diff --git a/RELEASE_CHECKLIST.md b/RELEASE_CHECKLIST.md index f1c7865..2aa7b7a 100644 --- a/RELEASE_CHECKLIST.md +++ b/RELEASE_CHECKLIST.md @@ -8,11 +8,12 @@ Please be sure to do the following when making a release. 5. Update release notes `RELEASENOTES.md`. 6. Update `docs/source/index.rst` if badges changed. 7. Restore fail-on-warning on .readthedocs.yaml if it was turned off. -8. Make a release on github. -9. Be sure the `stable` build of readthedocs points to the new release. -10. Be sure to create a version on readthedocs of the new release. -11. If the version is a patch, deactivate the docs version for the previous patch of the same minor version. (Only one docs version for each minor version should be active at a time.) -12. Be sure codecov website is switched to default to master branch. -13. Update Zenodo. -14. Move readthedocs latest to master branch. -15. Remove items 14 and 15 from this list. +8. Update all binder links in `docs/source/02_Modules.rst` to point to the upcoming version. +9. Make a release on github. +10. Be sure the `stable` build of readthedocs points to the new release. +11. Be sure to create a version on readthedocs of the new release. +12. If the version is a patch, deactivate the docs version for the previous patch of the same minor version. (Only one docs version for each minor version should be active at a time.) +13. Be sure codecov website is switched to default to master branch. +14. Update Zenodo. +15. Move readthedocs latest to master branch. +16. Remove items 14 and 15 from this list. diff --git a/docs/source/01_Getting_Started.rst b/docs/source/01_Getting_Started.rst index 5d14fcc..66e36f2 100644 --- a/docs/source/01_Getting_Started.rst +++ b/docs/source/01_Getting_Started.rst @@ -2,10 +2,8 @@ 1. Getting started ================== - ------- Binder ------- +====== .. image:: https://mybinder.org/badge_logo.svg :target: https://mybinder.org/v2/gh/villano-lab/galactic-spin-W1/master?labpath=binder @@ -13,9 +11,32 @@ Binder Binder is a website that hosts jupyter notebooks and allows users to run them on the web without any download or installation required from the user. If you only wish to run the notebooks, you can click on the binder button above to run them from your browser. ------------- Installation ------------- +============ Installation of this workshop is not needed. -Binder Project provides an easy access to Jupyter notebooks and their environments without the hassle of installation. Upon clicking on the provided Binder URLs, the modules of the workshop open in your browser. \ No newline at end of file +Binder Project provides an easy access to Jupyter notebooks and their environments without the hassle of installation. +Upon clicking on the provided Binder URLs, the modules of the workshop open in your browser. + +If you wish to work offline, you can run these notebooks in Jupyter Lab or Jupyter Notebooks. + +Requirements +------------ + +1. **Jupyter Lab** or **Jupyter Notebooks**, which are both included with `Anaconda Python `_. +2. The ability to install python modules, either through **pip**, **conda**, or `Anaconda Python `_. + +Instructions +------------ + +These instructions will assume that you will use Anaconda. +For experienced users with other setups, +please install the environment found in `binder/environment.yml` to run our notebooks. + +0. Install `Anaconda Python `_. +1. `Download `_ and unzip the repository somewhere inside your user directory, such as the "Documents" folder. +2. In Anaconda Navigator, go to "Environments," then select "Import." +3. Import from "Local drive" and select the file `binder/environment.yml` from the repository. Name the environment `galactic-spin`. Anaconda will start installing all other necessary dependencies; please be patient, as this will take some time. +4. Once the environment is finished building, from the "Home" menu of Anaconda Navigator, launch a prompt. The prompt will depend on your system -- for example, in Windows, you can choose "CMD.exe Prompt." +5. In the prompt, run the following command: `ipython kernel install --user --name=galactic-spin` +6. In Anaconda Navigator, launch "JupyterLab" and browse to your local copy of the repository, then enter the `binder` subdirectory. Enjoy! \ No newline at end of file diff --git a/docs/source/02_Modules.rst b/docs/source/02_Modules.rst index 1411eab..92a882e 100644 --- a/docs/source/02_Modules.rst +++ b/docs/source/02_Modules.rst @@ -2,6 +2,9 @@ 2. Modules ========== +.. role:: raw-html(raw) + :format: html + -------- Overview -------- @@ -9,29 +12,47 @@ Overview Description of the learning modules -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| **File Name** | **Short Description** | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `01_DM_Rotation_Curve_Intro.ipynb` | Animations and rotation curve plots demonstrating three types of rotational motion. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `02_Widget_NGC5533_DMonly.ipynb` | An interactive introduction to Dark Matter. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `03_Measured_Data_Plotting.ipynb` | Rotation curve plotting of measured velocities to visualize star and gas motions in a galaxy. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `04_Plotting_Rotation_Curves.ipynb` | Choose between 4 galaxies and plot the rotation curve of each component and their total velocity. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `05_Widget_NGC5533_All_Components.ipynb` | Interactive widget to adjust the components of the galaxy NGC 5533 and see how velocity changes. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `06_Plotting_SPARC_Data.ipynb` | Plotting the components of galactic rotation curves using the SPARC database of 175 galaxies. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `07_Bonus_Bulge_Rotation_Curve.ipynb` | Calculate the theoretical rotation curve of the bulge component using empirically derived parameters. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `08_Interactive_Fitting.ipynb` | Calculate the fitting parameters of the rotation curve to determine the amount of Dark Matter needed. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `09_Widget_SPARC_Galaxies.ipynb` | Interactive widget to visualize the components of multiple galaxies using the SPARC database of 175 galaxies. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ -| `10_Bonus_Black_Holes_as_DM.ipynb` | Considering tiny black holes as Dark Matter candidates. | -+------------------------------------------+----------------------------------------------------------------------------------------------------------------+ ++------------------------------------------+--------------------------------------------------------+ +| **File Name** | **Short Description** | ++------------------------------------------+--------------------------------------------------------+ +| `01_DM_Rotation_Curve_Intro.ipynb` | Animations and rotation curve plots demonstrating | +| | :raw-html:`
` | +| | three types of rotational motion. | ++------------------------------------------+--------------------------------------------------------+ +| `02_Widget_NGC5533_DMonly.ipynb` | An interactive introduction to Dark Matter. | ++------------------------------------------+--------------------------------------------------------+ +| `03_Measured_Data_Plotting.ipynb` | Rotation curve plotting of measured velocities to | +| | :raw-html:`
` | +| | visualize star and gas motions in a galaxy. | ++------------------------------------------+--------------------------------------------------------+ +| `04_Plotting_Rotation_Curves.ipynb` | Choose between 4 galaxies and plot the rotation curve | +| | :raw-html:`
` | +| | of each component and their total velocity. | ++------------------------------------------+--------------------------------------------------------+ +| `05_Widget_NGC5533_All_Components.ipynb` | Interactive widget to adjust the components of the | +| | :raw-html:`
` | +| | galaxy NGC 5533 and see how velocity changes. | ++------------------------------------------+--------------------------------------------------------+ +| `06_Plotting_SPARC_Data.ipynb` | Plotting the components of galactic rotation curves | +| | :raw-html:`
` | +| | using the SPARC database of 175 galaxies. | ++------------------------------------------+--------------------------------------------------------+ +| `07_Bonus_Bulge_Rotation_Curve.ipynb` | Calculate the theoretical rotation curve of the bulge | +| | :raw-html:`
` | +| | component using empirically derived parameters. | ++------------------------------------------+--------------------------------------------------------+ +| `08_Interactive_Fitting.ipynb` | Calculate the fitting parameters of the rotation curve | +| | :raw-html:`
` | +| | to determine the amount of Dark Matter needed. | ++------------------------------------------+--------------------------------------------------------+ +| `09_Widget_SPARC_Galaxies.ipynb` | Interactive widget to visualize the components of | +| | :raw-html:`
` | +| | multiple galaxies using the SPARC database of 175 | +| | :raw-html:`
` | +| | galaxies. | ++------------------------------------------+--------------------------------------------------------+ +| `10_Bonus_Black_Holes_as_DM.ipynb` | Considering tiny black holes as Dark Matter candidates.| ++------------------------------------------+--------------------------------------------------------+ -------------------------- 01_DM_Rotation_Curve_Intro diff --git a/docs/source/03_Glossary.rst b/docs/source/03_Glossary.rst index d291523..77f0810 100644 --- a/docs/source/03_Glossary.rst +++ b/docs/source/03_Glossary.rst @@ -5,88 +5,125 @@ Glossary .. glossary:: Arcsecond - Unit of an angle of how large something appears in the sky. + Unit of an angle denoting how large something appears in the sky. Bulge - Dense spherical core of the galaxy. + Dense, spherical core of the galaxy. Central mass density - The central mass density is the density at the center of the galaxy, changing this value changes the magnitude of the Dark Matter curve. + The density of dark matter at the center of the galaxy. Changing this value changes the magnitude of the dark matter curve. + Centripetal force + A force that causes circular motion. + Concentration parameter - Also known as the bulge Sersic parameter "describes the curvature of the profile in a radius-magnitude plot" (Noordermeer 2008). + Also known as the bulge Sersic parameter. "Describes the curvature of the profile in a radius-magnitude plot" [Noordermeer2008]_. Core radius - The core radius indicates where the density falls off by a factor of e (~2.7). Adjusting this factor changes where the "bump" of the curve is located. Related words: cutoff radius, scale radius. + Indicates the distance from the galactic center where the density falls off by a factor of *e* (~2.7). Adjusting this factor changes where the "bump" of the curve is located. Synonyms: cutoff radius, scale radius. Dark matter - Dark matter is a placeholder to account for the matter in spiral galaxies that is `missing` ... Related words: Dark Matter halo. + A placeholder to account for the matter in spiral galaxies that is `missing` based on our observations of galactic motion. Related words: Dark Matter halo, Halo. + Dark matter halo + A disk-shaped distribution of Dark Matter that is most dense at some distance from the galactic center. + Density profile The mass distribution of matter in the galaxy. Disk - The stellar disk of the galaxy is a relatively flat component of the galaxy. - - Inclination angle - The angle of the galaxy from the horizontal. - + A large, relatively flat component of the galaxy. + + Enclosed mass + The total mass of the area between the center of the galaxy or other body and the specified radius. + + Edge-on spiral galaxy + A galaxy which lies in the same plane as our viewing direction which results in us only seeing the outer edge of the galaxy and part of the central bulge. Alternatively, a face-on galaxy is perpendicular to our line of sight revealing its spiral structure. + Fitting - ... + The process of adjusting unknown parameters in order to match a theoretical equation to measured data. + Flat Rotation + Rotation whose curve plateaus at large radii. + Gravitational constant (G) - ... - + The constant of proportionality used to calculate effects of gravity. + In SI units, G = 6.67e-11 m^3 kg^-1 s^-2 + + Inclination angle + The angle of the galaxy from the horizontal, as viewed from Earth. For example, a face-on galaxy has an inclination angle of 0, and an edge-on galaxy has an inclination angle of 90°. + Interstellar gas - Gas between stars and galaxies. + Gas between stars and galaxies -- mostly Hydrogen. Synonyms: atomic gas. Isothermal - ... - - Luminous matter - All matter that we are able to `see` in galaxies. Related words: light matter, visible matter, baryonic matter. - + Having a constant temperature. In thermal physics, this affects the behavior of temperature-related properties, such as density. + + Keplerian model + A model of the orbital motion of planets in solar systems such that the orbital velocity is inversely proportional to the square root of the radius. Related words: planet-like motion. + kpc - Unit of distance. kiloparsec: 1 kpc = 3262 light years = 3.086e+19 meters = 1.917e+16 miles. + Unit of distance; kiloparsec. 1 kpc = 3262 light years = 3.086e+19 meters = 1.917e+16 miles. + Luminous matter + All matter that emits visible light in galaxies. Synonyms: light matter, visible matter, baryonic matter. + MACHO - Massive Compact Halo Object. + MAssive Compact Halo Object. A type of object that emits little to no light, such as brown dwarfs, rogue planets, or black holes. - Mass-to-light ratio - The ratio of how much mass there is compared to how much it is visible. How much mass it is expected from the light source. The variation in the mass-to-light ratio means there is a wider range of masses that are plausible for the stellar component. Related words: M/L + Mass-to-light ratio (M/L ratio) + The ratio of how much mass there is compared to how much light the body emits; how much mass it is expected from the light source. Variation in the mass-to-light ratio means there is a wider range of masses that are plausible for the stellar component. Measured datapoints - Measured velocities of stars and gas in a galaxy. Related words: measured velocities. + Measured velocities of stars and gas in a galaxy. Synonyms: measured velocities. Mpc - Unit of distance. Megaparsec: 1 Mpc = 1000 kpc. + Unit of distance; megaparsec: 1 Mpc = 1000 kpc. NGC New General Catalogue of galaxies. Photometry - ... + The measurement of light emitted from astronomical objects. + Planet-like rotation + Rotation whose curve resembles that of planets orbiting a star. Related words: Keplerian model. + Prefactor - ... Related words: scaling parameter, M/L ratio + A parameter that multiplies/directly scales the other information in an equation. Synonyms: scaling parameter. Related words: M/L ratio Radial velocity The speed stars and gas are moving at different distances from the center of the galaxy. Reduced chi-squared value - In a strictly statistical sense, a reduced chi-squared of zero represents a perfect fit. However, a reduced chi-squared much less than 1 often indicates that more parameters were used than represented by the physical system. We would be simply connecting the measured data points. + A measure of how close the data and theory are to one another. In a strictly statistical sense, a reduced chi-squared of zero represents a perfect fit. However, a reduced chi-squared much less than 1 often indicates that more parameters were used than represented by the physical system, and we may be simply connecting the measured data points. + Rigid body rotation + Rotation whose curve resembles that of a rigid object. Synonyms: frisbee rotation + Rotation curve A plot of a galaxy's radial velocity versus the radius or distance from the center. Solar mass - Mass of the Sun. Approximately equal to 1.989e30 kilograms + Mass of the Sun, equal to 1.989e30 kilograms. + + Spiral arms + In a spiral galaxy, these are the long parts protruding from the disc's otherwise elliptical shape. Related words: spiral galaxy. + + Spiral galaxy + Galaxies that have spiral structures. Components are bulge, disk, gas, and Dark Matter halo. Spiral galaxies are less luminous than elliptical galaxies on average and have active star formation. Related words: spiral arms. + + Surface brightness + The amount of flux from the galaxy per square arcsecond on the sky. Theoretical rotation curve - ... + A rotation curve that has been modeled from known parameters that is then used to match observed data. UGC Uppsala General Catalogue of galaxies. + + Uncertainty + A value representing what range of values a data point might differ from what we measured. Synonyms: error. Zero-point luminosity - ... \ No newline at end of file + A reference luminosity for a star that has a zero absolute bolometric magnitude [Mamajek2015]_. \ No newline at end of file diff --git a/docs/source/04_Citations.rst b/docs/source/04_Citations.rst index fe4d5d0..62431f2 100644 --- a/docs/source/04_Citations.rst +++ b/docs/source/04_Citations.rst @@ -8,7 +8,7 @@ How to cite If you decide to use this code, or if you want to add a reference to it, please cite the latest archived version, - Villano, A.N., Bergfalk, J., Hatami, R., Harris, K., Vititoe, F., and Johnston, J., 2022, Galactic Spin Workshop 1 - The Basics of Rotation Curves [Code, v1.0.0] [DOI:] + Villano, A.N., Bergfalk, J., Hatami, R., Harris, K., Vititoe, F., and Johnston, J., 2022, The Data Behind Dark Matter: Exploring Galactic Rotation [Code, v1.0.0] [DOI:10.5281/zenodo.6588351] .. raw:: html @@ -19,12 +19,12 @@ If you decide to use this code, or if you want to add a reference to it, please @software{galacticspinW1, author = {Villano, A.N., Bergfalk, J., Hatami, R., Harris, K., Vititoe, F., and Johnston, J.}, - title = {{Galactic Spin Workshop 1 - The Basics of Rotation Curves [Code, v1.0.0]}}, + title = {{The Data Behind Dark Matter: Exploring Galactic Rotation [Code, v1.0.1]}}, year = {2022}, - publisher = {}, - version = {v1.0.0}, - doi = {DOI:}, - url = {}, + publisher = {Zenodo}, + version = {v1.0.1}, + doi = {DOI:10.5281/zenodo.6588351}, + url = {https://zenodo.org/record/6588351}, howpublished={The code can be found under \url{https://github.com/villano-lab/galactic-spin-W1/}.} } diff --git a/docs/source/05_Release_History.rst b/docs/source/05_Release_History.rst index 432060b..ab716f1 100644 --- a/docs/source/05_Release_History.rst +++ b/docs/source/05_Release_History.rst @@ -2,6 +2,11 @@ Release history =============== +* xx.xx.2022: Release of `v1.0.2 `_ + Expand and elaborate on documentation. + Fix various documentation issues. +* 27.04.2022: Release of `v1.0.1 `_ + Fixed various documentation issues. * 27.04.2022: Release of `v1.0.0 `_ Initial release for RaCAS 2022. * 27.04.2022: Release of `v1.0.1 `_ diff --git a/docs/source/07_Contact.rst b/docs/source/07_Contact.rst index 69021f4..3bf3080 100644 --- a/docs/source/07_Contact.rst +++ b/docs/source/07_Contact.rst @@ -2,7 +2,7 @@ Contact & Support ================= -The authors of *Galactic Spin Workshop 1* are `A.N. Villano `_, `J. Bergfalk `_, `K. Harris `_, `R. Hatami `_, F. Vititoe, and J. Johnston. +The authors of *Galactic Spin Workshop 1* are `A.N. Villano `_, `J. Bergfalk `_, `K. Harris `_, `R. Hatami `_, `F. Vititoe `_, and `J. Johnston `_. For questions, support, bug reports, or other suggestions, please open an issue on `github `_. \ No newline at end of file diff --git a/docs/source/References.rst b/docs/source/References.rst index ea5305e..d45cc32 100644 --- a/docs/source/References.rst +++ b/docs/source/References.rst @@ -3,25 +3,25 @@ References ========== .. .. [ref] author, *title*, `journal <>`_ -.. [BOB] Carroll, Bradley W. and Ostlie, Dale A., *An Introduction to Modern Astrophysics*, Cambridge University Press (2006). -.. [Casertano] Stefano Casertano, *Rotation curve of the edge-on spiral galaxy NGC 5907: disc and halo masses*, `Monthly Notices of the Royal Astronomical Society 203 (1983) `_. -.. [Datathief] B. Tummers, *Software*, `(2006) `_. +.. [Carroll2006] Carroll, Bradley W. and Ostlie, Dale A., *An Introduction to Modern Astrophysics*, Cambridge University Press (2006). +.. [Casertano1983] Stefano Casertano, *Rotation curve of the edge-on spiral galaxy NGC 5907: disc and halo masses*, `Monthly Notices of the Royal Astronomical Society 203 (1983) `_. +.. [Datathief2006] B. Tummers, *Software*, `(2006) `_. .. [deNaray2006] Rachel Kuzio de Naray and Stacy S. McGaugh and W. J. G. de Blok and A. Bosma, *High-Resolution Optical Velocity Fields of 11 Low Surface Brightness Galaxies*, `The Astrophysical Journal Supplement Series 165 (2006) `_. .. [deNaray2008] Rachel Kuzio de Naray and Stacy S. McGaugh and W. J. G. de Blok, *Mass Models for Low Surface Brightness Galaxies with High-Resolution Optical Velocity Fields*, `The Astrophysical Journal 676 (2008) `_. -.. [Epinat] Epinat, B. and Amram, P. and Marcelin, M. and Balkowski, C. and Daigle, O. and Hernandez, O. and Chemin, L. and Carignan, C. and Gach, J.L. and Balard, P., *GHASP: an Hα kinematic survey of spiral and irregular galaxies – VI. New Hα data cubes for 108 galaxies*, `Monthly Notices of the Royal Astronomical Society 388 (2008) `_. -.. [Fraternali] Fraternali, F. and Sancisi, R. and Kamphuis, P, *A tale of two galaxies: light and mass in NGC~891 and NGC~7814*, `Astronomy & Astrophysics 531 (2011) `_. -.. [GIPSY] Kapteyn Astronomical Institute, *GIPSY, the GRONINGEN image processing system, Software*, `(1992) `_. -.. [Graham] Alister W. Graham, *An Investigation into the Prominence of Spiral Galaxy Bulges*, `American Astronomical Society 121 (2001) `_. -.. [Jimenez] Raul Jimenez, Licia Verde, and S. Peng Oh, *Dark halo properties from rotation curves*, `Monthly Notices of the Royal Astronomical Society 339 (2003) `_. -.. [Karukes] Karukes, E. V. and Salucci, P. and Gentile, G., *The dark matter distribution in the spiral NGC 3198 out to 0.22 Rvir*, `Astronomy & Astrophysics 578 (2015) `_. -.. [Megaparsec] Swinburne University of Technology, *Megaparsec: Cosmos*, `Astronomy SWIN `_. -.. [NASAplanets] Dave Williams, *Planetary Fact Sheet*, `NASA (2021) `_. -.. [Newville] Matt Newville, Renee Otten, Andrew Nelson, Antonino Ingargiola, Till Stensitzki, Dan Allan, Austin Fox, Faustin Carter, Michał, Ray Osborn, Dima Pustakhod, lneuhaus, Sebastian Weigand, Glenn, Christoph Deil, Mark, Allan L. R. Hansen, Gustavo Pasquevich, Leon Foks, … Arun Persaud., *lmfit/lmfit-py: 1.0.3 (1.0.3)*, `Zenodo (2021) `_. -.. [Noordermeer] Edo Noordermeer, *The rotation curves of flattened Sérsic bulges*, `Monthly Notices of the Royal Astronomical Society 385 (2008) `_. -.. [Noordermeer-Hulst] Noordermeer, E. and Van Der Hulst, J. M., *The stellar mass distribution in early-type disc galaxies: surface photometry and bulge–disc decompositions*, `Monthly Notices of the Royal Astronomical Society 376 (2007) `_. -.. [Richards] Richards, Emily E. and van Zee, L. and Barnes, K. L. and Staudaher, S. and Dale, D. A. and Braun, T. T. and Wavle, D. C. and Calzetti, D. and Dalcanton, J. J. and Bullock, J. S. and Chandar, R., *Baryonic distributions in the dark matter halo of NGC 5005*, `Monthly Notices of the Royal Astronomical Society 449 (2015) `_. -.. [SkyView] McGlynn, T. and Scollick, K. and White, N., *SKYVIEW: The Multi-Wavelength Sky on the Internet*, `SAO/NASA Astrophysics Data System (1998) `_. -.. [SmallestBH] Springer Nature, *The smallest known Black Hole*, `Scientific American (2008) `_. -.. [SPARC] Federico Lelli, Stacy S. McGaugh, and James M. Schombert, *SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves*, `The Astronomical Journal 152 (2016) `_. -.. [Taylor] Taylor, John R., *An Introduction to Error Analysis: The Study of Uncertainties in Physical Measurements*, University Science Books (1996). -.. [Zeropoint] Mamajek, E. E., Torres, G., Prsa, A., Harmanec, P., Asplund, M., Bennett, P. D., Capitaine, N., Christensen-Dalsgaard, J., Depagne, E., Folkner, W. M., Haberreiter, M., Hekker, S., Hilton, J. L., Kostov, V., Kurtz, D. W., Laskar, J., Mason, B. D., Milone, E. F., Montgomery, M. M., Richards, M. T., *IAU 2015 Resolution B2 on Recommended Zero Points for the Absolute and Apparent Bolometric Magnitude Scales*, `SAO/NASA Astrophysics Data System (2015) `_. \ No newline at end of file +.. [Epinat2008] Epinat, B. and Amram, P. and Marcelin, M. and Balkowski, C. and Daigle, O. and Hernandez, O. and Chemin, L. and Carignan, C. and Gach, J.L. and Balard, P., *GHASP: an Hα kinematic survey of spiral and irregular galaxies – VI. New Hα data cubes for 108 galaxies*, `Monthly Notices of the Royal Astronomical Society 388 (2008) `_. +.. [Fraternali2011] Fraternali, F. and Sancisi, R. and Kamphuis, P, *A tale of two galaxies: light and mass in NGC~891 and NGC~7814*, `Astronomy & Astrophysics 531 (2011) `_. +.. [GIPSY1992] Kapteyn Astronomical Institute, *GIPSY, the GRONINGEN image processing system, Software*, `(1992) `_. +.. [Graham2001] Alister W. Graham, *An Investigation into the Prominence of Spiral Galaxy Bulges*, `American Astronomical Society 121 (2001) `_. +.. [Jimenez2003] Raul Jimenez, Licia Verde, and S. Peng Oh, *Dark halo properties from rotation curves*, `Monthly Notices of the Royal Astronomical Society 339 (2003) `_. +.. [Karukes2015] Karukes, E. V. and Salucci, P. and Gentile, G., *The dark matter distribution in the spiral NGC 3198 out to 0.22 Rvir*, `Astronomy & Astrophysics 578 (2015) `_. +.. [SWIN] Swinburne University of Technology, *Megaparsec: Cosmos*, `Astronomy SWIN `_. +.. [Williams2021] Dave Williams, *Planetary Fact Sheet*, `NASA (2021) `_. +.. [Newville2021] Matt Newville, Renee Otten, Andrew Nelson, Antonino Ingargiola, Till Stensitzki, Dan Allan, Austin Fox, Faustin Carter, Michał, Ray Osborn, Dima Pustakhod, lneuhaus, Sebastian Weigand, Glenn, Christoph Deil, Mark, Allan L. R. Hansen, Gustavo Pasquevich, Leon Foks, … Arun Persaud., *lmfit/lmfit-py: 1.0.3 (1.0.3)*, `Zenodo (2021) `_. +.. [Noordermeer2008] Edo Noordermeer, *The rotation curves of flattened Sérsic bulges*, `Monthly Notices of the Royal Astronomical Society 385 (2008) `_. +.. [Noordermeer2007] Noordermeer, E. and Van Der Hulst, J. M., *The stellar mass distribution in early-type disc galaxies: surface photometry and bulge–disc decompositions*, `Monthly Notices of the Royal Astronomical Society 376 (2007) `_. +.. [Richards2015] Richards, Emily E. and van Zee, L. and Barnes, K. L. and Staudaher, S. and Dale, D. A. and Braun, T. T. and Wavle, D. C. and Calzetti, D. and Dalcanton, J. J. and Bullock, J. S. and Chandar, R., *Baryonic distributions in the dark matter halo of NGC 5005*, `Monthly Notices of the Royal Astronomical Society 449 (2015) `_. +.. [SkyView1998] McGlynn, T. and Scollick, K. and White, N., *SKYVIEW: The Multi-Wavelength Sky on the Internet*, `SAO/NASA Astrophysics Data System (1998) `_. +.. [Springer2008] Springer Nature, *The smallest known Black Hole*, `Scientific American (2008) `_. +.. [SPARC2016] Federico Lelli, Stacy S. McGaugh, and James M. Schombert, *SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves*, `The Astronomical Journal 152 (2016) `_. +.. [Taylor1996] Taylor, John R., *An Introduction to Error Analysis: The Study of Uncertainties in Physical Measurements*, University Science Books (1996). +.. [Mamajek2015] Mamajek, E. E., Torres, G., Prsa, A., Harmanec, P., Asplund, M., Bennett, P. D., Capitaine, N., Christensen-Dalsgaard, J., Depagne, E., Folkner, W. M., Haberreiter, M., Hekker, S., Hilton, J. L., Kostov, V., Kurtz, D. W., Laskar, J., Mason, B. D., Milone, E. F., Montgomery, M. M., Richards, M. T., *IAU 2015 Resolution B2 on Recommended Zero Points for the Absolute and Apparent Bolometric Magnitude Scales*, `SAO/NASA Astrophysics Data System (2015) `_. \ No newline at end of file diff --git a/docs/source/conf.py b/docs/source/conf.py index cce0533..3a428f4 100644 --- a/docs/source/conf.py +++ b/docs/source/conf.py @@ -79,4 +79,4 @@ def configureDoxyfile(input_dir, output_dir): # Add any paths that contain custom static files (such as style sheets) here, # relative to this directory. They are copied after the builtin static files, # so a file named "default.css" will overwrite the builtin "default.css". -html_static_path = [] +html_static_path = [] \ No newline at end of file diff --git a/docs/source/index.rst b/docs/source/index.rst index 8f82983..01c9a87 100644 --- a/docs/source/index.rst +++ b/docs/source/index.rst @@ -10,6 +10,9 @@ .. .. image:: https://mybinder.org/badge_logo.svg .. :target: https://mybinder.org/v2/gh/villano-lab/galactic-spin-W1/HEAD?labpath=binder .. :alt: Binder +.. .. image:: https://zenodo.org/badge/DOI/10.5281/zenodo.6588351.svg +.. :target: https://doi.org/10.5281/zenodo.6588351 +.. :alt: Zenodo DOI ========================================================== *Galactic Spin Workshop 1* - The Basics of Rotation Curves