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 CAS A 351.0231 59.0265 350.456601 58.751794 27.744986 54.948342 111.88943817 -1.95981315 208.1115 54876.0965740741 2009-02-14 02:19:04 54876.8363310185 2009-02-14 20:04:19 503080010 30.0355 30 30.0355 30.0355 0 30.0355 2 2 0 2 1 0 0 30.0731 30.0731 63.9139 0 PROCESSED 57545.551087963 2016-06-06 13:13:34 55330 2010-05-14 00:00:00 54892.9889699074 2009-03-02 23:44:07 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030127 Cas A is the youngest supernova remnant(SNR) in our Galaxy. Recently, the Spitzer Space Telescope discovered moving structures nearly at the speed of light outside the shell of the SNR. These structures are likely infrared echoes, where interstellar dust is heated by the outward moving photon shell of a bright flash. The bright flash is probably due to a giant flare from the central point source of Cas A, and if so, it requires that the central point source is a magnetar. Magnetars are known to emit luminous flares in the X-ray band, so it is expected that we can detect Fe-K fluorescence emission accompanied by IR echo. Here, we propose to observe on IR-emitting cloud around Cas A for 30ks to search for Fe-K emission which is naturally expected if the central point source is a magnetar. GALACTIC DIFFUSE EMISSION 5 C HIROYUKI AONO JAP 3 AO3 INVESTIGATION OF A X-RAY ECHO NEAR THE SUPERNOVA REMNANT CASSIOPEIA A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503080010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503080010'

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