The Experts below are selected from a list of 28950 Experts worldwide ranked by ideXlab platform
Brett C Addison - One of the best experts on this subject based on the ideXlab platform.
-
stellar obliquities and planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b and wasp 109b
The Astronomical Journal, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, D J Wright, D BaylissAbstract:We report measurements of the sky-projected spin-orbit angles for three transiting hot Jupiters, two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low-obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter-McLaughlin effect over the course of the transits from high-resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin-orbit angles are lambda = 7 degrees(+11)(-12 degrees)degrees, lambda = 79 degrees(+19)(-10 degrees)degrees, and lambda = 99 degrees(+10)(-9 degrees)degrees for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly 90 degrees from their host star's equator, while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with T-eff = 6250 +/- 120 K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with T-eff = 6900 +/- 120 K and F4 with T-eff = 6520 +/- 140 K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
-
stellar obliquities planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b wasp 109b
arXiv: Earth and Planetary Astrophysics, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, David Wright, D BaylissAbstract:We report measurements of the sky-projected spin--orbit angles for three transiting hot Jupiters: two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter--McLaughlin effect over the course of the transits from high resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin--orbit angles are $\lambda = {-7^{\circ}}^{+11^{\circ}}_{-12^{\circ}}$, $\lambda = {79^{\circ}}^{+19^{\circ}}_{-10^{\circ}}$, and $\lambda = {99^{\circ}}^{+10^{\circ}}_{-9^{\circ}}$ for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly $90^{\circ}$ from their host star's equator while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with $T_\mathrm{eff}=6250\pm120$K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with $T_\mathrm{eff}=6900\pm120$K and F4 with $T_\mathrm{eff}=6520\pm140$K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
D Bayliss - One of the best experts on this subject based on the ideXlab platform.
-
stellar obliquities and planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b and wasp 109b
The Astronomical Journal, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, D J Wright, D BaylissAbstract:We report measurements of the sky-projected spin-orbit angles for three transiting hot Jupiters, two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low-obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter-McLaughlin effect over the course of the transits from high-resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin-orbit angles are lambda = 7 degrees(+11)(-12 degrees)degrees, lambda = 79 degrees(+19)(-10 degrees)degrees, and lambda = 99 degrees(+10)(-9 degrees)degrees for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly 90 degrees from their host star's equator, while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with T-eff = 6250 +/- 120 K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with T-eff = 6900 +/- 120 K and F4 with T-eff = 6520 +/- 140 K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
-
stellar obliquities planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b wasp 109b
arXiv: Earth and Planetary Astrophysics, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, David Wright, D BaylissAbstract:We report measurements of the sky-projected spin--orbit angles for three transiting hot Jupiters: two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter--McLaughlin effect over the course of the transits from high resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin--orbit angles are $\lambda = {-7^{\circ}}^{+11^{\circ}}_{-12^{\circ}}$, $\lambda = {79^{\circ}}^{+19^{\circ}}_{-10^{\circ}}$, and $\lambda = {99^{\circ}}^{+10^{\circ}}_{-9^{\circ}}$ for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly $90^{\circ}$ from their host star's equator while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with $T_\mathrm{eff}=6250\pm120$K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with $T_\mathrm{eff}=6900\pm120$K and F4 with $T_\mathrm{eff}=6520\pm140$K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
Marshall C Johnson - One of the best experts on this subject based on the ideXlab platform.
-
stellar obliquities and planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b and wasp 109b
The Astronomical Journal, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, D J Wright, D BaylissAbstract:We report measurements of the sky-projected spin-orbit angles for three transiting hot Jupiters, two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low-obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter-McLaughlin effect over the course of the transits from high-resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin-orbit angles are lambda = 7 degrees(+11)(-12 degrees)degrees, lambda = 79 degrees(+19)(-10 degrees)degrees, and lambda = 99 degrees(+10)(-9 degrees)degrees for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly 90 degrees from their host star's equator, while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with T-eff = 6250 +/- 120 K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with T-eff = 6900 +/- 120 K and F4 with T-eff = 6520 +/- 140 K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
-
stellar obliquities planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b wasp 109b
arXiv: Earth and Planetary Astrophysics, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, David Wright, D BaylissAbstract:We report measurements of the sky-projected spin--orbit angles for three transiting hot Jupiters: two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter--McLaughlin effect over the course of the transits from high resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin--orbit angles are $\lambda = {-7^{\circ}}^{+11^{\circ}}_{-12^{\circ}}$, $\lambda = {79^{\circ}}^{+19^{\circ}}_{-10^{\circ}}$, and $\lambda = {99^{\circ}}^{+10^{\circ}}_{-9^{\circ}}$ for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly $90^{\circ}$ from their host star's equator while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with $T_\mathrm{eff}=6250\pm120$K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with $T_\mathrm{eff}=6900\pm120$K and F4 with $T_\mathrm{eff}=6520\pm140$K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
Songhu Wang - One of the best experts on this subject based on the ideXlab platform.
-
stellar obliquities and planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b and wasp 109b
The Astronomical Journal, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, D J Wright, D BaylissAbstract:We report measurements of the sky-projected spin-orbit angles for three transiting hot Jupiters, two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low-obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter-McLaughlin effect over the course of the transits from high-resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin-orbit angles are lambda = 7 degrees(+11)(-12 degrees)degrees, lambda = 79 degrees(+19)(-10 degrees)degrees, and lambda = 99 degrees(+10)(-9 degrees)degrees for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly 90 degrees from their host star's equator, while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with T-eff = 6250 +/- 120 K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with T-eff = 6900 +/- 120 K and F4 with T-eff = 6520 +/- 140 K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
-
stellar obliquities planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b wasp 109b
arXiv: Earth and Planetary Astrophysics, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, David Wright, D BaylissAbstract:We report measurements of the sky-projected spin--orbit angles for three transiting hot Jupiters: two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter--McLaughlin effect over the course of the transits from high resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin--orbit angles are $\lambda = {-7^{\circ}}^{+11^{\circ}}_{-12^{\circ}}$, $\lambda = {79^{\circ}}^{+19^{\circ}}_{-10^{\circ}}$, and $\lambda = {99^{\circ}}^{+10^{\circ}}_{-9^{\circ}}$ for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly $90^{\circ}$ from their host star's equator while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with $T_\mathrm{eff}=6250\pm120$K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with $T_\mathrm{eff}=6900\pm120$K and F4 with $T_\mathrm{eff}=6520\pm140$K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
C G Tinney - One of the best experts on this subject based on the ideXlab platform.
-
stellar obliquities and planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b and wasp 109b
The Astronomical Journal, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, D J Wright, D BaylissAbstract:We report measurements of the sky-projected spin-orbit angles for three transiting hot Jupiters, two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low-obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter-McLaughlin effect over the course of the transits from high-resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin-orbit angles are lambda = 7 degrees(+11)(-12 degrees)degrees, lambda = 79 degrees(+19)(-10 degrees)degrees, and lambda = 99 degrees(+10)(-9 degrees)degrees for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly 90 degrees from their host star's equator, while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with T-eff = 6250 +/- 120 K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with T-eff = 6900 +/- 120 K and F4 with T-eff = 6520 +/- 140 K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
-
stellar obliquities planetary alignments sopa i spin orbit measurements of three transiting hot jupiters wasp 72b wasp 100b wasp 109b
arXiv: Earth and Planetary Astrophysics, 2018Co-Authors: Brett C Addison, Songhu Wang, Marshall C Johnson, C G Tinney, David Wright, D BaylissAbstract:We report measurements of the sky-projected spin--orbit angles for three transiting hot Jupiters: two of which are in nearly polar orbits, WASP-100b and WASP-109b, and a third in a low obliquity orbit, WASP-72b. We obtained these measurements by observing the Rossiter--McLaughlin effect over the course of the transits from high resolution spectroscopic observations made with the CYCLOPS2 optical fiber Bundle System feeding the UCLES spectrograph on the Anglo-Australian Telescope. The resulting sky-projected spin--orbit angles are $\lambda = {-7^{\circ}}^{+11^{\circ}}_{-12^{\circ}}$, $\lambda = {79^{\circ}}^{+19^{\circ}}_{-10^{\circ}}$, and $\lambda = {99^{\circ}}^{+10^{\circ}}_{-9^{\circ}}$ for WASP-72b, WASP-100b, and WASP-109b, respectively. These results suggests that WASP-100b and WASP-109b are on highly inclined orbits tilted nearly $90^{\circ}$ from their host star's equator while the orbit of WASP-72b appears to be well-aligned. WASP-72b is a typical hot Jupiter orbiting a mid-late F star (F7 with $T_\mathrm{eff}=6250\pm120$K). WASP-100b and WASP-109b are highly irradiated bloated hot Jupiters orbiting hot early-mid F stars (F2 with $T_\mathrm{eff}=6900\pm120$K and F4 with $T_\mathrm{eff}=6520\pm140$K), making them consistent with the trends observed for the majority of stars hosting planets on high-obliquity orbits.
