Mean magnitude and position on the discovery images: 
                   2026 07 02.1857  2461223.6857  13.57  17:32:01.20 -15:02:03.7
 10.20773   9.99957 galactic  Ser  Second-epoch detections are separated by 3.3" and 9.4 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
527 Euryanthe               -4      3       5  13.7    -0    0
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits at 17:32:01.20 -15:02:03.7:  15.52 +/- 99.00  upperlimit
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits at 17:32:01.20 -15:02:03.7:  15.42 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits  wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits -crosshair 2651.96143 4976.61914 image    wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits -crosshair 2644.45532 4982.26758 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18567 17 32 01.20 -15 02 03.7          13.6 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18541 17 32 01.29 -15 02 04.6          13.6 R      V36
     TAU0008  C2026 07 02.18592 17 32 01.10 -15 02 02.7          13.6 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1857*  17 32 01.20 -15 02 03.7  13.6 U             Ser       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6857,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1857 13.57CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1857  2461223.6857  13.62  18:03:25.64 -16:06:07.8
 13.15308   2.94347 galactic  Sgr  Second-epoch detections are separated by 2.2" and 9.2 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
1216 Askania                 -1      1       1  13.8     0   -0
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits at 18:03:25.64 -16:06:07.8:  15.35 +/- 99.00  upperlimit
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits at 18:03:25.64 -16:06:07.8:  15.32 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits  wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits -crosshair 7231.68701 4307.41943 image    wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits -crosshair 7224.67236 4313.43506 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18567 18 03 25.64 -16 06 07.8          13.6 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18541 18 03 25.66 -16 06 08.9          13.6 R      V36
     TAU0008  C2026 07 02.18592 18 03 25.63 -16 06 06.7          13.6 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1857*  18 03 25.64 -16 06 07.8  13.6 U             Sgr       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6857,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1857 13.62CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1857  2461223.6857  12.41  17:47:36.15 -16:20:58.6
 11.03425   6.11048 galactic  Sgr  Second-epoch detections are separated by 1.2" and 8.9 pix   
The object was found in VSX
 2"  ASAS J174736-1621.1           
Type: M
#   Max.           Min./Amp.       JD0           Period
    12.500   V            15.100   V         2451955.00000        190.600000000000   C                            
The object was not found in astcheck.
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits at 17:47:36.15 -16:20:58.6:  13.58 +/- 0.07  detection
Forced photometry on wcs_Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits at 17:47:36.15 -16:20:58.6:  13.23 +/- 0.05  detection
Forced photometry reference-image weighted average:  13.37 +/- 0.04
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits


Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits


fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs   wcs_Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits -crosshair 4708.60059 2212.45435 image    wcs_Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits -crosshair 4657.22949 2196.72021 image    wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits -crosshair 4928.02832 4189.10889 image    wcs_fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits -crosshair 4921.15137 4194.74561 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-04-23_05-59-28_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-05-11_04-27-53_20.00sec_-4.90C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-26-49_20.00sec_4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9/fd_Sgr-01-Q2b1x1_2026-07-01_23-27-33_20.00sec_5.00C_LIGHT_0027.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-01-Q2b1x1_232934_TTUQ2b1x1_3617269_af5h8XE9

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18567 17 47 36.15 -16 20 58.6          12.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18541 17 47 36.13 -16 20 59.1          12.4 R      V36
     TAU0008  C2026 07 02.18592 17 47 36.17 -16 20 58.1          12.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1857*  17 47 36.15 -16 20 58.6  12.4 U             Sgr       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J174736-1621.1,2461223.6857,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J174736-1621.1 20260702.1857 12.41CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1889  2461223.6889  12.71  18:49:20.01 -21:15:58.4
 13.61180  -9.07752 galactic  Sgr  Second-epoch detections are separated by 0.4" and 10.4 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
211 Isolda                   1     -1       1  12.7    -0    0
Forced photometry on wcs_Sgr-02-Q2b1x1_2026-05-12_05-16-10_20.00sec_-5.00C_LIGHT_0457.fits at 18:49:20.01 -21:15:58.4:  15.24 +/- 99.00  upperlimit
Forced photometry on wcs_Sgr-02-Q2b1x1_2026-05-14_02-33-41_20.00sec_-5.00C_LIGHT_0094.fits at 18:49:20.01 -21:15:58.4:  15.03 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-02-Q2b1x1_2026-05-12_05-16-10_20.00sec_-5.00C_LIGHT_0457.fits


fd_Sgr-02-Q2b1x1_2026-07-01_23-31-15_20.00sec_4.90C_LIGHT_0032.fits


fd_Sgr-02-Q2b1x1_2026-07-01_23-32-27_20.00sec_4.90C_LIGHT_0033.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-05-12_05-16-10_20.00sec_-5.00C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-02-Q2b1x1_233536_TTUQ2b1x1_832026_itDeo7AM/fd_Sgr-02-Q2b1x1_2026-07-01_23-31-15_20.00sec_4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-02-Q2b1x1_233536_TTUQ2b1x1_832026_itDeo7AM/fd_Sgr-02-Q2b1x1_2026-07-01_23-32-27_20.00sec_4.90C_LIGHT_0033.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Sgr-02-Q2b1x1_2026-05-12_05-16-10_20.00sec_-5.00C_LIGHT_0457.fits  wcs_fd_Sgr-02-Q2b1x1_2026-07-01_23-31-15_20.00sec_4.90C_LIGHT_0032.fits -crosshair 6093.40283 1204.82910 image    wcs_fd_Sgr-02-Q2b1x1_2026-07-01_23-32-27_20.00sec_4.90C_LIGHT_0033.fits -crosshair 6099.19531 1196.19104 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-05-12_05-16-10_20.00sec_-5.00C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-05-14_02-33-41_20.00sec_-5.00C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-02-Q2b1x1_233536_TTUQ2b1x1_832026_itDeo7AM/fd_Sgr-02-Q2b1x1_2026-07-01_23-31-15_20.00sec_4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-02-Q2b1x1_233536_TTUQ2b1x1_832026_itDeo7AM/fd_Sgr-02-Q2b1x1_2026-07-01_23-32-27_20.00sec_4.90C_LIGHT_0033.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-02-Q2b1x1_233536_TTUQ2b1x1_832026_itDeo7AM

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18891 18 49 20.01 -21 15 58.4          12.7 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18849 18 49 20.00 -21 15 58.3          12.7 R      V36
     TAU0008  C2026 07 02.18932 18 49 20.02 -21 15 58.4          12.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1889*  18 49 20.01 -21 15 58.4  12.7 U             Sgr       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6889,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1889 12.71CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1964  2461223.6964  11.90  19:03:54.48 +04:28:51.1
 38.34072  -0.72361 galactic  Aql  Second-epoch detections are separated by 0.7" and 8.6 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
849 Ara                     -0     -0       0  11.8     0    0
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits at 19:03:54.48 +04:28:51.1:  15.75 +/- 99.00  upperlimit
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits at 19:03:54.48 +04:28:51.1:  15.75 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits  wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits -crosshair 6620.21094 2276.99365 image    wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits -crosshair 6611.81445 2278.77441 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19638 19 03 54.48 +04 28 51.1          11.9 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19601 19 03 54.50 +04 28 51.0          11.9 R      V36
     TAU0008  C2026 07 02.19676 19 03 54.46 +04 28 51.3          11.9 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1964*  19 03 54.48 +04 28 51.1  11.9 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6964,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1964 11.90CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1964  2461223.6964  12.44  18:59:44.91 +02:09:35.9
 35.80183  -0.86271 galactic  Aql  Second-epoch detections are separated by 0.7" and 8.6 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
480 Hansa                   -1      0       1  12.3    -0    0
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits at 18:59:44.91 +02:09:35.9:  15.70 +/- 99.00  upperlimit
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits at 18:59:44.91 +02:09:35.9:  15.70 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits  wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits -crosshair 5988.77783 870.96143 image    wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits -crosshair 5980.40674 872.76251 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-42-04_20.00sec_5.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml/fd_Ser-04-Q2b1x1_2026-07-01_23-43-10_20.00sec_5.00C_LIGHT_0047.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_234540_TTUQ2b1x1_1466845_0vzE0Oml

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19638 18 59 44.91 +02 09 35.9          12.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19601 18 59 44.92 +02 09 35.6          12.4 R      V36
     TAU0008  C2026 07 02.19676 18 59 44.90 +02 09 36.3          12.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1964*  18 59 44.91 +02 09 35.9  12.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6964,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1964 12.44CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1974  2461223.6974  11.89  19:03:54.42 +04:28:51.5
 38.34071  -0.72334 galactic  Aql  Second-epoch detections are separated by 0.4" and 10.0 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
849 Ara                     -0      0       0  11.8     0    0
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits at 19:03:54.42 +04:28:51.5:  15.74 +/- 99.00  upperlimit
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits at 19:03:54.42 +04:28:51.5:  15.74 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits  wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits -crosshair 6612.04150 2278.02490 image    wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits -crosshair 6619.20361 2271.07056 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19738 19 03 54.42 +04 28 51.5          11.9 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19706 19 03 54.44 +04 28 51.4          11.9 R      V36
     TAU0008  C2026 07 02.19771 19 03 54.41 +04 28 51.5          11.9 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1974*  19 03 54.42 +04 28 51.5  11.9 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6974,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1974 11.89CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1974  2461223.6974  12.47  18:59:44.87 +02:09:35.7
 35.80170  -0.86259 galactic  Aql  Second-epoch detections are separated by 0.4" and 10.1 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
480 Hansa                   -0     -0       0  12.3    -0    0
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits at 18:59:44.87 +02:09:35.7:  15.70 +/- 99.00  upperlimit
Forced photometry on wcs_Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits at 18:59:44.87 +02:09:35.7:  15.70 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits


fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits  wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits -crosshair 5980.73779 871.94983 image    wcs_fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits -crosshair 5987.96143 864.87329 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-17-37_20.00sec_-4.90C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-05-10_05-18-40_20.00sec_-4.90C_LIGHTs_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-43-35_20.00sec_5.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf/fd_Ser-04-Q2b1x1_2026-07-01_23-44-32_20.00sec_5.00C_LIGHT_0049.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Ser-04-Q2b1x1_235533_TTUQ2b1x1_1637017_WiUBweaf

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19738 18 59 44.87 +02 09 35.7          12.5 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19706 18 59 44.88 +02 09 35.7          12.4 R      V36
     TAU0008  C2026 07 02.19771 18 59 44.85 +02 09 35.8          12.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1974*  18 59 44.87 +02 09 35.7  12.5 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6974,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1974 12.47CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1823  2461223.6823  13.64  16:42:09.50 -15:19:19.1
  2.94591  19.78096 galactic  Oph  Second-epoch detections are separated by 2.3" and 7.6 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
159 Aemilia                 -1      1       1  13.4     0   -0
Forced photometry on wcs_Oph-07-Q2b1x1_2026-05-13_03-29-49_20.00sec_-4.90C_LIGHTs_0326.fits at 16:42:09.50 -15:19:19.1:  15.59 +/- 99.00  upperlimit
Forced photometry on wcs_Oph-07-Q2b1x1_2026-05-13_03-30-24_20.00sec_-5.00C_LIGHTs_0327.fits at 16:42:09.50 -15:19:19.1:  15.55 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Oph-07-Q2b1x1_2026-05-13_03-29-49_20.00sec_-4.90C_LIGHTs_0326.fits


fd_Oph-07-Q2b1x1_2026-07-01_23-21-51_20.00sec_5.00C_LIGHT_0020.fits


fd_Oph-07-Q2b1x1_2026-07-01_23-22-53_20.00sec_4.90C_LIGHT_0021.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-05-13_03-29-49_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-07-Q2b1x1_232735_TTUQ2b1x1_3284574_oFAh0lhE/fd_Oph-07-Q2b1x1_2026-07-01_23-21-51_20.00sec_5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-07-Q2b1x1_232735_TTUQ2b1x1_3284574_oFAh0lhE/fd_Oph-07-Q2b1x1_2026-07-01_23-22-53_20.00sec_4.90C_LIGHT_0021.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Oph-07-Q2b1x1_2026-05-13_03-29-49_20.00sec_-4.90C_LIGHTs_0326.fits  wcs_fd_Oph-07-Q2b1x1_2026-07-01_23-21-51_20.00sec_5.00C_LIGHT_0020.fits -crosshair 3166.05542 4807.07471 image    wcs_fd_Oph-07-Q2b1x1_2026-07-01_23-22-53_20.00sec_4.90C_LIGHT_0021.fits -crosshair 3160.06470 4811.67041 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-05-13_03-29-49_20.00sec_-4.90C_LIGHTs_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-05-13_03-30-24_20.00sec_-5.00C_LIGHTs_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-07-Q2b1x1_232735_TTUQ2b1x1_3284574_oFAh0lhE/fd_Oph-07-Q2b1x1_2026-07-01_23-21-51_20.00sec_5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-07-Q2b1x1_232735_TTUQ2b1x1_3284574_oFAh0lhE/fd_Oph-07-Q2b1x1_2026-07-01_23-22-53_20.00sec_4.90C_LIGHT_0021.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-07-Q2b1x1_232735_TTUQ2b1x1_3284574_oFAh0lhE

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18233 16 42 09.50 -15 19 19.1          13.6 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18197 16 42 09.56 -15 19 19.9          13.6 R      V36
     TAU0008  C2026 07 02.18268 16 42 09.44 -15 19 18.4          13.7 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1823*  16 42 09.50 -15 19 19.1  13.6 U             Oph       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6823,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1823 13.64CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1953  2461223.6953  12.05  18:56:48.53 -01:05:24.3
 32.57375  -1.69196 galactic  Aql  Second-epoch detections are separated by 1.1" and 5.2 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
57 Mnemosyne               -0     -0       0  11.9    -0   -0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:56:48.53 -01:05:24.3:  15.23 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:56:48.53 -01:05:24.3:  15.20 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits -crosshair 5609.86230 3740.60181 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits -crosshair 5609.01562 3745.77930 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19530 18 56 48.53 -01 05 24.3          12.1 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19504 18 56 48.56 -01 05 24.1          12.1 R      V36
     TAU0008  C2026 07 02.19557 18 56 48.49 -01 05 24.5          12.0 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1953*  18 56 48.53 -01 05 24.3  12.1 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6953,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1953 12.05CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1953  2461223.6953  12.41  18:59:44.99 +02:09:35.4
 35.80186  -0.86307 galactic  Aql  Second-epoch detections are separated by 0.8" and 5.5 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
480 Hansa                   -0     -0       0  12.3    -0    0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:59:44.99 +02:09:35.4:  15.72 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:59:44.99 +02:09:35.4:  15.76 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits -crosshair 6070.77344 5708.23584 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits -crosshair 6070.04346 5713.67432 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19530 18 59 44.99 +02 09 35.4          12.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19504 18 59 44.99 +02 09 35.0          12.4 R      V36
     TAU0008  C2026 07 02.19557 18 59 44.99 +02 09 35.9          12.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1953*  18 59 44.99 +02 09 35.4  12.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6953,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1953 12.41CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1953  2461223.6953  13.52  18:34:00.52 -03:17:53.9
 28.00617   2.36533 galactic  Ser  Second-epoch detections are separated by 0.5" and 5.2 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
663 Gerlinde                -0     -0       1  13.6     0    0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:34:00.52 -03:17:53.9:  15.53 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:34:00.52 -03:17:53.9:  15.52 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits -crosshair 2154.06738 2421.86743 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits -crosshair 2153.39331 2427.06592 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-40-41_20.00sec_5.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW/fd_Aql-03-Q2b1x1_2026-07-01_23-41-26_20.00sec_4.90C_LIGHT_0045.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_235734_TTUQ2b1x1_1787600_cn61UGCW

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19530 18 34 00.52 -03 17 53.9          13.5 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19504 18 34 00.52 -03 17 54.1          13.6 R      V36
     TAU0008  C2026 07 02.19557 18 34 00.51 -03 17 53.6          13.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1953*  18 34 00.52 -03 17 53.9  13.5 U             Ser       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6953,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1953 13.52CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1800  2461223.6800  13.07  18:04:17.54 -29:18:17.1
  1.73948  -3.70707 galactic  Sgr  Second-epoch detections are separated by 1.6" and 5.4 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
160 Una                     -1     -1       1  13.1     0   -0
Forced photometry on wcs_Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits at 18:04:17.54 -29:18:17.1:  13.90 +/- 99.00  upperlimit
Forced photometry on wcs_Sgr-04-Q2b1x1_2026-04-23_06-07-42_20.00sec_-4.90C_LIGHTs_0332.fits at 18:04:17.54 -29:18:17.1:  14.25 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits


fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits


fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits  wcs_fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits -crosshair 3445.36035 1185.07520 image    wcs_fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits -crosshair 3440.15991 1183.51855 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-23_06-07-42_20.00sec_-4.90C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18004 18 04 17.54 -29 18 17.1          13.1 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.17976 18 04 17.60 -29 18 17.2          13.0 R      V36
     TAU0008  C2026 07 02.18031 18 04 17.48 -29 18 16.9          13.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1800*  18 04 17.54 -29 18 17.1  13.1 U             Sgr       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6800,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1800 13.07CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1800  2461223.6800  13.32  18:30:20.17 -25:37:50.3
  7.71543  -7.09223 galactic  Sgr  Second-epoch detections are separated by 1.6" and 5.7 pix   
The object was found in VSX
 1"  V4051 Sgr                     
Type: M
#   Max.           Min./Amp.       JD0           Period
    13.500   R            17.200   R         2439026.00000        272.500000000000                                
The object was not found in astcheck.
Forced photometry on wcs_Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits at 18:30:20.17 -25:37:50.3:  14.46 +/- 99.00  upperlimit
Forced photometry on wcs_Sgr-04-Q2b1x1_2026-04-23_06-07-42_20.00sec_-4.90C_LIGHTs_0332.fits at 18:30:20.17 -25:37:50.3:  14.77 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits


fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits


fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits  wcs_fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits -crosshair 6961.50391 3377.90649 image    wcs_fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits -crosshair 6956.05566 3376.27490 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-17_03-53-06_20.00sec_-4.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-04-23_06-07-42_20.00sec_-4.90C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-18-41_20.00sec_5.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5/fd_Sgr-04-Q2b1x1_2026-07-01_23-19-29_20.00sec_4.90C_LIGHT_0017.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Sgr-04-Q2b1x1_232136_TTUQ2b1x1_2660432_metJnly5

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18004 18 30 20.17 -25 37 50.3          13.3 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.17976 18 30 20.20 -25 37 49.7          13.3 R      V36
     TAU0008  C2026 07 02.18031 18 30 20.13 -25 37 50.9          13.3 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1800*  18 30 20.17 -25 37 50.3  13.3 U             Sgr       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V4051 Sgr,2461223.6800,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V4051 Sgr 20260702.1800 13.32CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1994  2461223.6994  11.39  19:14:31.37 +12:03:52.7
 46.28006   0.44634 galactic  Aql  Second-epoch detections are separated by 0.8" and 7.8 pix   This object is listed in tns_transients_list.txt    0.9"  AT 2026rdg  2026-07-01.30 12.53
The object was found in VSX
 9"  Gaia DR3 4312997401222073344  
Type: L
#   Max.           Min./Amp.       JD0           Period
    16.420   G            16.670   G                                                 M                            
The object was not found in astcheck.
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits  wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits -crosshair 1979.53369 2073.89233 image    wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits -crosshair 1986.42615 2070.33081 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-35-13_20.00sec_0.00C_LIGHT_1324.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19944 19 14 31.37 +12 03 52.7          11.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19914 19 14 31.34 +12 03 52.8          11.4 R      V36
     TAU0008  C2026 07 02.19974 19 14 31.39 +12 03 52.5          11.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1994*  19 14 31.37 +12 03 52.7  11.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4312997401222073344,2461223.6994,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4312997401222073344 20260702.1994 11.39CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1994  2461223.6994  11.43  19:14:31.40 +12:03:53.0
 46.28019   0.44627 galactic  Aql  Second-epoch detections are separated by 0.2" and 7.7 pix   This object is listed in tns_transients_list.txt    0.8"  AT 2026rdg  2026-07-01.30 12.53
The object was found in VSX
10"  Gaia DR3 4312997401222073344  
Type: L
#   Max.           Min./Amp.       JD0           Period
    16.420   G            16.670   G                                                 M                            
The object was not found in astcheck.
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits  wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits -crosshair 1979.58887 2073.90698 image    wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits -crosshair 1986.44775 2070.34033 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-35-13_20.00sec_0.00C_LIGHT_1324.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-46-36_20.00sec_5.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t/fd_Aql-01-Q2b1x1_2026-07-01_23-47-27_20.00sec_5.00C_LIGHT_0053.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-02_CI_Aql-01-Q2b1x1_000132_TTUQ2b1x1_1994314_M747797t

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19944 19 14 31.40 +12 03 53.0          11.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19914 19 14 31.40 +12 03 52.9          11.4 R      V36
     TAU0008  C2026 07 02.19974 19 14 31.40 +12 03 53.1          11.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1994*  19 14 31.40 +12 03 53.0  11.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4312997401222073344,2461223.6994,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4312997401222073344 20260702.1994 11.43CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1876  2461223.6876  10.78  17:49:55.25 -06:23:52.4
 20.03780  10.58827 galactic  Oph  Second-epoch detections are separated by 0.3" and 8.8 pix   
The object was found in VSX
25"  ASASSN-V J174954.35-062413.0  
Type: SR
#   Max.           Min./Amp.       JD0           Period
    14.840   V            15.270   V         2457227.00000        581.000000000000                                
The object was found in astcheck.  
51 Nemausa                  0     -0       0  10.9    -0   -0
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits at 17:49:55.25 -06:23:52.4:  15.46 +/- 0.35  detection
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits at 17:49:55.25 -06:23:52.4:  15.28 +/- 0.30  detection
Forced photometry reference-image weighted average:  15.36 +/- 0.23
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits  wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits -crosshair 3285.37280 5368.16016 image    wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits -crosshair 3277.41479 5371.92432 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18759 17 49 55.25 -06 23 52.4          10.8 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18731 17 49 55.26 -06 23 52.3          10.8 R      V36
     TAU0008  C2026 07 02.18786 17 49 55.24 -06 23 52.5          10.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1876*  17 49 55.25 -06 23 52.4  10.8 U             Oph       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174954.35-062413.0,2461223.6876,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174954.35-062413.0 20260702.1876 10.78CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1876  2461223.6876  11.25  17:54:03.89 -06:58:00.6
 20.04183   9.41250 galactic  Oph  Second-epoch detections are separated by 0.8" and 8.9 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
216 Kleopatra               -1      1       1  11.5    -0   -0
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits at 17:54:03.89 -06:58:00.6:  13.25 +/- 0.05  detection
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits at 17:54:03.89 -06:58:00.6:  13.36 +/- 0.05  detection
Forced photometry reference-image weighted average:  13.30 +/- 0.03
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits  wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits -crosshair 3910.00244 5021.69043 image    wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits -crosshair 3901.97168 5025.58203 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18759 17 54 03.89 -06 58 00.6          11.2 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18731 17 54 03.92 -06 58 00.7          11.2 R      V36
     TAU0008  C2026 07 02.18786 17 54 03.86 -06 58 00.6          11.2 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1876*  17 54 03.89 -06 58 00.6  11.2 U             Oph       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6876,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1876 11.25CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1876  2461223.6876  13.46  18:07:03.29 -13:38:49.3
 15.72804   3.37424 galactic  Ser  Second-epoch detections are separated by 1.1" and 8.6 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
540 Rosamunde                0      0       0  13.4     0   -0
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits at 18:07:03.29 -13:38:49.3:  15.45 +/- 99.00  upperlimit
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits at 18:07:03.29 -13:38:49.3:  15.47 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits  wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits -crosshair 5821.40283 968.73169 image    wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits -crosshair 5813.83643 972.88220 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18759 18 07 03.29 -13 38 49.3          13.5 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18731 18 07 03.29 -13 38 49.8          13.4 R      V36
     TAU0008  C2026 07 02.18786 18 07 03.30 -13 38 48.7          13.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1876*  18 07 03.29 -13 38 49.3  13.5 U             Ser       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6876,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1876 13.46CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1876  2461223.6876  13.51  18:05:57.92 -08:35:23.4
 20.04417   6.04757 galactic  Ser  Second-epoch detections are separated by 0.8" and 8.8 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
205 Martha                  -1      1       1  13.4    -0   -0
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits at 18:05:57.92 -08:35:23.4:  15.68 +/- 99.00  upperlimit
Forced photometry on wcs_Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits at 18:05:57.92 -08:35:23.4:  15.69 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits


fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits  wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits -crosshair 5687.98828 4030.88867 image    wcs_fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits -crosshair 5680.07959 4034.80322 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-01-38_20.00sec_-0.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-05-16_03-02-19_20.00sec_-0.00C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-29-33_20.00sec_5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3/fd_Oph-06-Q2b1x1_2026-07-01_23-30-21_20.00sec_5.00C_LIGHT_0031.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Oph-06-Q2b1x1_233934_TTUQ2b1x1_1244336_ghpW3Up3

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.18759 18 05 57.92 -08 35 23.4          13.5 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.18731 18 05 57.94 -08 35 23.5          13.5 R      V36
     TAU0008  C2026 07 02.18786 18 05 57.89 -08 35 23.3          13.5 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1876*  18 05 57.92 -08 35 23.4  13.5 U             Ser       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6876,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1876 13.51CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1945  2461223.6945  12.07  18:56:48.60 -01:05:24.6
 32.57381  -1.69226 galactic  Aql  Second-epoch detections are separated by 0.5" and 8.8 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
57 Mnemosyne                0     -0       1  11.9    -0   -0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:56:48.60 -01:05:24.6:  15.23 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:56:48.60 -01:05:24.6:  15.20 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits -crosshair 5601.94824 3737.24121 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits -crosshair 5609.86279 3741.15039 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19447 18 56 48.60 -01 05 24.6          12.1 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19419 18 56 48.62 -01 05 24.6          12.1 R      V36
     TAU0008  C2026 07 02.19475 18 56 48.59 -01 05 24.6          12.1 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1945*  18 56 48.60 -01 05 24.6  12.1 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6945,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1945 12.07CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1945  2461223.6945  12.40  18:59:45.04 +02:09:35.0
 35.80185  -0.86331 galactic  Aql  Second-epoch detections are separated by 0.4" and 8.9 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
480 Hansa                   -0     -0       0  12.3    -0    0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:59:45.04 +02:09:35.0:  15.72 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:59:45.04 +02:09:35.0:  15.77 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits -crosshair 6062.94385 5704.95361 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits -crosshair 6070.91699 5708.92725 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19447 18 59 45.04 +02 09 35.0          12.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19419 18 59 45.02 +02 09 35.0          12.4 R      V36
     TAU0008  C2026 07 02.19475 18 59 45.05 +02 09 35.0          12.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1945*  18 59 45.04 +02 09 35.0  12.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6945,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1945 12.40CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1945  2461223.6945  13.69  18:34:00.54 -03:17:54.3
 28.00611   2.36521 galactic  Ser  Second-epoch detections are separated by 0.8" and 8.9 pix   
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.  
663 Gerlinde                -1     -1       1  13.6     0    0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:34:00.54 -03:17:54.3:  15.53 +/- 99.00  upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:34:00.54 -03:17:54.3:  15.52 +/- 99.00  upperlimit
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits


fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits  wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits -crosshair 2146.01514 2418.78369 image    wcs_fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits -crosshair 2154.00000 2422.63013 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-39-27_20.00sec_5.00C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS/fd_Aql-03-Q2b1x1_2026-07-01_23-40-16_20.00sec_5.00C_LIGHT_0043.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-03-Q2b1x1_234938_TTUQ2b1x1_1540565_0o1Pf1oS

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19447 18 34 00.54 -03 17 54.3          13.7 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19419 18 34 00.57 -03 17 54.5          13.6 R      V36
     TAU0008  C2026 07 02.19475 18 34 00.52 -03 17 54.1          13.8 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1945*  18 34 00.54 -03 17 54.3  13.7 U             Ser       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461223.6945,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260702.1945 13.69CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1986  2461223.6986  11.37  19:14:31.35 +12:03:53.3
 46.28017   0.44649 galactic  Aql  Second-epoch detections are separated by 0.4" and 7.1 pix   This object is listed in tns_transients_list.txt    0.4"  AT 2026rdg  2026-07-01.30 12.53
The object was found in VSX
 9"  Gaia DR3 4312997401222073344  
Type: L
#   Max.           Min./Amp.       JD0           Period
    16.420   G            16.670   G                                                 M                            
The object was not found in astcheck.
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits  wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits -crosshair 1985.13037 2070.24805 image    wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits -crosshair 1979.50586 2074.58252 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-35-13_20.00sec_0.00C_LIGHT_1324.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19859 19 14 31.35 +12 03 53.3          11.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19832 19 14 31.36 +12 03 53.3          11.4 R      V36
     TAU0008  C2026 07 02.19885 19 14 31.34 +12 03 53.3          11.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1986*  19 14 31.35 +12 03 53.3  11.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4312997401222073344,2461223.6986,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4312997401222073344 20260702.1986 11.37CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp

Mean magnitude and position on the discovery images: 
                   2026 07 02.1986  2461223.6986  11.38  19:14:31.41 +12:03:53.3
 46.28028   0.44627 galactic  Aql  Second-epoch detections are separated by 0.7" and 7.1 pix   This object is listed in tns_transients_list.txt    0.7"  AT 2026rdg  2026-07-01.30 12.53
The object was found in VSX
 9"  Gaia DR3 4312997401222073344  
Type: L
#   Max.           Min./Amp.       JD0           Period
    16.420   G            16.670   G                                                 M                            
The object was not found in astcheck.
Check this position in TNS.                         Manually check the ASAS-SN list of transients!
Search this object in SIMBAD.
Search this object in VizieR catalogs.  WISE atlas  Aladin Lite  SNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.

Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits


fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits

# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i ;done
# Display the solved FITS images
ds9 -frame lock wcs  wcs_Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits  wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits -crosshair 1985.16663 2070.26807 image    wcs_fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits -crosshair 1979.53345 2074.59790 image   

./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-34-34_20.00sec_0.00C_LIGHT_1323.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-05-17_05-35-13_20.00sec_0.00C_LIGHT_1324.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-45-25_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm/fd_Aql-01-Q2b1x1_2026-07-01_23-46-11_20.00sec_4.90C_LIGHT_0051.fits  && util/transients/search_for_transients_single_field.sh

REFERENCE_IMAGES=/data_ssd/NMW-TexasTech/reference_imgs  util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-01_CI_Aql-01-Q2b1x1_235332_TTUQ2b1x1_1630180_nquzALcm

Don't forget to copy the leading white spaces and change the observatory code! The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter. Make sure there are no trailing white spaces after the observatory code. The string should be exactly 80 characters long to conform to the MPC format.
Mean position:

     TAU0008  C2026 07 02.19859 19 14 31.41 +12 03 53.3          11.4 R      V36

Position measured on individual images:

     TAU0008  C2026 07 02.19832 19 14 31.42 +12 03 53.6          11.4 R      V36
     TAU0008  C2026 07 02.19885 19 14 31.39 +12 03 53.0          11.4 R      V36

You may copy/paste the above measurements to the following online services:
MPChecker (in case the button does not work)
NEOCMTChecker (NEO's and comets)
sat_id2 (artificial satellites; needs at least two observations to work)
fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)

Here is a stub line for reporting a new transient to the TOCP. Don't forget to set the constellation name and the number of days since the last non-detection!

TCP 2026 07 02.1986*  19 14 31.41 +12 03 53.3  11.4 U             Aql       9 0

Don't forget to change the observer code for the AAVSO and VSNET format data!

 **** AAVSO file format ****

#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4312997401222073344,2461223.6986,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS


 **** VSNET file format ****

# Here are some valid formatiing examples:
#CETFZ 20230815.9829   <13.5CV NMW
#CETFZ 20230818.9746    12.5CV NMW
#CETFZ 20230819.9732    12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4312997401222073344 20260702.1986 11.38CV NMW


The AAVSO data should be submitted to https://www.aavso.org/webobs

The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to  vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp