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 CYGNUS LOOP (P23) 312.4772 32.3587 311.966597 32.171629 327.828669 47.6396 75.1675214 -7.32455162 61.8892 54620.7530439815 2008-06-03 18:04:23 54621.1473842593 2008-06-04 03:32:14 503059010 19.457 15 19.457 19.457 0 19.457 1 1 0 1 1 0 0 17.2771 17.2771 34.0639 0 PROCESSED 57542.7106944444 2016-06-03 17:03:24 55003 2009-06-21 00:00:00 54636.2328240741 2008-06-19 05:35:16 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030074 The Cygnus Loop is a prototypical middle-aged SNR. Based on the previous observation, the shell region shows relatively low temperature with low metal abundance while the interior shows high temperature with high metal abundance. The plasma in the interior is the fossil of the progenitor star. Recently, we found a region in the central part of the Loop where the shell is very thin. The observation in this region will show the precise mass of the progenitor star. We found most of the shell region showed extremely low abundance. This may suggest that the plasma in the shell region consists of a thin thermal spectrum and a non-thermal spectrum. We may be able to find a region showing non-thermal emission. We propose to observe the Cygnus Loop for 180ks. GALACTIC DIFFUSE EMISSION 5 B HIROSHI TSUNEMI JAP 3 AO3 SUZAKU OBSERVATIONS OF THE CYGNUS LOOP XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503059010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503059010'

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