alx-ai/arxiv_papers · Datasets at Hugging Face

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Richardson, L. J., Deming, D., & Seager, S. 2003, ApJ, 597, 58 1
Rieke, G. H. et al. 2004, ApJS, 154, 25
Rodler, F., K¨ urster, M., & Henning, T. 2008, A&A, 485, 859
—. 2010, A&A, 514, A23+Rogers, J. C., Apai, D., L´ opez-Morales, M., Sing, D. K., &
Burrows, A. 2009, ApJ, 707, 1707
Rowe, J. F. et al. 2008, ApJ, 689, 1345
Seager, S., & Deming, D. 2009, ApJ, 703, 1884
Seager, S., Whitney, B. A., & Sasselov, D. D. 2000, ApJ, 540, 5 04
Seager, S., & Mall´ en-Ornelas, G. 2003, ApJ, 585, 1038
Sing, D. K., & L´ opez-Morales, M. 2009, A&A, 493, L31
Snellen, I. A. G., & Covino, E. 2007, MNRAS, 375, 307
Snellen, I. A. G., de Mooij, E. J. W., & Albrecht, S. 2009, Natu re,
459, 543
Snellen, I. A. G., de Mooij, E. J. W., & Burrows, A. 2010, A&A,
513, A76+
Spiegel, D. S., & Burrows, A. 2010, ApJ, 722, 871
Stevenson, K. B. et al. 2010, Nature, 464, 1161
Sudarsky, D., Burrows, A., & Hubeny, I. 2003, ApJ, 588, 1121
Sudarsky, D., Burrows, A., & Pinto, P. 2000, ApJ, 538, 885
Todorov, K., Deming, D., Harrington, J., Stevenson, K. B.,
Bowman, W. C., Nymeyer, S., Fortney, J. J., & Bakos, G. A.
2010, ApJ, 708, 498
Werner, M. W. et al. 2004, ApJS, 154, 1
Wheatley, P. J., et al. 2010, arXiv:1004.0836
Zahnle, K., Marley, M. S., Freedman, R. S., Lodders, K., &
Fortney, J. J. 2009, ApJ, 701, L20Albedo and Heat Recirculation on Hot Exoplanets 11
TABLE 1
Secondary Eclipses & Phase Variations of Exoplanets
Planet Tε=0[K]aλ[µm]bEclipse DepthcTbright[K] Phase AmplitudecDerived Quantitiesd
CoRoT-1b12424(84) 0.60(0.42) 1 .6(6)×10−42726(141) Td=2674(144) K
0.71(0.25) 1 .26(33)×10−42409(75) 1 .0(3)×10−4Aλ<0.1
2.10(0.02) 2 .8(5)×10−32741(125) Td(A= 0)=2515(84) K
2.15(0.32) 3 .36(42)×10−32490(157)
3.6(0.75) 4 .15(42)×10−32098(116)
4.5(1.0) 4 .82(42)×10−32084(106)
CoRoT-2b21964(42) 0.60(0.42) 6(2) ×10−52315(85) Td=1864(233) K
0.71(0.25) 1 .02(20)×10−42215(49) Aλ= 0.16(7)
1.65(0.25) <1.7×10−3(3σ) Td(A= 0)=2010(144) K
2.15(0.32) 1 .6(9)×10−31914(292)
3.6(0.75) 3 .55(20)×10−31798(40)
4.5(1.0)e4.75(19)×10−31791(33)
4.5(1.0) 5 .10(42)×10−3
8.0(2.9) 4 .1(1.1)×10−3
8.0(2.9)e4.09(80)×10−31318(143)
Gl 436b3934(41) 3.6(0.75) 4 .1(3)×10−41145(23) Td=1082(38) K
4.5(1.0) <1.0×10−4(3σ)
5.8(1.4) 3 .3(1.4)×10−4797(106)
8.0(2.9)e4.52(27)×10−4737(17)
8.0(2.9) 5 .7(8)×10−4
8.0(2.9) 5 .4(7)×10−4
16(5) 1 .40(27)×10−3963(126)
24(9) 1 .75(41)×10−31016(182)
HAT-P-1b41666(38) 3.6(0.75) 8 .0(8)×10−41420(47) Td=1439(59) K
4.5(1.0) 1 .35(22)×10−31507(100)
5.8(1.4) 2 .03(31)×10−31626(128)
8.0(2.9) 2 .38(40)×10−31564(151)
HAT-P-7b52943(95) 0.65(0.4) 1 .30(11)×10−43037(35) 1 .22(16)×10−4Td=2086(156) K
3.6(0.75) 9 .8(1.7)×10−42063(152) Aλ= 0.58(5)
4.5(1.0) 1 .59(22)×10−32378(179) Td(A= 0)=2830(86) K
5.8(1.4) 2 .45(31)×10−32851(235)
8.0(2.9) 2 .25(52)×10−32512(403)
HD 80606b61799(50) 8.0(2.9) 1 .36(18)×10−31137(73) Td=1137(113) K
HD 149026b71871(17) 8.0(2.9)e3.7(0.8)×10−4976(276) 2 .3(7)×10−4Td=1571(231) K
8.0(2.9) 8 .4(1.1)×10−4Tn=976(286) K
HD 189733b81537(16) 2.15(32) <4.0×10−4(1σ) Td=1605(52) K
3.6(0.75) 2 .56(14)×10−31639(34) Tn=1107(132) K
4.5(1.0) 2 .14(20)×10−31318(45)
5.8(1.4) 3 .10(34)×10−31368(69)
8.0(2.9) 3 .381(55)×10−3
8.0(2.9) 3 .91(22)×10−31.2(2)×10−3
8.0(2.9)e3.440(36)×10−31259(7) 1 .2(4)×10−3
16(5) 5 .51(30)×10−31338(52)
24(9) 5 .98(38)×10−3
24(9)e5.36(27)×10−31202(46) 1 .3(3)×10−3
HD 209458b91754(15) 0.5(0.3) 7(9) ×10−62368(156) Td=1486(53) K
2.15(0.32) <3×10−4(1σ) Aλ= 0.09(7)
3.6(0.75) 9 .4(9)×10−41446(45) Td(A= 0)=2031(128) K
4.5(1.0) 2 .13(15)×10−31757(57) Tn=1476(304) K
5.8(1.4) 3 .01(43)×10−31890(149)
8.0(2.9) 2 .40(26)×10−31480(94) <1.5×10−3(2σ)
24(9) 2 .60(44)×10−31131(143)
OGLE-TR-56b102874(84) 0.90(0.15) 3 .63(91)×10−42696(116) Td=2696(236) K
OGLE-TR-113b111716(33) 2.15(0.32) 1 .7(5)×10−31918(164) Td=1918(219) K
TrES-1b121464(16) 3.6(0.75) <1.5×10−3(1σ) Td=998(67) K
4.5(1.0) 6 .6(1.3)×10−4972(56)
8.0(2.9) 2 .25(36)×10−31152(94)
TrES-2b131917(21) 0.65(0.4) 1 .14(78)×10−52020(132) Td=1623(76) K
2.15(0.32) 6 .2(1.2)×10−41655(80) Aλ= 0.06(3)
3.6(0.75) 1 .27(21)×10−31490(84) Td(A= 0) = 1751(80) K
4.5(1.0) 2 .30(24)×10−31652(74)
5.8(1.4) 1 .99(54)×10−31373(177)
8.0(2.9) 3 .59(60)×10−31659(163)
TrES-3b142093(32) 0.7(0.3) <6.2×10−4(1σ) Td=1761(66) K
1.25(0.16) <5.1×10−4(3σ)
2.15(0.32) 2 .41(43)×10−3
2.15(0.32)e1.33(17)×10−31770(58)
3.6(0.75) 3 .46(35)×10−31818(73)12 Cowan & Agol
TABLE 1
Secondary Eclipses & Phase Variations of Exoplanets
4.5(1.0) 3 .72(54)×10−31649(107)

Richardson, L. J., Deming, D., & Seager, S. 2003, ApJ, 597, 58 1

Rieke, G. H. et al. 2004, ApJS, 154, 25

Rodler, F., K¨ urster, M., & Henning, T. 2008, A&A, 485, 859

—. 2010, A&A, 514, A23+Rogers, J. C., Apai, D., L´ opez-Morales, M., Sing, D. K., &

Burrows, A. 2009, ApJ, 707, 1707

Rowe, J. F. et al. 2008, ApJ, 689, 1345

Seager, S., & Deming, D. 2009, ApJ, 703, 1884

Seager, S., Whitney, B. A., & Sasselov, D. D. 2000, ApJ, 540, 5 04

Seager, S., & Mall´ en-Ornelas, G. 2003, ApJ, 585, 1038

Sing, D. K., & L´ opez-Morales, M. 2009, A&A, 493, L31

Snellen, I. A. G., & Covino, E. 2007, MNRAS, 375, 307

Snellen, I. A. G., de Mooij, E. J. W., & Albrecht, S. 2009, Natu re,

459, 543

Snellen, I. A. G., de Mooij, E. J. W., & Burrows, A. 2010, A&A,

513, A76+

Spiegel, D. S., & Burrows, A. 2010, ApJ, 722, 871

Stevenson, K. B. et al. 2010, Nature, 464, 1161

Sudarsky, D., Burrows, A., & Hubeny, I. 2003, ApJ, 588, 1121

Sudarsky, D., Burrows, A., & Pinto, P. 2000, ApJ, 538, 885

Todorov, K., Deming, D., Harrington, J., Stevenson, K. B.,

Bowman, W. C., Nymeyer, S., Fortney, J. J., & Bakos, G. A.

2010, ApJ, 708, 498

Werner, M. W. et al. 2004, ApJS, 154, 1

Wheatley, P. J., et al. 2010, arXiv:1004.0836

Zahnle, K., Marley, M. S., Freedman, R. S., Lodders, K., &

Fortney, J. J. 2009, ApJ, 701, L20Albedo and Heat Recirculation on Hot Exoplanets 11

TABLE 1

Secondary Eclipses & Phase Variations of Exoplanets

Planet Tε=0[K]aλ[µm]bEclipse DepthcTbright[K] Phase AmplitudecDerived Quantitiesd

CoRoT-1b12424(84) 0.60(0.42) 1 .6(6)×10−42726(141) Td=2674(144) K

0.71(0.25) 1 .26(33)×10−42409(75) 1 .0(3)×10−4Aλ<0.1

2.10(0.02) 2 .8(5)×10−32741(125) Td(A= 0)=2515(84) K

2.15(0.32) 3 .36(42)×10−32490(157)

3.6(0.75) 4 .15(42)×10−32098(116)

4.5(1.0) 4 .82(42)×10−32084(106)

CoRoT-2b21964(42) 0.60(0.42) 6(2) ×10−52315(85) Td=1864(233) K

0.71(0.25) 1 .02(20)×10−42215(49) Aλ= 0.16(7)

1.65(0.25) <1.7×10−3(3σ) Td(A= 0)=2010(144) K

2.15(0.32) 1 .6(9)×10−31914(292)

3.6(0.75) 3 .55(20)×10−31798(40)

4.5(1.0)e4.75(19)×10−31791(33)

4.5(1.0) 5 .10(42)×10−3

8.0(2.9) 4 .1(1.1)×10−3

8.0(2.9)e4.09(80)×10−31318(143)

Gl 436b3934(41) 3.6(0.75) 4 .1(3)×10−41145(23) Td=1082(38) K

4.5(1.0) <1.0×10−4(3σ)

5.8(1.4) 3 .3(1.4)×10−4797(106)

8.0(2.9)e4.52(27)×10−4737(17)

8.0(2.9) 5 .7(8)×10−4

8.0(2.9) 5 .4(7)×10−4

16(5) 1 .40(27)×10−3963(126)

24(9) 1 .75(41)×10−31016(182)

HAT-P-1b41666(38) 3.6(0.75) 8 .0(8)×10−41420(47) Td=1439(59) K

4.5(1.0) 1 .35(22)×10−31507(100)

5.8(1.4) 2 .03(31)×10−31626(128)

8.0(2.9) 2 .38(40)×10−31564(151)

HAT-P-7b52943(95) 0.65(0.4) 1 .30(11)×10−43037(35) 1 .22(16)×10−4Td=2086(156) K

3.6(0.75) 9 .8(1.7)×10−42063(152) Aλ= 0.58(5)

4.5(1.0) 1 .59(22)×10−32378(179) Td(A= 0)=2830(86) K

5.8(1.4) 2 .45(31)×10−32851(235)

8.0(2.9) 2 .25(52)×10−32512(403)

HD 80606b61799(50) 8.0(2.9) 1 .36(18)×10−31137(73) Td=1137(113) K

HD 149026b71871(17) 8.0(2.9)e3.7(0.8)×10−4976(276) 2 .3(7)×10−4Td=1571(231) K

8.0(2.9) 8 .4(1.1)×10−4Tn=976(286) K

HD 189733b81537(16) 2.15(32) <4.0×10−4(1σ) Td=1605(52) K

3.6(0.75) 2 .56(14)×10−31639(34) Tn=1107(132) K

4.5(1.0) 2 .14(20)×10−31318(45)

5.8(1.4) 3 .10(34)×10−31368(69)

8.0(2.9) 3 .381(55)×10−3

8.0(2.9) 3 .91(22)×10−31.2(2)×10−3

8.0(2.9)e3.440(36)×10−31259(7) 1 .2(4)×10−3

16(5) 5 .51(30)×10−31338(52)

24(9) 5 .98(38)×10−3

24(9)e5.36(27)×10−31202(46) 1 .3(3)×10−3

HD 209458b91754(15) 0.5(0.3) 7(9) ×10−62368(156) Td=1486(53) K

2.15(0.32) <3×10−4(1σ) Aλ= 0.09(7)

3.6(0.75) 9 .4(9)×10−41446(45) Td(A= 0)=2031(128) K

4.5(1.0) 2 .13(15)×10−31757(57) Tn=1476(304) K

5.8(1.4) 3 .01(43)×10−31890(149)

8.0(2.9) 2 .40(26)×10−31480(94) <1.5×10−3(2σ)

24(9) 2 .60(44)×10−31131(143)

OGLE-TR-56b102874(84) 0.90(0.15) 3 .63(91)×10−42696(116) Td=2696(236) K

OGLE-TR-113b111716(33) 2.15(0.32) 1 .7(5)×10−31918(164) Td=1918(219) K

TrES-1b121464(16) 3.6(0.75) <1.5×10−3(1σ) Td=998(67) K

4.5(1.0) 6 .6(1.3)×10−4972(56)

8.0(2.9) 2 .25(36)×10−31152(94)

TrES-2b131917(21) 0.65(0.4) 1 .14(78)×10−52020(132) Td=1623(76) K

2.15(0.32) 6 .2(1.2)×10−41655(80) Aλ= 0.06(3)

3.6(0.75) 1 .27(21)×10−31490(84) Td(A= 0) = 1751(80) K

4.5(1.0) 2 .30(24)×10−31652(74)

5.8(1.4) 1 .99(54)×10−31373(177)

8.0(2.9) 3 .59(60)×10−31659(163)

TrES-3b142093(32) 0.7(0.3) <6.2×10−4(1σ) Td=1761(66) K

1.25(0.16) <5.1×10−4(3σ)

2.15(0.32) 2 .41(43)×10−3

2.15(0.32)e1.33(17)×10−31770(58)

3.6(0.75) 3 .46(35)×10−31818(73)12 Cowan & Agol

TABLE 1

Secondary Eclipses & Phase Variations of Exoplanets

4.5(1.0) 3 .72(54)×10−31649(107)