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 NGC4418 186.7074 -0.9383 186.066307 -0.661629 186.526079 1.80107 290.03230216 61.31559989 292.8039 53929.4791898148 2006-07-13 11:30:02 53931.280775463 2006-07-15 06:44:19 701001010 68.3485 70 68.3485 68.3485 68.3485 68.3485 2 2 2 2 1 0 0 57.1103 57.1103 155.634 1 PROCESSED 57534.9858564815 2016-05-26 23:39:38 54408 2007-11-04 00:00:00 53942.4601388889 2006-07-26 11:02:36 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010001 We propose Suzaku observations at E > 10 keV of nearby ultraluminous infrared galaxies (ULIRGs), for which our infrared spectroscopy has strongly suggested the presence of luminous AGNs deeply buried in gas and dust. However, extreme starbursts are still a possibility. Through the proposed X-ray observations using Suzaku, we aim to distinguish clearly between buried AGNs (strong X-ray emitters) and extreme starbursts (weak X-ray emitters), and to obtain convincing evidence for luminous buried AGNs. Since buried AGNs in these ULIRGs' cores are likely to suffer from Compton-thick X-ray absorption, the high sensitivity at E > 10 keV achieved by Suzaku HXD PIN is crucial for the success of this experiment. EXTRAGALACTIC COMPACT SOURCES 7 A MASATOSHI IMANISHI JAP 1 AO1 COMPTON THICK BURIED AGNS IN NEARBY ULTRALUMINOUS INFRARED GALAXIES HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701001010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701001010'

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