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
1 VELA PWN NE1 129.3684 -44.9817 128.942936 -44.80588 153.830902 -60.001311 263.62243766 -2.36980886 142.6395 55916.6230439815 2011-12-21 14:57:11 55917.0070601852 2011-12-22 00:10:10 506041010 15.408 15 15.424 15.408 0 15.424 1 1 0 1 1 0 0 11.5681 11.5681 33.1759 1 PROCESSED 57604.1925347222 2016-08-04 04:37:15 56305 2013-01-13 00:00:00 55937.7788310185 2012-01-11 18:41:31 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061302 Located only ~290 pc from Earth, the Vela PWN is one of the best targets for the study of PWNe. Its radio and gamma-ray surface brightness peaks to the south of the pulsar, suggesting that the nebula was crushed by the reverse shock which propagated more rapidly from the north than the south through an inhomogeneous ambient medium. The X-ray morphology is not yet known. Recently, we found that the X-ray extent is larger than the radio extent in the northeastern and eastern directions. We here propose ten Suzaku XIS observations in these two directions to study the history of the Vela PWN; for instance, to investigate whether the radio-emitting PWN is the relic of PWN-reverse shock interactions, whereas the X-ray-emitting PWN is more recently formed by freshly injected particles. GALACTIC DIFFUSE EMISSION 5 C SATORU KATSUDA USA 6 AO6 THE X-RAY MORPHOLOGY OF THE VELA PULSAR WIND NEBULA XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506041010'

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