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improved readme
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README.md

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@@ -41,7 +41,7 @@ glomap mapper --database_path DATABASE_PATH --output_path OUTPUT_PATH --image_pa
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```
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For more details on the command line interface, one can type `glomap -h` or `glomap mapper -h` for help.
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We also provide a guide on improving the obtained reconstruction, which can be found [here](docs/getting_started.md)
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We also provide a guide on improving the obtained reconstruction, which can be found [here](docs/getting_started.md).
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Note:
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- GLOMAP depends on two external libraries - [COLMAP](https://github.com/colmap/colmap) and [PoseLib](https://github.com/PoseLib/PoseLib).

docs/getting_started.md

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The number of global positioning and bundle adjustment iterations can be limited
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using the `--GlobalPositioning.max_num_iterations` and
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`--BundleAdjustment.max_num_iterations` options.
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#### Enable GPU-based solver
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If Ceres 2.3 or above is installed and the cuDSS are installed, GLOMAP supports GPU
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accelerated optimization process now. The process can be largely speed up with flags
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`--GlobalPositioning.use_gpu 1 --BundleAdjustment.use_gpu`.

docs/rotation_averager.md

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@@ -50,8 +50,10 @@ The gravity direction file is expected to be of the following format
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```
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IMAGE_NAME GX GY GZ
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```
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The gravity direction $g$ should $[0, 1, 0]$ if the image is parallel to the ground plane, and the estimated rotation would have the property that $R_i \cdot [0, 1, 0]^\top = g$.
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If is acceptable if only a subset of all images have gravity direciton.
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The gravity direction $g$ should $[0, 1, 0]$ if the image is orthogonal to the ground plane, and the estimated rotation would have the property that $R_i \cdot [0, 1, 0]^\top = g$.
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More explicitly, suppose we can transpose a 3D point from the world coordinate to the image coordinate by RX + t = x, then the gravity direction should be the second column of the R.
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It is acceptable if only a subset of all images have gravity direciton.
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If the specified image name does not match any known image name from relative pose, it is ignored.
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### Output

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