diff --git a/Pipeline_flow_diagram.pdf b/Pipeline_flow_diagram.pdf
deleted file mode 100644
index 08c6042..0000000
Binary files a/Pipeline_flow_diagram.pdf and /dev/null differ
diff --git a/Stack_examples.pdf b/Stack_examples.pdf
deleted file mode 100644
index ad0a9ea..0000000
Binary files a/Stack_examples.pdf and /dev/null differ
diff --git a/potpyri/_version.py b/potpyri/_version.py
index 277a711..b6ae0b0 100644
--- a/potpyri/_version.py
+++ b/potpyri/_version.py
@@ -1,7 +1,14 @@
 # file generated by setuptools-scm
 # don't change, don't track in version control
 
-__all__ = ["__version__", "__version_tuple__", "version", "version_tuple"]
+__all__ = [
+    "__version__",
+    "__version_tuple__",
+    "version",
+    "version_tuple",
+    "__commit_id__",
+    "commit_id",
+]
 
 TYPE_CHECKING = False
 if TYPE_CHECKING:
@@ -9,13 +16,19 @@
     from typing import Union
 
     VERSION_TUPLE = Tuple[Union[int, str], ...]
+    COMMIT_ID = Union[str, None]
 else:
     VERSION_TUPLE = object
+    COMMIT_ID = object
 
 version: str
 __version__: str
 __version_tuple__: VERSION_TUPLE
 version_tuple: VERSION_TUPLE
+commit_id: COMMIT_ID
+__commit_id__: COMMIT_ID
 
-__version__ = version = '1.0.2.dev4'
-__version_tuple__ = version_tuple = (1, 0, 2, 'dev4')
+__version__ = version = '1.0.14.dev12'
+__version_tuple__ = version_tuple = (1, 0, 14, 'dev12')
+
+__commit_id__ = commit_id = 'g0f75b276d'
diff --git a/potpyri/stages/image_procs.py b/potpyri/stages/image_procs.py
index ab5e9e0..4a1d055 100755
--- a/potpyri/stages/image_procs.py
+++ b/potpyri/stages/image_procs.py
@@ -631,6 +631,9 @@ def create_mask(science_data, saturation, rdnoise, sigclip=3.5,
         else:
             print('Setting sky background to 2000.0')
 
+    # This needs to be done before data is modified to preserve bad pixels
+    mask_bp = (data==0.0) | np.isnan(data)
+
     # Set data background to skybkg
     data = data + skybkg
     # Also need to adjust the saturation level by SKYBKG for saturated pixels
@@ -638,8 +641,6 @@ def create_mask(science_data, saturation, rdnoise, sigclip=3.5,
     
     if log: log.info('Masking saturated pixels.')
 
-    mask_bp = (data==0.0) | np.isnan(data)
-
     mask_sat = np.zeros(data.shape).astype(bool) # create empty mask
     mask_sat = mask_sat.astype(np.uint8) #set saturated star mask type
     mask_sat[data >= saturation] = 4 #set saturated pixel flag
diff --git a/potpyri/stages/photometry.py b/potpyri/stages/photometry.py
index a95fffe..23f91bd 100755
--- a/potpyri/stages/photometry.py
+++ b/potpyri/stages/photometry.py
@@ -526,7 +526,8 @@ def photloop(stack, phot_sn_min=3.0, phot_sn_max=40.0, fwhm_init=5.0, log=None):
                       'snthresh_final': signal_to_noise}
         try:
             do_phot(stack, star_param=star_param) 
-        except:
+        except Exception as e:
+            log.error(e)
             signal_to_noise = signal_to_noise / 2.0
             continue
         break
diff --git a/potpyri/stages/solve_wcs.py b/potpyri/stages/solve_wcs.py
index e4a3c41..fe45d51 100755
--- a/potpyri/stages/solve_wcs.py
+++ b/potpyri/stages/solve_wcs.py
@@ -20,10 +20,10 @@
 import astropy.units as u
 from astropy.stats import sigma_clipped_stats
 from astropy.io import fits
-from astropy.io import ascii
 from astropy.coordinates import SkyCoord
 from astropy.coordinates import match_coordinates_sky
-from astropy.table import Table, Column
+from astropy.table import Column
+from astropy.table import Table
 from astropy.utils.exceptions import AstropyWarning
 from astropy.wcs import WCS
 from astropy.wcs.utils import fit_wcs_from_points
@@ -67,7 +67,10 @@ def get_gaia_catalog(input_file, log=None):
         try:
             cat = vizier.query_region(coord, width=20 * u.arcmin, 
                 catalog='I/355/gaiadr3')
-            break
+            if cat is None:
+                if log: log.error(f'Gaia did not return catalog.  Try #{tries+1}')
+            else:
+                break
         except requests.exceptions.ReadTimeout:
             if log: log.error(f'Gaia catalog timeout.  Try #{tries+1}')
             tries += 1
@@ -195,7 +198,7 @@ def solve_astrometry(file, tel, binn, paths, radius=0.5, replace=True,
 
     tries = 1
     good = False
-    while tries < 4 and not good:
+    while tries < 5 and not good:
         input_args = args + extra_opts
 
         if log: 
@@ -226,6 +229,13 @@ def solve_astrometry(file, tel, binn, paths, radius=0.5, replace=True,
                 extra_opts='--objs 15'
             elif tries==3:
                 extra_opts=''
+            elif tries==4:
+                # Try with no constraint on RA/Dec
+                args = '--scale-units arcsecperpix '
+                args += f'--scale-low {scale_low} --scale-high {scale_high} '
+                args += f'--no-plots -T '
+                args += f'--overwrite -N {newfile} --dir {directory} '
+                extra_opts=''
 
 
     file_exists=os.path.exists(newfile)
diff --git a/tests/test_photometry.py b/tests/test_photometry.py
index ecd3fe3..db182b5 100644
--- a/tests/test_photometry.py
+++ b/tests/test_photometry.py
@@ -22,6 +22,15 @@ def test_photometry(tmp_path):
         if key in [h.name for h in hdu]:
             del hdu[key]
 
+    # Sanitize error array
+    mask = np.isnan(hdu['ERROR'].data)
+    hdu['ERROR'].data[mask] = np.nanmedian(hdu['ERROR'].data)
+    mask = hdu['ERROR'].data < 0.0
+    hdu['ERROR'].data[mask] = np.nanmedian(hdu['ERROR'].data)
+    maxval = np.max(hdu['SCI'].data)
+    mask = np.isinf(hdu['ERROR'].data)
+    hdu['ERROR'].data[mask] = maxval
+
     hdu.writeto(file_path, overwrite=True)
 
     data_path, basefile = os.path.split(file_path)