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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201111010 V2400_OPH 258.15135 -24.2459 257.38821 -24.18691 259.20708 -1.24944 359.86634 8.73969 274.12526 60902.58963 2025-08-15 14:09:04 60907.21532 2025-08-20 05:10:04 237.744 200.000 237.744 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2025-08-30 07:49:54 2026-09-03 00:00:00 2025-08-31 07:49:54 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012196 Masses of white dwarfs (WDs) play an important role in understanding their formation and evolution. A unique way to estimate the mass of a WD in an Intermediate Polar (IP) is to estimate the gravitational redshift of emission lines. We propose 200 kilosec XRISM observations to carry out accurate estimation of the gravitational redshift of emission lines in an IP V2400 Oph and use these measurements to accurately estimate the mass of the WD. The proposed XRISM observation would also serve as a benchmark for carrying out similar investigations for several other moderately bright IPs in future cycles and to estimate the mass of the WDs. ACCRETING WHITE DWARFS AND NOVAE 2 B NAZMA ISLAM USA 1 NOR ESTIMATING THE MASS OF THE WHITE DWARF IN THE INTERMEDIATE POLAR V2400 OPH USING XRISM OBSERVATIONS archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201111010/ Quick Look 258.1227 -24.26847 258.17903 -24.27221 258.18231 -24.22959 258.17301 -24.22902 258.17374 -24.22058 258.12685 -24.21737 257.35945 -24.20935 257.41572 -24.21336 257.41925 -24.17075 257.40996 -24.17014 257.41074 -24.1617 257.36389 -24.15827 259.18289 -1.27408 259.23438 -1.27361 259.23389 -1.23088 259.22538 -1.23101 259.22536 -1.22254 259.18247 -1.22284 359.83245 8.74806 359.85924 8.70391 359.89626 8.72597 359.89179 8.73324 359.89917 8.73754 359.87693 8.77437 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201111010'

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