DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | PERSEUS CLUSTER | 49.9436 | 41.5175 | 49.116107 | 41.336843 | 58.603575 | 22.345195 | 150.56798595 | -13.25929387 | 66.0393 | 53976.788275463 | 2006-08-29 18:55:07 | 53980.0793865741 | 2006-09-02 01:54:19 | 101012010 | 150.9051 | 150 | 150.9051 | 150.9211 | 150.9371 | 150.9211 | 6 | 6 | 6 | 6 | 1 | 0 | 0 | 142.5334 | 142.5334 | 284.336 | 3 | PROCESSED | 57535.5159375 | 2016-05-27 12:22:57 | 53826 | 2006-04-01 00:00:00 | 54024.8648726852 | 2006-10-16 20:45:25 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 015016 | We propose the observation of Perseus cluster for 150ks. To recover the energy resolution of the XIS, we will try the periodic charge injection method. However, the charge injection will change calibrations such as gain, QE and so on dramatically. To study the change of the clibrations, Perseus cluster is one of the best targets, because it is extended over the whole XIS FOV and the iron K line from the cluster is extremely strong. For the first 50ks, the observation will be done with the normal mode without the charge injection. For the second and third 50ks, we will do the charge injections with every 54 and 108 rows, repectively. | CALIBRATION | 1 | A | HIRONORI MATSUMOTO | JAP | 1 | AO1 | PERSEUS OBSERVATION FOR CALIBRATIONS ON THE PERIODIC CHARGE INJECTION METHOD | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/101012010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '101012010'
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