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 VELAFRAGG TAIL 125.0448 -47.7009 124.65466 -47.541789 151.337516 -63.864294 264.09848727 -6.37839252 263.1844 55658.0366898148 2011-04-07 00:52:50 55658.8565162037 2011-04-07 20:33:23 506057010 49.3543 50 49.3703 49.3543 0 49.3703 3 2 0 2 1 0 0 43.9581 43.9581 70.8259 1 PROCESSED 57601.4287268518 2016-08-01 10:17:22 56043 2012-04-26 00:00:00 55673.1976736111 2011-04-22 04:44:39 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 062021 The Vela supernova remnant (SNR) displays remarkable features which appear to be ejecta ``shrapnel'' visible beyond the main shell. One of these shrapnel (A) is distinct from the others in that its X-ray spectrum exhibits a high Si abundance, while the other shrapnel exhibit enhanced O, Ne, and Mg abundances. One unexplored ejecta shrapnel (G) is located on the opposite side of the remnant from shrapnel A, suggesting that the SN explosion may have resulted in a jet-counterjet Si-rich structure, reminiscent of Cas A. We propose to observe this shrapnel for the first time to determine if it is also Si-rich like shrapnel A. If this is the case, the Vela SNR may be the first direct evidence of a jet-induced SN explosion. GALACTIC DIFFUSE EMISSION 5 A FABRIZIO BOCCHINO EUR 6 AO6 ASYMMETRIC SN EXPLOSION IN VELA SNR XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506057010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506057010'

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