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 G296.1-0.5N 177.8287 -62.3875 177.210977 -62.109277 215.982021 -55.076396 296.02814016 -0.3243747 322.3815 54321.2538541667 2007-08-09 06:05:33 54323.4522453704 2007-08-11 10:51:14 502068010 77.1759 67 77.1759 77.1759 0 77.1759 2 2 0 2 1 0 0 68.4846 68.4846 189.9237 1 PROCESSED 57539.4859953704 2016-05-31 11:39:50 54716 2008-09-07 00:00:00 54347.5137268518 2007-09-04 12:19:46 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021218 Supernova (SN) explosions within wind-blown bubbles are common among core-collapse (CC) SNe, and are expected to occur for some Type Ia SNe. We propose observations of an X-ray bright supernova remnant (SNR), G296.1-0.5, with very strong evidence for an explosion within a bubble. Spectroscopy with Suzaku will provide us with temperatures, abundances, and ionization ages of the X-ray emitting gas. If we detect SN ejecta, we will distinguish between a CC or a Type Ia progenitor. Gas temperatures will provide us with the shock speeds, while ionization ages will tell us when this gas was shocked. We will infer how progenitor winds affected the ambient medium prior to the explosion. The proposed observations will advance our knowledge of poorly understood SNR evolution in wind-blown bubbles. GALACTIC DIFFUSE EMISSION 5 B KAZIMIERZ BORKOWSKI USA 2 AO2 G296.1-0.5: A SUPERNOVA EXPLOSION WITHIN A BUBBLE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502068010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502068010'

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