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 G306.3-0.9 200.4753 -63.5602 199.643661 -63.298602 230.10249 -49.420915 306.31531317 -0.88874973 306.5675 56889.7845833333 2014-08-20 18:49:48 56894.0099768518 2014-08-25 00:14:22 509072010 190.0114 200 190.0181 190.0114 0 190.0114 2 2 0 2 1 0 0 14.4515 14.4515 20.22 0 PROCESSED 57616.5396759259 2016-08-16 12:57:08 57305 2015-10-10 00:00:00 56938.2302777778 2014-10-08 05:31:36 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 093109 The origin of the distorted, inhomogeneous structure of mixed-morphology SNRs (MM SNRs) is a mystery. Recently we have discovered recombining plasma from MM SNRs. The existence of recombining plasma implies rapid cooling process in past. Recombining plasma, together with the peculiar morphologies, would indicate a new SNR evolution scenario. Our systematic analysis of recombining SNRs shows that the recombination ages are almost the same, although their dynamical ages range over an order of magnitude. Such a trend can be explained by past rapid rarefaction. This hypothesis can be tested by measuring a recombination age of a dynamically young recombining SNR. We thus propose a 100-ks Suzaku observation of G306.3-0.9, a candidate of the youngest recombining SNR ever. GALACTIC DIFFUSE EMISSION 5 A MAKOTO SAWADA Reynolds,Matsumura JUS 9 AO9 THE DYNAMICS OF MIXED-MORPHOLOGY SNRS PROBED BY THE YOUNGEST RECOMBINING PLASMA XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509072010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509072010'

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