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 | G332.5-5.6 CENTER | 250.7335 | -54.5135 | 249.725841 | -54.419293 | 256.94436 | -31.940577 | 332.53119736 | -5.54004522 | 262.5079 | 54330.694224537 | 2007-08-18 16:39:41 | 54331.8731944444 | 2007-08-19 20:57:24 | 502066010 | 70.1488 | 80 | 70.1488 | 70.1488 | 0 | 70.1568 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 71.4907 | 71.4907 | 101.8399 | 0 | PROCESSED | 57539.62875 | 2016-05-31 15:05:24 | 54721 | 2008-09-12 00:00:00 | 54354.4910300926 | 2007-09-11 11:47:05 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021216 | We propose to observe G332.5-5.6, a puzzling supernova remnant with several unusual features: high radio polarization, central emission with bilaterally symmetric limbs, and evidence for enhanced nitrogen suggesting interaction with processed circumstellar material. Very little is known about G332.5-5.6, so our observations will provide information on the remnant shock speed, age, and evolutionary state; on the possible presence of nonthermal emission, either due to a pulsar in the center or to shock-accelerated electrons in the limbs; and on abundances, which might identify ejecta emission and allow the classification of the supernova. | GALACTIC DIFFUSE EMISSION | 5 | B | STEPHEN REYNOLDS | USA | 2 | AO2 | G332.5-5.6: AN UNUSUAL SUPERNOVA REMNANT WITH CIRCUMSTELLAR INTERACTION | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502066010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502066010'
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