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 G352.7-0.1 261.9227 -35.1119 261.088463 -35.070764 263.245639 -11.859611 352.75195989 -0.12120729 94.0335 55988.8605671296 2012-03-02 20:39:13 55993.5536111111 2012-03-07 13:17:12 506052010 201.5474 200 201.5474 201.5474 0 201.5474 2 2 0 2 1 0 0 171.544 171.544 405.4396 4 PROCESSED 57604.9422569445 2016-08-04 22:36:51 56375 2013-03-24 00:00:00 56008.397337963 2012-03-22 09:32:10 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061315 Supernova remnants showing strong Fe K emission are relatively rare, and primarily of Type Ia. We propose a long observation of one of the least well-studied Fe-rich Galactic SNRs, G352.7-0.1, with the goal of characterizing the Fe emission, confirming its likely identification as the remnant of a Type Ia supernova, and constraining the properties of ejected material and the dynamics of the explosion. Its thermal X-ray spectrum is strikingly similar to Tycho's SNR, but unexpectedly X-rays are uniformly distributed throughout the remnant. Our proposed observation will produce high-quality spectra, adequate for detailed studies with some spatial information, that will greatly aid in understanding of this very interesting young remnant. GALACTIC DIFFUSE EMISSION 5 C KAZIMIERZ BORKOWSKI USA 6 AO6 STRONG IRON EMISSION IN THE SUPERNOVA REMNANT G352.7-0.1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506052010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506052010'

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