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 2FGL J0923.5+1508 140.9887 15.0811 140.300178 15.296347 138.613889 -0.175811 215.96780071 40.48329137 287.9737 56046.2642939815 2012-04-29 06:20:35 56048.4933449074 2012-05-01 11:50:25 707007010 95.2554 90 95.2794 95.2554 0 95.2794 2 2 0 2 1 0 0 89.5878 89.5878 192.568 1 PROCESSED 57605.3423611111 2016-08-05 08:13:00 56434 2013-05-22 00:00:00 56068.6261921296 2012-05-21 15:01:43 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070024 We propose X-ray follow up observations of two high redshift blazar candidates in the Fermi/LAT unidentified sources. The aim of this proposal is to detect X-ray emissions from high redshift blazars (z >> 3) buried in unidentified Fermi/LAT sources and to find the most distant LAT detected blazar. Gamma-ray photons above 10 GeV are attenuated by interactions with UV photons which result in creating electron-positron pairs. Therefore, attenuation signatures are predicted to be observed in gamma-ray spectra and such attenuation of high redshift blazars with redshift up to z ~ 6 provide information about UV background out to the epoch of cosmological reionization. By utilizing the attenuation, we can investigate the UV radiation state of the early universe. EXTRAGALACTIC COMPACT SOURCES 7 B YOSUKE TAKAHASHI JAP 7 AO7 SUZAKU OBSERVATIONS OF HIGH REDSHIFT BLAZAR CANDIDATES IN THE FERMI UNIDENTIFIED SOURCE SAMPLE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707007010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707007010'

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