diff --git a/Figure/KT_Eri.pdf b/Figure/KT_Eri.pdf new file mode 100644 index 0000000..e4ff253 Binary files /dev/null and b/Figure/KT_Eri.pdf differ diff --git a/Figure/cost.pdf b/Figure/cost.pdf new file mode 100644 index 0000000..1f84cc3 Binary files /dev/null and b/Figure/cost.pdf differ diff --git a/Makefile b/Makefile index 8afcd93..0115089 100644 --- a/Makefile +++ b/Makefile @@ -1,3 +1,8 @@ +thesis: + rm -rf _build/auto + GHC_PACKAGE_PATH=${PUBSENGINE_ROOT}/.stack-work/install/x86_64-linux-tinfo6/3d751d21e6b97977106d82e2ec3961638329963dd4d98bc4115204782f5d4168/8.10.7/pkgdb:${HOME}/.stack/snapshots/x86_64-linux-tinfo6/3d751d21e6b97977106d82e2ec3961638329963dd4d98bc4115204782f5d4168/8.10.7/pkgdb:${GHC_PACKAGE_PATH} pubsEngine manuscript thesis +clean: + rm -rf _build article: rm -rf _build/auto GHC_PACKAGE_PATH=${PUBSENGINE_ROOT}/.stack-work/install/x86_64-linux-tinfo6/3d751d21e6b97977106d82e2ec3961638329963dd4d98bc4115204782f5d4168/8.10.7/pkgdb:${HOME}/.stack/snapshots/x86_64-linux-tinfo6/3d751d21e6b97977106d82e2ec3961638329963dd4d98bc4115204782f5d4168/8.10.7/pkgdb:${GHC_PACKAGE_PATH} pubsEngine manuscript article diff --git a/include/appendix3.md b/include/appendix3.md index ce40a49..0c46645 100644 --- a/include/appendix3.md +++ b/include/appendix3.md @@ -16,89 +16,6 @@ command can be used to help center extremely wide, landscape tables. The command `\movetabledown=1in` will move any rotated table down 1 inch. -\begin{longrotatetable} -\begin{deluxetable*}{lllrrrrrrll} -\tablecaption{Observable Characteristics of -Galactic/Magellanic Cloud novae with X-ray observations\label{chartable}} -\tablewidth{700pt} -\tabletypesize{\scriptsize} -\tablehead{ -\colhead{Name} & \colhead{V$_{max}$} & -\colhead{Date} & \colhead{t$_2$} & -\colhead{FWHM} & \colhead{E(B-V)} & -\colhead{N$_H$} & \colhead{Period} & -\colhead{D} & \colhead{Dust?} & \colhead{RN?} \\ -\colhead{} & \colhead{(mag)} & \colhead{(JD)} & \colhead{(d)} & -\colhead{(km s$^{-1}$)} & \colhead{(mag)} & \colhead{(cm$^{-2}$)} & -\colhead{(d)} & \colhead{(kpc)} & \colhead{} & \colhead{} -} -\startdata -CI Aql & 8.83 (1) & 2451665.5 (1) & 32 (2) & 2300 (3) & 0.8$\pm0.2$ (4) & 1.2e+22 & 0.62 (4) & 6.25$\pm5$ (4) & N & Y \\ -{\bf CSS081007} & \nodata & 2454596.5 & \nodata & \nodata & 0.146 & 1.1e+21 & 1.77 (5) & 4.45$\pm1.95$ (6) & \nodata & \nodata \\ -GQ Mus & 7.2 (7) & 2445352.5 (7) & 18 (7) & 1000 (8) & 0.45 (9) & 3.8e+21 & 0.059375 (10) & 4.8$\pm1$ (9) & N (7) & \nodata \\ -IM Nor & 7.84 (11) & 2452289 (2) & 50 (2) & 1150 (12) & 0.8$\pm0.2$ (4) & 8e+21 & 0.102 (13) & 4.25$\pm3.4$ (4) & N & Y \\ -{\bf KT Eri} & 5.42 (14) & 2455150.17 (14) & 6.6 (14) & 3000 (15) & 0.08 (15) & 5.5e+20 & \nodata & 6.5 (15) & N & M \\ -{\bf LMC 1995} & 10.7 (16) & 2449778.5 (16) & 15$\pm2$ (17) & \nodata & 0.15 (203) & 7.8e+20 & \nodata & 50 & \nodata & \nodata \\ -LMC 2000 & 11.45 (18) & 2451737.5 (18) & 9$\pm2$ (19) & 1700 (20) & 0.15 (203) & 7.8e+20 & \nodata & 50 & \nodata & \nodata \\ -{\bf LMC 2005} & 11.5 (21) & 2453700.5 (21) & 63 (22) & 900 (23) & 0.15 (203) & 1e+21 & \nodata & 50 & M (24) & \nodata \\ -{\bf LMC 2009a} & 10.6 (25) & 2454867.5 (25) & 4$\pm1$ & 3900 (25) & 0.15 (203) & 5.7e+20 & 1.19 (26) & 50 & N & Y \\ -{\bf SMC 2005} & 10.4 (27) & 2453588.5 (27) & \nodata & 3200 (28) & \nodata & 5e+20 & \nodata & 61 & \nodata & \nodata \\ -{\bf QY Mus} & 8.1 (29) & 2454739.90 (29) & 60: & \nodata & 0.71 (30) & 4.2e+21 & \nodata & \nodata & M & \nodata \\ -{\bf RS Oph} & 4.5 (31) & 2453779.44 (14) & 7.9 (14) & 3930 (31) & 0.73 (32) & 2.25e+21 & 456 (33) & 1.6$\pm0.3$ (33) & N (34) & Y \\ -{\bf U Sco} & 8.05 (35) & 2455224.94 (35) & 1.2 (36) & 7600 (37) & 0.2$\pm0.1$ (4) & 1.2e+21 & 1.23056 (36) & 12$\pm2$ (4) & N & Y \\ -{\bf V1047 Cen} & 8.5 (38) & 2453614.5 (39) & 6 (40) & 840 (38) & \nodata & 1.4e+22 & \nodata & \nodata & \nodata & \nodata \\ -{\bf V1065 Cen} & 8.2 (41) & 2454123.5 (41) & 11 (42) & 2700 (43) & 0.5$\pm0.1$ (42) & 3.75e+21 & \nodata & 9.05$\pm2.8$ (42) & Y (42) & \nodata \\ -V1187 Sco & 7.4 (44) & 2453220.5 (44) & 7: (45) & 3000 (44) & 1.56 (44) & 8.0e+21 & \nodata & 4.9$\pm0.5$ (44) & N & \nodata \\ -{\bf V1188 Sco} & 8.7 (46) & 2453577.5 (46) & 7 (40) & 1730 (47) & \nodata & 5.0e+21 & \nodata & 7.5 (39) & \nodata & \nodata \\ -{\bf V1213 Cen} & 8.53 (48) & 2454959.5 (48) & 11$\pm2$ (49) & 2300 (50) & 2.07 (30) & 1.0e+22 & \nodata & \nodata & \nodata & \nodata \\ -{\bf V1280 Sco} & 3.79 (51) & 2454147.65 (14) & 21 (52) & 640 (53) & 0.36 (54) & 1.6e+21 & \nodata & 1.6$\pm0.4$ (54) & Y (54) & \nodata \\ -{\bf V1281 Sco} & 8.8 (55) & 2454152.21 (55) & 15:& 1800 (56) & 0.7 (57) & 3.2e+21 & \nodata & \nodata & N & \nodata \\ -{\bf V1309 Sco} & 7.1 (58) & 2454714.5 (58) & 23$\pm2$ (59) & 670 (60) & 1.2 (30) & 4.0e+21 & \nodata & \nodata & \nodata & \nodata \\ -{\bf V1494 Aql} & 3.8 (61) & 2451515.5 (61) & 6.6$\pm0.5$ (61) & 1200 (62) & 0.6 (63) & 3.6e+21 & 0.13467 (64) & 1.6$\pm0.1$ (63) & N & \nodata \\ -{\bf V1663 Aql} & 10.5 (65) & 2453531.5 (65) & 17 (66) & 1900 (67) & 2: (68) & 1.6e+22 & \nodata & 8.9$\pm3.6$ (69) & N & \nodata \\ -V1974 Cyg & 4.3 (70) & 2448654.5 (70) & 17 (71) & 2000 (19) & 0.36$\pm0.04$ (71) & 2.7e+21 & 0.081263 (70) & 1.8$\pm0.1$ (72) & N & \nodata \\ -{\bf V2361 Cyg} & 9.3 (73) & 2453412.5 (73) & 6 (40) & 3200 (74) & 1.2: (75) & 7.0e+21 & \nodata & \nodata & Y (40) & \nodata \\ -{\bf V2362 Cyg} & 7.8 (76) & 2453831.5 (76) & 9 (77) & 1850 (78) & 0.575$\pm0.015$ (79) & 4.4e+21 & 0.06577 (80) & 7.75$\pm3$ (77) & Y (81) & \nodata \\ -{\bf V2467 Cyg} & 6.7 (82) & 2454176.27 (82) & 7 (83) & 950 (82) & 1.5 (84) & 1.4e+22 & 0.159 (85) & 3.1$\pm0.5$ (86) & M (87) & \nodata \\ -{\bf V2468 Cyg} & 7.4 (88) & 2454534.2 (88) & 10: & 1000 (88) & 0.77 (89) & 1.0e+22 & 0.242 (90) & \nodata & N & \nodata \\ -{\bf V2491 Cyg} & 7.54 (91) & 2454567.86 (91) & 4.6 (92) & 4860 (93) & 0.43 (94) & 4.7e+21 & 0.09580: (95) & 10.5 (96) & N & M \\ -V2487 Oph & 9.5 (97) & 2450979.5 (97) & 6.3 (98) & 10000 (98) & 0.38$\pm0.08$ (98) & 2.0e+21 & \nodata & 27.5$\pm3$ (99) & N (100) & Y (101) \\ -{\bf V2540 Oph} & 8.5 (102) & 2452295.5 (102) & \nodata & \nodata & \nodata & 2.3e+21 & 0.284781 (103) & 5.2$\pm0.8$ (103) & N & \nodata \\ -V2575 Oph & 11.1 (104) & 2453778.8 (104) & 20: & 560 (104) & 1.4 (105) & 3.3e+21 & \nodata & \nodata & N (105) & \nodata \\ -{\bf V2576 Oph} & 9.2 (106) & 2453832.5 (106) & 8: & 1470 (106) & 0.25 (107) & 2.6e+21 & \nodata & \nodata & N & \nodata \\ -{\bf V2615 Oph} & 8.52 (108) & 2454187.5 (108) & 26.5 (108) & 800 (109) & 0.9 (108) & 3.1e+21 & \nodata & 3.7$\pm0.2$ (108) & Y (110) & \nodata \\ -{\bf V2670 Oph} & 9.9 (111) & 2454613.11 (111) & 15: & 600 (112) & 1.3: (113) & 2.9e+21 & \nodata & \nodata & N (114) & \nodata \\ -{\bf V2671 Oph} & 11.1 (115) & 2454617.5 (115) & 8: & 1210 (116) & 2.0 (117) & 3.3e+21 & \nodata & \nodata & M (117) & \nodata \\ -{\bf V2672 Oph} & 10.0 (118) & 2455060.02 (118) & 2.3 (119) & 8000 (118) & 1.6$\pm0.1$ (119) & 4.0e+21 & \nodata & 19$\pm2$ (119) & \nodata & M \\ -V351 Pup & 6.5 (120) & 2448617.5 (120) & 16 (121) & \nodata & 0.72$\pm0.1$ (122) & 6.2e+21 & 0.1182 (123) & 2.7$\pm0.7$ (122) & N & \nodata \\ -{\bf V382 Nor} & 8.9 (124) & 2453447.5 (124) & 12 (40) & 1850 (23) & \nodata & 1.7e+22 & \nodata & \nodata & \nodata & \nodata \\ -V382 Vel & 2.85 (125) & 2451320.5 (125) & 4.5 (126) & 2400 (126) & 0.05: (126) & 3.4e+21 & 0.146126 (127) & 1.68$\pm0.3$ (126) & N & \nodata \\ -{\bf V407 Cyg} & 6.8 (128) & 2455266.314 (128) & 5.9 (129) & 2760 (129) & 0.5$\pm0.05$ (130) & 8.8e+21 & 15595 (131) & 2.7 (131) & \nodata & Y \\ -{\bf V458 Vul} & 8.24 (132) & 2454322.39 (132) & 7 (133) & 1750 (134) & 0.6 (135) & 3.6e+21 & 0.06812255 (136) & 8.5$\pm1.8$ (133) & N (135) & \nodata \\ -{\bf V459 Vul} & 7.57 (137) & 2454461.5 (137) & 18 (138) & 910 (139) & 1.0 (140) & 5.5e+21 & \nodata & 3.65$\pm1.35$ (138) & Y (140) & \nodata \\ -V4633 Sgr & 7.8 (141) & 2450895.5 (141) & 19$\pm3$ (142) & 1700 (143) & 0.21 (142) & 1.4e+21 & 0.125576 (144) & 8.9$\pm2.5$ (142) & N & \nodata \\ -{\bf V4643 Sgr} & 8.07 (145) & 2451965.867 (145) & 4.8 (146) & 4700 (147) & 1.67 (148) & 1.4e+22 & \nodata & 3 (148) & N & \nodata \\ -{\bf V4743 Sgr} & 5.0 (149) & 2452537.5 (149) & 9 (150) & 2400 (149) & 0.25 (151) & 1.2e+21 & 0.281 (152) & 3.9$\pm0.3$ (151) & N & \nodata \\ -{\bf V4745 Sgr} & 7.41 (153) & 2452747.5 (153) & 8.6 (154) & 1600 (155) & 0.1 (154) & 9.0e+20 & 0.20782 (156) & 14$\pm5$ (154) & \nodata & \nodata \\ -{\bf V476 Sct} & 10.3 (157) & 2453643.5 (157) & 15 (158) & \nodata & 1.9 (158) & 1.2e+22 & \nodata & 4$\pm1$ (158) & M (159) & \nodata \\ -{\bf V477 Sct} & 9.8 (160) & 2453655.5 (160) & 3 (160) & 2900 (161) & 1.2: (162) & 4e+21 & \nodata & \nodata & M (163) & \nodata \\ -{\bf V5114 Sgr} & 8.38 (164) & 2453081.5 (164) & 11 (165) & 2000 (23) & \nodata & 1.5e+21 & \nodata & 7.7$\pm0.7$ (165) & N (166) & \nodata \\ -{\bf V5115 Sgr} & 7.7 (167) & 2453459.5 (167) & 7 (40) & 1300 (168) & 0.53 (169) & 2.3e+21 & \nodata & \nodata & N (169) & \nodata \\ -{\bf V5116 Sgr} & 8.15 (170) & 2453556.91 (170) & 6.5 (171) & 970 (172) & 0.25 (173) & 1.5e+21 & 0.1238 (171) & 11$\pm3$ (173) & N (174) & \nodata \\ -{\bf V5558 Sgr} & 6.53 (175) & 2454291.5 (175) & 125 (176) & 1000 (177) & 0.80 (178) & 1.6e+22 & \nodata & 1.3$\pm0.3$ (176) & N (179) & \nodata \\ -{\bf V5579 Sgr} & 5.56 (180) & 2454579.62 (180) & 7: & 1500 (23) & 1.2 (181) & 3.3e+21 & \nodata & \nodata & Y (181) & \nodata \\ -{\bf V5583 Sgr} & 7.43 (182) & 2455051.07 (182) & 5: & 2300 (182) & 0.39 (30) & 2.0e+21 & \nodata & 10.5 & \nodata & \nodata \\ -{\bf V574 Pup} & 6.93 (183) & 2453332.22 (183) & 13 (184) & 2800 (184) & 0.5$\pm0.1$ & 6.2e+21 & \nodata & 6.5$\pm1$ & M (185) & \nodata \\ -{\bf V597 Pup} & 7.0 (186) & 2454418.75 (186) & 3: & 1800 (187) & 0.3 (188) & 5.0e+21 & 0.11119 (189) & \nodata & N (188) & \nodata \\ -{\bf V598 Pup} & 3.46 (14) & 2454257.79 (14) & 9$\pm1$ (190) & \nodata & 0.16 (190) & 1.4e+21 & \nodata & 2.95$\pm0.8$ (190) & \nodata & \nodata \\ -{\bf V679 Car} & 7.55 (191) & 2454797.77 (191) & 20: & \nodata & \nodata & 1.3e+22 & \nodata & \nodata & \nodata & \nodata \\ -{\bf V723 Cas} & 7.1 (192) & 2450069.0 (192) & 263 (2) & 600 (193) & 0.5 (194) & 2.35e+21 & 0.69 (195) & 3.86$\pm0.23$ (196) & N & \nodata \\ -V838 Her & 5 (197) & 2448340.5 (197) & 2 (198) & \nodata & 0.5$\pm0.1$ (198) & 2.6e+21 & 0.2975 (199) & 3$\pm1$ (198) & Y (200) & \nodata \\ -{\bf XMMSL1 J06} & 12 (201) & 2453643.5 (202) & 8$\pm2$ (202) & \nodata & 0.15 (203) & 8.7e+20 & \nodata & 50 & \nodata & \nodata \\ -\enddata -\end{deluxetable*} -\end{longrotatetable} - A handy "cheat sheet" that provides the necessary \latex to produce 17 different types of tables is available at \url{http://journals.aas.org/authors/aastex/aasguide.html#table_cheat_sheet}. diff --git a/include/appendix4.md b/include/appendix4.md index 4b37647..a1016d2 100644 --- a/include/appendix4.md +++ b/include/appendix4.md @@ -8,54 +8,9 @@ incorporate into v6.31 to help authors follow the IAU resolution. The general commands take this form: -\vskip12pt -\begin{center} -\begin{tabular}{@{\vrule height 14pt depth 6pt width0pt}lll} -Command&Example&Results\\ -\verb+\nom{}+&\verb+\nom{Q}+&\nom{Q}\\ -\verb+\Eenom{}+&\verb+\Eenom{Q}+&\Eenom{Q}\\ -\verb+\Epnom{}+&\verb+\Epnom{Q}+&\Epnom{Q}\\ -\verb+\Jenom{}+&\verb+\Jenom{Q}+&\Jenom{Q}\\ -\verb+\Jpnom{}+&\verb+\Jpnom{Q}+&\Jpnom{Q}\\ -\end{tabular} -\end{center} -\vskip12pt - -which can be used for any units the author requires. Examples of -the most common uses would be: - -\vskip12pt -\begin{tabular}{@{\vrule height 14pt depth 6pt width 0pt}llllp{3in}} -1.&\verb+\nom{(GM)}+& \nom{(GM)} &=& nominal solar mass parameter\\ -2.&\verb+\nom{R}+&\nom{R} &=& nominal solar radius\\ -3.&\verb+\nom{S}+& \nom{S}&=& nominal total solar irradiance\\ -4.&\verb+\nom{L}+& \nom{L} &=&nominal solar luminosity\\ -\end{tabular} -\vskip12pt - AASTeX v6.31 also contains specific commands for other commonly used units. These are: -\vskip24pt -\begin{tabular}{@{\vrule height 14pt depth 6pt width 0pt}llllp{3in}} -1.&\verb+\nomSolarEffTemp+& \nomSolarEffTemp&=& nominal solar effective temperature\\ -2.&\verb+\nomTerrEqRadius+&\nomTerrEqRadius &=& nominal terrestrial -equatorial radius\\ -&\verb+\nomTerrPolarRadius+ &\nomTerrPolarRadius &=& nominal -terrestrial polar radius\\ -&\verb+\nomTerrEqRadius+&\nomTerrEqRadius&& should be used if equatorial -vs.~polar radius is not explicitly specified.\\ -3.&\verb+\nomJovianEqRadius+&\nomJovianEqRadius&=& nominal one-bar equatorial radii of -Jupiter\\ -&\verb+\nomJovianPolarRadius+&\nomJovianPolarRadius &=& nominal polar radii of Jupiter\\ -&\verb+\nomJovianEqRadius+&\nomJovianEqRadius&& should be used if Jovian equatorial -vs.~polar radius is not explicitly specified.\\ -4.&\verb+\nomTerrMass+ &\nomTerrMass &=& nominal terrestrial mass -parameter\\ -&\verb+\nomJovianMass+ &\nomJovianMass &=& nominal Jovian mass parameter\\ -\end{tabular} -\vskip12pt - All of these commands work equally well in text and math mode. # Using Chinese, Japanese, and Korean characters diff --git a/manuscript.bib b/manuscript.bib index 8093e24..e8738f4 100644 --- a/manuscript.bib +++ b/manuscript.bib @@ -315,3 +315,43 @@ archivePrefix = {arXiv}, adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...793..127V}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } +@article{Reference1, + Abstract = {We have developed an enhanced Littrow configuration extended cavity diode laser (ECDL) that can be tuned without changing the direction of the output beam. The output of a conventional Littrow ECDL is reflected from a plane mirror fixed parallel to the tuning diffraction grating. Using a free-space Michelson wavemeter to measure the laser wavelength, we can tune the laser over a range greater than 10 nm without any alteration of alignment.}, + Author = {C. J. Hawthorn and K. P. Weber and R. E. Scholten}, + Journal = {Review of Scientific Instruments}, + Month = {12}, + Number = {12}, + Numpages = {3}, + Pages = {4477--4479}, + Title = {Littrow Configuration Tunable External Cavity Diode Laser with Fixed Direction Output Beam}, + Volume = {72}, + Url = {http://link.aip.org/link/?RSI/72/4477/1}, + Year = {2001}} + +@article{Reference3, + Abstract = {Operating a laser diode in an extended cavity which provides frequency-selective feedback is a very effective method of reducing the laser's linewidth and improving its tunability. We have developed an extremely simple laser of this type, built from inexpensive commercial components with only a few minor modifications. A 780~nm laser built to this design has an output power of 80~mW, a linewidth of 350~kHz, and it has been continuously locked to a Doppler-free rubidium transition for several days.}, + Author = {A. S. Arnold and J. S. Wilson and M. G. Boshier and J. Smith}, + Journal = {Review of Scientific Instruments}, + Month = {3}, + Number = {3}, + Numpages = {4}, + Pages = {1236--1239}, + Title = {A Simple Extended-Cavity Diode Laser}, + Volume = {69}, + Url = {http://link.aip.org/link/?RSI/69/1236/1}, + Year = {1998}} + +@article{Reference2, + Abstract = {We present a review of the use of diode lasers in atomic physics with an extensive list of references. We discuss the relevant characteristics of diode lasers and explain how to purchase and use them. We also review the various techniques that have been used to control and narrow the spectral outputs of diode lasers. Finally we present a number of examples illustrating the use of diode lasers in atomic physics experiments. Review of Scientific Instruments is copyrighted by The American Institute of Physics.}, + Author = {Carl E. Wieman and Leo Hollberg}, + Journal = {Review of Scientific Instruments}, + Keywords = {Diode Laser}, + Month = {1}, + Number = {1}, + Numpages = {20}, + Pages = {1--20}, + Title = {Using Diode Lasers for Atomic Physics}, + Volume = {62}, + Url = {http://link.aip.org/link/?RSI/62/1/1}, + Year = {1991}} + diff --git a/manuscript.md b/manuscript.md index a824563..cc14c1d 100644 --- a/manuscript.md +++ b/manuscript.md @@ -10,11 +10,31 @@ author: affiliation: "My City University" address: "Orenomachi, Orenoshi, Orenoken, Japan" email: "one@myuni.ac.jp" + url: "http://thegreatme.org" - number: 2 name: "Author Two" affiliation: "My Other City University" address: "Hokanomachi, Orenoshi, Orenoken, Japan" email: "two@myuni.ac.jp" +thesis: + degree: "Doctor of Philosophy" + univ: + name: "My City University" + url: "http://mycity.ac.jp" + department: + name: "My Great Department" + url: "http://mydepartment.ac.jp" + group: + name: "My Research Group" + url: "http://myresearch.group.ac.jp" + faculty: + name: "My Faculty Name" + url: "http://myfaculty.ac.jp" + supervisor: + name: "My Best Supervisor" + url: "http://thegreatsupervisor.ac.jp" + quotation: "include/quotation" + dedicatory: "include/dedicatory" collaborator: theme: "AAS Journal Data Editors" person: @@ -57,7 +77,7 @@ appendix: - include/appendix3 - include/appendix4 - include/appendix5 -graphicpaths: +graphicspath: - Figure abstract: | This example manuscript is intended to serve as a tutorial and template for @@ -106,6 +126,8 @@ header-includes: | \usepackage{hologo} \usepackage{xspace} \usepackage{chemfig} + \usepackage{amsmath} + \usepackage{graphicx} \newcommand\mC[1]{\multicolumn{1}{c}{#1}} \newcommand{\vdag}{(v)^\dagger} \newcommand\aastex{AAS\TeX} @@ -967,7 +989,6 @@ encapsulated postscript (EPS) or portable document format (PDF) files, \begin{enumerate} \item ORCID support for preprints, \item improved author, affiliation and collaboration mark up, - \item reintroduced the old AASTeX v5.2 `\received`, `\revised`, `\accepted`, and `\published` commands plus added the new `\submitjournal` command to document which AAS Journal the manuscript was submitted to, plus \item new typeset style options including ` modern`. \end{enumerate} \item{v6.2} @@ -976,7 +997,6 @@ encapsulated postscript (EPS) or portable document format (PDF) files, \item Titles no longer put in all caps, \item No page skip between the title page and article body, \item re-introduce RevTeX's widetext environment for long lines in two column style formats, and - \item upgrade to the `\doi` command. \end{enumerate} \item{v6.3} \begin{enumerate} @@ -1290,49 +1310,10 @@ the `\splitdeluxetable` command. The `\colnumbers` option is on to show how the automatic column numbering carries through the second table component, see Section \ref{subsubsec:autonumber}. -\begin{splitdeluxetable*}{lccccBcccccBcccc} -\tabletypesize{\scriptsize} -\tablewidth{0pt} -\tablenum{5} -\tablecaption{Measurements of Emission Lines: two breaks \label{tab:deluxesplit}} -\tablehead{ -\colhead{Model} & \colhead{Component}& \colhead{Shift} & \colhead{FWHM} & -\multicolumn{10}{c}{Flux} \\ -\colhead{} & \colhead{} & \colhead{($\rm -km~s^{-1}$)}& \colhead{($\rm km~s^{-1}$)} & \multicolumn{10}{c}{($\rm -10^{-17}~erg~s^{-1}~cm^{-2}$)} \\ -\cline{5-14} -\colhead{} & \colhead{} & -\colhead{} & \colhead{} & \colhead{Ly$\alpha$} & \colhead{N\,{\footnotesize -V}} & \colhead{Si\,{\footnotesize IV}} & \colhead{C\,{\footnotesize IV}} & -\colhead{Mg\,{\footnotesize II}} & \colhead{H$\gamma$} & \colhead{H$\beta$} -& \colhead{H$\alpha$} & \colhead{He\,{\footnotesize I}} & -\colhead{Pa$\gamma$} -} -\colnumbers -\startdata -{ }& BELs& -97.13 & 9117$\pm 38$& 1033$\pm 33$&$< 35$&$< 166$& 637$\pm 31$& 1951$\pm 26$& 991$\pm 30$& 3502$\pm 42$& 20285$\pm 80$& 2025$\pm 116$& 1289$\pm 107$\\ -{Model 1}& IELs& -4049.123 & 1974$\pm 22$& 2495$\pm 30$&$< 42$&$< 109$& 995$\pm 186$& 83$\pm 30$& 75$\pm 23$& 130$\pm 25$& 357$\pm 94$& 194$\pm 64$& 36$\pm 23$\\ -{ }& NELs& \nodata & 641$\pm 4$& 449$\pm 23$&$< 6$&$< 9$& -- & 275$\pm 18$& 150$\pm 11$& 313$\pm 12$& 958$\pm 43$& 318$\pm 34$& 151$\pm 17$\\ -\hline -{ }& BELs& -85 & 8991$\pm 41$& 988$\pm 29$&$< 24$&$< 173$& 623$\pm 28$& 1945$\pm 29$& 989$\pm 27$& 3498$\pm 37$& 20288$\pm 73$& 2047$\pm 143$& 1376$\pm 167$\\ -{Model 2}& IELs& -51000 & 2025$\pm 26$& 2494$\pm 32$&$< 37$&$< 124$& 1005$\pm 190$& 72$\pm 28$& 72$\pm 21$& 113$\pm 18$& 271$\pm 85$& 205$\pm 72$& 34$\pm 21$\\ -{ }& NELs& 52 & 637$\pm 10$& 477$\pm 17$&$< 4$&$< 8$& -- & 278$\pm 17$& 153$\pm 10$& 317$\pm 15$& 969$\pm 40$& 325$\pm 37$& - 147$\pm 22$\\ -\enddata -\tablecomments{This is an example of how to split a deluxetable. You can -split any table with this command into two or three parts. The location of -the split is given by the author based on the placement of the ``B`` -indicators in the column identifier preamble. For more information please -look at the new \aastex instructions.} -\end{splitdeluxetable*} - ## Figures -%% The "ht!" tells LaTeX to put the figure "here" first, at the "top" next -%% and to override the normal way of calculating a float position \begin{figure}[ht!] -\plotone{cost.pdf} +\includegraphics{cost} \caption{The subscription (squares) and author publication (asterisks) costs from 1991 to 2013. Subscription cost are on the left Y axis while the author costs are on the right Y axis. All numbers in US dollars and @@ -1365,7 +1346,7 @@ used to position the two image files side by side. Both `\plotone` and `\plottwo` take a `\caption` and an optional `\figurenum` command to specify the figure number\footnote{It is better to not use -`\figurenum` and let \latex auto-increment all the figures. If you +figurenum and let \latex auto-increment all the figures. If you do use this command you need to mark all of them accordingly.}. Each is based on the ` graphicx` package command, `\includegraphics`. Authors are welcome to use @@ -1401,21 +1382,6 @@ Figure \ref{fig:pyramid} shows an inverted pyramid of individual figure constructed with six individual EPS files using the `\gridline` option. -\begin{figure*} -\gridline{\fig{V2491_Cyg.pdf}{0.3\textwidth}{(a)} - \fig{HV_Cet.pdf}{0.3\textwidth}{(b)} - \fig{LMC_2009.pdf}{0.3\textwidth}{(c)} - } -\gridline{\fig{RS_Oph.pdf}{0.3\textwidth}{(d)} - \fig{U_Sco.pdf}{0.3\textwidth}{(e)} - } -\gridline{\fig{KT_Eri.pdf}{0.3\textwidth}{(f)}} -\caption{Inverted pyramid figure of six individual files. The nova are -(a) V2491 Cyg, (b) HV Cet, (c) LMC 2009, (d) RS Oph, (e) U Sco, and (f) -KT Eri. These individual figures are taken from \citet{2011ApJS..197...31S}. -\label{fig:pyramid}} -\end{figure*} - ## Enhanced graphics Enhanced graphics have an example figure to serve as an example for the @@ -1451,62 +1417,8 @@ but is now included. Note that when an article with figure set is compiled in \latex none of the component figures are shown and a floating Figure Set caption will appear in the resulting PDF. -\figsetstart -\figsetnum{4} -\figsettitle{Swift X-ray light curves} - -\figsetgrpstart -\figsetgrpnum{1.1} -\figsetgrptitle{KT Eri} -\figsetplot{KT_Eri.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of KT Eri.} -\figsetgrpend - -\figsetgrpstart -\figsetgrpnum{1.2} -\figsetgrptitle{RS Oph} -\figsetplot{RS_Oph.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of RS Oph.} -\figsetgrpend - -\figsetgrpstart -\figsetgrpnum{1.3} -\figsetgrptitle{U Sco} -\figsetplot{U_Sco.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of U Sco.} -\figsetgrpend - -\figsetgrpstart -\figsetgrpnum{1.4} -\figsetgrptitle{V2491 Cyg} -\figsetplot{V2491_Cyg.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of V2491 Cyg.} -\figsetgrpend - -\figsetgrpstart -\figsetgrpnum{1.5} -\figsetgrptitle{Nova LMC 2009} -\figsetplot{LMC_2009.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of nova LMC 2009.} -\figsetgrpend - -\figsetgrpstart -\figsetgrpnum{1.6} -\figsetgrptitle{HV Cet} -\figsetplot{HV_Cet.pdf} -\figsetgrpnote{The Swift/XRT X-ray light curve for the first year after -outburst of HV Cet.} -\figsetgrpend - -\figsetend - \begin{figure} -\plotone{KT_Eri.pdf} +\includegraphics{KT_Eri.pdf} \caption{The Swift/XRT X-ray light curve for the first year after outburst of the suspected recurrent nova KT Eri. At a maximum count rate of 328 ct/s, KT Eri was the brightest nova in X-rays observed to date. All @@ -1535,18 +1447,6 @@ including start and stop times and the video duration. Authors should review the AAS animation guidelines in the graphics guide at \url{https://journals.aas.org/graphics-guide/#animations}. -\begin{figure} -\begin{interactive}{animation}{movie.mp4} -\plotone{f4.pdf} -\end{interactive} -\caption{Figure 1 from \citet{2018ApJ...868L..33L}. AIA 171\AA (a,b), -AIA 131\AA (c), and AIA 304\AA images are shown. The red rectangle -in (a) shows the field of view of the other panels. An animation of -panels (b-d) is available. It covers 8 hours of observing beginning -at 01:00 UT on 2012 January 19. The video duration is 20 seconds. -\label{fig:video}} -\end{figure} - Animations and interactive figures (Section \ref{sec:interactive}) should use the `\begin{interactive}` environment in the figure call. This environment @@ -1588,25 +1488,6 @@ to external javascript libraries. Ideally, the javascript should be included with the submitted package of interactive files to minimize external dependencies within the published article. -\begin{figure} -\begin{interactive}{js}{interactive.tar.gz} -\plotone{f5.pdf} -\end{interactive} -\caption{Figure 4 from \citet{2018AJ....156...82C}. \emph{Upper panel}: the -cumulative median observing time to measure the $3\sigma$ RV masses of TESS -planets as a function of host star spectral type and up to $10^3$ hours. -The \emph{dashed blue curves} represent the results from the optical -spectrograph whereas the \emph{solid red curves} represent the near-IR -spectrograph. \emph{Lower panel}: the time derivative of the cumulative -observing time curves used to indicate the RV planet detection efficiency. -The \emph{horizontal dashed line} highlights the value of the detection -efficiency at 20 hours per detection. Note that unlike the lower panels, -the upper panels do not share a common ordinate due to the differing number -of planet detections around stars in each spectral type bin. The -interactive version has two buttons that allows one to turn the optical and -NIR layers. \label{fig:interactive}} -\end{figure} - Authors should consult the online tutorials at \url{https://journals.aas.org/graphics-guide/#interactive_figures} for more information on what is currently supported and links to @@ -1684,22 +1565,6 @@ Authors sometimes use color to highlight changes to their manuscript in response to editor and referee comments. In \aastex new commands have been introduced to make this easier and formalize the process. -The first method is through a new set of editing mark up commands that -specifically identify what has been changed. These commands are -`\added{}`, `\deleted{}`, and -`\replaced{\`{\}}. To activate these -commands the ` trackchanges` option must be used in the -`\documentclass` call. When compiled this will produce the -marked text in red. The `\explain{}` can be used to add -text to provide information to the reader describing the change. Its -output is purple italic font. To see how `\added{}`, `\deleted{}`, -`\replaced{}{}` and -`\explain{}` commands will produce -\added{important added information}\deleted{, deleted text, and } -\replaced{old data}{and replaced data,} toggle between versions compiled with -and without the ` \trackchanges` option.\explain{text explaining -the change} - A summary list of all these tracking commands can be produced at the end of the article by adding the `\listofchanges` just before the `\end{document}` call. The page number for each change will be @@ -1714,10 +1579,6 @@ multiple revisions. The commands are `\edit1{}`, `\edit2{}` and `\edit3{}` and they produce `` that is highlighted in bold, bold+italic and bold+underline, respectively. Authors should use the first command to -\edit1{indicated which text has been changed from the first revision.} The -second command is to highlight \edit2{new or modified text from a second -revision}. If a third revision is needed then the last command should be used -\edit3{to show this changed text}. Since over 90\% of all manuscripts are accepted after the 3rd revision these commands make it easy to identify what text has been added and when. Once the article is accepted all the highlight color can be turned off simply by adding the @@ -1758,7 +1619,7 @@ In the bibliography the format for data or code follows this format: \citet{2015ApJ...805...23C} provides a example of how the citation in the article references the external code at -\doi{10.5281/zenodo.15991}. Unfortunately, bibtex does +`\doi{10.5281/zenodo.15991}`. Unfortunately, bibtex does not have specific bibtex entries for these types of references so the ``@misc`` type should be used. The Repository tutorial explains how to code the ``@misc`` type correctly. The most recent aasjournal.bst file,