov 2010

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https://ui.adsabs.harvard.edu/abs/2010HiA....15..535V

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Vernet, J., Kerber, F., Mainieri, V., Rauch, T., Saitta, F., D'Odorico, S., Bohlin, R., Ivanov, V., Lidman, C., Mason, E., Smette, A., Walsh, J., Fosbury, R., Goldoni, P., Groot, P., Hammer, F., Kaper, L., Horrobin, M., Kjaergaard-Rasmussen, P., & Royer, F. (2010). Building-up a database of spectro-photometric standards from the UV to the NIR. Highlights of Astronomy, 15, 535. https://doi.org/10.1017/S1743921310010574

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title = "Building-up a database of spectro-photometric standards from the UV to the NIR",

abstract = "We present results of a project aimed at establishing a set of 12 spectro-photometric standards over a wide wavelength range from 320 to 2500 nm. Currently no such set of standard stars covering the near-IR is available. Our strategy is to extend the useful range of existing well-established optical flux standards (Oke 1990, Hamuy et al. 1992, 1994) into the near-IR by means of integral field spectroscopy with SINFONI at the VLT combined with state-of-the-art white dwarf stellar atmospheric models (TMAP, Holberg et al. 2008). As a solid reference, we use two primary HST standard white dwarfs GD71 and GD153 and one HST secondary standard BD+17 4708. The data were collected through an ESO “Observatory Programme” over ~40 nights between February 2007 and September 2008.",

author = "J. Vernet and F. Kerber and V. Mainieri and T. Rauch and F. Saitta and S. D'Odorico and R. Bohlin and V. Ivanov and C. Lidman and E. Mason and A. Smette and J. Walsh and R. Fosbury and P. Goldoni and P. Groot and F. Hammer and L. Kaper and M. Horrobin and P. Kjaergaard-Rasmussen and F. Royer",

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Vernet, J, Kerber, F, Mainieri, V, Rauch, T, Saitta, F, D'Odorico, S, Bohlin, R, Ivanov, V, Lidman, C, Mason, E, Smette, A, Walsh, J, Fosbury, R, Goldoni, P, Groot, P, Hammer, F, Kaper, L, Horrobin, M, Kjaergaard-Rasmussen, P & Royer, F 2010, 'Building-up a database of spectro-photometric standards from the UV to the NIR', Highlights of Astronomy, vol. 15, pp. 535. https://doi.org/10.1017/S1743921310010574

TY - JOUR

T1 - Building-up a database of spectro-photometric standards from the UV to the NIR

AU - Vernet, J.

AU - Kerber, F.

AU - Mainieri, V.

AU - Rauch, T.

AU - Saitta, F.

AU - D'Odorico, S.

AU - Bohlin, R.

AU - Ivanov, V.

AU - Lidman, C.

AU - Mason, E.

AU - Smette, A.

AU - Walsh, J.

AU - Fosbury, R.

AU - Goldoni, P.

AU - Groot, P.

AU - Hammer, F.

AU - Kaper, L.

AU - Horrobin, M.

AU - Kjaergaard-Rasmussen, P.

AU - Royer, F.

PY - 2010/11/1

Y1 - 2010/11/1

N2 - We present results of a project aimed at establishing a set of 12 spectro-photometric standards over a wide wavelength range from 320 to 2500 nm. Currently no such set of standard stars covering the near-IR is available. Our strategy is to extend the useful range of existing well-established optical flux standards (Oke 1990, Hamuy et al. 1992, 1994) into the near-IR by means of integral field spectroscopy with SINFONI at the VLT combined with state-of-the-art white dwarf stellar atmospheric models (TMAP, Holberg et al. 2008). As a solid reference, we use two primary HST standard white dwarfs GD71 and GD153 and one HST secondary standard BD+17 4708. The data were collected through an ESO “Observatory Programme” over ~40 nights between February 2007 and September 2008.

AB - We present results of a project aimed at establishing a set of 12 spectro-photometric standards over a wide wavelength range from 320 to 2500 nm. Currently no such set of standard stars covering the near-IR is available. Our strategy is to extend the useful range of existing well-established optical flux standards (Oke 1990, Hamuy et al. 1992, 1994) into the near-IR by means of integral field spectroscopy with SINFONI at the VLT combined with state-of-the-art white dwarf stellar atmospheric models (TMAP, Holberg et al. 2008). As a solid reference, we use two primary HST standard white dwarfs GD71 and GD153 and one HST secondary standard BD+17 4708. The data were collected through an ESO “Observatory Programme” over ~40 nights between February 2007 and September 2008.

U2 - 10.1017/S1743921310010574

DO - 10.1017/S1743921310010574

M3 - Article

VL - 15

SP - 535

JO - Highlights of Astronomy

JF - Highlights of Astronomy

ER -

Building-up a database of spectro-photometric standards from the UV to the NIR

Abstract

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