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 G21.5-0.9 278.4038 -10.5066 277.711815 -10.545632 278.460388 12.687474 21.56207071 -0.86897985 103.5553 54190.0674074074 2007-03-31 01:37:04 54191.7405671296 2007-04-01 17:46:25 502065020 53.5261 100 53.5261 53.551 0 53.5661 1 2 0 1 1 0 0 48.618 48.618 144.5418 0 PROCESSED 57538.0817013889 2016-05-30 01:57:39 54695 2008-08-17 00:00:00 54200.5054861111 2007-04-10 12:07:54 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021211 We propose an observation of the supernova remnant (SNR) G21.5--0.9. This SNR has a centrally peaked X-ray morphology which coupled with its non-thermal emission, suggested that the SNR's central engine was an undetected pulsar. Last year, a radio pulsar associated with the remnant was discovered (Gupta et al. 2005; Camilo et al. 2006). These announcements concur on the period of the pulsar and its period derivative making it the second highest spin-down luminosity pulsar. Deep Chandra imaging uncovered the missing shell (Matheson & Safi-Harb, 2005). Recent INTEGRAL and SWIFT/BAT slew observations detected G21.5--0.9 at more than 10 and 8 sigma respectively. The proposed observation will be the first self-consistent broad-band timing and spectral analysis from soft to very hard X-ray. GALACTIC DIFFUSE EMISSION 5 B ILANA HARRUS USA 2 AO2 SUZAKU OBSERVATIONS OF THE SUPERNOVA REMNANT G21.5-0.9 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502065020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502065020'

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